WorldWideScience

Sample records for alma los informes

  1. Ingenieros del alma: los informes sobre canción popular, ensayo y Ciencias Sociales de los servicios de inteligencia de la dictadura militar argentina sobre América Latina Engineers of the soul: reports from the Argentine military dictatorship's intelligence services on Latin American popular song, essays, and the social sciences

    OpenAIRE

    Patricia Funes

    2007-01-01

    El artículo se propone reconstruir y analizar los informes de los servicios de inteligencia sobre la producción acerca de América Latina durante la última dictadura militar argentina (1976-1983). Partimos de la hipótesis que el concepto "América Latina" es connotado a priori como "subversivo, "comunista", "revolucionario". Lo anterior podría explicar la profusión de informes de inteligencia sobre las ciencias sociales latinoamericanas de los años sesenta y setenta, así como también los centro...

  2. Ingenieros del alma: los informes sobre canción popular, ensayo y Ciencias Sociales de los servicios de inteligencia de la dictadura militar argentina sobre América Latina Engineers of the soul: reports from the Argentine military dictatorship's intelligence services on Latin American popular song, essays, and the social sciences

    Directory of Open Access Journals (Sweden)

    Patricia Funes

    2007-12-01

    Full Text Available El artículo se propone reconstruir y analizar los informes de los servicios de inteligencia sobre la producción acerca de América Latina durante la última dictadura militar argentina (1976-1983. Partimos de la hipótesis que el concepto "América Latina" es connotado a priori como "subversivo, "comunista", "revolucionario". Lo anterior podría explicar la profusión de informes de inteligencia sobre las ciencias sociales latinoamericanas de los años sesenta y setenta, así como también los centros de estudio, las revistas, e incluso la canción popular encontrados en el Archivo de la ex Dirección de Inteligencia de la Policía de la Provincia de Buenos Aires [DIPBA], fondo privilegiado para la reconstrucción sobre las formas y significados de la construcción de la categoría "delincuente subversivo" por parte de los servicios de inteligencia sobre el campo cultural argentino.The paper aims to trace, to reconstruct and to analyze the records of the Intelligence Services regarding the production of Latin-American social sciences in the period 1976-1983. The object "Latin America" is to the services of intelligence a priori associated with and connoting "communist", "revolutionary" or "subversive". All the above led to an exhaustive work of exegesis and research on the production of Latin-American Social Sciences describing a double process: introducing professionalism in politics and political radicalization. The documents found in the Archive of the former Direction of Intelligence of the Police of the Province of Buenos Aires [DIPBA] -(containing reports of other services of intelligence allow to infer the importance and the degree of "danger" that the dictatorships attributed to this production. This research will analyze reports issued by Intelligence Offices on popular music, essays and, particularly, classic works produced by Latin American Social Sciences.

  3. ALMA science operations

    Science.gov (United States)

    Nyman, Lars-Åke; Andreani, Paola; Hibbard, John; Okumura, Sachiko K.

    2010-07-01

    The ALMA (Atacama Large Millimeter/submillimeter Array) project is an international collaboration between Europe, East Asia and North America in cooperation with the Republic of Chile. The ALMA Array Operations Site (AOS) is located at Chajnantor, a plateau at an altitude of 5000 m in the Atacama desert in Chile, and the ALMA Operations Support Facility (OSF) is located near the AOS at an altitude of 2900 m. ALMA will consist of an array of 66 antennas, with baselines up to 16 km and state-of-the-art receivers that cover all the atmospheric windows up to 1 THz. An important component of ALMA is the compact array of twelwe 7-m and four 12-m antennas (the Atacama Compact Array, ACA), which will greatly enhance ALMA's ability to image extended sources. Construction of ALMA started in 2003 and will be completed in 2013. Commissioning started in January 2010 and Early Science Operations is expected to start during the second half of 2011. ALMA science operations is provided by the Joint ALMA Observatory (JAO) in Chile, and the three ALMA Regional Centers (ARCs) located in each ALMA region - Europe, North America and East Asia. ALMA observations will take place 24h per day, interrupted by maintenance periods, and will be done in service observing mode with flexible (dynamic) scheduling. The observations are executed in the form of scheduling blocks (SBs), each of which contains all information necessary to schedule and execute the observations. The default output to the astronomer will be pipeline-reduced images calibrated according to the calibration plan. The JAO is responsible for the data product quality. All science and calibration raw data are captured and archived in the ALMA archive, a distributed system with nodes at the OSF, the Santiago central office and the ARCs. Observation preparation will follow a Phase 1/Phase 2 process. During Phase 1, observation proposals will be created using software tools provided by the JAO and submitted for scientific and

  4. La metáfora de la luz como expresión del alma en “Livia y los sueños” de Jesús Gardea

    OpenAIRE

    María del Rosario Lara

    2014-01-01

    En el presente artículo exploramos la expresión artística de la idea de alma a través de la metáfora de la luz tal y como aparece en “Livia y los sueños” . Para ello, nos basare - mos en los postulados filosóficos de María Zambrano referentes a las concepciones de alma, ser humano y destino. En nuestra investigación también abordaremos la forma como tiempo y espacio en la obra de Gardea integran un cronotopo específico, como base donde la idea de alma puede desplegarse en toda su plenitud....

  5. Observaci\\'on de lentes gravitatorias con ALMA

    CERN Document Server

    Bonilla, A; Fuentes, I; Motta, V

    2016-01-01

    Gravitational lensing is a fundamental tool for cosmology. A recent instrument which will provide more information for models of these objects is ALMA. Our goal is to select lens candidates to observe with ALMA and then model them using GravLens Software. We had selected 12 quadruple images systems from the CASTLES database, which show a high probability of observing extended sources in the submillimetric range. These new data will allow us to improve existing models. Las lentes gravitatorias son una herramienta fundamental para la cosmolog\\'ia. Un nuevo instrumento que nos proporcionar\\'a mayor informaci\\'on para los modelos de estos objetos, es ALMA. Nuestro objetivo es seleccionar lentes candidatas para observar con ALMA y posteriormente modelarlas mediante el programa GravLens. Seleccionamos de la base de datos de CASTLES, 12 sistemas cu\\'adruples, los cuales tienen mayor probabilidad de observar fuentes extendidas en el rango submilim\\'etrico. Estos nuevos datos nos permitir\\'an mejorar los modelos exite...

  6. ALMA Observations of TNOs

    Science.gov (United States)

    Butler, Bryan J.; Brown, Michael E.

    2016-10-01

    Some of the most fundamental properties of TNOs are still quite poorly constrained, including diameter and density. Observations at long thermal wavelengths, in the millimeter and submillimeter, hold promise for determining these quantities, at least for the largest of these bodies (and notably for those with companions). Knowing this information can then yield clues as to the formation mechanism of these bodies, allowing us to distinguish between pairwise accretion and other formation scenarios.We have used the Atacama Large Millimeter/Submillimeter Array (ALMA) to observe Orcus, Quaoar, Salacia, and 2002 UX25 at wavelengths of 1.3 and 0.8 mm, in order to constrain the sizes of these bodies. We have also used ALMA to make astrometric observations of the Eris-Dysnomia system, in an attempt to measure the wobble of Eris and hence accurately determine its density. Dysnomia should also be directly detectable in those data, separate from Eris (ALMA has sufficient resolution in the configuration in which the observations were made). Results from these observations will be presented and discussed.

  7. ALMA telescope reaches new heights

    Science.gov (United States)

    2009-09-01

    the electromagnetic spectrum. Light at these wavelengths comes from some of the coldest, but also from some of the most distant objects in the cosmos. These include cold clouds of gas and dust where new stars are being born and remote galaxies towards the edge of the observable universe. The Universe is relatively unexplored at submillimetre wavelengths, as the telescopes need extremely dry atmospheric conditions, such as those at Chajnantor, and advanced detector technology. More information The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile. ESO is the European partner in ALMA. ALMA, the largest astronomical project in existence, is a revolutionary telescope, comprising an array of 66 giant 12-metre and 7-metre diameter antennas observing at millimetre and submillimetre wavelengths. ALMA will start scientific observations in 2011. ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a

  8. ALMA measures Calama earthquake

    Science.gov (United States)

    Brito, R.; Shillue, B.

    2010-04-01

    On 4 March 2010, the ALMA system response to an extraordinarily large disturbance was measured when a magnitude 6.3 earthquake struck near Calama, Chile, relatively close to the ALMA site. Figures 1 through 4 demonstrate the remarkable performance of the ALMA system to a huge disturbance that was more than 100 times the specification for correction accuracy.

  9. ALMA science data management

    OpenAIRE

    Stoehr, Felix

    2015-01-01

    ALMA has transitioned now from the construction to the operation phase. We review the Science Data Management of ALMA including the concepts of Data Reduction, Quality Assurance as well as of the Science Archive. We also place the Science Data Management of ALMA into the larger context.

  10. ALMA Pipeline: Current Status

    Science.gov (United States)

    Shinnaga, H.; Humphreys, E.; Indebetouw, R.; Villard, E.; Kern, J.; Davis, L.; Miura, R. E.; Nakazato, T.; Sugimoto, K.; Kosugi, G.; Akiyama, E.; Muders, D.; Wyrowski, F.; Williams, S.; Lightfoot, J.; Kent, B.; Momjian, E.; Hunter, T.; ALMA Pipeline Team

    2015-12-01

    The ALMA Pipeline is the automated data reduction tool that runs on ALMA data. Current version of the ALMA pipeline produces science quality data products for standard interferometric observing modes up to calibration process. The ALMA Pipeline is comprised of (1) heuristics in the form of Python scripts that select the best processing parameters, and (2) contexts that are given for book-keeping purpose of data processes. The ALMA Pipeline produces a "weblog" that showcases detailed plots for users to judge how each step of calibration processes are treated. The ALMA Interferometric Pipeline was conditionally accepted in March 2014 by processing Cycle 0 and Cycle 1 data sets. From Cycle 2, ALMA Pipeline is used for ALMA data reduction and quality assurance for the projects whose observing modes are supported by the ALMA Pipeline. Pipeline tasks are available based on CASA version 4.2.2, and the first public pipeline release called CASA 4.2.2-pipe has been available since October 2014. One can reduce ALMA data both by CASA tasks as well as by pipeline tasks by using CASA version 4.2.2-pipe.

  11. ADMIT: The ALMA Data Mining Toolkit

    Science.gov (United States)

    Teuben, P.; Pound, M.; Mundy, L.; Rauch, K.; Friedel, D.; Looney, L.; Xu, L.; Kern, J.

    2015-09-01

    ADMIT (ALMA Data Mining ToolkiT), a toolkit for the creation of new science products from ALMA data, is being developed as an ALMA Development Project. It is written in Python and, while specifically targeted for a uniform analysis of the ALMA science products that come out of the ALMA pipeline, it is designed to be generally applicable to (radio) astronomical data. It first provides users with a detailed view of their science products created by ADMIT inside the ALMA pipeline: line identifications, line ‘cutout' cubes, moment maps, emission type analysis (e.g., feature detection). Using descriptor vectors the ALMA data archive is enriched with useful information to make archive data mining possible. Users can also opt to download the (small) ADMIT pipeline product, then fine-tune and re-run the pipeline and inspect their hopefully improved data. By running many projects in a parallel fashion, data mining between many astronomical sources and line transitions will also be possible. Future implementations of ADMIT may include EVLA and other instruments.

  12. El alma de Venezuela en los proyectos de Estado-Nación de 1947 y de 1999

    Directory of Open Access Journals (Sweden)

    Dilia Flores Díaz

    2003-01-01

    Full Text Available El presente artículo es parte de una investigación que lleva por título: El imaginario galleguiano ¿Y un nuevo paradigma? En dicho artículo se hace una breve revisión histórica de los diferentes períodos constitucionales que remiten a una realidad más profunda que refleja, en cierta forma, cómo ha “evolucionado” el Estado-Nación en manos de “elegidos”. El objetivo del mismo es contrastar la posición asumida por dos actores que pertenecen a épocas diferentes, pero enmarcados en el mismo contexto histórico-geográfico como son Santos Luzardo,creado y recreado en el imaginario de Rómulo Gallegosy el otro, Hugo Rafael Chávez Frías, creado y recreado por su propia persona; por el “soberano” y relegitimado por una avalancha de votos que lo lleva a la Presidencia de Venezuela. Ambos aspiran en su imaginario cumplir con unamisión:construir un nuevo país.

  13. ALMA Common Software - UTFSM Group

    Science.gov (United States)

    Araya, M.; Avarias, J.; Mora, M.; Tobar, R.

    The ACS-UTFSM Group was created as a distributed systems research team on astronomical and non-astronomical applications on the year 2004. The choice of the ALMA Common Software framework (ACS) as the development platform came from the experience gained during summerjobs at ESO observatories. After three years of informal contributions to ACS development, the team presented a technology exchange initiative to the ALMA-CONICYT Fund 2006, which was granted in 2007. Through the past years, the UTFSM helped the ACS team with "nice-to-have" applications and testing. Currently the ACS-UTFSM is involved in several contributions to ACS, and the development of a flexible telescope control system (gTCS) framework which aims to encapsulate common requirements and will provide a uniform software. In preparation for this challenging objective, several small projects are currently being developed. The other interesting edge of the team work is the technology transfer initiatives. Several inter-universities collaborations are flourishing (PUC, UCN, UV) after the first ACS Workshop held at the UTFSM this year. Today three former team members are working at NRAO's ALMA Test Facility in Socorro, New Mexico. Two other students will have a summer job next year to work in ALMA related development.

  14. First two ALMA antennas successfully linked

    Science.gov (United States)

    2009-05-01

    a millionth of a second between equipment located many kilometers apart. The extreme environment where the ALMA observatory is located, with its strong winds, high altitude, and wide range of temperatures, just adds to the complexity of the observatory and to the fascinating engineering challenges we face", comments Richard Murowinski, ALMA Project Engineer. The astronomical target in this scientific milestone was the planet Mars. The astronomers measured the distinctive "fringes" -- a regular pattern of alternating strong and weak signals -- detected by the interferometer as the planet moved across the sky. The hardware used in this successful first test included two 12-metre diameter ALMA antennas as well as the complex series of electronic processing components needed to combine the signals. Such pairs of antennas are the basic building blocks of imaging systems that enable radio telescopes to deliver pictures that approach or even exceed the resolving power of visible light telescopes. Each antenna is combined electronically with every other antenna to form a multitude of antenna pairs. Each pair contributes unique information that is used to build a highly detailed image of the astronomical object under observation. When completed in early in the next decade, ALMA's 66 antennas will provide over a thousand such antenna pairings, with distances between antennas up to 16 kilometres. This will enable ALMA to see with a sharpness surpassing that of the best space telescopes, and to complement ground-based optical interferometers such as the ESO Very Large Telescope Interferometer (VLTI). "We are on target to do the first interferometry tests at the 5000-metre high-altitude site by the end of this year, and by the end of 2011 we plan to have at least 16 antennas working together as a single giant telescope," said Thijs de Graauw, ALMA Director. Notes for editors ALMA is a revolutionary astronomical telescope, comprising an array of 66 giant 12-metre and 7-metre

  15. Las Opiniones sacadas de los más auténticos y antigos philósofos que sobre la alma escrivieron i sus definiciones, de Daniel Arón Afia.

    Directory of Open Access Journals (Sweden)

    2008-06-01

    Full Text Available Included in a volume published in 1568 in Venice alongside the first Spanish translation of Leon Hebreo’s Diálogos de amor, the Opiniones sacadas de los más auténticos y antigos philósofos que sobre la alma escrivieron y sus difiniciones, were written by Aron Daniel Afia, an important Latin and Philosophy scholar in the Salonika of the second half of the 16th c. Descendant of a Converso family returned to Judaism after settlement in Ottoman lands, his short twelve folio work is a compendium of definitions of the soul proposed by thinkers from Antiquity to Renaissance, being a precious example of the intellectual activity (in Latin, Spanish and Hebrew of the Conversos who chose exile in the Levant. The volume, dedicated to Philip II, shows the attachment of former Conversos to Spanish culture.Las Opiniones sacadas de los más auténticos y antigos philósofos que sobre la alma escrivieron y sus definiciones fueron publicadas en 1568 en Venecia, junto con la primera traducción española de los Diálogos de amor de León Hebreo. Escritas por Daniel Arón Afia, profesor de latín y filosofía establecido en la Salónica de la segunda mitad del siglo XVI, este autor de familia conversa vuelta al judaísmo tras su establecimiento en tierras otomanas. El opúsculo de apenas doce folios es un compendio de definiciones del alma propuestas por pensadores, desde la Antigüedad hasta el Renacimiento, muestra de la actividad intelectual desarrollada en hebreo, latín y castellano de los conversos que escogieron la vía del exilio en el Levante mediterráneo. El volumen fue dedicado a Felipe II y muestra el apego de su promotor a la cultura hispánica.

  16. ALMA Pipeline Heuristics

    Science.gov (United States)

    Lightfoot, J.; Wyrowski, F.; Muders, D.; Boone, F.; Davis, L.; Shepherd, D.; Wilson, C.

    2006-07-01

    The ALMA (Atacama Large Millimeter Array) Pipeline Heuristics system is being developed to automatically reduce data taken with the standard observing modes. The goal is to make ALMA user-friendly to astronomers who are not experts in radio interferometry. The Pipeline Heuristics system must capture the expert knowledge required to provide data products that can be used without further processing. Observing modes to be processed by the system include single field interferometry, mosaics and single dish `on-the-fly' maps, and combinations of these modes. The data will be produced by the main ALMA array, the ALMA Compact Array (ACA) and single dish antennas. The Pipeline Heuristics system is being developed as a set of Python scripts. For interferometry these use as data processing engines the CASA/AIPS++ libraries and their bindings as CORBA objects within the ALMA Common Software (ACS). Initial development has used VLA and Plateau de Bure data sets to build and test a heuristic script capable of reducing single field data. In this paper we describe the reduction datapath and the algorithms used at each stage. Test results are presented. The path for future development is outlined.

  17. ACS: ALMA Common Software

    Science.gov (United States)

    Chiozzi, Gianluca; Šekoranja, Matej

    2013-02-01

    ALMA Common Software (ACS) provides a software infrastructure common to all ALMA partners and consists of a documented collection of common patterns and components which implement those patterns. The heart of ACS is based on a distributed Component-Container model, with ACS Components implemented as CORBA objects in any of the supported programming languages. ACS provides common CORBA-based services such as logging, error and alarm management, configuration database and lifecycle management. Although designed for ALMA, ACS can and is being used in other control systems and distributed software projects, since it implements proven design patterns using state of the art, reliable technology. It also allows, through the use of well-known standard constructs and components, that other team members whom are not authors of ACS easily understand the architecture of software modules, making maintenance affordable even on a very large project.

  18. Fideísmo y racionalismo en las tres potencias del alma

    Directory of Open Access Journals (Sweden)

    José Andrés Calvo Rodríguez

    2004-12-01

    Full Text Available Dentro de la gnoseología luliana, las tres potencias del alma racional (Voluntad, Memoria y Entendimiento adquieren una especial importancia por ser los instrumentos del alma que permiten el acceso y el conocimiento del amor divino. A este respecto escribe Cruz Hernández: «Las potencias del alma, además, tanto por su naturaleza como por su actividad, reflejan las virtudes divinas; y, de un modo eminente, la Trinidad personal».1 De esta manera, no hay mejor espejo de Dios en el hombre que el alma, donde reside la presencia divina. Por esto, el Libro de amigo y Amado, considerando la reiterativa presencia de las tres potencias del alma que presenta, simplemente propone un viaje errático por el interior del alma humana en busca de Dios y, en definitiva, en busca del propio yo del místico.

  19. ALMA Achieves Major Milestone With Antenna-Link Success

    Science.gov (United States)

    2007-03-01

    The Atacama Large Millimeter/submillimeter Array (ALMA), an international telescope project, reached a major milestone on March 2, when two ALMA prototype antennas were first linked together as an integrated system to observe an astronomical object. The milestone achievement, technically termed "First Fringes," came at the ALMA Test Facility (ATF) on the grounds of the National Radio Astronomy Observatory's (NRAO) Very Large Array (VLA) radio telescope in New Mexico. NRAO is a facility of the National Science Foundation (NSF), managed by Associated Universities, Incorporated (AUI). AUI also is designated by NSF as the North American Executive for ALMA. ALMA Test Facility ALMA Test Facility, New Mexico: VertexRSI antenna, left; AEC antenna, right. CREDIT: Drew Medlin, NRAO/AUI/NSF Click on image for page of graphics and full information Faint radio waves emitted by the planet Saturn were collected by the two ALMA antennas, then processed by new, state-of-the-art electronics to turn the two antennas into a single, high-resolution telescope system, called an interferometer. Such pairs of antennas are the basic building blocks of multi-antenna imaging systems such as ALMA and the VLA. In such a system, each antenna is combined electronically with every other antenna to form a multitude of pairs. Each pair contributes unique information that is used to build a highly-detailed image of the astronomical object under observation. When completed in 2012, ALMA will have 66 antennas. The successful Saturn observation began at 7:13 p.m., U.S. Mountain Time Friday (0213 UTC Saturday). The planet's radio emissions at a frequency of 104 GigaHertz (GHz) were tracked by the ALMA system for more than an hour. "Our congratulations go to the dedicated team of scientists, engineers and technicians who produced this groundbreaking achievement for ALMA. Much hard work and many long hours went into this effort, and we appreciate it all. This team should be very proud today," said NRAO

  20. Alma Data Mining Toolkit

    Science.gov (United States)

    Friedel, Douglas; Looney, Leslie; Teuben, Peter J.; Pound, Marc W.; Rauch, Kevin P.; Mundy, Lee; Harris, Robert J.; Xu, Lisa

    2016-06-01

    ADMIT (ALMA Data Mining Toolkit) is a Python based pipeline toolkit for the creation and analysis of new science products from ALMA data. ADMIT quickly provides users with a detailed overview of their science products, for example: line identifications, line 'cutout' cubes, moment maps, and emission type analysis (e.g., feature detection). Users can download the small ADMIT pipeline product (web browser and command line interface available for this purpose. By analyzing multiple data cubes simultaneously, data mining between many astronomical sources and line transitions are possible. Users are also able to enhance the capabilities of ADMIT by creating customized ADMIT tasks satisfying any special processing needs. We will present some of the salient features of ADMIT and example use cases.

  1. ALMA correlator computer systems

    Science.gov (United States)

    Pisano, Jim; Amestica, Rodrigo; Perez, Jesus

    2004-09-01

    We present a design for the computer systems which control, configure, and monitor the Atacama Large Millimeter Array (ALMA) correlator and process its output. Two distinct computer systems implement this functionality: a rack- mounted PC controls and monitors the correlator, and a cluster of 17 PCs process the correlator output into raw spectral results. The correlator computer systems interface to other ALMA computers via gigabit Ethernet networks utilizing CORBA and raw socket connections. ALMA Common Software provides the software infrastructure for this distributed computer environment. The control computer interfaces to the correlator via multiple CAN busses and the data processing computer cluster interfaces to the correlator via sixteen dedicated high speed data ports. An independent array-wide hardware timing bus connects to the computer systems and the correlator hardware ensuring synchronous behavior and imposing hard deadlines on the control and data processor computers. An aggregate correlator output of 1 gigabyte per second with 16 millisecond periods and computational data rates of approximately 1 billion floating point operations per second define other hard deadlines for the data processing computer cluster.

  2. Admit: Alma Data Mining Toolkit

    Science.gov (United States)

    Friedel, Douglas; Looney, Leslie; Xu, Lisa; Pound, Marc W.; Teuben, Peter J.; Rauch, Kevin P.; Mundy, Lee; Kern, Jeffrey S.

    2015-06-01

    ADMIT (ALMA Data Mining Toolkit) is a toolkit for the creation and analysis of new science products from ALMA data. ADMIT is an ALMA Development Project written purely in Python. While specifically targeted for ALMA science and production use after the ALMA pipeline, it is designed to be generally applicable to radio-astronomical data. ADMIT quickly provides users with a detailed overview of their science products: line identifications, line 'cutout' cubes, moment maps, emission type analysis (e.g., feature detection), etc. Users can download the small ADMIT pipeline product (data mining between many astronomical sources and line transitions will be possible. Users will also be able to enhance the capabilities of ADMIT by creating customized ADMIT tasks satisfying any special processing needs. Future implementations of ADMIT may include EVLA and other instruments.

  3. Microbiological quality and antimicrobial susceptibility of informally traded milk in Cruz das Almas county, Bahia Qualidade microbiológica e suscetibilidade antimicrobiana do leite in natura comercializado em Cruz das Almas, Bahia

    Directory of Open Access Journals (Sweden)

    Norma Suely Evangelista Barreto

    2012-12-01

    Full Text Available The microbiological quality as well as the antimicrobial susceptibility of bacteria isolated from raw milk obtained from 25 food stores in Cruz das Almas, Bahia were evaluated. The analysis included counts of mesophilic and psicrotrophic microorganisms, molds and yeast, Staphylococcus spp., coagulase-positive Staphylococcus, coliforms (at 35ºC and 45ºC, and the presence of Salmonella spp. and Escherichia coli. The average count for mesophilic and psicrotrophic microorganisms, molds and yeast, and coliforms at 35°C and 45°C were 1.6 x 109 CFU.mL-1, 9.6 x 104 CFU.mL-1, 3.8 x 108 CFU. mL-1, 4.0 x 105 MPN.mL-1 and 3.8 x 105 MPN.mL-1, respectively. Coagulase positive Staphylococcus was found in 44% of the samples (mean value of 7.3 x 105 CFU.mL-1, and E. coli was present in 76% of them. Salmonella was not detected in any of the samples tested. E. coli showed resistance (57.9% to tetracycline, to ampicillin and chloramphenicol (10.5%, and cephalotin (5.3%, while coagulase-positive Staphylococcus strains were resistant to amicacin (18% and vancomicin (18%. The raw milk besides to present poor microbiological quality, becoming a health risk of the consumers, it may contribute to the dissemination of resistant bacteria to various antimicrobial agents. Para a avaliação da qualidade microbiológica do leite in natura, bem como a suscetibilidade antimicrobiana das bactérias isoladas, foram analisados 25 estabelecimentos comerciais em Cruz das Almas, Ba. Para isso realizou-se a quantificação de micro-organismos heterotróficos mesófilos e psicrotróficos aeróbios, bolores e leveduras, Staphylococcus spp., Staphylococcus coagulase positiva, coliformes (35ºC e 45ºC e presença de Salmonella spp. e Escherichia coli. A contagem média de micro-organismos heterotróficos mesófilos foi de 1,6 x 109 UFC.mL-1, psicrotróficos 9,6 x 104 UFC. mL-1, bolores e leveduras 3,8 x 108 UFC.mL-1, coliformes a 35°C 4 x 105 NMP.mL-1 e a 45°C 3,8 x 105 NMP.mL-1

  4. The ALMA software architecture

    Science.gov (United States)

    Schwarz, Joseph; Farris, Allen; Sommer, Heiko

    2004-09-01

    The software for the Atacama Large Millimeter Array (ALMA) is being developed by many institutes on two continents. The software itself will function in a distributed environment, from the 0.5-14 kmbaselines that separate antennas to the larger distances that separate the array site at the Llano de Chajnantor in Chile from the operations and user support facilities in Chile, North America and Europe. Distributed development demands 1) interfaces that allow separated groups to work with minimal dependence on their counterparts at other locations; and 2) a common architecture to minimize duplication and ensure that developers can always perform similar tasks in a similar way. The Container/Component model provides a blueprint for the separation of functional from technical concerns: application developers concentrate on implementing functionality in Components, which depend on Containers to provide them with services such as access to remote resources, transparent serialization of entity objects to XML, logging, error handling and security. Early system integrations have verified that this architecture is sound and that developers can successfully exploit its features. The Containers and their services are provided by a system-orienteddevelopment team as part of the ALMA Common Software (ACS), middleware that is based on CORBA.

  5. ALMA and Cosmology

    CERN Document Server

    Combes, F

    2005-01-01

    ALMA is a privileged instrument to tackle high redshift galaxies, due to the negative K-correction in the millimeter domain. Many dusty star-forming galaxies, invisible in the optical or NIR, will be detected easily through the peak of their emission in the FIR redshifted in the submm between z=10 and z=5. Their mass and dynamics will be determined through the CO lines, together with the efficiency of star formation. Normal intervening galaxies at all z will be studied through absorption lines in front of quasars, exploring the dense tail of the column density spectrum. CMB anisotropies could be detected at the arcsecond scale, the secondary effects (SZ, Vishniak-Ostriker) could test the re-ionization and the nature of dark energy. The detection of the SZ effect on a few arcsec scales will allow to map in detail clusters and proto-clusters.

  6. The Atacama Large Millimeter Array (ALMA)

    Science.gov (United States)

    1999-06-01

    . The road ahead The three-year design and development phase of the project is now underway as a collaboration between Europe and the U.S., and Japan may also join in this effort. Assuming the construction phase begins about two years from now, limited operations of the array may begin in 2005 and the full array may become operational by 2009. Notes [1] Press Releases about this event have also been issued by some of the other organisations participating in this project: * CNRS (in French) * MPG (in German) * NOVA (in Dutch) * NRAO * NSF (ASCII and HTML versions) * PPARC [2] "ALMA" means "soul" in Spanish. [3] Additional information about ALMA is available on the web: * Articles in the ESO Messenger - "The Large Southern Array" (March 1998), "European Site Testing at Chajnantor" (December 1998) and "The ALMA Project" (June 1999), cf. http://www.eso.org/gen-fac/pubs/messenger/ * ALMA website at ESO at http://www.eso.org/projects/alma/ * ALMA website at the U.S. National Radio Astronomy Observatory (NRAO) at http://www.mma.nrao.edu/ * ALMA website in The Netherlands about the detectors at http://www.sron.rug.nl/alma/ ALMA/Chajnantor Video Clip and Photos ESO PR Video Clip 03/99 [MPEG-version] ESO PR Video Clip 03/99 (2450 frames/1:38 min) [MPEG Video; 160x120 pix; 2.1Mb] [MPEG Video; 320x240 pix; 10.0Mb] [RealMedia; streaming; 700k] [RealMedia; streaming; 2.3M] About ESO Video Clip 03/99 : This video clip about the ALMA project contains two sequences. The first shows a panoramic scan of the Chajnantor plain from approx. north-east to north-west. The Chajnantor mountain passes through the field-of-view and the perfect cone of the Licancabur volcano (5900 m) on the Bolivian border is seen at the end (compare also with ESO PR 24e/99 below. The second is a 52-sec animation with a change of viewing perspective of the array and during which the antennas move in unison. For convenience, the clip is available in four versions: two MPEG files of different sizes and two streamer

  7. ALMA Telescope Passes Major Milestone with Successful Antenna Link

    Science.gov (United States)

    2009-05-01

    The Atacama Large Millimeter/submillimeter Array (ALMA), an immense international telescope project under construction in northern Chile, reached a major milestone on April 30, when two ALMA antennas were linked together as an integrated system to observe an astronomical object for the first time. The milestone achievement, technically termed "First Fringes," came at ALMA’s Operations Support Facility, 9,500 feet above sea level. Faint radio waves emitted by the planet Mars were collected by the two 12-meter diameter ALMA antennas, then processed by state-of-the-art electronics to turn the two antennas into a single, high-resolution telescope system, called an interferometer. Such pairs of antennas are the basic building blocks of imaging systems that enable radio telescopes to deliver pictures that approach or even exceed the resolving power of visible light telescopes. In such a system, each antenna is combined electronically with every other antenna to form a multitude of antenna pairs. Each pair contributes unique information that is used to build a highly-detailed image of the astronomical object under observation. When completed early in the next decade, ALMA’s 66 antennas will provide over a thousand such antenna pairings, with distances between antennas exceeding ten miles. This will enable ALMA to see with a sharpness surpassing that of the best space telescopes. The antennas will operate at an altitude of 16,500 feet, high above the OSF, in one of the best locations on Earth for millimeter-wavelength astronomy, the Chajnantor Plateau in Chile’s Atacama Desert. Last week’s successful Mars observation was conducted at an observing frequency of 104.2 GHz. Astronomers measured the distinctive varying “fringes” detected by the interferometer as the planet moved across the sky. “This is a great success,” said Adrian Russell, North American ALMA Project Director at the National Radio Astronomy Observatory (NRAO), “not because we observed a

  8. The ALMA Observation Support Tool

    CERN Document Server

    Heywood, I; Williams, C J

    2011-01-01

    The ALMA Observation Support Tool (OST) is an ALMA simulator which is interacted with solely via a standard web browser. It is aimed at users who may or may not be experts in interferometry, or those that do not wish to familarise themselves with the simulation components of a data reduction package. It has been designed to offer full imaging simulation capability for an arbitrary ALMA observation while maintaining the accessibility of other online tools such as the ALMA Sensitivity Calculator. Simulation jobs are defined by selecting and entering options on a standard web form. The user can specify the standard parameters that would need to be considered for an ALMA observation (e.g. pointing direction, frequency set up, duration), and there is also the option to upload arbitrary sky models in FITS format. Once submitted, jobs are sequentially processed by a remote server running a CASA-based back-end system. The user is notified by email when the job is complete, and directed to a standard web page which co...

  9. Informe Signos Vitales de los CDC Obesidad infantil - (Childhood Obesity)

    Centers for Disease Control (CDC) Podcasts

    2013-08-06

    Este podcast se basa en el informe Signos Vitales de los CDC de agosto del 2013. La tasa de obesidad entre los niños en edad prescolar de bajos ingresos ha disminuido, pero todavía uno de cada seis niños hispanos es obeso. Este programa habla brevemente sobre lo que se puede hacer.  Created: 8/6/2013 by Centers for Disease Control and Prevention (CDC).   Date Released: 8/6/2013.

  10. ALMA Telescope Reaches New Heights

    Science.gov (United States)

    2009-09-01

    The ALMA (Atacama Large Millimeter/submillimeter Array) astronomical observatory took another step forward and upward, as one of its state-of-the-art antennas was carried for the first time to Chile's 16,500-foot-high plateau of Chajnantor on the back of a giant, custom-built transporter. The 40-foot-diameter antenna, weighing about 100 tons, was moved to ALMA's high-altitude Array Operations Site, where the extremely dry and rarefied air is ideal for observing the Universe. The conditions at the Array Operations Site on Chajnantor, while excellent for astronomy, are also very harsh. Only about half as much oxygen is available as at sea level, making it very difficult to work there. This is why ALMA's antennas are assembled and tested at the lower 9,500-foot altitude of the ALMA Operations Support Facility (OSF). It was from this relatively hospitable base camp that the ALMA antenna began its journey to the high Chajnantor site. "The successful transport of the first ALMA Antenna to the high site marks the start of the next phase of the project. Now that we are starting to move the ALMA antennas to the high site, the real work begins and the exciting part is just beginning," said Adrian Russell, North American ALMA Project Manager. The antenna's trip began when one of the two ALMA transporters lifted the antenna onto its back, carrying its heavy load along the 17-mile road from the Operations Support Facility up to the Array Operations Site. While the transporter is capable of speeds of up to 8 miles per hour when carrying an antenna, this first journey was made more slowly to ensure that everything worked as expected, taking about seven hours. The ALMA antennas use state-of-the-art technology, and are the most advanced submillimeter-wavelength antennas ever made. They are designed to operate fully exposed in the harsh conditions of the Array Operations Site, to survive strong winds and extreme temperatures, to point precisely enough that they could pick out a golf

  11. ALMA Cycle 0 Publication Statistics

    CERN Document Server

    Stoehr, Felix; Meakins, Silvia; Bishop, Marsha; Uchida, Ayako; Testi, Leonardo; Iono, Daisuke; Tatematsu, Kenichi; Wootten, Al

    2016-01-01

    The scientific impact of a facility is the most important measure of its success. Monitoring and analysing the scientific return can help to modify and optimise operations and adapt to the changing needs of scientific research. The methodology that we have developed to monitor the scientific productivity of the ALMA Observatory, as well as the first results, are described. We focus on the outcome of the first cycle (Cycle 0) of ALMA Early Science operations. Despite the fact that only two years have passed since the completion of Cycle 0 and operations have already changed substantially, this analysisconfirms the effectiveness of the underlying concepts. We find that ALMA is fulfilling its promise as a transformational facility for the observation of the Universe in the submillimetre.

  12. The North American ALMA Science Center

    Science.gov (United States)

    Lonsdale, Carol J.; Hibbard, J. E.; Staff, NAASC

    2010-01-01

    The North American ALMA Science Center at the National Radio Astronomy Observatory, NRAO, in Charlottesville, Virginia, in partnership with the Herzberg Institute of Astrophysics in Victoria, Canada, will support the North American community in their observations with the Atacama Large Millimeter Array, ALMA. Our goal is to promote successful observations with ALMA for both novice users, with no experience in either interferometry or millimeter astronomy, and experts alike. We will describe the services that the Science Center will provide for the community, from education about the capabilities of ALMA, though proposal preparation to data analysis. The Science Center will host a website with a Helpdesk that includes FAQs and a growing knowledgebase of ALMA expertise, and will support extensive demos and tutorials on observation preparation and data reduction with ALMA. The Science Center also promotes science-themed meetings. The staff of the Science Center will provide expert assistance for observers at all stages of development and execution of their program. There are visitor and postdoc opportunities at the Science Center. The North American ALMA Science Center is one of three regional centers around the globe that will support ALMA observations. Our partners are the European ALMA Regional Center at ESO in Garching, Germany, and the East Asian ALMA Region Center in Tokyo, Japan.

  13. A Web-based Dashboard for the High-level Monitoring of ALMA

    OpenAIRE

    Pietriga, Emmanuel; Filippi, Giorgio; Véliz, Luis; Del Campo, Fernando; Ibsen, Jorge

    2014-01-01

    International audience The ALMA radio-telescope's operations depend on the availability of high-level, easy-to-understand status information about all of its components. The ALMA Dashboard aims at providing an all-in-one-place near-real-time overview of the observatory's key elements and figures to both line and senior management. The Dashboard covers a wide range of elements beyond antennas, such as pads, correlator and central local oscillator. Data can be displayed in multiple ways, inc...

  14. Una Nueva Perspectiva de los Informes Financieros en Contabilidad Pública: Los Indicadores de Gestión

    OpenAIRE

    Isabel Brusca Alijarde

    1997-01-01

    El desarrollo alcanzado por los sistemas contables de las administraciones públicas en los últimos años ha sido intenso, tanto a nivel nacional como internacional, con el objetivo de que éstos proporcionen la información demandada por los usuarios para la toma de decisiones. Esto ha llevado a la implantación de informes financieros de contenido similar a los del sector empresarial, ampliando así la tradicional información presupuestaria. Ahora bien, una de las novedades más importantes es el ...

  15. The ALMA Telescope Control System

    Science.gov (United States)

    Farris, A.; Marson, Ralph; Kern, Jeff

    2005-10-01

    The Atacama Large Millimeter Array (ALMA) is a joint project between North America, Europe and Japan. ALMA is an aperture synthesis radio telescope consisting of 50 12-meter antennas located at an elevation of 5,000 meters in Llano de Chajnantor, Chile. These antennas will operate at frequencies ranging from 31.3 GHz to 950 GHz. The antennas can be moved and placed in different configurations, with baselines between the antennas varying from 150 meters to 20 km. The 50 antennas are supplemented by sixteen additional ones, known as the ALMA Compact Array (ACA): 12 7-meter antennas and 4 12-meter antennas. The ALMA control system will consist of over 70 computers separated by distances of over 20 km. Two aspects of the system are apparent: its distributed nature and its need to accurately synchronize events across many computers separated by large distances. In this paper we describe key features of the architecture of the ALMA Control System, focusing on its properties as a distributed system and on the mechanisms employed to achieve its time synchronization goals. This control system is a distributed system that uses the ALMA Common Software (ACS) as a middleware system layered on top of CORBA. The architecture of the control system extensively employs the component/container model in ACS. In addition, the use of CORBA allows us to employ Java in the higher levels of the control system, leaving C++ to the lower time-critical levels. Python as a scripting language is used by astronomers, to craft standard observing programs, and engineers, in a testing and debugging mode. Key to the concept of an aperture synthesis telescope is a special purpose hardware system known as a correlator, responsible for making various delay model corrections and correlating the signals from the antennas. There are two correlators in ALMA, one for the array of 50 antennas and one for the ACA. This entire system operates under a control system that must synchronize events across the

  16. Medidas procesales especiales y proteccíon de los derechos humanos Informe general

    NARCIS (Netherlands)

    Vervaele, J.A.E.

    2009-01-01

    El objetivo del informe general es realizar un análisis comparativo de los informes nacionales para evidenciar los procesos de transformación de los sistemas nacionales de justicia penal, en particular del proceso penal, en el que se han introducido medidas procesales especiales para hacer frente al

  17. ALMA Band 5 Cartridge Performance

    Science.gov (United States)

    Billade, Bhushan; Lapkin, I.; Nystrom, O.; Sundin, E.; Fredrixon, M.; Finger, R.; Rashid, H.; Desmaris, V.; Meledin, D.; Pavolotsky, A.; Belitsky, Victor

    2010-03-01

    Work presented here concerns the design and performance of the ALMA Band 5 cold cartridge, one of the 10 frequency channels of ALMA project, a radio interferometer under construction at Atacama Desert in Chile. The Band 5 cartridge is a dual polarization receiver with the polarization separation performed by orthomode transducer (OMT). For each polarization, Band 5 receiver employs sideband rejection (2SB) scheme based on quadrature layout, with SIS mixers covering 163-211 GHz with 4-8 GHz IF. The LO injection circuitry is integrated with mixer chip and is implemented on the same substrate, resulting in a compact 2SB assembly. Amongst the other ALMA bands, the ALMA Band 5 being the lowest frequency band that uses all cold optics, has the largest mirror. Consequently, ALMA Band 5 mirror along with its support structure leaves very little room for placing OMT, mixers and IF subsystems. The constraints put by the size of cold optics and limited cartridge space, required of us to revise the original 2SB design and adopt a design where all the components like OMT, mixer, IF hybrid, isolators and IF amplifier are directly connected to each other without using any co-ax cables in-between. The IF subsystem uses the space between 4 K and 15 K stage of the cartridge and is thermally connected to 4 K stage. Avoiding co-ax cabling required use of custom designed IF hybrid, furthermore, due to limited cooling capacity at 4 K stage, resistive bias circuitry for the mixers is moved to 15 K stage and the IF hybrid along with an integrated bias-T is implemented using superconducting micro-strip lines. The E-probes for both LO and RF waveguide-to-microstrip transitions are placed perpendicular to the wave direction (back-piece configuration). The RF choke at the end of the probes provides a virtual ground for the RF/LO signal, and the choke is DC grounded to the chassis. The on-chip LO injection is done using a microstrip line directional coupler with slot-line branches in the

  18. Una Nueva Perspectiva de los Informes Financieros en Contabilidad Pública: Los Indicadores de Gestión

    Directory of Open Access Journals (Sweden)

    Isabel Brusca Alijarde

    1997-12-01

    Full Text Available El desarrollo alcanzado por los sistemas contables de las administraciones públicas en los últimos años ha sido intenso, tanto a nivel nacional como internacional, con el objetivo de que éstos proporcionen la información demandada por los usuarios para la toma de decisiones. Esto ha llevado a la implantación de informes financieros de contenido similar a los del sector empresarial, ampliando así la tradicional información presupuestaria. Ahora bien, una de las novedades más importantes es el interés demostrado para dar respuesta a la necesidad de proporcionar información sobre la economía, eficiencia y eficacia en el contexto de las administraciones públicas, apareciendo los indicadores de gestión como un nuevo componente de los informes financieros. The development reached by public accounting systems over the last few years has been intense, both at the national and international level, with the aim of providing the information demanded by the users for the decision making process. This has led to the introduction of financial reports with similar disclosure to those of the business sector. Thereby extending the traditional budgetary reporting. However, one of the most important new developments is the interest shown in meeting the objective of supplying information about economy, efficiency and effectiveness in public administration context, with performance indicators appearing as a new component of financial reports.

  19. ALMA to Help Solving Acute Mountain Sickness Mystery

    Science.gov (United States)

    2007-04-01

    , family and social isolation, commuting, intermittent high altitude exposure and other environmental challenges such as low temperatures. "An adequate acclimatisation to 2500m altitude requires around two weeks, and we can thus speculate that going to 5000m would require more than one month to achieve complete acclimatisation," said Professor Juan Silva Urra, from the University of Antofagasta. However, short and long term effects of regular commuting between sea level and high altitude have scarcely been studied in biomedical terms. Scientifically based guidelines for appropriate preventive handling and care under these conditions are lacking and the new study will help bridging this gap. Among the studies to be done, some involve continuous monitoring of the human body through portable devices, including measurements of hormone levels and application of psychometric tests. All measurements at 5000m will be carried out on a voluntary basis, under strict safety protocols, with the presence of a doctor from the investigation team, paramedic personnel form ALMA and an ambulance. The symptoms of Acute Mountain Sickness are headache, sicknesses, gastrointestinal inconveniences, fatigue and insomnia that, depending on their intensities, decrease the capacity to carry out the most routine activities. The valuable data collected will enhance our knowledge of human physiology in extreme environments, generating recommendations that will improve wellbeing and health not only in high-altitude observatories, but also in mining and Antarctic personnel. "We are pleased that ALMA is contributing to other disciplines, like medicine, even before the antennas begin to explore the universe," said Felix Mirabel, ESO's representative in Chile. "This outstanding long-term research that will provide crucial information of human physiology to experts worldwide, has been made possible thanks to the combined effort of Chilean and European universities, in collaboration with ALMA". The Atacama

  20. Kemanda Çalma Teknikleri

    OpenAIRE

    ÇUHADAR, Yrd. Doç. C. Hakan

    2013-01-01

    Keman ortaya çıkışından bugüne kadar üzerinde en çok eser yazılan ve çalma tekniği geliştirilen çalgılardan birisidir Hemen hemen tüm doğu ve batı müziklerinde önemli bir yeri bulunmaktadır Özellikle gelişen yay ve çalma teknikleri sayesinde batı müziğinin en önemli üyesi olmuştur Batı dünyasında 1600 yıllarında geliştirilmeye başlanan keman İtalyan ustalar Amati Guarnerius ve Stradivarius sayesinde bugünkü şeklini elde etmiştir Keman çalmada önemli bir unsur olan yay ise Fransız yay ...

  1. El alma colombiana. Idiosincrasia e identidades culturales en Colombia

    Directory of Open Access Journals (Sweden)

    P. Pedro José Díaz Camacho

    2012-01-01

    Full Text Available La presente investigación tiene el propósito de averiguar sobre los rasgos anímicos y temperamentales que se expresan en el modo de ser y en la conducta de los colombianos, según las distintas regiones y grupos socioculturales; es decir, sobre cómo ha llegado a ser en el siglo XXI la índole y el alma del pueblo colombiano. Bajo este panorama, se indaga acerca de algunos factores que intervienen en la configuración y expresión del modo de ser, pensar, sentir, percibir y actuar de los colombianos, junto con la forma diversa como se manifiesta su idiosincrasia y la identidad cultural, según lo expuesto por algunos estudiosos de las cuestiones antropológicas, históricas y sociológicas del pueblo colombiano.

  2. Morphologies of protostellar outflows: An ALMA view

    CERN Document Server

    Peters, Thomas; Seifried, Daniel; Banerjee, Robi; Klessen, Ralf S

    2014-01-01

    The formation of stars is usually accompanied by the launching of protostellar outflows. Observations with the Atacama Large Millimetre/sub-millimetre Array (ALMA) will soon revolutionalise our understanding of the morphologies and kinematics of these objects. In this paper, we present synthetic ALMA observations of protostellar outflows based on numerical magnetohydrodynamic collapse simulations. We find significant velocity gradients in our outflow models and a very prominent helical structure within the outflows. We speculate that the disk wind found in the ALMA Science Verification Data of HD 163296 presents a first instance of such an observation.

  3. Los alcances de los nuevos programas informáticos para el desarrollo de la econometría

    OpenAIRE

    Guillermo Noel Gutiérrez Cárdenas

    2013-01-01

    El presente ensayo, es una aproximación de la econometría a la informática, mostrando su origen e importancia para las Ciencias Económicas, pero principalmente para el investigador y analista de datos. Pasando brevemente por su historia y los dilemas que a enfrentado en la economía. Pretende así, ser una guía completa que repasa los principales programas informáticos en econometría con sus respectivos enlaces WEB para que puedan ser descargados conforme al uso que se le quiera dar. Así, esta ...

  4. Interstellar Isotopes: Prospects with ALMA

    Science.gov (United States)

    Charnley Steven B.

    2010-01-01

    Cold molecular clouds are natural environments for the enrichment of interstellar molecules in the heavy isotopes of H, C, N and O. Anomalously fractionated isotopic material is found in many primitive Solar System objects, such as meteorites and comets, that may trace interstellar matter that was incorporated into the Solar Nebula without undergoing significant processing. Models of the fractionation chemistry of H, C, N and O in dense molecular clouds, particularly in cores where substantial freeze-out of molecules on to dust has occurred, make several predictions that can be tested in the near future by molecular line observations. The range of fractionation ratios expected in different interstellar molecules will be discussed and the capabilities of ALMA for testing these models (e.g. in observing doubly-substituted isotopologues) will be outlined.

  5. Two years of ALMA bibliography - lessons learned

    CERN Document Server

    Meakins, Silvia; Bishop, Marsha J; Stoehr, Felix; Tatematsu, Ken

    2014-01-01

    Telescope bibliographies are integral parts of observing facilities. They are used to associate the published literature with archived observational data, to measure an observatory's scientific output through publication and citation statistics, and to define guidelines for future observing strategies. The ESO and NRAO librarians as well as NAOJ jointly maintain the ALMA (Atacama Large Millimeter/submillimeter Array) bibliography, a database of refereed papers that use ALMA data. In this paper, we illustrate how relevant articles are identified, which procedures are used to tag entries in the database and link them to the correct observations, and how results are communicated to ALMA stakeholders and the wider community. Efforts made to streamline the process will be explained and evaluated, and a first analysis of ALMA papers published after two years of observations will be given.

  6. New Inspiring Planetarium Show Introduces ALMA to the Public

    Science.gov (United States)

    2009-03-01

    As part of a wide range of education and public outreach activities for the International Year of Astronomy 2009 (IYA2009), ESO, together with the Association of French Language Planetariums (APLF), has produced a 30-minute planetarium show, In Search of our Cosmic Origins. It is centred on the global ground-based astronomical Atacama Large Millimeter/submillimeter Array (ALMA) project and represents a unique chance for planetariums to be associated with the IYA2009. ESO PR Photo 09a/09 Logo of the ALMA Planetarium Show ESO PR Photo 09b/09 Galileo's first observations with a telescope ESO PR Photo 09c/09 The ALMA Observatory ESO PR Photo 09d/09 The Milky Way band ESO PR Video 09a/09 Trailer in English ALMA is the leading telescope for observing the cool Universe -- the relic radiation of the Big Bang, and the molecular gas and dust that constitute the building blocks of stars, planetary systems, galaxies and life itself. It is currently being built in the extremely arid environment of the Chajnantor plateau, at 5000 metres altitude in the Chilean Andes, and will start scientific observations around 2011. ALMA, the largest current astronomical project, is a revolutionary telescope, comprising a state-of-the-art array of 66 giant 12-metre and 7-metre diameter antennas observing at millimetre and submillimetre wavelengths. In Search of our Cosmic Origins highlights the unprecedented window on the Universe that this facility will open for astronomers. "The show gives viewers a fascinating tour of the highest observatory on Earth, and takes them from there out into our Milky Way, and beyond," says Douglas Pierce-Price, the ALMA Public Information Officer at ESO. Edited by world fulldome experts Mirage3D, the emphasis of the new planetarium show is on the incomparable scientific adventure of the ALMA project. A young female astronomer guides the audience through a story that includes unique animations and footage, leading the viewer from the first observations by Galileo

  7. Fernando Vallejo,  Almas en pena chapolas negras

    Directory of Open Access Journals (Sweden)

    Daniel García

    2012-05-01

    Full Text Available En uno de sus aforismos Ciorán se pregunta por qué no ha sido un motivo de suicidio para nadie el solo hecho de pensar que otro escribiría su biografía. Fernando Vallejo, por su parte, reconoce la miseria de este género espurio y no puede imaginarse un oficio peor que el de los biógrafos, « metidos en archivos y bibliotecas entre papeles polvosos, viejos, viviendo las infamias del pasado », más muertos que los muertos. La anécdota que abre Almas en pena chapolas negras, la biografía de José A...

  8. A web-based dashboard for the high-level monitoring of ALMA

    Science.gov (United States)

    Pietriga, Emmanuel; Filippi, Giorgio; Véliz, Luis; del Campo, Fernando; Ibsen, Jorge

    2014-07-01

    The ALMA radio-telescope's operations depend on the availability of high-level, easy-to-understand status information about all of its components. The ALMA Dashboard aims at providing an all-in-one-place near-real-time overview of the observatory's key elements and figures to both line and senior management. The Dashboard covers a wide range of elements beyond antennas, such as pads, correlator and central local oscillator. Data can be displayed in multiple ways, including: a table view, a compact view fitting on a single screen, a timeline showing detailed information over time, a logbook, a geographical map.

  9. Supporting Student Learning in Computer Science Education via the Adaptive Learning Environment ALMA

    Directory of Open Access Journals (Sweden)

    Alexandra Gasparinatou

    2015-10-01

    Full Text Available This study presents the ALMA environment (Adaptive Learning Models from texts and Activities. ALMA supports the processes of learning and assessment via: (1 texts differing in local and global cohesion for students with low, medium, and high background knowledge; (2 activities corresponding to different levels of comprehension which prompt the student to practically implement different text-reading strategies, with the recommended activity sequence adapted to the student’s learning style; (3 an overall framework for informing, guiding, and supporting students in performing the activities; and; (4 individualized support and guidance according to student specific characteristics. ALMA also, supports students in distance learning or in blended learning in which students are submitted to face-to-face learning supported by computer technology. The adaptive techniques provided via ALMA are: (a adaptive presentation and (b adaptive navigation. Digital learning material, in accordance with the text comprehension model described by Kintsch, was introduced into the ALMA environment. This material can be exploited in either distance or blended learning.

  10. Evolución de los informes de auditoria calificados en los sectores: financiero y de la construcción

    OpenAIRE

    Iváñez Mingot, Marco

    2015-01-01

    El informe de auditoría es el producto final del proceso de auditoría. El auditor muestra a través de él, a los usuarios de la información contable, su valoración sobre la calidad de los contenidos en el Informe Anual. Evolución de dicha calidad y en consecuencia de la calificación de los informes.

  11. Los objetos con alma: legitimidad de la esclavitud en el discurso de Aristóteles y Alonso de Sandoval. Una aproximación desde la construcción del cuerpo

    Directory of Open Access Journals (Sweden)

    Catalina Ariza Montañez

    2005-01-01

    Full Text Available En este artículo se hace un estudio comparativo entre las obras de Aristóteles y del jesuita del siglo XVII, Alonso de Sandoval, en especial el Tractatus de Instauranda de Aethiopum Salute (1627, con el fin de comparar la concepción de la esclavitud que tenía este filósofo de la Grecia Antigua y los teólogos españoles del periodo colonial. Se toma como referente la construcción social y cultural del cuerpo, siguiendo las ideas propuestas por David Le Bretón. Se argumenta que desde la Antigüedad la legitimación de la esclavitud se basó en la idea de una inferioridad natural inscrita en los cuerpos de los esclavos. Esta aproximación corporal ayuda a dilucidar las redes de significación que dieron sentido a la esclavitud, permitiendo resaltar las diferencias, semejanzas, correlaciones, superposiciones, contradicciones en la obra de los dos autores.

  12. La ciencia del alma en IBN Bayya (Avempace

    Directory of Open Access Journals (Sweden)

    Lomba, Joaquín

    2007-01-01

    Full Text Available Não possui resumo em portugês El objetivo de este trabajo es la interpretación de del más importante aspecto de la filosofía de Ibn Bayya (Avempace a base de la lectura de su Kitab al nafs, primer comentario del De anima de Aristóteles en Occidente. Este estudio sobre el alma es, para Avempace, constituye la principal ciencia porque sin el análisis de la propia alma es imposible conocer el resto de las ciencias y del mundo. Este autor, en todas sus obras encentra el ideal del filósofo y del hombre sabio, sobre todo, en la progresiva desmaterialización de toda su vida. Este objetivo se obtiene mediante el transcendeer de tres formas de vida, concretamente, las formas materiales, el primer nivel espiritual y, por fin, el segundo nivel espiritual. La culminación de este itinerario es alcanzar el segundo nivel espiritual, concretamente, la unión con el Intelecto Agente mediante un misticismo espiritual o «amor Dei intellectualis». Los materiales básicos de esta filosofía están conteniddos en este comentario al aristotélico al De anima. $$bspa

  13. First North American Antenna Enables Next Phase in Joint ALMA Observatory

    Science.gov (United States)

    2009-02-01

    project. With two antennas now on site, we begin the real work of combining signals from them. We are advancing toward ALMA's ultimate goal of surpassing by tenfold existing technology in this area,” explained Philip Puxley, the NSF’s ALMA Program Manager. ALMA officials expect the pace of antenna acceptance to accelerate. “We have nine (North American) antennas on site already,” said Adrian Russell, NRAO’s ALMA Project Director, “and following handover of Number Three we plan to get one through the test procedure each month. Additional North American antennas will be arriving in Chile at a rate of one every two months, and General Dynamics is on track to complete delivery of these systems within days of the original schedule.” When completed early next decade, ALMA will have a total of sixty-six antennas (with the option of further expansion) provided by partners in North America, Europe, and East Asia. The first European antennas, produced under the auspices of the European Organization for Astronomical Research in the Southern Hemisphere (ESO) are scheduled to begin arriving early this year. The ALMA Project is a partnership between the scientific communities of East Asia, Europe and North America with Chile. ALMA is funded in North America by the U.S. National Science Foundation in cooperation with the National Research Council of Canada and the National Science Council of Taiwan. ALMA construction and operations are led on behalf of North America by the National Radio Astronomy Observatory, which is operated under cooperative agreement by Associated Universities, Inc. Notes for Editors * High-resolution images associated with this press release: o Antenna o Antenna on Transporter 1 o Antenna on Transporter 2 * Additional information about ALMA * ALMA will be the leading astronomical instrument for observing the cool Universe - the molecular gas and dust that constitute the building blocks of stars, planetary systems, galaxies, and of life itself. * ALMA

  14. Los alcances de los nuevos programas informáticos para el desarrollo de la econometría

    Directory of Open Access Journals (Sweden)

    Guillermo Noel Gutiérrez Cárdenas

    2013-01-01

    Full Text Available El presente ensayo, es una aproximación de la econometría a la informática, mostrando su origen e importancia para las Ciencias Económicas, pero principalmente para el investigador y analista de datos. Pasando brevemente por su historia y los dilemas que a enfrentado en la economía. Pretende así, ser una guía completa que repasa los principales programas informáticos en econometría con sus respectivos enlaces WEB para que puedan ser descargados conforme al uso que se le quiera dar. Así, esta guía mostrará las ventajas y falencias de cada uno de ellos. Siempre entregando un fundamento de que este tipo de programas son un complemento y no reemplaza a la econometría como técnica fundamental en la investigación científica.

  15. Estética y lógica social en las mesas para las almas maya-chortís

    OpenAIRE

    López García, Julián

    2000-01-01

    Los mayas-chortís del oriente de Guatemala preparan mesas para los difuntos en unas celebraciones rituales llamadas sikines. El presente artículo trata de la estética y la lógica social asociada a la preparación de esas mesas donde llegan a comer las almas de los difuntos. En las mesas para las almas se dispone una amplia gama de alimentos pero hay que observar algunas restricciones: no se podrá poner carne grasienta (como la de cerdo), no se podrán colocar bebidas esp...

  16. The First Six ALMA Band 10 Receivers

    Science.gov (United States)

    Fujii, Y.; Gonzalez, A.; Kroug, M.; Kaneko, K.; Miyachi, A.; Yokoshima, T.; Kuroiwa, K.; Ogawa, H.; Makise, K.; Wang, Z.; Uzawa, Y.

    2013-01-01

    The first six Atacama Large Millimeter/submillimeter Array (ALMA) Band 10 (787-950 GHz) receivers have been developed and characterized during the receiver preproduction phase. State-of-the-art measurement systems at THz frequencies have been implemented and successfully used to measure the performance of the first six receivers. Extensive tests ranging from receiver sensitivity and stability to optical aperture efficiency on the secondary antenna have been performed. Performance of all six receivers is well within the stringent ALMA requirements. Moreover, our extensive tests have shown that there are no big performance differences between receivers. These results indicate that the ALMA Band 10 receiver is ready for the production phase, during which an additional 67 receivers will be produced and characterized.

  17. Common Software for the ALMA project

    CERN Document Server

    Chiozzi, G; Jeram, B; Sivera, P; Plesko, M; Sekoranja, M; Tkacik, G; Dovc, J; Kadunc, M; Milcinski, G; Verstovsek, I; Zagar, K

    2001-01-01

    The Atacama Large Millimeter Array (ALMA) is a joint project between astronomical organizations in Europe, USA and Japan. ALMA will consist of at least 64 12-meter antennas operating in the millimeter and sub-millimeter wavelength range, with baselines up to 10 km. It will be located at an altitude above 5000m in the Chilean Atacama desert[1]. The ALMA Common Software (ACS) provides a software infrastructure common to all partners and consists of a documented collection of common patterns in control systems and of components, which implement those patterns. The heart of ACS is an object model of controlled devices, called Distributed Objects (DOs), implemented as CORBA network objects. Components such as antenna mount, power supply, etc. are defined by means of DOs. A code generator creates Java Bean components for each DO. Programmers can write Java client applications by connecting those Beans with data-manipulation and visualization Beans using commercial visual development tools or programmatically. ACS i...

  18. Business Intelligence Applied to the ALMA Software Integration Process

    Science.gov (United States)

    Zambrano, M.; Recabarren, C.; González, V.; Hoffstadt, A.; Soto, R.; Shen, T.-C.

    2012-09-01

    Software quality assurance and planning of an astronomy project is a complex task, specially if it is a distributed collaborative project such as ALMA, where the development centers are spread across the globe. When you execute a software project there is much valuable information about this process itself that you might be able to collect. One of the ways you can receive this input is via an issue tracking system that will gather the problem reports relative to software bugs captured during the testing of the software, during the integration of the different components or even worst, problems occurred during production time. Usually, there is little time spent on analyzing them but with some multidimensional processing you can extract valuable information from them and it might help you on the long term planning and resources allocation. We present an analysis of the information collected at ALMA from a collection of key unbiased indicators. We describe here the extraction, transformation and load process and how the data was processed. The main goal is to assess a software process and get insights from this information.

  19. ALMA Observatory Equipped with its First Antenna

    Science.gov (United States)

    2008-12-01

    High in the Atacama region of northern Chile one of the world’s most advanced telescopes has just passed a major milestone. The first of many state-of-the-art antennas has been handed over to the Atacama Large Millimeter/submillimeter Array (ALMA) project. ALMA is being built by a global partnership whose North American partners are led by the National Radio Astronomy Observatory (NRAO). With ALMA, astronomers will study the cool Universe, the molecular gas and tiny dust grains from which stars, planetary systems, galaxies and even life are formed. ALMA will provide new, much-needed insights into the formation of stars and planets, and will reveal distant galaxies in the early Universe, which we see as they were over ten billion years ago. ALMA will initially comprise 66 high-precision antennas, with the option to expand in the future. There will be an array of fifty 12-meter diameter antennas, acting together as a single giant telescope, and a compact array composed of 7-meter and 12-meter antennas. The first 12-meter antenna to be handed over to the observatory was built by Mitsubishi Electric Corporation for the National Astronomical Observatory of Japan, one of the ALMA partners. It will shortly be joined by North American and European antennas. “Our Japanese colleagues have produced this state-of-the-art antenna to exacting specifications. We are very excited about the handover because now we can fully equip this antenna for scientific observations,” said Thijs de Graauw, ALMA Director. Antennas arriving at the ALMA site undergo a series of tests to ensure that they meet the strict requirements of the telescope. The antennas have surfaces accurate to less than the thickness of a human hair, and can be pointed precisely enough to pick out a golf ball at a distance of 9 miles. “The handover of the first Japanese antenna is the crowning achievement of the ALMA Project to date,” said Adrian Russell, the North American ALMA Project Director at NRAO. The

  20. TELCAL: The On-line Calibration Software for ALMA

    Science.gov (United States)

    Broguière, D.; Lucas, R.; Pardo, J.; Roche, J.-C.

    2011-07-01

    The ALMA on-line calibration regroups all the operations needed to maintain the ALMA interferometer optimally tuned to successfully execute the planned observations. The results of the calibrations are used in quasi-real time by the ALMA Control System. Since the first ALMA antennas were put into operation in 2009, TELCAL has been used for all the basic calibration operations and is still being improved following the project advancement. We describe here the calibrations done by TELCAL, its relationships with the other ALMA software subsystems and, briefly, the architecture of the software based on CORBA.

  1. First ALMA Transporter Ready for Challenging Duty

    Science.gov (United States)

    2008-07-01

    The first of two ALMA transporters -- unique vehicles designed to move high-tech radio-telescope antennas in the harsh, high-altitude environment of the Atacama Large Millimeter/submillimeter Array -- has been completed and passed its initial operational tests. The 130-ton machine moves on 28 wheels and will be able to transport a 115-ton antenna and set it down on a concrete pad within millimeters of a prescribed position. ALMA Transporter The ALMA Transporter on a Test Run CREDIT: ESO Click on image for high-resolution file (244 KB) The ALMA transporter rolled out of its hangar and underwent the tests at the Scheuerle Fahrzeugfabrik company site near Nuremberg, Germany. The machine is scheduled for delivery at the ALMA site in Chile by the end of 2007, and a second vehicle will follow about three months later. ALMA is a giant, international observatory under construction in the Atacama Desert of northern Chile at an elevation of 16,500 feet. Using at least 66 high-precision antennas, with the possibility of increasing the number in the future, ALMA will provide astronomers with an unprecedented ability to explore the Universe as seen at wavelengths of a few millimeters to less than a millimeter. By moving the antennas from configurations as compact as 150 meters to as wide as 15 kilometers, the system will provide a zoom-lens ability for scientists. "The ability to move antennas to reconfigure the array is vital to fulfilling ALMA's scientific mission. The operations plan calls for moving antennas on a daily basis to provide the flexibility that will be such a big part of ALMA's scientific value. That's why the transporters are so important and why this is such a significant milestone," said Adrian Russell, North American Project Manager for ALMA. "The ALMA antennas will be assembled and their functionality will be verified at a base camp, located at an altitude of 2900 meters (9500 feet) and the transporters will in a first step bring the telescopes up to the

  2. The exciting future of (sub-)millimeter interferometry: ALMA

    CERN Document Server

    Casasola, V

    2010-01-01

    The Atacama Large Millimeter/submillimeter Array (ALMA), presently under construction, is a revolutionary astronomical interferometer, that will operate at (sub)millimeter wavelengths. With unprecedented sensitivity, resolution, and imaging capability, ALMA will explore the (sub-)mm Universe, one of astronomy's last frontiers. ALMA is expected to provide insight in star- and galaxy formation in the early Universe and to image local star- and planet formation in great detail. The ALMA Commissioning and Science Verification phase is currently in course, preparing the path for Early Science. The Call for ALMA Early Science proposals is expected to be released before the end of 2010. In this contribution we will describe the ALMA project, the array and its receivers, its science goals, and its scientific and technological potential. We will outline the organizational structure of the ALMA Regional Centres, that will play an important role in providing support to the users, with particular attention to the Italian...

  3. «Con llanto en los ojos, / con luto y duelo en el alma»: el moro como forjador identitario en la tradición dramática del levante peninsular

    Directory of Open Access Journals (Sweden)

    Sáez Raposo, Francisco

    2013-06-01

    Full Text Available The festival of Moors and Christians in the town of Caudete (Albacete, one of the oldest known, came into being within a dramatic tradition that goes back to the late Sixteenth Century. As a paradigmatic example of the dramatic creation process based on rewriting, the original play has been adapted to the audience’s ever changing horizons of expectations to constitute Episodios caudetanos, the core of nowadays celebration. History, religion, legend and literature complement each other in order to form a cultural phenomenon that transcends its mere playful essence as a popular festival. Through the archetypical figure of the moor, the identity of a community has been shaped (and, by extension, that of a whole nation from the concept of a polarized universe that historical documentation insists on denying.La fiesta de moros y cristianos de la villa albaceteña de Caudete, una de las más antiguas que se conocen, tiene su origen en una tradición dramática que se remonta a finales del siglo XVI. Ejemplo paradigmático del proceso de creación teatral basado en la reescritura, la obra primigenia se ha ido adaptando a los cambiantes horizontes de expectativas del público hasta conformar los Episodios caudetanos, médula de la actual celebración. Historia, religión, leyenda y literatura se complementan para configurar un fenómeno cultural que trasciende la mera esencia lúdica de un festejo popular. Mediante la figura prototípica del moro se ha moldeado la identidad de una comunidad (y, por extensión, de toda una nación a partir del concepto de un universo polarizado que la documentación histórica se empeña en refutar.

  4. ALMA communication backbone in Chile goes optical

    Science.gov (United States)

    Filippi, G.; Ibsen, J.; Jaque, Sandra; Liello, F.; Navarro, C.

    2014-07-01

    High-bandwidth communication has become a key factor for scientific installations as Observatories. This paper describes the technical, organizational, and operational goals and the level of completion of the ALMA Optical Link Project. The project focus is the creation and operation of an effective and sustainable communication infrastructure to connect the ALMA Observatory, located in the Atacama Desert, in the Northern region of Chile, with the point of presence in ANTOFAGASTA, about 400km away, of the EVALSO infrastructure, and from there to the Central Office in the Chilean capital, Santiago. This new infrastructure that will be operated in behalf of ALMA by REUNA, the Chilean National Research and Education Network, will use state of the art technologies, like dark fiber from newly built cables and DWDM transmission, allowing extending the reach of high capacity communication to the remote region where the Observatory is located. When completed, the end-to-end Gigabit-per-second (Gbps) capable link will provide ALMA with a modern, effective, robust, communication infrastructure capable to cope with present and future demands, like those coming from fast growing data transfer to rapid response mode, from remote monitoring and engineering to virtual presence.

  5. Alma Flor Ada: Writer, Translator, Storyteller.

    Science.gov (United States)

    Brodie, Carolyn S.

    2003-01-01

    Discusses the work of children's author Alma Flor Ada, a Cuban native who has won awards honoring Latino writers and illustrators. Includes part of an interview that explores her background, describes activity ideas, and presents a bibliography of works written by her (several title published in both English and Spanish) as well as sources of…

  6. Catalogación de los dispositivos de entretenimiento de los fondos museográficos del Museo de Informática

    OpenAIRE

    LÓPEZ GARCÍA, IVÁN

    2015-01-01

    [ES] En este proyecto se plantea el estudio y catalogación de las consolas, videojuegos y dispositivos periféricos pertenecientes a los fondos del Museo de Informática de la Escuela Técnica Superior de Ingeniería Informática de la Universidad Politécnica de Valencia. El estudio incluye un análisis cronológico de los videojuegos a lo largo de la historia, de donde se han confeccionado los datos relacionados con el origen de los dispositivos de entretenimiento del museo, de fo...

  7. The ALMA Real Time Control System

    Science.gov (United States)

    Kern, Jeffrey S.; Juerges, Thomas A.; Marson, Ralph G.

    2009-01-01

    The Atacama Large Millimeter Array (ALMA) is a revolutionary millimeter and submillimeter array being developed on the Atacama plateau of northern Chile. An international partnership lead by NRAO, ESO, and NAOJ this powerful and flexible telescope will provide unprecedented observations of this relatively unexplored frequency range. The control subsystem for the Atacama Large Millimeter Array must coordinate the monitor and control of at least sixty six antennas (in four different styles), two correlators, and all of the ancillary equipment (samplers, local oscillators, front ends, etc.). This equipment will be spread over tens of kilometers and operated remotely. Operation of the array requires a robust, scalable, and maintainable real time control system. The real time control system is responsible for monitoring and control of any devices where there are fixed deadlines. Examples in the ALMA context are antenna pointing and fringe tracking. Traditionally the real time portion of a large software system is an intricate and error prone portion of the software. As a result the real time portion is very expensive in terms of effort expended both during construction and during maintenance phases of a project. The ALMA real time control system uses a Linux based real time operating system to interact with the hardware and the CORBA based ALMA Common Software to communicate in the distributed computing environment. Mixing the requirements of real time computing and the non-deterministic CORBA middleware has produced an interesting design. We discuss the architecture, design, and implementation of the ALMA real time control system. Highlight some lessons learned along the way, and justify our assertion that this should be the last large scale real time control system in radio astronomy.

  8. Caracterización de los delitos informáticos en Colombia

    Directory of Open Access Journals (Sweden)

    Iván Manjarrés Bolaño

    2012-07-01

    Full Text Available ResumenEs evidente que los avances tecnológicos demuestran la evolución del hombre, y eso lo podemos comprobar a través de los medios que permiten el almacenamiento, la transmisión y la administración de la información. Avances que han modificado el vivir diario de las personas y de las organizaciones, las cuales reflejan el aumento de transacciones comerciales, comercio electrónico, comunicaciones en línea, los procesos industriales, las investigaciones, la seguridad, la sanidad, etc., pero los sistemas de información que han permitido mejorar ostensiblemente los procesos al interior de las organizaciones, son los que al mismo tiempo han generado una serie de comportamientos ilícitos, que se les denomina “Delitos Informáticos”, y es el tema a abordar en este artículo de investigación, que se enmarca dentro del proyecto interdisciplinar titulado La seguridad en los Delitos informáticos desarrollado por estudiantes y docentes de los programas de Derecho e Ingeniería de Sistemas de la Corporación Universitaria Americana. AbstractIt is clear that technological advances show the evolution of man, and we can check through the means for storage, transmission and information management. Advances that have changed the daily life of individuals and organizations, which reflect increased business transactions, electronic commerce, online communications , industrial processes , research , safety , health, etc. . , But systems information that allowed significantly improve processes within organizations are at the same time have created a series of unlawful conduct, which are called “ Computer Crimes “ and is the subject addressed in this research article, that is part of the interdisciplinary project entitled security in cybercrime developed by students and teachers of law programs and Systems Engineering of the American University Corporation.

  9. [Parenting Information: Drugs. Informacion Para los Padres: Sobre las Drojas.

    Science.gov (United States)

    Moreno, Steve

    These two booklets provide basic information about drugs and drug abuse and are part of a series of 22 booklets, designed specifically to help parents understand their children and help them to learn. "Let's Talk about Drug Abuse," (booklet #18), reviews foreign substances or drugs young people are often exposed to (i.e., tobacco, alcohol,…

  10. La informática en los centros educativos: entre el ideal y la acción

    OpenAIRE

    Cerdá, Ernesto Pedro; Moyetta, Adriana M.; Schwartz, Gladys; Solivellas, Daniela Beatriz; Angeli, Sandra E.; Guazzone, Jorge O.; Ferreira Szpiniak, Ariel

    2005-01-01

    El presente trabajo brinda resultados obtenidos en el Proyecto de Investigación “Modelos de aplicación de la informática en los Centros Educativos” (perteneciente a la Universidad Nacional de Río Cuarto), en relación a las posturas que poseen los directivos de Centros Educativos de nivel primario en cuanto a la informática en la escuela y a las actividades que los profesionales encargados de los laboratorios de computación llevan a cabo en los mismos. La incorporación de la Informática en ...

  11. El surgimiento de la doctrina de la transmigración de las almas en la India

    OpenAIRE

    Kahle Armbruster, Marcos David

    2011-01-01

    En este trabajo se estudia el complejo proceso de configuración de la doctrina de la transmigración de las almas en la literatura védica. Después de una parte introductoria en la que se revisan los diferentes textos, sus escuelas y su localización, se estudian aquellos elementos de los himnos védicos que se pueden considerar antecedentes de esta doctrina y que han conducido o contribuido a su formulación. En los brāhmanas, los comentarios rituales, se desarrollan las distintas teorías que con...

  12. Referencias al contrabando en los informes de los «oidores» de la Real Audiencia de Extremadura

    Directory of Open Access Journals (Sweden)

    Eusebio MEDINA GARCÍA

    2009-11-01

    Full Text Available RESUMEN: En este artículo se recogen y se comentan las principales referencias sobre el contrabando tradicional en la frontera de España y Portugal, contenidas en los informes de los «oidores» (1791 y en otras disposiciones de la Real Audiencia de Extremadura. Además de resaltar la importancia que tuvo la instauración de la Real Audiencia de Extremadura en el proceso de consolidación de la Administración central en la región, ponemos de manifiesto el enorme interés de la autoridad real por conocer, para erradicar, los tráficos ilegales; siendo la recién estrenada —Real Audiencia—, un instrumento fundamental para implementar esa política de represión del contrabando en la frontera de Portugal, a finales del siglo XVIII.ABSTRACT: In this article the main references on the traditional smuggling in the border between Spain and Portugal, contained in the reports the «oidores» (1791 and in other regulations of the Royal Court of Extremadura are gathered and commented. Besides highlighting the great importance that the establishment of the Royal Court of Extremadura had in the process of consolidation of the state administration in the region, we point out the enormous interest of the Royal Authority in knowing the illegal trafficking to eradicate it. In this sense, the new Royal Court was a fundamental instrument to implement this policy of smuggling repression in the border at the end of 18th century.

  13. Detecting the First Quasars with ALMA

    Science.gov (United States)

    Schleicher, Dominik R. G.; Spaans, Marco; Klessen, Ralf S.

    2010-05-01

    We show that ALMA is the first telescope that can probe the dust-obscured central region of quasars at z > 5 with a maximum resolution of ~ 30 pc employing the 18 km baseline. We explore the possibility of detecting the first quasars with ALMA (Schleicher, Spaans, & Klessen 2009). For this purpose, we adopt the Seyfert 2 galaxy NGC 1068 as a reference system and calculate the expected fluxes if this galaxy were placed at high redshift. This choice is motivated by the detailed observations available for this system and the absence of any indication for an evolution in metallicity in high-redshift quasars. It is a conservative choice due to the moderate column densities in NGC 1068, leading to moderate fluxes.

  14. CURA MÉDICA DE ALMAS (CMA

    Directory of Open Access Journals (Sweden)

    Ancisar Restrepo Toro

    2001-01-01

    Full Text Available La «Cura médica de almas» tiene como objetivo señalar otra zona de aplicación de la Logoterapia, el acercamiento al hombre que sufre, al homo patiens, pero no ya a su sufrimiento en sí mismo sino a su humanidad. Si la Logoterapia, en su sentido más estricto, es la terapia indicada para las neurosis noógenas o en otros casos es complementaria de las psicoterapias, en el caso de la «Cura médica de almas» ya no es intervención terapéutica sino, específicamente, ejercicio de la humanidad del terapeuta en contacto con la humanidad de su paciente.

  15. Prospects for Asymmetric PNe with ALMA

    CERN Document Server

    Huggins, P J

    2010-01-01

    Millimeter and sub-millimeter observations have made fundamental contributions to our current understanding of the transition from AGB stars to white dwarfs. The approaching era of ALMA brings significantly enhanced observing capabilities at these wavelengths and promises to push back the frontiers in a number of ways. We examine the scientific prospects of this new era for PNe, with an emphasis on how developments may contribute to the goals of the asymmetric PNe community.

  16. Performance highlights of the ALMA correlators

    Science.gov (United States)

    Baudry, Alain; Lacasse, Richard; Escoffier, Ray; Webber, John; Greenberg, Joseph; Platt, Laurence; Treacy, Robert; Saez, Alejandro F.; Cais, Philippe; Comoretto, Giovanni; Quertier, Benjamin; Okumura, Sachiko K.; Kamazaki, Takeshi; Chikada, Yoshihiro; Watanabe, Manabu; Okuda, Takeshi; Kurono, Yasutake; Iguchi, Satoru

    2012-09-01

    Two large correlators have been constructed to combine the signals captured by the ALMA antennas deployed on the Atacama Desert in Chile at an elevation of 5050 meters. The Baseline correlator was fabricated by a NRAO/European team to process up to 64 antennas for 16 GHz bandwidth in two polarizations and another correlator, the Atacama Compact Array (ACA) correlator, was fabricated by a Japanese team to process up to 16 antennas. Both correlators meet the same specifications except for the number of processed antennas. The main architectural differences between these two large machines will be underlined. Selected features of the Baseline and ACA correlators as well as the main technical challenges met by the designers will be briefly discussed. The Baseline correlator is the largest correlator ever built for radio astronomy. Its digital hybrid architecture provides a wide variety of observing modes including the ability to divide each input baseband into 32 frequency-mobile sub-bands for high spectral resolution and to be operated as a conventional 'lag' correlator for high time resolution. The various observing modes offered by the ALMA correlators to the science community for 'Early Science' are presented, as well as future observing modes. Coherently phasing the array to provide VLBI maps of extremely compact sources is another feature of the ALMA correlators. Finally, the status and availability of these large machines will be presented.

  17. Application development using the ALMA common software

    Science.gov (United States)

    Chiozzi, G.; Caproni, A.; Jeram, B.; Sommer, H.; Wang, V.; Plesko, M.; Sekoranja, M.; Zagar, K.; Fugate, D. W.; Harrington, S.; Di Marcantonio, P.; Cirami, R.

    2006-06-01

    The ALMA Common Software (ACS) provides the software infrastructure used by ALMA and by several other telescope projects, thanks also to the choice of adopting the LGPL public license. ACS is a set of application frameworks providing the basic services needed for object oriented distributed computing. Among these are transparent remote object invocation, object deployment and location based on a container/component model, distributed error, alarm handling, logging and events. ACS is based on CORBA and built on top of free CORBA implementations. Free software is extensively used wherever possible. The general architecture of ACS was presented at SPIE 2002. ACS has been under development for 6 years and it is midway through its development life. Many applications have been written using ACS; the ALMA test facility, APEX and other telescopes are running systems based on ACS. This is therefore a good time to look back and see what have been until now the strong and the weak points of ACS in terms of architecture and implementation. In this perspective, it is very important to analyze the applications based on ACS, the feedback received by the users and the impact that this feedback has had on the development of ACS itself, by favoring the development of some features with respect to others. The purpose of this paper is to describe the results of this analysis and discuss what we would like to do in order to extend and improve ACS in the coming years, in particular to make application development easier and more efficient.

  18. The Criticality Safety Information Resource Center at Los Alamos National Laboratory

    International Nuclear Information System (INIS)

    The mission of the Criticality Safety Information Resource Center (CSIRC) at Los Alamos National Laboratory (LANL) is the preservation of primary documentation supporting criticality safety. In many cases, but not all, this primary documentation consists of experimentalists' logbooks. Experience has shown that the logbooks and other primary information are vulnerable to being discarded. Destruction of these logbooks results in a permanent loss to the criticality safety community

  19. ESO and NSF Sign Agreement on ALMA

    Science.gov (United States)

    2003-02-01

    Green Light for World's Most Powerful Radio Observatory On February 25, 2003, the European Southern Observatory (ESO) and the US National Science Foundation (NSF) are signing a historic agreement to construct and operate the world's largest and most powerful radio telescope, operating at millimeter and sub-millimeter wavelength. The Director General of ESO, Dr. Catherine Cesarsky, and the Director of the NSF, Dr. Rita Colwell, act for their respective organizations. Known as the Atacama Large Millimeter Array (ALMA), the future facility will encompass sixty-four interconnected 12-meter antennae at a unique, high-altitude site at Chajnantor in the Atacama region of northern Chile. ALMA is a joint project between Europe and North America. In Europe, ESO is leading on behalf of its ten member countries and Spain. In North America, the NSF also acts for the National Research Council of Canada and executes the project through the National Radio Astronomy Observatory (NRAO) operated by Associated Universities, Inc. (AUI). The conclusion of the ESO-NSF Agreement now gives the final green light for the ALMA project. The total cost of approximately 650 million Euro (or US Dollars) is shared equally between the two partners. Dr. Cesarsky is excited: "This agreement signifies the start of a great project of contemporary astronomy and astrophysics. Representing Europe, and in collaboration with many laboratories and institutes on this continent, we together look forward towards wonderful research projects. With ALMA we may learn how the earliest galaxies in the Universe really looked like, to mention but one of the many eagerly awaited opportunities with this marvellous facility". "With this agreement, we usher in a new age of research in astronomy" says Dr. Colwell. "By working together in this truly global partnership, the international astronomy community will be able to ensure the research capabilities needed to meet the long-term demands of our scientific enterprise, and

  20. The 492 GHz emission of Sgr A* constrained by ALMA

    Science.gov (United States)

    Liu, Hauyu Baobab; Wright, Melvyn C. H.; Zhao, Jun-Hui; Mills, Elisabeth A. C.; Requena-Torres, Miguel A.; Matsushita, Satoki; Martín, Sergio; Ott, Jürgen; Morris, Mark R.; Longmore, Steven N.; Brinkerink, Christiaan D.; Falcke, Heino

    2016-09-01

    Aims: Our aim is to characterize the polarized continuum emission properties including intensity, polarization position angle, and polarization percentage of Sgr A* at ~492 GHz. This frequency, well into the submillimeter bump where the emission is supposed to become optically thin, allows us to see down to the event horizon. Hence the reported observations contain potentially vital information on black hole properties. We have compared our measurements with previous, lower frequency observations, which provides information in the time domain. Methods: We report continuum emission properties of Sgr A* at ~492 GHz, based on Atacama Large Millimeter Array (ALMA) observations. We measured flux densities of Sgr A* from the central fields of our ALMA mosaic observations. We used calibration observations of the likely unpolarized continuum emission of Titan and the observations of Ci line emission, to gauge the degree of spurious polarization. Results: The flux density of 3.6 ± 0.72 Jy which we measured during our run is consistent with extrapolations from previous, lower frequency observations. We found that the continuum emission of Sgr A* at ~492 GHz shows large amplitude differences between the XX and the YY correlations. The observed intensity ratio between the XX and YY correlations as a function of parallactic angle can be explained by a constant polarization position angle of ~158°± 3°. The fitted polarization percentage of Sgr A* during our observational period is 14% ± 1.2%. The calibrator quasar J1744-3116 we observed on the same night can be fitted to Stokes I = 252 mJy, with 7.9% ± 0.9% polarization at position angle PA = 14°± 4.2°. Conclusions: The observed polarization percentage and polarization position angle in the present work appear consistent with those expected from longer wavelength observations in the period of 1999-2005. In particular, the polarization position angle at 492 GHz expected from the previously fitted 167°± 7° intrinsic

  1. ESO Signs Largest-Ever European Industrial Contract For Ground-Based Astronomy Project ALMA

    Science.gov (United States)

    2005-12-01

    coordinating consortiums in charge of complex, high-performance ground systems." ALMA is an international astronomy facility. It is a partnership between Europe, North America and Japan, in cooperation with the Republic of Chile. The European contribution is funded by ESO and Spain, with the construction and operations being managed by ESO. A matching contribution is being made by the USA and Canada, who will also provide 25 antennas. Japan will provide additional antennas, thus making this a truly worldwide endeavour. ALMA will be located on the 5,000m high Llano de Chajnantor site in the Atacama Desert of Northern Chile. ALMA will consist of a giant array of 12-m antennas separated by baselines of up to 18 km and is expected to start partial operation by 2010-2011. The excellent site, the most sensitive receivers developed so far, and the large number of antennas will allow ALMA to have a sensitivity that is many times better than any other comparable instrument. "ALMA will bring to sub-millimetre astronomy the aperture synthesis techniques of radio astronomy, enabling precision imaging to be done on sub-arcsecond angular scales, and will nicely complement the ESO VLT/VLTI observatory", said Dr. Hans Rykaczewski, the ALMA European Project Manager. Millimetre-wave astronomy is the study of the universe in the spectral region between what is traditionally considered radio waves and infrared radiation. In this realm, ALMA will study the evolution of galaxies, including very early stages, gather crucial data on the formation of stars, proto-planetary discs, and planets, and provide new insights on the familiar objects of our own solar system. A prototype antenna had already been built by Alcatel Alenia Space and European Industrial Engineering and thoroughly tested along with prototypes antennas from Vertex/LSI and Mitsubishi at the ALMA Antenna Test Facility located at the Very Large Array site in Socorro, New Mexico. For more information on the ALMA project, please go to http://www.eso.org/projects/alma/.

  2. Informe anual sobre el medio ambiente y los recursos naturales 2000

    OpenAIRE

    Banco Interamericano de Desarrollo (BID)

    2001-01-01

    El presente informe sobre medio ambiente y los recursos naturales abarca las acciones y sucesos ocurridos durante el año 2000. Las operaciones crediticias del BID destinadas al medio ambiente en 2000 totalizaron 531 millones de dólares. El Banco aprobó 13 préstamos para el medio ambiente y los recursos naturales. Estos préstamos se destinaron a programas de desarrollo urbano, incluyendo suministro de agua y saneamiento (357 millones de dólares), conservación de recursos naturales (93 millones...

  3. Mejora de la calidad de los informes de los ensayos clínicos aleatorio controlados. Recomendaciones del grupo de trabajo CONSORT

    Directory of Open Access Journals (Sweden)

    Begg Colin

    1998-01-01

    Full Text Available Este trabajo corresponde a la traducción al español de la Colaboración Especial publicada en The Journal of the American Medical Association en agosto de 1996, junto con el editorial How to report Randomized Controlled Trials. The Consort Statement, publicada en el mismo número. En ella se describe la elaboración de las Normas Consolidadas para la elaboración de los Informes de los Ensayos Clínicos Controlados, por un grupo de trabajo formado por los componentes del grupo SORT y del Grupo de Trabajo Asilomar, junto con el director de una revista y el autor del informe de un ensayo clínico. El trabajo se realizó mediante un proceso Delphi y el resultado fue una lista de comprobación (checklist y un diagrama de flujo. La primera está compuesta por 21 puntos que se refieren principalmente a los métodos, resultados y discusión del informe de un ensayo clínico controlado, identificándose la información necesaria para poder evaluar la validez interna y externa del ensayo, valorándose la mejora como positiva, tanto para los pacientes, como para los editores de las revistas y los revisores de las mismas.

  4. Los informes anuales de la Comisión Interamericana de Derechos Humanos, 1991-2000

    OpenAIRE

    2000-01-01

    Los informes que anualmente presenta la Comisión a la Asamblea General de la OEA han variado en la última década tanto en el tipo de situaciones que considera para revisión como en su forma de presentación. En lo que se refiere al contenido, ha habido un aumento del interés de la Comisión por los derechos sociales económicos y culturales, cuando en un principio su actividad se concentraba en los derechos civiles y políticos. También ha habido un interés creciente por la situación de grupos po...

  5. Italian Science Case for ALMA Band 2+3

    CERN Document Server

    Beltran, M T; Brand, J; Casasola, V; Cesaroni, R; Codella, C; Fontani, F; Gregorini, L; Guidi, G; Hunt, L; Liuzzo, E; Marconi, A; Massardi, M; Moscadelli, L; Paladini, R; Podio, L; Prandoni, I; Rygl, K L J; Rivilla, V; .,; Testi, L

    2015-01-01

    The Premiale Project "Science and Technology in Italy for the upgraded ALMA Observatory - iALMA" has the goal of strengthening the scientific, technological and industrial Italian contribution to the Atacama Large Millimeter/submillimeter Array (ALMA), the largest ground based international infrastructure for the study of the Universe in the microwave. One of the main objectives of the Science Working Group (SWG) inside iALMA, the Work Package 1, is to develop the Italian contribution to the Science Case for the ALMA Band 2 or Band 2+3 receiver. ALMA Band 2 receiver spans from ~67 GHz (bounded by an opaque line complex of ozone lines) up to 90 GHz which overlaps with the lower frequency end of ALMA Band 3. Receiver technology has advanced since the original definition of the ALMA frequency bands. It is now feasible to produce a single receiver which could cover the whole frequency range from 67 GHz to 116 GHz, encompassing Band 2 and Band 3 in a single receiver cartridge, a so called Band 2+3 system. In addit...

  6. El (reconocimiento de la madre en La mitad del alma

    Directory of Open Access Journals (Sweden)

    Sandra J. Schumm

    2011-01-01

    Full Text Available Resumen: La mitad del alma de Carme Riera, en que C rememora a su madre, enfatiza la importancia del reconocimiento de las mujeres en la memoria histórica. Desde el mito griego de Atena, quien ignoraba a su madre Metis, la sociedad patriarcal ha excluido a la madre, lo cual promete que la hija conlleve negación también, según Amber Jacobs en On Matricide. Jacobs observa que en La Oresteia hay crímenes sancionados contra las mujeres, las hijas están deprimidas, existe incesto contra la hija, la reproducción familiar se paraliza, toda la sociedad sufre y la hija se desperdicia también cuando la madre es menospreciada. Jacobs afirma que este desprecio de la madre que transcurría en los mitos griegos continúa en la sociedad y la psicología hoy en día. En esta novela de Riera, la hija protagonista, quien desconoce a su madre, sufre de un estado depresivo, la falta de creatividad y una conexión demasiado fuerte con su padre, semejante a lo que Jacobs observa en los mitos, pero la escritura de C sobre su madre la integrará en la consciencia y mejorará la situación de la hija y, últimamente, la de toda la civilización.Summary: Carme Riera‟s La mitad del alma, in which C recollects her mother, emphasizes the importance of the recognition of women in historic memory. Ever since the Greek myth of Athena, who was ignorant of the existence of her mother, Metis, patriarchal society has excluded the mother, a fact which promises that the daughter will also experience negation, according to Amber Jacobs in On Matricide. Jacobs observes that in La Oresteia there are sanctioned crimes against women, the daughters are depressed, there is incest against the daughter, she is dishonored, family reproduction stops, and all of society suffers when the mother is not appreciated. Jacobs affirms that the distain of the mother that took place in Greek myths continues in society and psychology today. In this novel by Riera, the protagonist/daughter, who

  7. Los servicios de salud mental se enredan en la informática

    OpenAIRE

    Moreno-Küstner, Berta

    2015-01-01

    Con los últimos adelantos en la tecnología informática, cada vez resulta más fácil diseñar, alimentar y gestionar grandes bases de datos, estandarizar la entrada y salida de la información, mejorar su accesibilidad, facilitar las tareas administrativas y repetitivas como informes, recetas, circulares,… en definitiva suponen una mejora en la gestión de la información clínica. Efectivamente se está avanzando en el desarrollo informático aplicado al ámbito sanitario, sin embargo, el gran avance ...

  8. Goodbye to WIMPs: A Scalable Interface for ALMA Operations

    Science.gov (United States)

    Schwarz, J.; Pietriga, E.; Schilling, M.; Grosbol, P.

    2011-07-01

    The operators of the ALMA Observatory will monitor and control more than 50 mm/submm radio antennas and their associated instrumentation from an operations site that is separated from this hardware by 35-50 km. Software that enables them to identify trouble spots and react to failures quickly in this environment will be critical to the safe and efficient functioning of the observatory. Early commissioning of ALMA uses a operator interface implemented with a standard window, icon, menu, pointing device (WIMP) toolkit. Early experience indicates that this paradigm will not scale well as the number of antennas approaches its full complement. Operators lose time as they manipulate overlapping or tabbed windows to drill-down to detailed diagnostic data, losing a feeling for "where they are" in the process. The WIMP model reaches its limits when there is so much information to present to users that they cannot focus on details while maintaining a view from above. To simplify the operators' tasks and let them concentrate on the real issues at hand rather than continually re-organizing their use of screen space, we are replacing the existing top-level interface with a multi-scale interface that takes advantage of semantic zooming, dynamic network visualization and other advanced filtering, navigation and visualization features. Following the first of several planned participatory design workshops, we have developed prototypes to show how users' needs can be met with the kinds of navigation that become possible when the restrictions of the WIMP model are lifted. Cycles of design and implementation coupled with active user feedback will characterize this project up through deployment.

  9. La inmortalidad del alma: historia de un argumento político

    OpenAIRE

    Saralegui Benito, Miguel Manuel

    2013-01-01

    Se examina una cuestión fundamental y poco estudiada de la teología política: la relación entre la defensa de la inmortalidad del alma y el mantenimiento del orden público. Se realiza un recorrido histórico por autores como Pietro Pomponazzi y Tomás Moro, que aceptan motivos políticos para defenderla, y David Hume, quien considera que no existe ningún motivo político para mantener dicha relación. Por último, se analizan los argumentos esgrimidos para mostrar que su eficacia está condicionada ...

  10. Dos revistas similares pero distintas: “El Olivo” y “Alma100”

    Directory of Open Access Journals (Sweden)

    Carlos Arbelos

    2006-01-01

    Así aparecen dos revistas similares pero diferentes, si bien ambas se proponen la difusión y divulgación del flamenco, una El Olivo lo hace desde una perspectiva más tradicional y Alma100 lo aborda desde conceptos más ligados a lo que se ha denominado postmodernidad. La otra gran diferencia es que mientras la primera depende económicamente casi exclusivamente de una subvención institucional, la segunda lo hace desde los recursos propios que genera la publicidad que se inserta en la publicación

  11. Medidas procesales especiales y proteccíon de los derechos humanos Informe general

    Directory of Open Access Journals (Sweden)

    John A.E. Vervaele

    2009-10-01

    Full Text Available El objetivo del informe general es realizar un análisis comparativo de los informes nacionales para evidenciar los procesos de transformación de los sistemas nacionales de justicia penal, en particular del proceso penal, en el que se han introducido medidas procesales especiales para hacer frente al terrorismo y al crimen organizado, y determinar si esto ha llevado a los países a apartarse de sus propias normas fundamentales, procedimientos, principios y estándares de derechos humanos aplicables. Partiendo de la premisa de que el sistema integrado de derecho penal tiene tres dimensiones – la protección de las personas (la dimensión de escudo, la disposición de instrumentos de aplicación de la ley (la dimensión de la espada y de pesos y contrapesos / trias politica (la dimensión constitucional – el informe ofrece un panorama general de las transformaciones relacionadas entre sí, principalmente en la fase previa al juicio, que han afectado a tales dimensiones como consecuencia de tres oleadas de ‘guerras’ (contra las drogas, el crimen organizado y el terrorismo. En muchos países, las garantías procesales y los principios que protegen frente a violaciones del derecho a un juicio justo son considerados una carga para la eficacia de la persecución de los delitos graves. Estas reformas han dado lugar a una clara expansión del estado punitivo y a que queden difuminadas las distinciones clásicas, y no favorecen al estado de derecho. El actuar centrado en la seguridad pública y en la investigación coactiva preventiva socava el sistema de justicia penal. Con un sistema de justicia penal utilizado crecientemente como instrumento para regular el presente y/o el futuro en lugar de para castigar el comportamiento pasado, y un proceso penal en el que la investigación previa al juicio no se dirige a conocer la verdad en relación con el delito cometido, sino a la construcción y de-construcción de la peligrosidad social, los

  12. Las relaciones entre los sectores formal e informal. Una exploración sobre su naturaleza

    Directory of Open Access Journals (Sweden)

    Víctor E. Tokman

    2001-12-01

    Full Text Available Desde que la OIT adoptó el concepto de sector informal, se han suscitado intrincadas discusiones que sirvieron, al menos, para estimular el debate sobre el subdesarrollo y permitir una mejor comprensión de sus problemas y soluciones. De este modo se procura estudiar el fenómeno limitado, pero decisivo, de las relaciones que mantiene elsector informal con el resto de la economía. El análisis de estas relaciones es un punto de partida muy fructífero pues permite ordenar los distintos puntos de vista teóricos sobre el sector informal. En efecto, estos criterios pueden distinguirse por el tipo de vinculaciones que establecen entre la economía informal y formal. Así, en la primera parte, el autor presenta los enfoques contrapuestosde las relaciones <> y las de explotación, con sus diversas variantes y esboza una perspectiva propia en la que sostiene que aquellas relaciones son de <>. En la segunda parte ensaya una estimación para Chile, de la <> del sector informal en relación con el resto de la economía basado en información procedente de las cuentas nacionales; para culminar, en la tercera parte, con la interpretación de los datos de encuestas realizadas en Santiago sobre las características y desempeño del comercio informal.---Since the ILO adopted the concept of informal sector, intricate discussions have emerged that, at least, gave a stimulus to the debate on development and permitted a better understanding of its problems and solutions. It is then of interest to study the limited but critical phenomenon of the relationships between the informal sector and the rest of the economy. The study of these relations is a very fruitful starting point because it permits to organize different theoretical points of view on the informal sector. In fact, these criteria can be distinguished by the type of relations they establish between the formal and informal economies. Thus, in the

  13. ALMA Observations of the Orion Proplyds

    CERN Document Server

    Mann, Rita K; Johnstone, Doug; Andrews, Sean M; Williams, Jonathan P; Bally, John; Ricci, Luca; Hughes, A Meredith; Matthews, Brenda C

    2014-01-01

    We present ALMA observations of protoplanetary disks ("proplyds") in the Orion Nebula Cluster. We imaged 5 individual fields at 856um containing 22 HST-identified proplyds and detected 21 of them. Eight of those disks were detected for the first time at submillimeter wavelengths, including the most prominent, well-known proplyd in the entire Orion Nebula, 114-426. Thermal dust emission in excess of any free-free component was measured in all but one of the detected disks, and ranged between 1-163 mJy, with resulting disk masses of 0.3-79 Mjup. An additional 26 stars with no prior evidence of associated disks in HST observations were also imaged within the 5 fields, but only 2 were detected. The disk mass upper limits for the undetected targets, which include OB stars, theta1Ori C and theta1Ori F, range from 0.1-0.6 Mjup. Combining these ALMA data with previous SMA observations, we find a lack of massive (>3 Mjup) disks in the extreme-UV dominated region of Orion, within 0.03 pc of O-star theta1Ori C. At large...

  14. ALMA Nutator Design and Preliminary Performance

    CERN Document Server

    Martin-Cocher, Pierre; Koch, Patrick M; Ni, Chih-Wen; Chen, Wei-Long; Chen, Ming-Tang; Raffin, Philippe; Ong, Chin-Long; Ho, Paul T P; Symmes, Arthur

    2013-01-01

    We report the past two years of collaboration between the di?erent actors on the ALMA nutator. Building on previous developments, the nutator has seen changes in much of the design. A high-modulus carbon ?fiber structure has been added on the back of the mirror in order to transfer the voice coils forces with less deformation, thus reducing delay problems due to flexing. The controller is now an off?-the-shelf National Instrument NI-cRIO, and the ampli?fier a class D servo drive from Advanced Motion Controls, with high peak power able to drive the coils at 300 Volts DC. The stow mechanism has been totally redesigned to improve on the repeatability and precision of the stow position, which is also the reference for the 26 bits Heidenhain encoders. This also improves on the accuracy of the stow position with wind loading. Finally, the software, written largely with National Instrument's LabView, has been developed. We will discuss these changes and the preliminary performances achieved to date. Keywords: ALMA, ...

  15. Las relaciones entre los sectores formal e informal. Una exploración sobre su naturaleza

    OpenAIRE

    Víctor E. Tokman

    2001-01-01

    Desde que la OIT adoptó el concepto de sector informal, se han suscitado intrincadas discusiones que sirvieron, al menos, para estimular el debate sobre el subdesarrollo y permitir una mejor comprensión de sus problemas y soluciones. De este modo se procura estudiar el fenómeno limitado, pero decisivo, de las relaciones que mantiene elsector informal con el resto de la economía. El análisis de estas relaciones es un punto de partida muy fructífero pues permite ordenar los distintos puntos de ...

  16. Quasi-optical attenuators for ALMA band 10 receiver

    Science.gov (United States)

    Gonzalez, A.; Fujii, Y.; Kaneko, K.; Uzawa, Y.

    2011-12-01

    Simple quasi-optical attenuators based on beam truncation have been designed, fabricated and tried on ALMA band 10 receivers (787-950 GHz) with optimal results. The design is based on physical-optics simulations considering effects of diffraction. The use of these attenuators allows flexibility in the design of the local oscillator (LO) quasi-optical injection scheme depending on the specific performance of components for each of the 73 ALMA band 10 receivers. In particular, they have proven very effective to keep system noise within the stringent ALMA requirements (230 K at 80% of 787-950 GHz band).

  17. World-Wide Effort Bringing ALMA Telescope Into Reality

    Science.gov (United States)

    2008-02-01

    In the thin, dry air of northern Chile's Atacama Desert, at an altitude of 16,500 feet, an amazing new telescope system is taking shape, on schedule to provide the world's astronomers with unprecedented views of the origins of stars, galaxies, and planets. The Atacama Large Millimeter/submillimeter Array (ALMA) will open an entirely new "window" on the Universe, allowing scientists to unravel longstanding and important astronomical mysteries. ALMA Artist's Concept Artist's Concept of Completed ALMA CREDIT: ALMA/ESO/NRAO/NAOJ Click on image for high-resolution file (182 KB) "Most of the photons in the Universe are in the wavelength range that ALMA will receive, and ALMA will give us our first high-resolution views at these wavelengths. This will be a tremendous advancement for astronomy and open one of our science's last frontiers," Anneila Sargent, a Caltech professor and ALMA Board member, told the American Association for the Advancement of Science at its meeting in Boston, Mass. The millimeter and submillimeter wavelength range lies between what is traditionally considered radio waves and infrared waves. ALMA, a system using up to 66 high-precision dish antennas working together, will provide astronomers with dramatically greater sensitivity, the ability to detect faint objects, and resolving power, the ability to see fine detail, than has ever before been available in this range. "This ambitious project is the product of an international collaboration that spans the globe," Sargent said. "ALMA truly will enable transformational science and providing this capability has required a massive, world-wide effort," she added. The ALMA project is a partnership between Europe, Japan and North America in cooperation with the Republic of Chile. ALMA is funded in Europe by ESO, in Japan by the National Institutes of Natural Sciences in cooperation with the Academia Sinica in Taiwan and in North America by the U.S. National Science Foundation in cooperation with the

  18. La informática forense y los delitos informáticos

    Directory of Open Access Journals (Sweden)

    Alex Canedo Estrada

    2010-07-01

    Full Text Available ResumenEste artículo da una mirada general acerca de la informática forense, su definición y su implicaciónen la forma como se trata la información en el mundo. Además, muestra la importancia de lainformática forense y su puesta en práctica de manera efectiva, de la mano con diferentesherramientas tecnológicas. En definitiva, explica su aplicación, así como la legislación existenteen materia de delitos informáticos en nuestro país.Palabras claves: Informática forense, delito informático, auditoría informática, seguridad. AbstractThis paper gives a general look about the forensic computer science, its definition and maincharacteristics. Also, it shows the importance that the forensic computer science is put into practicein an effective way, together with deferent technology tools. Finally, explains the application, aswell the existent legislation for computer science crime in our country. Key Words: Forensic computer science, computer science crime, computer science audit,computer science security, technology and tools.

  19. Testing Wave Propagation Properties in the Solar Chromosphere with ALMA and IRIS

    Science.gov (United States)

    Fleck, Bernard; Straus, Thomas; Wedemeyer, Sven

    2016-05-01

    Waves and oscillations are interesting not only from the point of view that they can propagate energy into the chromosphere and dissipate that energy to produce non-radiative heating, they also carry information about the structure of the atmosphere in which they propagate. Since the late 80s there is substantial evidence that the chromospheric wave field is dominated by a non-propagating component, presumably resulting from wave reflection at the transition region. Observations of Doppler oscillations measured in the Ca II infrared tripet lines, Ca II K, and He 10830 all show vanishing phase lags (i.e. vanishing travel time differences) between the various lines, in particular also for frequencies above the cut-off frequency. Why is the apparent phase speed of high frequency acoustic waves in the chromosphere so high? Are these results misleading because of complex radiation transfer effects in these optically thick lines? ALMA, which acts as a linear thermometer of the solar chromosphere, will provide measurements of the local plasma conditions that should be, at least in principle, much easier to interpret. Multi-wavelength time series of ALMA observations of the temperature fluctuations of inter-network oscillations should allow travel time measurements between different heights as these disturbances propagate through the chromosphere and thus should finally settle the long-standing question about the propagation characteristics of high frequency acoustic waves in the chromosphere. We plan to combine ALMA mm-observations with high resolution IRIS observations in the Mg II h and k lines, and until ALMA observations are available, will study the expected signals using time series of mm-maps from 3D radiation hydrodynamics simulations that are being prepared within the framework of the Solar Simulations for the Atacama Large Millimeter Observatory Network (SSALMON).

  20. ALMA Observations of the Sun in Cycle 4 and Beyond

    CERN Document Server

    Wedemeyer, S; Battaglia, M; Labrosse, N; Fleishman, G; Hudson, H; Antolin, P; Alissandrakis, C; Ayres, T; Ballester, J; Bastian, T; Black, J; Benz, A; Brajsa, R; Carlsson, M; Costa, J; DePontieu, B; Doyle, G; de Castro, G Gimenez; Gunár, S; Harper, G; Jafarzadeh, S; Loukitcheva, M; Nakariakov, V; Oliver, R; Schmieder, B; Selhorst, C; Shimojo, M; Simões, P; Soler, R; Temmer, M; Tiwari, S; Van Doorsselaere, T; Veronig, A; White, S; Yagoubov, P; Zaqarashvili, T

    2016-01-01

    This document was created by the Solar Simulations for the Atacama Large Millimeter Observatory Network (SSALMON) in preparation of the first regular observations of the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA), which are anticipated to start in ALMA Cycle 4 in October 2016. The science cases presented here demonstrate that a large number of scientifically highly interesting observations could be made already with the still limited solar observing modes foreseen for Cycle 4 and that ALMA has the potential to make important contributions to answering long-standing scientific questions in solar physics. With the proposal deadline for ALMA Cycle 4 in April 2016 and the Commissioning and Science Verification campaign in December 2015 in sight, several of the SSALMON Expert Teams composed strategic documents in which they outlined potential solar observations that could be feasible given the anticipated technical capabilities in Cycle 4. These documents have been combined and supplemented w...

  1. ALMA observations of the Orion proplyds

    International Nuclear Information System (INIS)

    We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of protoplanetary disks ('proplyds') in the Orion Nebula Cluster. We imaged five individual fields at 856 μm containing 22 Hubble Space Telescope (HST)-identified proplyds and detected 21 of them. Eight of those disks were detected for the first time at submillimeter wavelengths, including the most prominent, well-known proplyd in the entire Orion Nebula, 114-426. Thermal dust emission in excess of any free-free component was measured in all but one of the detected disks, and ranged between 1 and 163 mJy, with resulting disk masses of 0.3-79 M jup. An additional 26 stars with no prior evidence of associated disks in HST observations were also imaged within the 5 fields, but only 2 were detected. The disk mass upper limits for the undetected targets, which include OB stars, θ1 Ori C, and θ1 Ori F, range from 0.1 to 0.6 M jup. Combining these ALMA data with previous Submillimeter Array observations, we find a lack of massive (≳3 M jup) disks in the extreme-UV-dominated region of Orion, within 0.03 pc of θ1 Ori C. At larger separations from θ1 Ori C, in the far-UV-dominated region, there is a wide range of disk masses, similar to what is found in low-mass star forming regions. Taken together, these results suggest that a rapid dissipation of disk masses likely inhibits potential planet formation in the extreme-UV-dominated regions of OB associations, but leaves disks in the far-UV-dominated regions relatively unaffected.

  2. Los informes de visita ad limina del cardenal Lorenzana en Toledo (1772-1800

    Directory of Open Access Journals (Sweden)

    Fernández Collado, Ángel

    2002-12-01

    Full Text Available Analysis of the visits ad limina of the cardinal Lorenzana during the years 1776, 1780, 1784, 1788, 1792 and 1796. It is accomplished with a synthesis of each report, that are included as documental appendix in its original draft language.

    Análisis de las visitas ad limina del cardenal Lorenzana de los años 1776, 1780, 1784, 1788, 1792 y 1796. Se realiza una síntesis de cada informe, que se incluyen como apéndice documental en su lengua de redacción original.

  3. ALMA Partners Break Ground on World's Largest Millimeter Wavelength Telescope

    Science.gov (United States)

    2003-11-01

    Scientists and dignitaries from North America, Europe, and Chile broke ground today (Thursday, November 6, 2003) on what will be the world's largest, most sensitive radio telescope operating at millimeter wavelengths. ALMA - the Atacama Large Millimeter Array - will be a single instrument composed of 64 high-precision antennas located on the Chajnantor plain of the Chilean Andes in the District of San Pedro de Atacama, 16,500 feet (5,000 meters) above sea level. ALMA's primary function will be to observe and image with unprecedented clarity the enigmatic cold regions of the Universe, which are optically dark, yet shine brightly in the millimeter portion of the electromagnetic spectrum. ALMA Array Artist's Conception of ALMA Array in Compact Configuration (Click on Image for Larger Version) Other Images Available: Artist's conception of the antennas for the Atacama Large Millimeter Array Moonrise over ALMA test equipment near Cerro Chajnantor, Chile VertexRSI antenna at the VLA test site The Atacama Large Millimeter Array is an international astronomy facility. ALMA is an equal partnership between Europe and North America, in cooperation with the Republic of Chile, and is funded in North America by the U.S. National Science Foundation (NSF) in cooperation with the National Research Council of Canada (NRC), and in Europe by the European Southern Observatory (ESO) and Spain. ALMA construction and operations are led on behalf of North America by the National Radio Astronomy Observatory (NRAO), which is managed by Associated Universities, Inc. (AUI), and on behalf of Europe by ESO. "The U.S. National Science Foundation joins today with our North American partner, Canada, and with the European Southern Observatory, Spain, and Chile to prepare for a spectacular new instrument," said Dr. Rita Colwell, director of the U.S. National Science Foundation. "The Atacama Large Millimeter Array will expand our vision of the Universe with "eyes" that pierce the shrouded mantles of

  4. U.S., European ALMA Partners Award Prototype Antenna Contracts

    Science.gov (United States)

    2000-03-01

    The U.S. and European partners in the Atacama Large Millimeter Array (ALMA) project have awarded contracts to U.S. and Italian firms, respectively, for two prototype antennas. ALMA is a planned telescope array, expected to consist of 64 millimeter-wave antennas with 12-meter diameter dishes. The array will be built at a high-altitude, extremely dry mountain site in Chile's Atacama desert, and is scheduled to be completed sometime in this decade. On February 22, 2000, Associated Universities Inc. (AUI) signed an approximately $6.2 million contract with Vertex Antenna Systems, of Santa Clara, Calif., for construction of one prototype ALMA antenna. AUI operates the U.S. National Radio Astronomy Observatory (NRAO) for the National Science Foundation under a cooperative agreement. The European partners contracted with the consortium of European Industrial Engineering and Costamasnaga, of Mestre, Italy, on February 21, 2000, for the production of another prototype. (Mestre is located on the inland side of Venice.) The two antennas must meet identical specifications, but will inherently be of different designs. This will ensure that the best possible technologies are incorporated into the final production antennas. Only one of the designs will be selected for final production. Several technical challenges must be met for the antennas to perform to ALMA specifications. Each antenna must have extremely high surface accuracy (25 micrometers, or one-third the diameter of a human hair, over the entire 12-meter diameter). This means that, when completed, the surface accuracy of the ALMA dishes will be 20 times greater than that of the Very Large Array (VLA) antennas, and about 50 times greater than dish antennas for communications or radar. The ALMA antennas must also have extremely high pointing accuracy (0.6 arcseconds). An additional challenge is that the antennas, when installed at the ALMA site in Chile, will be exposed to the ravages of weather at 16,500 feet (5000 meters

  5. Exploring remote operation for ALMA Observatory

    Science.gov (United States)

    Shen, Tzu-Chiang; Soto, Ruben; Ovando, Nicolás.; Velez, Gaston; Fuica, Soledad; Schemrl, Anton; Robles, Andres; Ibsen, Jorge; Filippi, Giorgio; Pietriga, Emmanuel

    2014-08-01

    The Atacama Large Millimeter /submillimeter Array (ALMA) will be a unique research instrument composed of at least 66 reconfigurable high-precision antennas, located at the Chajnantor plain in the Chilean Andes at an elevation of 5000 m. The observatory has another office located in Santiago of Chile, 1600 km from the Chajnantor plain. In the Atacama desert, the wonderful observing conditions imply precarious living conditions and extremely high operation costs: i.e: flight tickets, hospitality, infrastructure, water, electricity, etc. It is clear that a purely remote operational model is impossible, but we believe that a mixture of remote and local operation scheme would be beneficial to the observatory, not only in reducing the cost but also in increasing the observatory overall efficiency. This paper describes the challenges and experience gained in such experimental proof of the concept. The experiment was performed over the existing 100 Mbps bandwidth, which connects both sites through a third party telecommunication infrastructure. During the experiment, all of the existent capacities of the observing software were validated successfully, although room for improvement was clearly detected. Network virtualization, MPLS configuration, L2TPv3 tunneling, NFS adjustment, operational workstations design are part of the experiment.

  6. $\\eta$ Carinae Baby Homunculus Uncovered by ALMA

    CERN Document Server

    Abraham, Zulema; Beaklini, Pedro P B

    2014-01-01

    We report observations of $\\eta$ Carinae obtained with ALMA in the continuum of 100, 230, 280 and 660 GHz in 2012 November, with a resolution that varied from 2.88" to 0.45" for the lower and higher frequencies respectively. The source is not resolved, even at the highest frequency; its spectrum is characteristic of thermal bremsstrahlung of a compact source, but different from the spectrum of optically thin wind. The recombination lines H42$\\alpha$, He42$\\alpha$, H40$\\alpha$, He40$\\alpha$, H50$\\beta$, H28$\\alpha$, He28$\\alpha$, H21$\\alpha$ and He21$\\alpha$ were also detected and their intensities reveal non local thermodynamic equilibrium (NLTE) effects. We found that the line profiles could only be fit by an expanding shell of dense and ionized gas, which produces a slow shock in the surroundings of $\\eta$ Carinae. Combined with fittings to the continuum, we were able to constrain the shell size, radius, density, temperature and velocity. The detection of the He recombination lines is compatible with the hi...

  7. Solving the polarization problem in ALMA-VLBI observations

    CERN Document Server

    Marti-Vidal, I; Alef, W; Conway, J; Lindqvist, M; Zensus, A J

    2015-01-01

    The Atacama Large mm-submm Array (ALMA) is, by far, the most sensitive mm/submm telescope in the World. The ALMA Phasing Project (APP) will allow us to phase-up all the ALMA antennas and use them as one single VLBI station. This will be a key component of the Event Horizon Telescope (EHT), a Global VLBI array at millimeter wavelengths. A problem in the APP is the calibration and conversion of the polarization channels. Most VLBI stations record their signals in a circular basis, but the ALMA receivers record in a linear basis. The strategy that will be followed in the phased-ALMA VLBI observations will be to correlate in "mixed" basis (i.e., linear versus circular) and convert the visibilities to a pure circular basis after the correlation. We have developed an algorithm to perform such a polarization conversion of the VLBI visibilities. In these proceedings, we present the basics of the PolConvert algorithm and discuss on the polarization conversion in the general case were single dishes (besides phased arra...

  8. VIDEO AT OSF - Interview to David Rabanus, ESO, on the ALMA OSF site, at 2900 m

    CERN Multimedia

    2015-01-01

    In this interview, recorded on the ALMA OSF (Operations and Support Facilities) site, at 2900 m on the Chajnantor highlands, physicist David Rabanus of ESO/ ALMA takes us inside the heart of the ALMA antennas, to reveal how the antennas detect millimetric and submillimetric radiowaves.

  9. New Eyes on the Sun — Solar Science with ALMA

    Science.gov (United States)

    Wedemeyer, S.

    2016-03-01

    In Cycle 4, which starts in October 2016, the Atacama Large Millimeter/submillimeter Array (ALMA) will be open for regular observations of the Sun for the first time. ALMA’s impressive capabilities have the potential to revolutionise our understanding of our host star, with far-reaching implications for our knowledge about stars in general. The radiation emitted at ALMA wavelengths originates mostly from the chromosphere — a complex and dynamic layer between the photosphere and the corona that is prominent during solar eclipses. Despite decades of intensive research, the chromosphere is still elusive due to its complex nature and the resulting challenges to its observation. ALMA will change the scene substantially by opening up a new window on the Sun, promising answers to long-standing questions.

  10. The Soul of Lupus with ALMA (SOLA) Project Overview

    Science.gov (United States)

    Saito, M.; de Gregorio, I.; Team SOLA

    2015-12-01

    The SOLA (Soul of Lupus with ALMA) project is conducting comprehensive studies of the Lupus Molecular Clouds and their star formation processes. Our goal is to exploit ALMA and other facilities over a wide wavelength range to establish a prototypical low-mass star forming scenario based on the Lupus region. We focus mainly on 10-104 au scale physics, kinematics, density, and temperature, together with detailed modelling of radiative transfer. Our unique source catalog so far contains more than 700 sources at various evolutionary stages and we have obtained complementary data with Mopra, APEX, etc. In the poster, we will report the latest status of SOLA and the expected outcome in observing runs in the near future, including ALMA Cycle 3.

  11. Verificación de los informes de sostenibilidad de las empresas cotizadas en Alemania

    OpenAIRE

    MARTÍ PÉREZ, ARANTXA

    2015-01-01

    Tradicionalmente, la información publicada por las empresas se basaba en términos financieros y puramente obligatorios. Sin embargo, en los últimos años se está dando lugar un cambio de estrategia empresarial donde cobra gran importancia el desempeño ético, social y medioambiental. De este modo, en el presente trabajo se analizan los principales motivos a los que se debe esta transformación en el contexto de los negocios. Por un lado, debido a la difícil valoración de los activos intangibl...

  12. Alternativas a los ftalatos en adhesivos y tintas: Informe de vigilancia tecnológica

    OpenAIRE

    Cano Serrano, Encarnación; Cerezo García, Lidia; Urbina Fraile, Marina

    2008-01-01

    Los plastificantes mejoran la flexibilidad y el procesado de los polímeros. Los más empleados en todo el mundo son los ésteres de ácido ftálico como el DEHP (ftalato de bis(2-etilhexilo)), el DIDP (ftalato de diisodecilo), el DITDP (ftalato de diisotridecilo) y el DINP (ftalato de diisononilo)), existiendo más de 30 tipos diferentes de ftalatos en el mercado. La mayoría de los ftalatos poseen excelentes propiedades plastificantes y adhesivas, por lo que son empleados en la industria química p...

  13. Python code parallelization for ALMA, challenges and alternatives

    OpenAIRE

    Gonzalez, Justo; Taylor, Julian; Castro, Sandra; Kern, Jeff; Knudstrup, Jens; Zampieri, Stefano; Manning, Alisdair

    2015-01-01

    In the last few years development of Python code for science and data reduction purposes has gained significant popularity. ESO in itself uses a Python-based archiving  system for VLT and ALMA data. Also the data reduction suite for ALMA data is python-based. Rapid development is fostered by a big community and a wide range of already available packages. However Python enforces locking mechanisms, to ensure thread safety, that effectively reduce the capacity of Python to use only one cor...

  14. The limits of information in the negotiated debates/ Los límites de la información en los debates pactados

    Directory of Open Access Journals (Sweden)

    Dr. Xosé Soengas Pérez

    2009-01-01

    Full Text Available Resumen: La Academia de Televisión fue el escenario considerado neutral por el PSOE y por el PP para organizar los debates electorales previstos entre los candidatos de ambos partidos con motivo de las elecciones generales del 9-M de 2008, emitidos el 25 de febrero y el 3 de marzo. El análisis de los dos cara a cara que mantuvieron José Luis Rodríguez Zapatero y Mariano Rajoy pretende conocer las circunstancias en las que se fraguaron ambos encuentros, valorar su utilidad y determinar el grado de previsibilidad que ofreció la confrontación dialéctica entre los líderes de los dos partidos políticos mayoritarios, cuyas intervenciones fueron acordadas previamente, tanto los contenidos como la puesta en escena. Nos interesa comprobar hasta qué punto es compatible la libertad de información con los debates pactados y con la imposición de unos moderadores a los que se deja sin atribuciones. Los protagonistas conocían las preguntas que se les iban a formular y tenían la seguridad de que no se plantearían determinadas cuestiones por ninguna de las dos partes porque habían negociado qué temas les convenía abordar y cuáles preferían no comentar. Además del contenido, consideramos muy importante el contexto en el que se desarrollaron los encuentros entre Zapatero y Rajoy porque en España hay una falta de tradición de programas de estas características (el último fue en 1993 entre Felipe González y José María Aznar y se generaron muchas expectativas ante algo extraordinario. Por eso queremos comprobar si el debate estuvo a la altura de las circunstancias.Abstract: The Academy of Television was the allegedly neutral scenario for the organization of the debate between the PSOE and the PP of the Spanish general elections of March the 9th 2008, which were on air in February the 25th and March the 3rd. The analysis of both face to face between candidates José Luis Rodríguez Zapatero and Mariano Rajoy aims to know the circumstances

  15. Los físicos en la Facultad de Informática de Barcelona, 1976-1992

    OpenAIRE

    Fornés de Juan, Jordi

    2013-01-01

    En la España de la transición, la profesionalización de la informática y el nacimiento de los primeros estudios reglados universitarios en esta materia ofrecieron nuevas oportunidades a otras disciplinas científicas. Así, mientras los informáticos daban sus primeros pasos en las publicaciones científicas, otro colectivo, el de los físicos, se aproximó a la FIB en busca de técnicas y métodos de computación, de programación paralela, de potencia de cálculo y de puestos académicos. Una consecuen...

  16. La inmortalidad del alma: historia de un argumento político

    Directory of Open Access Journals (Sweden)

    Miguel Saralegui

    2014-01-01

    Full Text Available Se examina una cuestión fundamental y poco estudiada de la teología política: la relación entre la defensa de la inmortalidad del alma y el mantenimiento del orden público. Se realiza un recorrido histórico por autores como Pietro Pomponazzi y Tomás Moro, que aceptan motivos políticos para defenderla, y David Hume, quien considera que no existe ningún motivo político para mantener dicha relación. Por último, se analizan los argumentos esgrimidos para mostrar que su eficacia está condicionada por la situación histórica.

  17. THE 2014 ALMA LONG BASELINE CAMPAIGN: AN OVERVIEW

    Energy Technology Data Exchange (ETDEWEB)

    Partnership, ALMA [Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF (United Kingdom); Fomalont, E. B.; Vlahakis, C.; Corder, S.; Remijan, A.; Barkats, D.; Dent, W. R. F.; Phillips, N.; Cox, P.; Hales, A. S. [Joint ALMA Observatory, Alonso de Córdova 3107, Vitacura, Santiago (Chile); Lucas, R. [Institut de Planétologie et d’Astrophysique de Grenoble (UMR 5274), BP 53, F-38041 Grenoble Cedex 9 (France); Hunter, T. R.; Brogan, C. L.; Amestica, R.; Cotton, W. [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Asaki, Y. [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Matsushita, S. [Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 106, Taiwan (China); Hills, R. E. [Astrophysics Group, Cavendish Laboratory, JJ Thomson Avenue, Cambridge CB3 0HE (United Kingdom); Richards, A. M. S. [Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL (United Kingdom); Broguiere, D., E-mail: efomalon@nrao.edu [Institut de Radioastronomie Millime´trique (IRAM), 300 rue de la Piscine, Domaine Universitaire, F-38406 Saint Martin d’Hères (France); and others

    2015-07-20

    A major goal of the Atacama Large Millimeter/submillimeter Array (ALMA) is to make accurate images with resolutions of tens of milliarcseconds, which at submillimeter (submm) wavelengths requires baselines up to ∼15 km. To develop and test this capability, a Long Baseline Campaign (LBC) was carried out from 2014 September to late November, culminating in end-to-end observations, calibrations, and imaging of selected Science Verification (SV) targets. This paper presents an overview of the campaign and its main results, including an investigation of the short-term coherence properties and systematic phase errors over the long baselines at the ALMA site, a summary of the SV targets and observations, and recommendations for science observing strategies at long baselines. Deep ALMA images of the quasar 3C 138 at 97 and 241 GHz are also compared to VLA 43 GHz results, demonstrating an agreement at a level of a few percent. As a result of the extensive program of LBC testing, the highly successful SV imaging at long baselines achieved angular resolutions as fine as 19 mas at ∼350 GHz. Observing with ALMA on baselines of up to 15 km is now possible, and opens up new parameter space for submm astronomy.

  18. Revealing the dynamics of Class 0 protostellar discs with ALMA

    CERN Document Server

    Seifried, D; Walch, S; Banerjee, R

    2016-01-01

    We present synthetic ALMA observations of Keplerian, protostellar discs in the Class 0 stage studying the emission of molecular tracers like $^{13}$CO, C$^{18}$O, HCO$^+$, H$^{13}$CO$^+$, N$_2$H$^+$, and H$_2$CO. We model the emission of discs around low- and intermediate-mass protostars. We show that under optimal observing conditions ALMA is able to detect the discs already in the earliest stage of protostellar evolution, although the emission is often concentrated to the innermost 50 AU. Therefore, a resolution of a few 0.1" might be too low to detect Keplerian discs around Class 0 objects. We also demonstrate that under optimal conditions Keplerian rotation signatures are recognisable and protostellar masses can be determined with high fidelity for edge-on discs. Furthermore, we show that it is possible to reveal Keplerian rotation even for strongly inclined discs and that ALMA should be able to detect possible signs of fragmentation in face-on discs. In order to give some guidance for future ALMA observa...

  19. Alma Flor Ada and the Quest for Change

    Science.gov (United States)

    Manna, Anthony, L.; Hill, Janet; Kellogg, Kathy

    2004-01-01

    Alma Flor Ada, a folklorist, novelist, scholar, teacher, and children's book author has passionate dedication to education for social justice, equality, and peace. As a faculty member at the University of San Francisco, Ada has developed programs that help students and others transform their lives and has written several bilingual legends and…

  20. Circumnuclear molecular gas in M87 detected with ALMA

    Science.gov (United States)

    Vlahakis, Catherine E.

    2016-01-01

    We present the detection of circumnuclear molecular gas residing within 100 pc of the supermassive black hole (SMBH) in the galaxy M87 (3C 274), using the Atacama Large Millimeter/submillimeter Array (ALMA) to image the gas on spatial scales from 100 to 10 pc. The proximity of M87, the archetypical giant elliptical radio galaxy at the centre of the Virgo galaxy cluster, presents a unique opportunity to investigate in detail the circumnuclear molecular gas revealed first by single-dish observations and recently imaged for the first time with ALMA (Vlahakis et al., in prep). ALMA's unique long baseline capability now allows us to make the first detailed investigation of the properties of the interstellar medium around the galaxy's SMBH on scales down to 10 pc (0.1 arcsec). Here, we present results of ALMA Band 3 CO J=1-0 observations obtained at different angular resolutions. With this data we are able to trace the bulk of the molecular gas as well as the continuum emission, providing the deepest and highest spatial resolution images yet of the molecular gas content of this giant elliptical galaxy. The highest resolution data allow us to unambiguously resolve the molecular gas structures for the first time and investigate, in unprecedented detail, the nature and origin of molecular gas that resides within the sphere of influence of the SMBH.

  1. Alma-0: an imperative language that supports declarative programming

    NARCIS (Netherlands)

    Apt, K.R.; Brunekreef, J.; Partinton, V.; Schaerf, A.

    1997-01-01

    We describe here an implemented small programming language, called Alma, that augments the expressive power of imperative programming by a limited number of features inspired by the logic programming paradigm. These additions encourage declarative programming and make it a more attractive vehicle fo

  2. The High Redshift Universe Seen Through the Eyes of ALMA

    Science.gov (United States)

    Wiklind, Tommy

    2012-07-01

    The Atacama Large Millimeter/submm Array (ALMA) is an interferometric telescope currently under construction on the Chajnantor Plateau in northern Chile. It is situated at an altitude of 5000m, in one of the driest places in the world. The combination of the meteorological conditions, increased total collecting area and the use of state-of-the-art receivers means that the fully operational ALMA is a factor 10-1000 more sensitive than existing facilities, depending on the wavelength. When completed in 2013, ALMA will consists of 66 antennas, with maximum baselines of up to 15 km and it will be able to observe at wavelengths from 10 millimeter to ~350micron. ALMA will be able to provide an angular resolution of ~0.05 arcseconds. ALMA is still under construction, but has started producing science in an 'Early Science' phase. The goal with ALMA has from the beginning been to provide very high sensitivity as well as an angular resolution matching that of space based optical observatories such as the HST. One of three main drivers when designing ALMA has been the ability to study the high redshift universe. The main reason behind this is that almost half of the integrated background radiation comes from the far-infrared wavelength regime. This emission is interpreted as originating from dust re-radiated stellar emission in high redshift galaxies. Interstellar dust is almost invariably associated with molecular gas, that can be studied using molecular rotational transitions. The shape of the dust spectral energy distribution ensures that the observed flux at a fixed wavelength long-ward of the far-infrared peak (about 100micron) remains more or less constant over a redshift range z=1-10. This aspect makes dust continuum emission extraordinarily important for studying galaxies and Active Galactic Nuclei at high redshift. Through observations of line emission from molecular transitions it is possible to study the associated molecular gas distribution and its kinematics. The

  3. Informe Especial sobre el Manejo de los Residuos Sólidos en Panamá. Panamá,

    OpenAIRE

    2007-01-01

    La Defensoría del Pueblo, atenta al mandato consagrado en la Ley No. 7 de 5 de febrero de 1997, reformada por la Ley No. 41 de 1 de diciembre de 2005, ha elaborado este informe especial sobre la creciente problemática de los residuos sólidos en la República de Panamá y cuya finalidad es proporcionar elementos que faciliten la toma de decisiones gubernamentales relacionadas con su manejo. El inadecuado manejo y disposición final de los residuos sólidos, que en su mayoría son depositados dentro...

  4. Educando el alma psicológica

    Directory of Open Access Journals (Sweden)

    Matthew Curtis

    2007-01-01

    Full Text Available Este trabajo retoma aspectos de una exploración de los trabajos de cuatro importantes psicólogos educativos estadounidenses –Granville Stanley Hall, William James, John Dewey y Edward Thorndike– para concentrarse en los principios rectores del desarrollo de los niños. Los trabajos de estos autores están considerados como funciones que psicologizan al niño como un proceso de llegar a ser humano, que deba ser educado con fines éticos e inteligentes. Dos puntos de partida históricos se abordan en este artículo: (1 explorar la psicología como una formación de la moral del niño y (2 la clasificación y el orden del ser de forma razonada a partir de una psicología que abre el interior del niño a la supervisión y al calculo. Este enfoque explora la psicología educativa como una maquinaria de prácticas discusivas, intelectuales y materiales que invitan al estudiante a ver /ser visto y formar/ser formado de formas particulares. Educar al yo autónomo requería métodos modernos

  5. Atomic carbon as a tracer of molecular gas in high-redshift galaxies: perspectives for ALMA

    CERN Document Server

    Tomassetti, Matteo; Romano-Diaz, Emilio; Ludlow, Aaron D; Papadopoulos, Padelis P

    2014-01-01

    We use a high-resolution simulation that tracks the non-equilibrium abundance of molecular hydrogen, H2, within a massive high-redshift galaxy to produce mock ALMA maps of the fine-structure lines of atomic carbon CI 1-0 and CI 2-1. Inspired by recent observational and theoretical work, we assume that CI is thoroughly mixed in giant molecular clouds and demonstrate that its emission is an excellent proxy for H2. The entire H2 mass of a galaxy at redshift z<4 can be detected using a compact interferometric configuration with a large synthesized beam (that does not resolve the target galaxy) in less than 1 hour of integration time. Low-resolution imaging of the CI lines (in which the target galaxy is resolved into 3-4 beams) will detect nearly 50-60 per cent of the molecular hydrogen in less than 12 hours. In this case, the data cube also provides valuable information regarding the dynamical state of the galaxy. We conclude that ALMA observations of the CI 1-0 and 2-1 emission will widely extend the interval...

  6. Informe sobre los elementos prefabricados de yeso utilizados hoy día en Francia

    Directory of Open Access Journals (Sweden)

    Courivaud, I.

    1965-03-01

    Full Text Available Not availableAunque la fabricación de losetas o placas de yeso no es una industria nueva en Francia, aproximadamente en el año 1920 cuando empiezan a aparecer en el mercado francés los primeros elementos prefabricados de yeso. Por primera vez estos elementos fabricados industrialmente tenían sus dimensiones perfectamente "calibradas y presentaban sus paramentos perfectamente lisos; no requiriendo una vez montados los tradicionales enlucidos para su acabado.

  7. Informações dos adolescentes sobre métodos anticoncepcionais Informaciones los adolescentes sobre los métodos anticonceptivos Teenagers' information about anticonceptive methods

    Directory of Open Access Journals (Sweden)

    Alzira Maria d'Ávila Nery Guimarães

    2003-06-01

    Full Text Available Realizou-se estudo de corte transversal, com o objetivo de identificar, em escolares do ensino médio, informações relativas aos métodos anticoncepcionais. A amostra compreendeu 816 adolescentes de ambos os sexos de escolas públicas de Aracaju, Sergipe. Em relação a essas informações, foram investigados também aspectos demográficos, pedagógicos, comportamentais e reprodutivos. Verificou-se que 59% dos adolescentes possuíam vida sexual ativa e 57,7% afirmaram não receber informações sobre métodos anticoncepcionais nas escolas. As fontes de informações, revistas, livros e jornais, alcançaram o percentual de 28% e o condon masculino (84,5% foi o método mais conhecido. A análise possibilitou identificar a necessidade de maior discussão na escola e a inserção dos pais nesse processo.Se realizó un estudio de corte transversal, con el objetivo de identificar en estudiantes de enseñanza media, informaciones relacionadas con los métodos anticonceptivos. La muestra comprendió 816 adolescentes de ambos sexos de escuelas públicas de Aracaju Estado de Sergipe. Se averiguaron aspectos demográficos, pedagógicos, comportamentales y reproductivos. Se encontró que 59% de los adolescentes tienen vida sexual activa y 57,7% afirmaron no haber recibido informaciones sobre los métodos anticonceptivos en las escuelas. Las fuentes de información, revistas, libros y periódicos alcanzaron un porcentaje de 28% y el condón masculino 84,5%, fue el método más conocido. El análisis hizo posible identificar la necesidad de mayor discusión en la escuela y la inclusión de los padres en este proceso.A transversal study was realized in order to identify information about anticonceptive methods in high school students. The sample included 816 adolescents of both genders from public schools in Aracaju, Sergipe. With respect to this information, demographic, pedagogical, behavioral and reproductive aspects were also analyzed. It was verified

  8. Integración de los campos del saber Informático y Humanístico : Proyecto: “Comunidad de lectores de los profesorados de la Facultad de Humanidades y Cs. Sociales de la UNPSJB”

    OpenAIRE

    Gómez, Susana; Uviña, Patricia Ruth; Uviña, Paulina Carmen; Gutiérrez, José María; Lorenzo, Alicia Noemí; Diez, Marina Soledad; Belcastro, Ángela; Blengino, Sonia; Solsona, Lucila Elisa

    2005-01-01

    “Comunidad de lectores de los profesorados de la Fac. de Humanidades y Cs. Sociales. Un enfoque sociosemiótico”, es un proyecto de investigación interdisciplinario, integra los campos del saber informático y humanístico. Desde el campo Informático se aportan sistemas de software aplicados a la educación, creando productos de apoyo para la descripción, análisis e intervención en los procesos de lectura de estudiantes de carreras específicas de Humanidades. Algunos productos son muy simples y a...

  9. Construcción temática y marcas enunciativas en los informes de estudiantes universitarios

    Directory of Open Access Journals (Sweden)

    Marcela Oyanedel

    2006-06-01

    Full Text Available Este artículo aborda la construcción discursiva de las figuras de productor y receptor en los informes escritos de estudiantes universitarios de segundo año. Los textos estudiados revelan la representación de un saber complejo, que incluye mecanismos discursivos para la construcción del enunciador –el estudiante– y delreceptor: el profesor que evalúa. A lo largo del artículo se ilustra con ejemplos tomados de informes de Ciencias Biológicas y de Ciencias Humanas y Sociales. Se destaca el empleo de marcas de didacticidad para orientar al receptor como mecanismo específico de estos últimos informes. Se concluye que la variedad e inestabilidad en las estrategias para construir a los actores involucrados en este intercambio académico responden, por una parte, a las diferencias que son propias del campo disciplinar y de la clase de informe y, por otra, al nivel de alfabetización en el que se encuentran los productores. (This paper addresses the discoursive construction of producer and recipient in written research reports made by second-year university students. Texts analysed reveal the representation of a complex kind of knowledge, including discoursive mechanisms for the construction of the writer –the student– and the reader – the evaluating professor. Throughout the article this is illustrated by examples taken from Biological, Human and Social Sciences reports. Didactic resources used to guide the reader are highlighted as a mechanism specific to reports in Social Sciences. The paper concludes that the variety and instability shown by strategies for the construction of actors involved in this academic exchange reflect differences proper to the discipline and report classes, as well to text producers’ literacy level.

  10. Phase Correction for ALMA with 183 GHz Water Vapour Radiometers

    CERN Document Server

    Nikolic, Bojan; Graves, Sarah F; Hills, Richard E; Richer, John S

    2013-01-01

    Fluctuating properties of the atmosphere, and in particular its water vapour content, give rise to phase fluctuations of astronomical signals which, if uncorrected, lead to rapid deterioration of performance of (sub)-mm interferometers on long baselines. The Atacama Large Millimetre/submillimeter Array (ALMA) uses a 183 GHz Water Vapour Radiometer (WVR) system to help correct these fluctuations and provide much improved performance on long baselines and at high frequencies. Here we describe the design of the overall ALMA WVR system, the choice of design parameters and the data processing strategy. We also present results of initial tests that demonstrate both the large improvement in phase stability that can be achieved and the very low contribution to phase noise from the WVRs. Finally, we describe briefly the main limiting factors to the accuracy of phase correction seen in these initial tests; namely, the degrading influence of cloud and the residual phase fluctuations that are most likely to be due to var...

  11. Star and Stellar Cluster Formation: ALMA-SKA Synergies

    CERN Document Server

    Fuller, G A; Rathborne, J M; Longmore, S; Molinari, S

    2015-01-01

    Over the next decade, observations conducted with ALMA and the SKA will reveal the process of mass assembly and accretion onto young stars and will be revolutionary for studies of star formation. Here we summarise the capabilities of ALMA and discuss recent results from its early science observations. We then review infrared and radio variability observations of both young low-mass and high-mass stars. A time domain SKA radio continuum survey of star forming regions is then outlined. This survey will produce radio light-curves for hundreds of young sources, providing for the first time a systematic survey of radio variability across the full range of stellar masses. These light-curves will probe the magnetospheric interactions of young binary systems, the origins of outflows, trace episodic accretion on the central sources and potentially constrain the rotation rates of embedded sources.

  12. Sistema informático para análisis y procesamiento de datos de los computadores de a bordo de la serie AGM-200X

    OpenAIRE

    Javier Lorenzo; Roberto Sepúlveda Lima; Alejandro Rosete Suárez; Juan Carlos Sepúlveda Peña; Carlos Lago González

    2011-01-01

    Con el auge de las Tecnologías de la Información y las Comunicaciones  y el abaratamiento del uso de los sistemas de navegación asistidos por satélites, cada día son más comunes los sistemas de control de flota y los computadores de a bordo, con el objetivo de elevar la eficiencia en el uso de los recursos técnicos y humanos. Tanto los sistemas de control de flota como los computadores de a bordo precisan de un autómata y un sistema informático que procese los datos registrados por el autómat...

  13. The 1976 Illini: Sweet Memories of Alma Mater

    OpenAIRE

    Diya Dutt

    1996-01-01

    The purpose of this article is to explore the attitudes of graduates of the class of 1976 from the University of Illinois toward their alma mater over a period of fifteen years. The central question addressed in this article is: How do former students feel about their educational institution as time passes? Early research suggests that students' attachment to their educational institution becomes weaker with the passage of time. This panel data on alumni attitudes towards the academic environ...

  14. The ALMA assembly, integration, and verification project: a retrospective analysis

    Science.gov (United States)

    Lopez, B.; Knee, L. B. G.; Jager, H.; Whyborn, N.; McMullin, J.; Murowinski, R.; Peck, A.; Corder, S.

    2014-08-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) is a joint project between astronomical organizations in Europe, North America, and East Asia, in collaboration with the Republic of Chile. ALMA consists of 54 twelve-meter antennas and 12 seven-meter antennas operating as an aperture synthesis array in the (sub)millimeter wavelength range. Assembly, Integration, and Verification (AIV) of the antennas was completed at the end of the year 2013, while the final optimization and complete expansion to validate all planned observing modes will continue. This paper compares the actually obtained results of the period 2008-2013 with the baselines that had been laid out in the early project-planning phase (2005-2007). First plans made for ALMA AIV had already established a two-phased project life-cycle: phase 1 for setting up necessary infrastructure and common facilities, and taking the first three antennas to the start of commissioning; and phase 2 focused on the steady state processing of the remaining units. Throughout the execution of the project this lifecycle was refined and two additional phases were added, namely a transition phase between phases 1 and 2, and a closing phase to address the project ramp-down. A sub-project called Accelerated Commissioning and Science Verification (ACSV) was carried out during the year 2009 in order to provide focus to the whole ALMA organization, and to accomplish the start-of-commissioning milestone. Early phases of CSV focused on validating the basic performance and calibration. Over time additional observing modes have been validated as capabilities expanded both in hardware and software. This retrospective analysis describes the originally presented project staffing plans and schedules, the underlying assumptions, identified risks and operational models, among others. For comparison actual data on staffing levels, the resultant schedule, additional risks identified and those that actually materialized, are presented. The

  15. Solar ALMA Observations - A new view of our host star

    CERN Document Server

    Wedemeyer, Sven; Brajsa, Roman; Barta, Miroslav; Shimojo, Masumi; Hales, Antonio; Yagoubov, Pavel; Hudson, Hugh

    2015-01-01

    ALMA provides the necessary spatial, temporal and spectral resolution to explore central questions in contemporary solar physics with potentially far-reaching implications for stellar atmospheres and plasma physics. It can uniquely constraint the thermal and magnetic field structure in the solar chromosphere with measurements that are highly complementary to simultaneous observations with other ground-based and space-borne instruments. Here, we highlight selected science cases.

  16. A deep ALMA image of the Hubble Ultra Deep Field

    CERN Document Server

    Dunlop, J S; Biggs, A D; Geach, J E; Michalowski, M J; Ivison, R J; Rujopakarn, W; van Kampen, E; Kirkpatrick, A; Pope, A; Scott, D; Swinbank, A M; Targett, T A; Aretxaga, I; Austermann, J E; Best, P N; Bruce, V A; Chapin, E L; Charlot, S; Cirasuolo, M; Coppin, K E K; Ellis, R S; Finkelstein, S L; Hayward, C C; Hughes, D H; Ibar, E; Khochfar, S; Koprowski, M P; Narayanan, D; Papovich, C; Peacock, J A; Robertson, B; Vernstrom, T; van der Werf, P P; Wilson, G W; Yun, M

    2016-01-01

    We present the results of the first, deep ALMA imaging covering the full 4.5 sq arcmin of the Hubble Ultra Deep Field (HUDF) as previously imaged with WFC3/IR on HST. Using a mosaic of 45 pointings, we have obtained a homogeneous 1.3mm image of the HUDF, achieving an rms sensitivity of 35 microJy, at a resolution of 0.7 arcsec. From an initial list of ~50 >3.5sigma peaks, a rigorous analysis confirms 16 sources with flux densities S(1.3) > 120 microJy. All of these have secure galaxy counterparts with robust redshifts ( = 2.15), and 12 are also detected at 6GHz in new deep JVLA imaging. Due to the wealth of supporting data in this unique field, the physical properties of the ALMA sources are well constrained, including their stellar masses (M*) and UV+FIR star-formation rates (SFR). Our results show that stellar mass is the best predictor of SFR in the high-z Universe; indeed at z > 2 our ALMA sample contains 7 of the 9 galaxies in the HUDF with M* > 2 x 10^10 Msun and we detect only one galaxy at z > 3.5, re...

  17. Final tests and performances verification of the European ALMA antennas

    Science.gov (United States)

    Marchiori, Gianpietro; Rampini, Francesco

    2012-09-01

    The Atacama Large Millimeter Array (ALMA) is under erection in Northern Chile. The array consists of a large number (up to 64) of 12 m diameter antennas and a number of smaller antennas, to be operated on the Chajnantor plateau at 5000 m altitude. The antennas will operate up to 950 GHz so that their mechanical performances, in terms of surface accuracy, pointing precision and dimensional stability, are very tight. The AEM consortium constituted by Thales Alenia Space France, Thales Alenia Space Italy, European Industrial Engineering (EIE GROUP), and MT Mechatronics is assembling and testing the 25 antennas. As of today, the first set of antennas have been delivered to ALMA for science. During the test phase with ESO and ALMA, the European antennas have shown excellent performances ensuring the specification requirements widely. The purpose of this paper is to present the different results obtained during the test campaign: surface accuracy, pointing error, fast motion capability and residual delay. Very important was also the test phases that led to the validation of the FE model showing that the antenna is working with a good margin than predicted at design level thanks also to the assembly and integration techniques.

  18. Future mmVLBI Research with ALMA: A European vision

    CERN Document Server

    Tilanus, R P J; Zensus, J A; Baudry, A; Bremer, M; Falcke, H; Giovannini, G; Laing, R; van Langevelde, H J; Vlemmings, W; Abraham, Z; Afonso, J; Agudo, I; Alberdi, A; Alcolea, J; Altamirano, D; Asadi, S; Assaf, K; Augusto, P; Baczko, A-K; Boeck, M; Boller, T; Bondi, M; Boone, F; Bourda, G; Brajsa, R; Brand, J; Britzen, S; Bujarrabal, V; Cales, S; Casadio, C; Casasola, V; Castangia, P; Cernicharo, J; Charlot, P; Chemin, L; Clenet, Y; Colomer, F; Combes, F; Cordes, J; Coriat, M; Cross, N; D'Ammando, F; Dallacasa, D; Desmurs, J-F; Eatough, R; Eckart, A; Eisenacher, D; Etoka, S; Felix, M; Fender, R; Ferreira, M; Freeland, E; Frey, S; Fromm, C; Fuhrmann, L; Gabanyi, K; Galvan-Madrid, R; Giroletti, M; Goddi, C; Gomez, J; Gourgoulhon, E; Gray, M; di Gregorio, I; Greimel, R; Grosso, N; Guirado, J; Hada, K; Hanslmeier, A; Henkel, C; Herpin, F; Hess, P; Hodgson, J; Horns, D; Humphreys, E; Kramer, B Hutawarakorn; Ilyushin, V; Impellizzeri, V; Ivanov, V; Julião, M; Kadler, M; Kerins, E; Klaassen, P; Klooster, K van 't; Kording, E; Kozlov, M; Kramer, M; Kreikenbohm, A; Kurtanidze, O; Lazio, J; Leite, A; Leitzinger, M; Lepine, J; Levshakov, S; Lico, R; Lindqvist, M; Liuzzo, E; Lobanov, A; Lucas, P; Mannheim, K; Marcaide, J; Markoff, S; Martí-Vidal, I; Martins, C; Masetti, N; Massardi, M; Menten, K; Messias, H; Migliari, S; Mignano, A; Miller-Jones, J; Minniti, D; Molaro, P; Molina, S; Monteiro, A; Moscadelli, L; Mueller, C; Müller, A; Muller, S; Niederhofer, F; Odert, P; Olofsson, H; Orienti, M; Paladino, R; Panessa, F; Paragi, Z; Paumard, T; Pedrosa, P; Pérez-Torres, M; Perrin, G; Perucho, M; Porquet, D; Prandoni, I; Ransom, S; Reimers, D; Rejkuba, M; Rezzolla, L; Richards, A; Ros, E; Roy, A; Rushton, A; Savolainen, T; Schulz, R; Silva, M; Sivakoff, G; Soria-Ruiz, R; Soria, R; Spaans, M; Spencer, R; Stappers, B; Surcis, G; Tarchi, A; Temmer, M; Thompson, M; Torrelles, J; Truestedt, J; Tudose, V; Venturi, T; Verbiest, J; Vieira, J; Vielzeuf, P; Vincent, F; Wex, N; Wiik, K; Wiklind, T; Wilms, J; Zackrisson, E; Zechlin, H

    2014-01-01

    Very long baseline interferometry at millimetre/submillimetre wavelengths (mmVLBI) offers the highest achievable spatial resolution at any wavelength in astronomy. The anticipated inclusion of ALMA as a phased array into a global VLBI network will bring unprecedented sensitivity and a transformational leap in capabilities for mmVLBI. Building on years of pioneering efforts in the US and Europe the ongoing ALMA Phasing Project (APP), a US-led international collaboration with MPIfR-led European contributions, is expected to deliver a beamformer and VLBI capability to ALMA by the end of 2014 (APP: Fish et al. 2013, arXiv:1309.3519). This report focuses on the future use of mmVLBI by the international users community from a European viewpoint. Firstly, it highlights the intense science interest in Europe in future mmVLBI observations as compiled from the responses to a general call to the European community for future research projects. A wide range of research is presented that includes, amongst others: - Imagin...

  19. ALMA Binary Data Transport Mechanism using VOTable Headers

    Science.gov (United States)

    Wicenec, A.; Meuss, H.; Pisano, J.

    2006-07-01

    ALMA will produce very large data rates and volumes. In full operation the correlator will generate up to 60 MB/s of visibility data. These data have to be transported from the correlator on the high site (5000 m) to the ALMA archive, the telescope calibration and the quick-look subsystems, which are all located at the low site (2500 m) some 40 km away. A dedicated fiber connection between the sites is under construction and the interfaces between the subsystems are under development. The actual transport format produced by the correlator has been defined and implemented and is described in this paper in more detail. The format is derived from the SOAP with attachments [1], but instead of the SOAP XML envelope it is using a slightly modified VOTable [2] to keep the description of the binary data. The VOTable uses content ID pointers (CID, RFC2111 [3]) to refer to the binary parts contained in the same Multipart/Related (RFC2387 [4]) container. Such Multipart/Related containers are constructed for each ALMA integration and sent through a multimedia streaming connection implemented in CORBA (TAO[5, 6]).

  20. An Overview of the 2014 ALMA Long Baseline Campaign

    CERN Document Server

    Partnership, ALMA; Vlahakis, C; Corder, S; Remijan, A; Barkats, D; Lucas, R; Hunter, T R; Brogan, C L; Asaki, Y; Matsushita, S; Dent, W R F; Hills, R E; Phillips, N; Richards, A M S; Cox, P; Amestica, R; Broguiere, D; Cotton, W; Hales, A S; Hiriart, R; Hirota, A; Hodge, J A; Impellizzeri, C M V; Kern, J; Kneissl, R; Liuzzo, E; Marcelino, N; Marson, R; Mignano, A; Nakanishi, K; Nikolic, B; Perez, J E; Pérez, L M; Toledo, I; Aladro, R; Butler, B; Cortes, J; Cortes, P; Dhawan, V; Di Francesco, J; Espada, D; Galarza, F; Garcia-Appadoo, D; Guzman-Ramirez, L; Humphreys, E M; Jung, T; Kameno, S; Laing, R A; Leon, S; Mangum, J; Marconi, G; Nagai, H; Nyman, L -A; Perley, R; Radiszcz, M; Rodón, J A; Sawada, T; Takahashi, S; Tilanus, R P J; van Kempen, T; Vilaro, B Vila; Watson, L C; Wiklind, T; Gueth, F; Tatematsu, K; Wootten, A; Castro-Carrizo, A; Chapillon, E; Dumas, G; de Gregorio-Monsalvo, I; Francke, H; Gallardo, J; Garcia, J; Gonzalez, S; Hibbard, J E; Hill, T; Kaminski, T; Karim, A; Krips, M; Kurono, Y; Lopez, C; Martin, S; Maud, L; Morales, F; Pietu, V; Plarre, K; Schieven, G; Testi, L; Videla, L; Villard, E; Whyborn, N; Zwaan, M A; Alves, F; Andreani, P; Avison, A; Barta, M; Bedosti, F; Bendo, G J; Bertoldi, F; Bethermin, M; Biggs, A; Boissier, J; Brand, J; Burkutean, S; Casasola, V; Conway, J; Cortese, L; Dabrowski, B; Davis, T A; Trigo, M Diaz; Fontani, F; Franco-Hernandez, R; Fuller, G; Madrid, R Galvan; Giannetti, A; Ginsburg, A; Graves, S F; Hatziminaoglou, E; Hogerheijde, M; Jachym, P; Serra, I Jimenez; Karlicky, M; Klaasen, P; Kraus, M; Kunneriath, D; Lagos, C; Longmore, S; Leurini, S; Maercker, M; Magnelli, B; Vidal, I Marti; Massardi, M; Maury, A; Muehle, S; Muller, S; Muxlow, T; O'Gorman, E; Paladino, R; Petry, D; Pineda, J; Randall, S; Richer, J S; Rossetti, A; Rushton, A; Rygl, K; Monge, A Sanchez; Schaaf, R; Schilke, P; Stanke, T; Schmalzl, M; Stoehr, F; Urban, S; van Kampen, E; Vlemmings, W; Wang, K; Wild, W; Yang, Y; Iguchi, S; Hasegawa, T; Saito, M; Inatani, J; Mizuno, N; Asayama, S; Kosugi, G; Morita, K -I; Chiba, K; Kawashima, S; Okumura, S K; Ohashi, N; Ogasawara, R; Sakamoto, S; Noguchi, T; Huang, Y -D; Liu, S -Y; Kemper, F; Koch, P M; Chen, M -T; Chikada, Y; Hiramatsu, M; Iono, D; Shimojo, M; Komugi, S; Kim, J; Lyo, A -R; Muller, E; Herrera, C; Miura, R E; Ueda, J; Chibueze, J; Su, Y -N; Trejo-Cruz, A; Wang, K -S; Kiuchi, H; Ukita, N; Sugimoto, M; Kawabe, R; Hayashi, M; Miyama, S; Ho, P T P; Kaifu, N; Ishiguro, M; Beasley, A J; Bhatnagar, S; Braatz, J A; Brisbin, D G; Brunetti, N; Carilli, C; Crossley, J H; D'Addario, L; Meyer, J L Donovan; Emerson, D T; Evans, A S; Fisher, P; Golap, K; Griffith, D M; Hale, A E; Halstead, D; Hardy, E J; Hatz, M C; Holdaway, M; Indebetouw, R; Jewell, P R; Kepley, A A; Kim, D -C; Lacy, M D; Leroy, A K; Liszt, H S; Lonsdale, C J; Matthews, B; McKinnon, M; Mason, B S; Moellenbrock, G; Moullet, A; Myers, S T; Ott, J; Peck, A B; Pisano, J; Radford, S J E; Randolph, W T; Venkata, U Rao; Rawlings, M; Rosen, R; Schnee, S L; Scott, K S; Sharp, N K; Sheth, K J; Simon, R S; Tsutsumi, T; Wood, S J

    2015-01-01

    A major goal of the Atacama Large Millimeter/submillimeter Array (ALMA) is to make accurate images with resolutions of tens of milliarcseconds, which at submillimeter (submm) wavelengths requires baselines up to ~15 km. To develop and test this capability, a Long Baseline Campaign (LBC) was carried out from September to late November 2014, culminating in end-to-end observations, calibrations, and imaging of selected Science Verification (SV) targets. This paper presents an overview of the campaign and its main results, including an investigation of the short-term coherence properties and systematic phase errors over the long baselines at the ALMA site, a summary of the SV targets and observations, and recommendations for science observing strategies at long baselines. Deep ALMA images of the quasar 3C138 at 97 and 241 GHz are also compared to VLA 43 GHz results, demonstrating an agreement at a level of a few percent. As a result of the extensive program of LBC testing, the highly successful SV imaging at long...

  1. Los informes del desarrollo humano y el plan milenio de la ONU: una evaluación para México

    OpenAIRE

    Asael Mercado Maldonado; Luis Jesús Luna Cano

    2006-01-01

    Este artículo documenta los informes de la ONU sobre desarrollo humano de 1990 a 2005, así como la aparición del Proyecto del Milenio —un intento mundial para que la humanidad supere los enormes problemas que la globalización ha acentuado, como desigualdad, pobreza y deterioro de la ecología—, que propone ocho objetivos fundamentales para disminuir las desigualdades entre los seres humanos

  2. Los tratos con el cuerpo

    OpenAIRE

    Musachi, Graciela

    2012-01-01

    Sigmund Freud bien podría haber usufructuado de una figura clásica como la del filósofo acostado. Sócrates, Descartes, Diderot, Tolstoi, Proust, Becket consideraron que, en la postura de abandono, es posible acoger una revelación sobre el “interior” de nuestro cuerpo. Pero, a partir de Descartes se pierde la connaturalidad de esa percepción ya que hay las percepciones que atribuimos a los objetos fuera del cuerpo, aquellas que atribuimos a nuestro cuerpo y las que atribuimos al alma. La se...

  3. Síntomas en la menopausia y el cuidado de los nietos. Informe preliminar

    Directory of Open Access Journals (Sweden)

    Rosalinda García Campos

    2008-01-01

    Full Text Available Introducción. La menopausia es un proceso restringido al ser humano. La mujer tiene una etapa post-reproductiva prolongada en la que aparecen síntomas que deterioran su calidad de vida. El valor adaptativo de la menopausia se ha atribuido al papel de las abuelas en la crianza de los nietos. También se ha planteado como explicación la teoría del conflicto reproductivo entre generaciones. Es importante definir la posible relación entre los síntomas en la menopausia y su papel en el cuidado de los nietos. Método. Efectuamos un estudio epidemiológico en sección transversal en 386 mujeres post-menopáusicas, con edad de 55 a 75 años. Se colectaron los datos antropométricos,antecedentes gineco-obstétricos, nivel socioeconómico, relaciones con hijos y nietos, y los síntomas: bochornos, sequedad vaginal, pérdida del interés sexual, depresión, ansiedad, síntomas no específicos de depresión y el síndrome del nido vacío. Se midieron glucosa, colesterol, estradiol y FSH en una muestra de sangre en ayuno. Resultados. Las voluntarias tuvieron edad media de 63 años, menopausia a los 47.7 años, 5.6 hijos y 13.1 nietos. Se encontró mayor pérdida del interés sexual en las mujeres que veían con frecuencia a sus hijos y en quienes cuidaban a sus nietos. Las calificaciones más bajas del síndrome del nido vacío, se encontraron en el grupo sin hijos o nietos. El grupo sin nietos tenía además calificaciones más bajas de síntomas no específicos de depresión. En cuanto a los factores asociados con los síntomas, la edad se asoció inversamente a bochornos y ansiedad; la escolaridad tuvo relación inversa con bochornos, depresión, ansiedad y síndrome del nido vacío. El índice de masa corporal se asoció negativamente con sequedad vaginal, pérdida del interés sexual y síntomas no específicos de depresión. FSH se asoció negativamente con la pérdida del interés sexual. Los bochornos se asociaron con el ejercicio. El n

  4. Los informes contables externos y la legitimidad organizacional con el entorno: estudio de un caso en Colombia

    Directory of Open Access Journals (Sweden)

    Mauricio Gómez Villegas

    2009-08-01

    Full Text Available Este documento es una aproximación académica a la contabilidad y a los informes contables externos. Su preocupación es la caracterización y comprensión del papel de la contabilidad en las organizaciones y en la sociedad. Por ello sintetiza la visión económica dominante y algunas de las perspectivas sociales e institucionales sobre el rol de la contabilidad y la información contable financiera. Parte de la pregunta: ¿Aporta la contabilidad al propósito de legitimidad organizacional con el entorno? Así, el objetivo del trabajo es realizar una síntesis de las visiones que explican el papel de los informes contables externos, los estados financieros particularmente, desde la visión dominante y desde una perspectiva neoinstitucional en contabilidad. Para ello el documento recoge un primer estudio de caso, que pretende aportar a la necesaria contrastación empírica para la comprensión del rol de la contabilidad en Colombia. Adoptamos la visión según la cual, ante todo, la información contable desempeña un rol institucional, como mecanismo de legitimación de la organización con su entorno

  5. Informe a la nación indica que los índices de muertes por cáncer siguen bajando

    Science.gov (United States)

    Los índices de mortalidad por todos los cánceres combinados para hombres, mujeres y niños siguieron bajando en Estados Unidos entre 2004 y 2008, según el Informe Anual a la Nación sobre el Estado del Cáncer de 1975 a 2008. El índice general de diagnóstico

  6. Una aproximación a la situación de la mujer en los estudios universitarios de informática

    Directory of Open Access Journals (Sweden)

    Maritxalar, Montse

    2008-10-01

    Full Text Available En los últimos años, la baja participación de la mujer y la tendencia al descenso de los porcentajes de alumnas matriculadas en los estudios universitarios de informática ha sido objeto de estudio para investigadoras/es en Estados Unidos, Europa y otros países. Habiendo constatado también en la Facultad de Informática de San Sebastián (FISS de la Universidad del País Vasco (UPV/EHU dicho descenso, nuestro objetivo ha sido recopilar información estadística para determinar si esta tendencia se ha producido también en otras universidades del Estado español. El estudio incluye, en primer lugar, porcentajes de mujeres inscritas en Ingeniería Informática comparados con los porcentajes en el área técnica en su conjunto. Por otra parte, recoge datos del tercer ciclo y porcentajes de profesoras de los departamentos que imparten docencia en la FISS, comparados con los porcentajes en los mismos departamentos en el conjunto del Estado. Por último, se presentan datos de inserción en el mundo laboral para las promociones 1998-2002 de egresadas/os en la UPV/EHU. Los datos revelan los bajos porcentajes de mujeres que se han matriculado en Ingeniería Informática los últimos años y la tendencia al descenso, las diferencias entre distintas universidades, y que apenas hay sesgo de género en los datos de inserción en el mundo laboral.En los últimos años, la baja participación de la mujer y la tendencia al descenso de los porcentajes de alumnas matriculadas en los estudios universitarios de informática ha sido objeto de estudio para investigadoras/es en Estados Unidos, Europa y otros países. Habiendo constatado también en la Facultad de Informática de San Sebastián (FISS de la Universidad del País Vasco (UPV/EHU dicho descenso, nuestro objetivo ha sido recopilar información estadística para determinar si esta tendencia se ha producido también en otras universidades del Estado español. El estudio incluye, en primer lugar

  7. El futuro de los recursos humanos en informática. Un estudio empírico con estudiantes secundarios argentinos

    Directory of Open Access Journals (Sweden)

    Mariano Zukerfeld

    2015-12-01

    Full Text Available El sector de software y servicios informáticos ha tenido un crecimiento notable en la Argentina de la última década, sin embargo los recursos humanos son vistos por los actores del sector como el principal limitante para el desarrollo futuro de este. La pregunta general que fundamenta la investigación es: ¿en qué medida los adolescentes presentan potencialidades para desempeñarse en el futuro cercano, en procesos productivos de software? se preven algunas respuestas a través de tres ejes: tecnológico (cantidad y calidad del uso de tecnologías digitales e internet, subjetivo (la compatibilidad entre los gustos y habilidades de los jóvenes y los que son útiles en los procesos productivos de software e intersubjetivo (representaciones sobre los programadores, el mercado de trabajo y las carreras profesionales. Asimismo, se consideran las divergencias de género y las potencialidades de los jóvenes para, más allá de la producción de software, participar del trabajo informacional. Metodológicamente, su desarrollo se basa en información primaria surgida de una encuesta realizada a 627 estudiantes secundarios. Las conclusiones muestran que las actividades informáticas, en las tres dimensiones, las mujeres presentan una lejanía mayor que los varones. Asimismo, pese a que encontramos algunas habilidades subjetivas promisorias, en la dimensión intersubjetiva emergen fuertes limitaciones para identificarse con un horizonte laboral en informática. Finalmente, se considera que quiénes manifiestan deseos de avanzar en una educación universitaria en informática, no son los alumnos que declaran tener prácticas actuales en esa actividad. Se sugieren algunas líneas de acción respaldadas por políticas públicas.

  8. El trabajo informal de los vagoneros en el Metro de la Ciudad de México

    Directory of Open Access Journals (Sweden)

    Eloísa Ramírez Cárdenas

    2016-01-01

    Full Text Available Resumen El objetivo principal de este artículo es presentar un estudio exploratorio a partir de un caso que explica de qué forma las condiciones laborales propias del sector informal pudieran determinar la decisión de los vendedores ambulantes de permane- cer en este en su modalidad de comercio ambulante, específicamente en la venta de artículos apócrifos. La manera en que se operacionalizaron las proposiciones planteadas en la presente investigación fue a través del uso de la observación participante en calidad de compradores y de la aplicación de ocho entrevistas a los vendedores ambulantes mayores de 25 años que se dedi- can a la venta de discos compactos (CD’s piratas dentro de los vagones del Sistema de Transporte Colectivo (STC Metro de la Línea 8 de la Ciudad de México. Los resultados arrojan que el ingreso, las remuneraciones, la jornada de trabajo y la satisfacción que da el trabajar en el sector informal hace que los sujetos de estudio decidan trabajar en el marco de la informalidad. Palabras clave: Comercio ambulante, Sector informal, Precariedad laboral, Vagoneros. Abstract This paper focuses on analysis of the decisions made by peddlers to continue working on the streets, specifically selling apocryphal items. Those decisions are based on the working conditions in the informal sector. To collect data, the participant observation was used, as buyers; 8 interviews with vendors, aged over 25, were conducted. These sellers are engaged in the sale of pirate compact discs (CDs inside the wagons of the Sistema de Transporte Colectivo (STC Metro Line 8 in Mexico City. The results show that economic income, financial compensation, the working day and the satisfaction of working in the informal sector makes those people keep on working within the framework of informality. Key words: Street vendors, Informal sector, Job insecurity, Wagon drivers. Resumo O principal objetivo deste artigo é apresentar um estudo

  9. Los nuevos derechos humanos: gobierno electrónico e informática comunitaria

    Directory of Open Access Journals (Sweden)

    Javier Bustamante Donas

    2007-05-01

    Full Text Available Este artículo analiza la relación entre derechos humanos, tecnología y democracia. En particular, la relaciónentre el uso de Internet, las políticas de inclusión digital y el desarrollo del gobierno electrónico, con referencias alos casos de Brasil y España. Se identifican factores que suponen un cambio real en la definición de los límites de lademocracia y en el concepto de ciudadanía. El movimiento Linux, las comunidades virtuales y la ética de hackersson manifestaciones de una primera generación de usos alternativos de profundo poder transformador. Los conceptosde ciudadanía y de derechos humanos se redefinen en este nuevo entorno a partir de un nuevo conjunto devalores y metáforas, de un nuevo paradigma ético.

  10. La computación en la nube, como solución a los problemas de disponibilidad y continuidad en los servicios informáticos de la aeronáutica civil

    OpenAIRE

    Páez Murcia, Omar Iván

    2012-01-01

    Tener acceso a la información desde cualquier sitio, utilizando dispositivos móviles, ha permitido a los miembros de las organizaciones agilizar sus relaciones comerciales y realizar sus actividades laborales, sin la necesidad de estar presentes en las oficinas de la compañía. Esto se ha logrado gracias a modelos tecnológicos como la computación en la nube, en el cual los servicios informáticos se procesan fuera de los centros de datos propiedad de las empresas y se acceden desde intern...

  11. Informe final. Manejo y monitoreo de las mareas rojas en las regiones de los Lagos, Aysén y Magallanes IV etapa, 2010.

    OpenAIRE

    Guzmán Méndez, F. L.; Vidal Santana, G.; Pizarro Nova, G.; Vivanco Tapia, X.; Iriarte Bustamante, L.; Alarcón Zapata, C.; Arenas Sepúlveda, V.; Mercado Leal, S.; Pacheco Valles, H.; Mejías Wagner, P.; Salgado Garrido, P.; Palma Alarcón, M.; Espinoza Alvarado, C.; Fernández-Niño Azócar, E.; Monsalve Montecinos, J.

    2011-01-01

    En el presente informe se muestran los resultados de la cuarta etapa de un estudio diseñado para monitorear las variaciones espacio temporales del veneno paralizante de los mariscos (VPM), el veneno diarreíco de los mariscos (VDM), el veneno amnésico de los mariscos (VAM) en especies transvectoras centinelas, y de especies de microalgas nocivas o potencialmente nocivas, además de variables ambientales de tipo hidrográficas y meteorólogicas, además, de fitoplancton cualitativo y cuantitativo....

  12. Informe final. Manejo y monitoreo de las mareas rojas, en las regiones de Los Lagos, Aysén y Magallanes. IV etapa, 2010.

    OpenAIRE

    Guzmán Méndez, F. L.; Vidal Santana, G.; Pizarro Nova, G.; Iriarte Bustamante, L.; Alarcón Zapata, C.; Arenas Sepúlveda, V.; Mercado Leal, S.; Pacheco Valles, H.; Mejías Wagner, P.; Salgado Garrido, P.; Palma Alarcón, M.; Espinoza Alvarado, C.; Fernández-Niño Azócar, E.; Monsalve Montecinos, J.; Zamora Amstein, C.

    2011-01-01

    En el presente informe se muestran los resultados de la cuarta etapa de un estudio diseñado para monitorear las variaciones espacio temporales del veneno paralizante de los mariscos (VPM), el veneno diarreíco de los mariscos (VDM), el veneno amnésico de los mariscos (VAM) en especies transvectoras centinelas, y de especies de microalgas nocivas o potencialmente nocivas, además de variables ambientales de tipo hidrográficas y meteorólogicas, además, de fitoplancton cualitativo y cuantitativo....

  13. Comprensión pública de la nanociencia y la nanotecnología. Informe de los resultados de un estudio Delphi

    OpenAIRE

    Gómez Ferri, Javier

    2013-01-01

    Según datos de los Eurobarómetros que periódicamente realiza la Comisión Europea y de estudios recientes más específicos, los niveles de cultura científica de la sociedad española se encuentran entre los más bajos de Europa. En el caso de la nanotecnología el desconocimiento es especialmente significativo. El presente informe recoge los principales resultados de una investigación realizada entre expertos sobre comprensión pública de la nanociencia y la nanotecnología. el obj...

  14. An ALMA view of the post-AGB object HD 101584

    Science.gov (United States)

    Olofsson, H.; Vlemmings, W.; Maercker, M.; Humphreys, E.; Lindqvist, M.; Nyman, L.; Ramstedt, S.

    2016-07-01

    ALMA cycles 1 and 3 observations of CO isotopologues and 1.3mm continuum are used in a study of the circumstellar environment of the binary HD 101584, a post-AGB star and a low-mass companion that is most likely a post-common-envelope-evolution system. These data are supplemented with new information from OH maser emission. It is inferred that the large- scale circumstellar medium has a bipolar hour-glass structure, seen almost pole-on, formed by an energetic, ≥⃒ 150 km s-1, jet. Significant amount of material still resides in the central region. It is proposed that the circumstellar morphology is related to an event which took place ≤⃒ 500 yr ago, possibly a capture event where the companion spiralled in towards the AGB star. Several observed features remain to be explained, and may hint to a more complicated scenario.

  15. Sistema informático para análisis y procesamiento de datos de los computadores de a bordo de la serie AGM-200X

    Directory of Open Access Journals (Sweden)

    Javier Lorenzo

    2011-10-01

    Full Text Available Con el auge de las Tecnologías de la Información y las Comunicaciones  y el abaratamiento del uso de los sistemas de navegación asistidos por satélites, cada día son más comunes los sistemas de control de flota y los computadores de a bordo, con el objetivo de elevar la eficiencia en el uso de los recursos técnicos y humanos. Tanto los sistemas de control de flota como los computadores de a bordo precisan de un autómata y un sistema informático que procese los datos registrados por el autómata. El presente artículo versa sobre del Sistema Informático de Recuperación, Análisis y Procesamiento de Datos de los Computadores de a bordo de la serie AGM-200X aplicados en la agricultura, el cual ya ha sido probado exitosamente en empresas de Brasil y Australia. Este sistema fue desarrollado a partir del modelo de Sistema de Análisis de Datos de Ordenadores de a Bordo (SIANDOB. Se detallan los módulos y capas que forman el modelo y las características del software resultante de su aplicación práctica.

  16. El culteranismo cartujo de 'Alma de Dios' (1637), de Miguel de Dicastillo

    OpenAIRE

    Mata-Induráin, C. (Carlos)

    2002-01-01

    El estilo poético del tafallés Miguel de Dicastillo, religioso cartujo, presenta rasgos característicos del culteranismo, cuya obra destacada es un libro de poemas titulado 'Alma de Dios', de 1637. ---------------------- The poetic style of Miguel de Dicastillo has features characteristic of culteranism; his outstanding work is a book of poems entitled 'Alma de Dios', from 1637.

  17. SXDF-ALMA 2-arcmin2 deep survey: 1.1-mm number counts

    NARCIS (Netherlands)

    Hatsukade, Bunyo; Kohno, Kotaro; Umehata, Hideki; Aretxaga, Itziar; Caputi, Karina I.; Dunlop, James S.; Ikarashi, Soh; Iono, Daisuke; Ivison, Rob J.; Lee, Minju; Makiya, Ryu; Matsuda, Yuichi; Motohara, Kentaro; Nakanishi, Kouichiro; Ohta, Kouji; Tadaki, Ken-ich; Tamura, Yoichi; Wang, Wei-Hao; Wilson, Grant W.; Yamaguchi, Yuki; Yun, Min S.

    2016-01-01

    We report 1.1-mm number counts revealed with the Atacama Large Millimeter/submillimeter Array (ALMA) in the Subaru/XMM-Newton Deep Survey Field (SXDF). The advent of ALMA enables us to reveal millimeter-wavelength number counts down to the faint end without source confusion. However, previous studie

  18. Design and development of a 600-720 GHz receiver for ALMA Band 9

    NARCIS (Netherlands)

    Baryshev, A. M.; Hesper, R.; Mena, F. P.; Jackson, B. D.; Adema, J.; Schaeffer, H.; Barkhof, J.; Wild, W.; Candotti, M.; Lodewijk, C.; Loudkov, D.; Zijlstra, T.; Noroozian, 0.; Klapwijk, T. M.

    2006-01-01

    This paper describes the design and development of the ALMA Band 9 receiver cartridges. The ALMA project is a collaboration between Europe, North America, and Japan to build an aperture synthesis telescope consisting of at least 64 12-m antennas located at 5000 m altitude in Chile. In its full confi

  19. Preparación de los docentes desde la informática y la pedagogía para el uso de moodle

    OpenAIRE

    Sahara María Blanco Hernández; Febe Ángel Ciudad Ricardo; Úrsula Puentes Puentes

    2015-01-01

    Actualmente los especialistas informáticos desarrollan software para la enseñanza, soportados en las Tecnologías de la Información y las Comunicaciones (TIC), como es el caso de Moodle y utilizan conceptos que ya tienen una sistematización científica en otras ciencias, como las Pedagógicas. Es por ello que este trabajo tiene el propósito de socializar los resultados del diagnóstico realizado a los docentes de la Universidad de las Ciencias Informáticas (UCI), con respecto a la preparación que...

  20. Los nuevos derechos humanos: gobierno electrónico e informática comunitaria

    OpenAIRE

    Javier Bustamante Donas

    2007-01-01

    Este artículo analiza la relación entre derechos humanos, tecnología y democracia. En particular, la relaciónentre el uso de Internet, las políticas de inclusión digital y el desarrollo del gobierno electrónico, con referencias alos casos de Brasil y España. Se identifican factores que suponen un cambio real en la definición de los límites de lademocracia y en el concepto de ciudadanía. El movimiento Linux, las comunidades virtuales y la ética de hackersson manifestaciones de una primera gene...

  1. Astronomers Break Ground on Atacama Large Millimeter Array (ALMA) - World's Largest Millimeter Wavelength Telescope

    Science.gov (United States)

    2003-11-01

    Scientists and dignitaries from Europe, North America and Chile are breaking ground today (Thursday, November 6, 2003) on what will be the world's largest, most sensitive radio telescope operating at millimeter wavelengths . ALMA - the "Atacama Large Millimeter Array" - will be a single instrument composed of 64 high-precision antennas located in the II Region of Chile, in the District of San Pedro de Atacama, at the Chajnantor altiplano, 5,000 metres above sea level. ALMA 's primary function will be to observe and image with unprecedented clarity the enigmatic cold regions of the Universe, which are optically dark, yet shine brightly in the millimetre portion of the electromagnetic spectrum. The Atacama Large Millimeter Array (ALMA) is an international astronomy facility. ALMA is an equal partnership between Europe and North America, in cooperation with the Republic of Chile, and is funded in North America by the U.S. National Science Foundation (NSF) in cooperation with the National Research Council of Canada (NRC), and in Europe by the European Southern Observatory (ESO) and Spain. ALMA construction and operations are led on behalf of North America by the National Radio Astronomy Observatory (NRAO), which is managed by Associated Universities, Inc. (AUI), and on behalf of Europe by ESO. " ALMA will be a giant leap forward for our studies of this relatively little explored spectral window towards the Universe" , said Dr. Catherine Cesarsky , Director General of ESO. "With ESO leading the European part of this ambitious and forward-looking project, the impact of ALMA will be felt in wide circles on our continent. Together with our partners in North America and Chile, we are all looking forward to the truly outstanding opportunities that will be offered by ALMA , also to young scientists and engineers" . " The U.S. National Science Foundation joins today with our North American partner, Canada, and with the European Southern Observatory, Spain, and Chile to prepare

  2. The ALMA common software: dispatch from the trenches

    Science.gov (United States)

    Schwarz, J.; Sommer, H.; Jeram, B.; Sekoranja, M.; Chiozzi, G.; Grimstrup, A.; Caproni, A.; Paredes, C.; Allaert, E.; Harrington, S.; Turolla, S.; Cirami, R.

    2008-07-01

    The ALMA Common Software (ACS) provides both an application framework and CORBA-based middleware for the distributed software system of the Atacama Large Millimeter Array. Building upon open-source tools such as the JacORB, TAO and OmniORB ORBs, ACS supports the development of component-based software in any of three languages: Java, C++ and Python. Now in its seventh major release, ACS has matured, both in its feature set as well as in its reliability and performance. However, it is only recently that the ALMA observatory's hardware and application software has reached a level at which it can exploit and challenge the infrastructure that ACS provides. In particular, the availability of an Antenna Test Facility(ATF) at the site of the Very Large Array in New Mexico has enabled us to exercise and test the still evolving end-to-end ALMA software under realistic conditions. The major focus of ACS, consequently, has shifted from the development of new features to consideration of how best to use those that already exist. Configuration details which could be neglected for the purpose of running unit tests or skeletal end-to-end simulations have turned out to be sensitive levers for achieving satisfactory performance in a real-world environment. Surprising behavior in some open-source tools has required us to choose between patching code that we did not write or addressing its deficiencies by implementing workarounds in our own software. We will discuss these and other aspects of our recent experience at the ATF and in simulation.

  3. Radio measurements of constant variation, and perspectives with ALMA

    Science.gov (United States)

    Combes, Françoise

    2010-11-01

    In the radio domain, absorption lines in front of quasars of CO, HI, OH, HCO+, HCN, up to NH3 and CII are providing interesting constraints on fundamental constant variation (α and μ). With more absorbing systems, and a wider redshift range, they could be more competitive than optical studies. This could come with ALMA, with more than one order of magnitude in sensitivity. Up to now, at intermediate and high redshift, between z = 0.25 to z = 0.89, only four absorption lines systems have been detected in the millimeter range and a fifth system at 0.765, at the OH-18cm lines (Kanekar et al. 2005). Out of these 5 systems, 3 are intervening lensing galaxies (and the background quasar is multiply imaged), and 2 correspond to an absorption of the host (PKS1413+135, B3-1504+377, for an overview see Combes & Wiklind 1996; Wiklind & Combes 1994 to 1998). A global comparison of all molecular lines observed with the HI-21cm absorption lines in PKS1413 and B0218 systems, the two narrowest line systems, have given quite stringent constraints on y = α2 gp μ, Δ y/y = (-0.20 ± 0.44) 10-5 and Δ y/y = (-0.16 ± 0.54) 10-5 respectively (Murphy et al. 2001). The precision is comparable to the MM method (Murphy et al. 2003), with a limited number of absorbing systems. The high sensitivity if the NH3 inversion lines to variation in the μ ratio (Flambaum & Kozlov 2007) was used by Henkel et al. (2009) in a recent multi-line study of PKS1830 at z ~ 0.9, and Murphy et al. (2008) for B0218 at z ~ 0.7. They find a limit of Δμ/μ 100 for NH3). Fortunately, the sensitivity of ALMA will be able to detect many more continuum sources, to search for absorption lines, and at larger redshifts. ALMA will have a much wider bandwidth, allowing the search of absorption, even if not previously detected in the optical or HI-21cm. The redshift will be obtained directly in the millimeter. It is possible to predict the number of continuum sources that can be selected as targets for absorption

  4. Los programas de mejora de la ciudad informal, herramientas de lucha contra la pobreza

    Directory of Open Access Journals (Sweden)

    Colavidas, Felipe

    2004-06-01

    Full Text Available The paper contains a discussion of the chief approachesand objectives of new policies for improving precariousLatin American barrios implemented by multilateral,national and/or municipal organizations. With a census of25 million extremely precarious living quarters, theseneighbourhoods have a combined population of 125million. A precise estimate of the investment required toimprove, enlarge and/or refurbish this sub-standardhousing amounts to US$170 billion. In this vein, therelevance and specific contribution of three programmes(“Chile Barrio”, “Favela Barrio” and “Obras con SaldoPedagógico” are critically reviewed from the standpointof their utility as tools for combating poverty.Se presentan los principales enfoques y objetivos de lasnuevas políticas de mejora de barrios precarios enLatinoamérica emprendidas por organismos multilaterales,nacionales y/o municipales. Barrios, en los que secontabilizan más de 25 millones de soluciones habitacionalesextremadamente precarias, en las que se alojan unos 125millones de habitantes. Se ha estimado de forma precisa, quela inversión necesaria para el mejoramiento, ampliacióny/o dotación de estas infraviviendas supondría unos 170.000millones de $USA. Igualmente, se presenta una síntesiscrítica de tres programas (Chile Barrio, Favela Barrio yObras con Saldo Pedagógico, desde la óptica de supertinencia y aportes concretos como herramientas para lalucha contra la pobreza.

  5. ALMA Observations of HD141569's Circumstellar Disk

    CERN Document Server

    White, J A; Hughes, A M; Flaherty, K M; Ford, E; Wilner, D; Corder, S; Payne, M

    2016-01-01

    We present ALMA band 7 (345 GHz) continuum and $^{12}$CO(J = 3-2) observations of the circumstellar disk surrounding HD141569. At an age of about 5 Myr, the disk has a complex morphology that may be best interpreted as a nascent debris system with gas. Our $870\\rm~\\mu m$ ALMA continuum observations resolve a dust disk out to approximately $ 56 ~\\rm au$ from the star (assuming a distance of 116 pc) with $0."38$ resolution and $0.07 ~ \\rm mJy~beam^{-1}$ sensitivity. We measure a continuum flux density for this inner material of $3.8 \\pm 0.4 ~ \\rm mJy$ (including calibration uncertainties). The $^{12}$CO(3-2) gas is resolved kinematically and spatially from about 30 to 210 au. The integrated $^{12}$CO(3-2) line flux density is $15.7 \\pm 1.6~\\rm Jy~km~s^{-1}$. We estimate the mass of the millimeter debris and $^{12}$CO(3-2) gas to be $\\gtrsim0.04~\\rm M_{\\oplus}$ and $\\sim2\\times 10^{-3}~\\rm M_{\\oplus}$, respectively. If the millimeter grains are part of a collisional cascade, then we infer that the inner disk ($&...

  6. ALMA images of discs: are all gaps carved by planets?

    CERN Document Server

    Gonzalez, Jean-François; Maddison, Sarah T; Pinte, Christophe; Ménard, François

    2015-01-01

    Protoplanetary discs are now routinely observed and exoplanets, after the numerous indirect discoveries, are starting to be directly imaged. To better understand the planet formation process, the next step is the detection of forming planets or of signposts of young planets still in their disc, such as gaps. A spectacular example is the ALMA science verification image of HL Tau showing numerous gaps and rings in its disc. To study the observability of planet gaps, we ran 3D hydrodynamical simulations of a gas and dust disc containing a 5 M J gap-opening planet and characterised the spatial distribution of migrating, growing and fragmenting dust grains. We then computed the corresponding synthetic images for ALMA. For a value of the dust fragmentation threshold of 15 m s --1 for the collisional velocity, we identify for the first time a self-induced dust pile up in simulations taking fragmentation into account. This feature, in addition to the easily detected planet gap, causes a second apparent gap that could...

  7. Measuring protoplanetary disk gas surface density profiles with ALMA

    CERN Document Server

    McPartland, Jonathan P Williams Conor

    2016-01-01

    The gas and dust are spatially segregated in protoplanetary disks due to the vertical settling and radial drift of large grains. A fuller accounting of the mass content and distribution in disks therefore requires spectral line observations. We extend the modeling approach presented in Williams & Best (2014) to show that gas surface density profiles can be measured from high fidelity 13CO integrated intensity images. We demonstrate the methodology by fitting ALMA observations of the HD 163296 disk to determine a gas mass, Mgas = 0.048 solar masse, and accretion disk characteristic size Rc = 213au and gradient gamma = 0.39. The same parameters match the C18O 2--1 image and indicates an abundance ratio [13CO]/[C18O] of 700 independent of radius. To test how well this methodology can be applied to future line surveys of smaller, lower mass T Tauri disks, we create a large 13CO 2--1 image library and fit simulated data. For disks with gas masses 3-10 Jupiter masses at 150pc, ALMA observations with a resolutio...

  8. Unveiling the dust nucleation zone of IRC+10216 with ALMA

    CERN Document Server

    Cernicharo, J; Castro-Carrizo, A; Agundez, M; Marcelino, N; Joblin, C; Goicoechea, J R; Guélin, M

    2013-01-01

    We report the detection in IRC+10216 of lines of HNC $J$=3-2 pertaining to 9 excited vibrational states with energies up to $\\sim$5300 K. The spectrum, observed with ALMA, also shows a surprising large number of narrow, unidentified lines that arise in the vicinity of the star. The HNC data are interpreted through a 1D--spherical non--local radiative transfer model, coupled to a chemical model that includes chemistry at thermochemical equilibrium for the innermost regions and reaction kinetics for the external envelope. Although unresolved by the present early ALMA data, the radius inferred for the emitting region is $\\sim$0.06'' (i.e., $\\simeq$ 3 stellar radii), similar to the size of the dusty clumps reported by IR studies of the innermost region ($r <$ 0.3''). The derived abundance of HNC relative to H$_2$ is $10^{-8} <$ $\\chi$(HNC) $< 10^{-6}$, and drops quickly where the gas density decreases and the gas chemistry is dominated by reaction kinetics. Merging HNC data with that of molecular species...

  9. ALMA Observations of the Active Nucleus of NGC 7469

    CERN Document Server

    Izumi, Takuma; Aalto, Susanne; Doi, Akihiro; Espada, Daniel; Fathi, Kambiz; Harada, Nanase; Hatsukade, Bunyo; Hattori, Takashi; Hsieh, Pei-Ying; Ikarashi, Soh; Imanishi, Masatoshi; Iono, Daisuke; Ishizuki, Sumio; Krips, Melanie; Martín, Sergio; Matsushita, Satoki; Meier, David S; Nagai, Hiroshi; Nakai, Naomasa; Nakajima, Taku; Nakanishi, Kouichiro; Nomura, Hideko; Regan, Michael W; Schinnerer, Eva; Sheth, Kartik; Takano, Shuro; Tamura, Yoichi; Terashima, Yuichi; Tosaki, Tomoka; Turner, Jean L; Umehata, Hideki; Wiklind, Tommy

    2015-01-01

    We present ALMA Cycle 1 observations of the central kpc region of the luminous type-1 Seyfert galaxy NGC 7469 with unprecedented high resolution (0.5$"$ $\\times$ 0.4$"$ = 165 pc $\\times$ 132 pc) at submillimeter wavelengths. Utilizing the wide-bandwidth of ALMA, we simultaneously obtained HCN(4-3), HCO$^+$(4-3), CS(7-6), and partially CO(3-2) line maps, as well as the 860 $\\mu$m continuum. The region consists of the central $\\sim$ 1$"$ component and the surrounding starburst ring with a radius of $\\sim$ 1.5$"$-2.5$"$. Several structures connect these components. Except for CO(3-2), these dense gas tracers are significantly concentrated towards the central $\\sim$ 1$"$, suggesting their suitability to probe the nuclear regions of galaxies. Their spatial distribution resembles well those of centimeter and mid-infrared continuum emissions, but it is anti-correlated with the optical one, indicating the existence of dust obscured star formation. The integrated intensity ratios of HCN(4-3)/HCO$^+$(4-3) and HCN(4-3)/...

  10. Possibility of Terahertz Observations at the ALMA site

    CERN Document Server

    Matsushita, Satoki

    2011-01-01

    Observational rates under terahertz (THz) opacities less than 3.0 and 2.0 at the Atacama Large Millimeter/submillimeter Array (ALMA) site have been calculated using the 225 GHz tipping radiometer monitoring data and the opacity correlation between 225 GHz and THz opacities. The observational rate with THz opacity condition less than 3.0 is 12.4% in a year, and in winter (November - April) it is about twice higher than in summer (May - October). This observational rate shows a large sinusoidal annual variation, and it seems to have relation with the El Ni\\~no and La Ni\\~na phenomena; the La Ni\\~na years tend to have high observational rates, but the El Ni\\~no years show low rates. On the other hand, the observational rate with the THz opacity condition less than 2.0 is only 1.9%, and no obvious annual and seasonal variations are observed. This indicates that THz observations under low opacity condition of less than 2.0 at the ALMA site are very difficult to be performed.

  11. ALMA band 8 continuum emission from Orion Source I

    CERN Document Server

    Hirota, Tomoya; Matsushita, Yuko; Motogi, Kazuhito; Matsumoto, Naoko; Kim, Mi Kyoung; Burns, Ross A; Honma, Mareki

    2016-01-01

    We have measured continuum flux densities of a high-mass protostar candidate, a radio source I in the Orion KL region (Orion Source I) using the Atacama Large Millimeter/Submillimeter Array (ALMA) at band 8 with an angular resolution of 0.1". The continuum emission at 430, 460, and 490 GHz associated with Source I shows an elongated structure along the northwest-southeast direction perpendicular to the so-called low-velocity bipolar outflow. The deconvolved size of the continuum source, 90 au times 20 au, is consistent with those reported previously at other millimeter/submillimeter wavelength. The flux density can be well fitted to the optically thick black-body spectral energy distribution (SED), and the brightness temperature is evaluated to be 700-800 K. It is much lower than that in the case of proton-electron or H- free-free radiations. Our data are consistent with the latest ALMA results by Plambeck & Wright (2016), in which the continuum emission have been proposed to arise from the edge-on circum...

  12. A CORBA event system for ALMA common software

    Science.gov (United States)

    Fugate, David W.

    2004-09-01

    The ALMA Common Software notification channel framework provides developers with an easy to use, high-performance, event-driven system supported across multiple programming languages and operating systems. It sits on top of the CORBA notification service and hides nearly all CORBA from developers. The system is based on a push event channel model where suppliers push events onto the channel and consumers process these asynchronously. This is a many-to-many publishing model whereby multiple suppliers send events to multiple consumers on the same channel. Furthermore, these event suppliers and consumers can be coded in C++, Java, or Python on any platform supported by ACS. There are only two classes developers need to be concerned with: SimpleSupplier and Consumer. SimpleSupplier was designed so that ALMA events (defined as IDL structures) could be published in the simplest manner possible without exposing any CORBA to the developer. Essentially all that needs to be known is the channel's name and the IDL structure being published. The API takes care of everything else. With the Consumer class, the developer is responsible for providing the channel's name as well as associating event types with functions that will handle them.

  13. An overview of the ALMA Common Software (ACS) .

    Science.gov (United States)

    Di Marcantonio, P.; Cirami, R.; Caproni, A.; Chiozzi, G.; Jeram, B.; Sommer, H.; Harrington, S.; Zagar, K.; Plesko, M.; Sekoranja, M.

    The ALMA Common Software (ACS) is an application framework designed to provide a common and homogeneous software architecture and infrastructure, spanning the end to end needs of an Astronomical observatory, from the Telescope Control system to high-level data flow management. ACS offers, at the lower level, several basic services needed for object-oriented distributed computing like transparent remote object invocation, object deployment and location, distributed error, alarm handling, logging and events. On top of this it provides an application architecture based on the Component/Container paradigm that fosters sharing and reusing of software components. Although developed for the ALMA project, ACS is now used by several other projects worldwide, among which the Italian Sardinia Radio Telescope (SRT). Besides, there is an active community that shares ideas, concepts and actual software components. Major drivers for this diffusion were the choice of adopting the LGPL public license and the adoption of CORBA, a free but reliable and widely used middleware software. In this paper we present an overview of the main features of ACS, emphasizing in particular the role of INAF-OAT in this project.

  14. Container-component model and XML in ALMA ACS

    Science.gov (United States)

    Sommer, Heiko; Chiozzi, Gianluca; Zagar, Klemen; Voelter, Markus

    2004-09-01

    ALMA software, from high-level data flow applications down to instrument control, is built using the ACS framework. To meet the challenges of developing distributed software in distributed teams, ACS offers a container/component model that integrates the use of XML transfer objects. ACS containers are built on top of CORBA and are available for C++, Java, and Python, so that ALMA software can be written as components in any of these languages. The containers perform technical aspects of the software system, while components can focus on the implementation of functional requirements. Like Web services, components can use XML to exchange structured data by value. For Java components, the container seamlessly integrates the use of XML binding classes, which are Java classes that encapsulate access to XML data through type-safe methods. Binding classes are generated from XML schemas, allowing the Java compiler to enforce compliance of application code with the XML schemas. This presentation will explain the capabilities of the ACS container/component model, and how it relates to other middleware technologies that are popular in industry.

  15. Testing particle trapping in transition disks with ALMA

    CERN Document Server

    Pinilla, P; Pérez, L M; van Dishoeck, E F; Andrews, S; Birnstiel, T; Herczeg, G; Pontoppidan, K M; van Kempen, T

    2015-01-01

    We present new ALMA continuum observations at 336 GHz of two transition disks, SR 21 and HD 135344B. In combination with previous ALMA observations from Cycle 0 at 689 GHz, we compare the visibility profiles at the two frequencies and calculate the spectral index ($\\alpha_{\\rm{mm}}$). The observations of SR 21 show a clear shift in the visibility nulls, indicating radial variations of the inner edge of the cavity at the two wavelengths. Notable radial variations of the spectral index are also detected for SR 21 with values of $\\alpha_{\\rm{mm}}\\sim3.8-4.2$ in the inner region ($r\\lesssim35$ AU) and $\\alpha_{\\rm{mm}}\\sim2.6-3.0$ outside. An axisymmetric ring ("ring model") or a ring with the addition of an azimuthal Gaussian profile, for mimicking a vortex structure ("vortex model"), is assumed for fitting the disk morphology. For SR 21, the ring model better fits the emission at 336 GHz, conversely the vortex model better fits the 689 GHz emission. For HD 135344B, neither a significant shift in the null of the...

  16. ALMA Observations of Asteroid 3 Juno at 60 Kilometer Resolution

    CERN Document Server

    Partnership, ALMA; Kneissl, R; Moullet, A; Brogan, C L; Fomalont, E B; Vlahakis, C; Asaki, Y; Barkats, D; Dent, W R F; Hills, R; Hirota, A; Hodge, J A; Impellizzeri, C M V; Liuzzo, E; Lucas, R; Marcelino, N; Matsushita, S; Nakanishi, K; Perez, L M; Phillips, N; Richards, A M S; Toledo, I; Aladro, R; Broguiere, D; Cortes, J R; Cortes, P C; Dhawan, V; Espada, D; Galarza, F; Garcia-Appadoo, D; Guzman-Ramirez, L; Hales, A S; Humphreys, E M; Jung, T; Kameno, S; Laing, R A; Leon, S; Marconi, G; Nikolic, B; Nyman, L -A; Radiszcz, M; Remijan, A; Rodon, J A; Sawada, T; Takahashi, S; Tilanus, R P J; Vilaro, B Vila; Watson, L C; Wiklind, T; de Gregorio, I; Di Francesco, J; Mangum, J; Francke, H; Gallardo, J; Garcia, J; Gonzalez, S; Hill, T; Kaminski, T; Kurono, Y; Lopez, C; Morales, F; Plarre, K; Randall, S; van kempen, T; Videla, L; Villard, E; Andreani, P; Hibbard, J E; Tatematsu, K

    2015-01-01

    We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm continuum images of the asteroid 3 Juno obtained with an angular resolution of 0.042 arcseconds (60 km at 1.97 AU). The data were obtained over a single 4.4 hr interval, which covers 60% of the 7.2 hr rotation period, approximately centered on local transit. A sequence of ten consecutive images reveals continuous changes in the asteroid's profile and apparent shape, in good agreement with the sky projection of the three-dimensional model of the Database of Asteroid Models from Inversion Techniques. We measure a geometric mean diameter of 259pm4 km, in good agreement with past estimates from a variety of techniques and wavelengths. Due to the viewing angle and inclination of the rotational pole, the southern hemisphere dominates all of the images. The median peak brightness temperature is 215pm13 K, while the median over the whole surface is 197pm15 K. With the unprecedented resolution of ALMA, we find that the brightness temperature varies ...

  17. Simulating ALMA Observations of High-Redshift Submillimeter Galaxies

    Science.gov (United States)

    Carilli, Michael; Wagg, J.

    2007-12-01

    Until now, the coarse angular resolution of single-dish submm/mm telescopes has limited the depth of extragalactic surveys through confusion noise, meaning that only 20-30% of the 850 micron background can be resolved. However, the majority of this population should have flux densities of 1 mJy or fainter, and so either cannot be resolved or would require prohibitively long integration times to conduct surveys with existing interferometers. This will change with the advent of the Atacama Large Millimeter Array (ALMA); beginning operation within the next decade, it will provide an order of magnitude increase in sensitivity over that of current interferometers. To better plan for future surveys with this facility, I have prepared a set of simulated 850 micron and 1 mm maps covering 16 square arcminutes with an angular resolution of 1 arcsecond. The input models used to create these simulations are based on our current constraints on the 850 micron and 1 mm number counts, as well as a heuristic model which assumes an evolving 60 micron IRAS luminosity function. This work shows how ALMA will constrain the number counts well below the sub-mJy level. Research was conducted as part of the National Science Foundation's Research Experience for Undergraduates program.

  18. Preparación de los docentes desde la informática y la pedagogía para el uso de moodle

    Directory of Open Access Journals (Sweden)

    Sahara María Blanco Hernández

    2015-07-01

    Full Text Available Actualmente los especialistas informáticos desarrollan software para la enseñanza, soportados en las Tecnologías de la Información y las Comunicaciones (TIC, como es el caso de Moodle y utilizan conceptos que ya tienen una sistematización científica en otras ciencias, como las Pedagógicas. Es por ello que este trabajo tiene el propósito de socializar los resultados del diagnóstico realizado a los docentes de la Universidad de las Ciencias Informáticas (UCI, con respecto a la preparación que poseen, para operar con el significado de los conceptos referidos, en la configuración y uso de Moodle y los conocimientos que pueden ser objeto de aprendizaje, desde la Informática y la Pedagogía. El presente trabajo está enmarcado en el proyecto: La calidad de la formación de los ingenieros, con sustento en el vínculo universidad – industria y las TIC. En este proyecto se ha considerado la capacitación de los profesores como uno de los problemas a resolver. Los métodos teóricos utilizados fueron el de análisis-síntesis y el inductivo- deductivo. Se utilizaron como métodos empíricos la entrevista, el producto de la actividad y el estudio de caso, este último, apoyado por el diferencial semántico como técnica que permitió apreciar el valor de la propuesta realizada.

  19. EL TRABAJO INFORMAL DE LOS VAGONEROS EN EL METRO DE LA CIUDAD DE MÉXICO

    Directory of Open Access Journals (Sweden)

    Eloísa Ramírez Cárdenas

    2016-05-01

    Full Text Available This paper focuses on analysis of the decisions made by peddlers to continue working on the streets, specifically selling apocryphal items. Those decisions are based on the working conditions in the informal sector. To collect data, the participant observation was used, as buyers; 8 interviews with vendors, aged over 25, were conducted. These sellers are engaged in the sale of pirate compact discs (CDs inside the wagons of the Sistema de Transporte Colectivo (STC Metro Line 8 in Mexico City. The results show that economic income, financial compensation, the working day and the satisfaction of working in the informal sector makes those people keep on working within the framework of informality.

  20. Geographic Information System (GIS) Emergency Support for the May 2000 Cerro Grande Wildfire, Los Alamos, New Mexico, USA

    Energy Technology Data Exchange (ETDEWEB)

    C.R.Mynard; G.N.Keating; P.M.Rich; D.R. Bleakly

    2003-05-01

    In May 2000 the Cerro Grande wildfire swept through Los Alamos, New Mexico, burning approximately 17,400 ha (43,000 acres) and causing evacuation of Los Alamos National Laboratory (LANL) and the communities of Los Alamos and White Rock. An integral part of emergency response during the fire was the use of geographic information system (GIS) technology, which continues to be used in support of post-fire restoration and environmental monitoring. During the fire Laboratory GIS staff and volunteers from other organizations worked to produce maps and provide support for emergency managers, including at an emergency GIS facility in Santa Fe. Subsequent to the fire, Laboratory GIS teams supported the multiagency Burned Area Emergency Rehabilitation (BAER) team to provide GIS data and maps for planning mitigation efforts. The GIS teams continue to help researchers, operations personnel, and managers deal with the tremendous changes caused by the fire. Much of the work is under the auspices of the Cerro Grande Rehabilitation Project (CGRP) to promote recovery from fire damage, improve information exchange, enhance emergency management, and conduct mitigation activities. GIS efforts during the fire provided important lessons about institutional matters, working relationships, and emergency preparedness. These lessons include the importance of (1) an integrated framework for assessing natural and human hazards in a landscape context; (2) a strong GIS capability for emergency response; (3) coordinated emergency plans for GIS operations; (4) a method for employees to report their whereabouts and receive authoritative information during an evacuation; (5) GIS data that are complete, backed-up, and available during an emergency; (6) adaptation of GIS to the circumstances of the emergency; (7) better coordination in the GIS community; (8) better integration of GIS into LANL operations; and (9) a central data warehouse for data and metadata. These lessons are important for planning

  1. Informática I (Fundamentos de la informática para los nuevos estudiantes de Grado) (2009/2010)

    OpenAIRE

    Grimaldo Moreno, Francisco; Giménez Sánchez, Juan Vicente; Navalón Martínez, José Ángel

    2009-01-01

    Esta asignatura cubre los fundamentos de las Tecnologías de la Información y la Comunicación (TIC), la arquitectura de los computadores y los conceptos generales de los algoritmos. Además, introduce los sistemas operativos y las redes de comunicación, junto con una formación avanzada con paquetes de ofimática.

  2. Informe del NCI y los CDC sobre el tabaco sin humo

    Science.gov (United States)

    El primer informe sobre el consumo mundial del tabaco sin humo y sus consecuencias en la salud pública reveló que más de 300 millones de personas en al menos 70 países usan estos productos dañinos.

  3. Prototype Implementation of Web and Desktop Applications for ALMA Science Verification Data and the Lessons Learned

    OpenAIRE

    Eguchi, Satoshi; Kawasaki, Wataru; Shirasaki, Yuji; Komiya, Yutaka; Kosugi, George; Ohishi, Masatoshi; Mizumoto, Yoshihiko

    2012-01-01

    ALMA is estimated to generate TB scale data during only one observation; astronomers manage to identify which part of the data they are really interested in. Now we have been developing new GUI software for this purpose utilizing the VO interface: ALMA Web Quick Look System (ALMAWebQL) and ALMA Desktop Application (Vissage). The former is written in JavaScript and HTML5 generated from Java codes by Google Web Toolkit, and the latter is in pure Java. An essential point of our approach is how t...

  4. Os sete graus de atividade da alma humana no De quantitate animae de Santo Agostinho

    Directory of Open Access Journals (Sweden)

    Sérgio Ricardo Strefling

    2014-12-01

    Full Text Available A alma é, sem dúvida, um dos problemas que mais interessou a Santo Agostinho; ele a define como uma substância partícipe da razão adequada ao governo de um corpo. A alma não tem quantidade corporal, contudo, é uma coisa grande. Este estudo pretende refletir sobre os sete graus de atividade da alma, os quais o autor apresenta na sua obra De quantitate animae. São eles: a animação, a sensação, a arte, a virtude, a tranquilidade, o ingresso e a contemplação.

  5. The Science Case for ALMA Band 2 and Band 2+3

    CERN Document Server

    Fuller, G A; Beltran, M; Casasola, V; Caselli, P; Cicone, C; Costagliola, F; De Breuck, C; Hunt, L; Jimenez-Serra, I; Laing, R; Longmore, S; Massardi, M; Paladino, R; Ramstedt, S; Richards, A; Testi, L; Vergani, D; Viti, S; Wagg, J

    2016-01-01

    We discuss the science drivers for ALMA Band 2 which spans the frequency range from 67 to 90 GHz. The key science in this frequency range are the study of the deuterated molecules in cold, dense, quiescent gas and the study of redshifted emission from galaxies in CO and other species. However, Band 2 has a range of other applications which are also presented. The science enabled by a single receiver system which would combine ALMA Bands 2 and 3 covering the frequency range 67 to 116 GHz, as well as the possible doubling of the IF bandwidth of ALMA to 16 GHz, are also considered.

  6. La música de los números: descubrimiento y aplicación de las proporciones sonoras

    OpenAIRE

    Martínez González, Francisco

    2014-01-01

    La conferencia se plantea remontarse a los orígenes de la relación entre la música y los números, aunque previamente se acerca a los más antiguos mitos griegos relacionados con el arte de los sonidos (Orfeo, Dionisos, Marsias, Sirenas). A continuación se muestra cómo los pitagóricos nos revelaron la naturaleza musical del cosmos y, a través de ella, la naturaleza relacional y procesual de la realidad. A su vez, fueron ellos los descubridores del alma, y los que definieron a ésta y a la música...

  7. LEARNIG TO BE INFORMED ON THE INTERNET: ¿ARE STUDENTS EFFECTIVE IN SEEKING AND SELECTING ONLINE INFORMATION? APRENDER A INFORMARSE EN LA RED: ¿SON LOS ESTUDIANTES EFICIENTES BUSCANDO Y SELECCIONANDO INFORMACIÓN?

    Directory of Open Access Journals (Sweden)

    María José Hernández Serrano

    2011-03-01

    Full Text Available From an educational perspective, taking the Internet as an informational resource for education, the article analyzes the scope of the new information skills in regard to the concepts of literacy and information competence. This brief description of skills leads to the question of how students perform in their searching and selecting practices with online information. The main conclusions abstracted from the recent author’s research are brought to debate in order to respond questions raised about the skills needed to being effective in accessing and managing online information. Finally, since the new ways to locate and operate with the information contributes to the reorganization of both the traditional models of teaching/learning and the roles of the educational stakeholders, we understand that preparing students to meet the informational demands requires of teachers as mediators or facilitators of the informational process; thus, in the final section of the article, a proposal for teaching strategies in searching and selecting online information is explored, by describing several useful activities.Desde una óptica educativa, tomando la Red como recurso de información para la educación, el artículo analiza qué suponen las nuevas habilidades informativas, en lo que respecta a los conceptos de alfabetización y competencia informacional. Esta breve descripción y recapitulación de habilidades nos lleva a preguntarnos, en la práctica, por cómo los estudiantes realizan los procesos de búsqueda y selección de información en línea. Traemos a debate las principales conclusiones abstraídas de los resultados de algunas de las investigaciones más relevantes de las autoras, que dan respuesta a los interrogantes planteados en torno a las habilidades necesarias para acceder y manejar eficazmente la información digital. Finalmente, y puesto que los nuevos modos para localizar y operar con la información precisan reorganizaciones tanto de

  8. The ALMA Front-end Archive Setup and Performance

    Science.gov (United States)

    Wicenec, A.; Chen, A.; Checcucci, A.; Jeram, B.; Meuss, H.; Persson, A.; Burgos, P.; Cirami, R.

    2010-12-01

    The ALMA front-end archive system has to capture up to 64 MB/s for a period of several days plus the data of about 100,000 monitor points from all 66 antennas and the correlators. The main science data is delivered through corba based audio/video streams and finally stored on SATA disk arrays hosted on 6 computers and controlled by 12 daemons. All data is collected by software components running on computers in the antennas and then sent through dedicated fiber links to the Array Operations Site at 5000 m and from there to the Operations Support Facility (OSF) at 3000 m elevation. The various hardware and software components have been tuned and tested to be able to meet the performance requirements. This paper describes the setup and the various components in more detail and gives results of various test runs.

  9. The Millimeter Astronomy Legacy Team 90 GHz Survey (MALT90) and ALMA

    CERN Document Server

    Foster, Jonathan B; Jackson, James M; Longmore, Steve N; Whitaker, Scott; Hoq, Sadia

    2013-01-01

    ALMA will revolutionize our understanding of star formation within our galaxy, but before we can use ALMA we need to know where to look. The Millimeter Astronomy Legacy Team 90 GHz (MALT90) Survey is a large international project to map the molecular line emission of over 2,000 dense clumps in the Galactic plane. MALT90 serves as a pathfinder for ALMA, providing a large public database of dense molecular clumps associated with high-mass star formation. In this proceedings, we describe the survey parameters and share early science highlights from the survey, including (1) a comparison between galactic and extragalactic star formation relations, (2) chemical trends in MALT90 clumps, (3) the distribution of high-mass star formation in the Milky Way, and (4) a discussion of the Brick, the target of successful ALMA Cycle 0 and Cycle 1 proposals.

  10. JCMT in the Post-Herschel ERA of Alma

    Science.gov (United States)

    Johnstone, Doug

    2013-07-01

    The James Clerk Maxwell Telescope (JCMT), with a 15m dish, is the largest single-dish astronomical telescope in the world designed specifically to operate in the sub-mm wavelength regime. The JCMT is located close to the summit of Mauna Kea, Hawaii, at an altitude of 4092m. The most recent addition to the JCMT's suite of instruments is the 10,000 bolometer sub-mm continuum instrument: SCUBA-2. SCUBA-2 operates simultaneously with 7' x7' foot print sub-arrays at both 450 and 850-microns. SCUBA-2's wide field surveying potential, combined with a 65% shared view of the sky from both sites, makes it the ideal instrument to provide complementary data for the ALMA Project. Furthermore, the SCUBA-2 sub-millimetre wavelength coverage and angular resolution complement existing Herschel observations. A set of comprehensive surveys of the submillimetre sky is underway at the James Clerk Maxwell Telescope (JCMT) using SCUBA-2 and HARP, a heterodyne array receiver operating between 325 and 375 GHz. The JCMT Legacy Survey (JLS) is comprised of seven survey projects, and ranges in scope from the study of nearby debris disk systems, the study of star formation in nearby molecular cloud systems and more distant structures in our Galactic Plane, to the structure and composition of galaxies in our local neighbourhood and the number and evolution of submillimetre galaxies at high redshifts in the early Universe. In addition to the JLS, the COHR survey is imaging the Galactic plane in CO (3-2) and a JAC Staff-led project is using SCUBA-2 to survey the Galactic Centre. This poster highlights the significant survey capabilities of SCUBA-2 and HARP and reveals the continuing importance of the JCMT in a post-Herschel, ALMA world.

  11. ACA phase calibration scheme with the ALMA water vapor radiometers

    Science.gov (United States)

    Asaki, Yoshiharu; Matsushita, Satoki; Morita, Koh-Ichiro; Nikolic, Bojan

    2012-09-01

    In Atacama Large Millimeter/submillimeter Array (ALMA) commissioning and science verification we have conducted a series of experiments of a novel phase calibration scheme for Atacama Compact Array (ACA). In this scheme water vapor radiometers (WVRs) devoted to measurements of tropospheric water vapor content are attached to ACA’s four total-power array (TP Array) antennas surrounding the 7 m dish interferometer array (7 m Array). The excess path length (EPL) due to the water vapor variations aloft is fitted to a simple two-dimensional slope using WVR measurements. Interferometric phase fluctuations for each baseline of the 7 m Array are obtained from differences of EPL inferred from the two-dimensional slope and subtracted from the interferometric phases. In the experiments we used nine ALMA 12-m antennas. Eight of them were closely located in a 70-m square region, forming a compact array like ACA. We supposed the most four outsiders to be the TP Array while the inner 4 antennas were supposed to be the 7 m Array, so that this phase correction scheme (planar-fit) was tested and compared with the WVR phase correction. We estimated residual root-mean-square (RMS) phases for 17- to 41-m baselines after the planar-fit phase correction, and found that this scheme reduces the RMS phase to a 70 - 90 % level. The planar-fit phase correction was proved to be promising for ACA, and how high or low PWV this scheme effectively works in ACA is an important item to be clarified.

  12. ALMA 1.3 mm observations of the Fomalhaut System

    Science.gov (United States)

    White, Jacob; Boley, Aaron C.; Ford, Eric B.; Payne, Matthew John; Dent, William; Corder, Stuartt

    2016-10-01

    We present ALMA Band 6 (1.3 mm) observations of Fomalhaut and its debris disk. Since the system is relatively close at 7.7 pc, it has been the target of numerous studies at multiple wavelengths, and can serve as a testbed for debris disk evolution models and planet-disk interactions. Outstanding issues that need to be resolved to properly characterize the debris include tightening constraints on the spectral index in the submm/mm regime and determining whether there is indeed excess over the stellar emission, indicating the presence of an inner debris disk or ring.These ALMA 1.3 mm observations provide the highest resolution observations to date of the mm grains the outer ring. Tight constraints are placed on the geometry of the disk and on the mm-wavelength spectral index. We explore fitting the debris disk model in the image plane in addition to the standard method of fitting the visibilities. The results are compared and potential advantages/disadvantages of each approach are discussed.The central emission detected is indistinguishable from a point source, with 0.89 mJy being the best fit flux of the host star for Fomalhaut itself. This implies that any inner debris component must contribute little to the total central emission. Moreover, the stellar flux is less than 70% of that predicted by extrapolating a blackbody from the constrained photosphere temperature and just over 70% of the flux if extrapolating from the far infrared. This behavior is similar to that seen in the Sun for submm/mm wavelengths, but even more pronounced. Currently, insufficient data exists to properly constrain the degree to which stellar atmospheres affect the observed flux in the submm/mm regime. This result is part of an ongoing larger project focused on measuring the emission from stellar atmospheres at submm/mm wavelengths, which directly impacts inferred excesses for debris disk studies.

  13. Espías entre el franquismo y la democracia: los informes confidenciales del Servicio Central de Documentación (SECED) entre 1974 y 1977

    OpenAIRE

    Villar Cirujano, Ernesto

    2015-01-01

    La Transición española es uno de los períodos de la historia de este país más profundamente estudiados. La presente tesis doctoral, ¿Espías entre el franquismo y la democracia: los informes confidenciales del Servicio Central de Documentación (SECED) entre 1974 y 1977¿ se acerca a este período desde un punto de vista no abordado hasta ahora: la información que manejaron los servicios secretos del Gobierno en el último año del Franquismo y los dos primeros de la Monarquía, hasta las elecciones...

  14. Resolving the extended atmosphere and the inner wind of Mira ($o$ Ceti) with long ALMA baselines

    CERN Document Server

    Wong, K T; Menten, K M; Wyrowski, F

    2016-01-01

    The prototypical Mira variable, $o$ Cet (Mira), has been observed as a Science Verification target in the 2014 ALMA Long Baseline Campaign with a longest baseline of 15 km. ALMA clearly resolves the images of the continuum and molecular line emission/absorption at an angular resolution of ~30 mas at 220 GHz. We image the data of the $^{28}$SiO v=0, 2 $J$=5-4 and H$_2$O $\

  15. Planet gaps in the dust layer of 3D proto-planetary disks: Observability with ALMA

    CERN Document Server

    Gonzalez, Jean-François; Maddison, Sarah T; Ménard, François

    2013-01-01

    Among the numerous known extrasolar planets, only a handful have been imaged directly so far, at large orbital radii and in rather evolved systems. The Atacama Large Millimeter/submillimeter Array (ALMA) will have the capacity to observe these wide planetary systems at a younger age, thus bringing a better understanding of the planet formation process. Here we explore the ability of ALMA to detect the gaps carved by planets on wide orbits.

  16. Supporting Student Learning in Computer Science Education via the Adaptive Learning Environment ALMA

    OpenAIRE

    Alexandra Gasparinatou; Maria Grigoriadou

    2015-01-01

    This study presents the ALMA environment (Adaptive Learning Models from texts and Activities). ALMA supports the processes of learning and assessment via: (1) texts differing in local and global cohesion for students with low, medium, and high background knowledge; (2) activities corresponding to different levels of comprehension which prompt the student to practically implement different text-reading strategies, with the recommended activity sequence adapted to the student’s learning style;...

  17. Software Development for ALMA in Chile: The ACS-UTFSM Group.

    Science.gov (United States)

    von Brand, H. H.

    ALMA Common Software (ACS) provides a common software framework for ALMA, the Atacama Large Millimeter Array in Chile. ACS is a collection of well-documented patterns for controlling systems and a set of components written to those patterns. In its core, ACS is a distributed, object-oriented system, written on top of CORBA. The ACS-UTFSM Group started as some students of informatics did summer jobs at the La Silla Observatory of ESO, where they became acquainted with ACS. Their interest led them to continue working on ACS on their own, and they eventually became official developers of the package. Now the group is being funded by project ALMA-CONICYT 31060008 ``Software Development for ALMA: Building Up Expertise to Meet ALMA Software Requirements within a Chilean University''. Several members of the original group are now working for ALMA, which fullfills one of the goals of the project. Some parts of ACS developed by the ACS-UTFSM Group include H3E (Hardware End-to-End Example), a Lego model of a telescope and its controlling software for training and demonstration purposes; and CDBChecker, a tool to verify the consistency of the configuration database for a ACS deployment. Currently we are working towards a general framework for telescope control using ACS, in order to simplify the deployment of new instruments; and repackaging ACS so it is easier to install and use. A master's thesis is exploring the real-time requirements of ACS.

  18. Aplicación de la teoría general de sistemas al análisis de los sistemas informáticos

    OpenAIRE

    Zubenko, Yuriy; Cataldi, Zulma; Lage, Fernando Javier

    2001-01-01

    Utilizando la metodología del análisis de sistemas y la teoría general de sistemas se pueden resolver tres tareas pertinentes a los sistemas informáticos en estadíos diferentes: el análisis de sistema de computación (en forma estática), el análisis de los sistemas de programación (en estática y dinámica) y el pronóstico de la evolución de los sistemas de computación (evolución cíclica). Para ello, se usa el esquema o modelo general del sistema informático para representar cada tarea del siste...

  19. Métricas de riesgos para los proyectos productivos de la Universidad de las Ciencias Informáticas. Risk Metrics for the Productive Projects at the University of Informatics Sciences

    OpenAIRE

    Neysis Hernández Díaz; Betsy Cuza García; Rachel Rachel Seijó

    2012-01-01

    En el presente trabajo se proponen métricas para disminuir el impacto negativo de los riesgos en los proyectos productivos de la Universidad de las Ciencias Informáticas, basado en el modelo CMMI. Las métricas pueden medir el avance del proyecto, así como contribuir a la prevención de los riesgos y en caso de ocurrir un riesgo, permite a los líderes tomar decisiones correctas ante los problemas presentados. Múltiples factores influyen en el desarrollo de software con calidad: los recursos hum...

  20. Informe final. Monitoreo complementario de las mareas rojas en las regiones de los Lagos, Aysén y Magallanes

    OpenAIRE

    Guzmán Méndez, F. L.; Vidal Santana, G.; Pizarro Nova, G.M.; Vivanco Tapia, X.; Iriarte Bustamante, L.; Alarcón Zapata, C.H.; Arenas Sepúlveda, V.; Mercado Leal, S.I.; Pacheco Valles, H.; Mejías Wagner, P.; Palma Alarcón, M.; Niño Azócar, E.; Monsalve Montecinos, J.; Espinoza Alvarado, C.; Zamora Amstein, C.V.

    2012-01-01

    Se presentan las bases de datos de los monitoreos de fitoplancton cualitativo y cuantitativo, incluyendo estimadores de abundancia relativa de siete taxones nocivos, además de resultados de los bioensayos para evaluar la presencia y/o concentración en mariscos de veneno paralizante y veneno diarreico, y estimaciones de veneno amnésico mediante cromatografía líquida. Asimismo, se entregan los datos oceanográficos y meteorológicos recogidos de cada uno de los sitios de muestreo, incluyendo el r...

  1. EL INFORME SOCIAL EN LOS PROCESOS DE INCLUSIÓN: ANÁLISIS DE LA REALIDAD SOCIAL DE UNA PERSONA SIN HOGAR

    OpenAIRE

    Castillo-Sánchez, María José

    2015-01-01

    El Informe Social en los Procesos de Inclusión: Análisis de la Realidad Social de una Persona sin Hogar.Centro de Orientación e Intervención Social (COIS). Negociado de Personas Sin Hogar. Ayuntamiento de Sevilla

  2. Políticas de austeridad y cambios en las pautas de uso de los servicios sanitarios. Informe SESPAS 2014

    Directory of Open Access Journals (Sweden)

    Rosa Urbanos Garrido

    2014-06-01

    Full Text Available Se analizan los principales cambios en los patrones de utilización sanitaria que se están produciendo en España como consecuencia de la crisis y de las medidas adoptadas frente a ella. Se examina el impacto de la reforma en el diseño del copago farmacéutico, que ofrece como resultado una importante reducción en el número de recetas dispensadas en las oficinas de farmacia, si bien sus efectos sobre la adherencia al tratamiento, el acceso a tratamientos necesarios y efectivos, y en última instancia la salud, aún se desconocen. Asimismo, el artículo constata que en los años más recientes de la crisis se han producido aumentos en los tiempos y listas de espera de intervenciones quirúrgicas, y en la insatisfacción que los ciudadanos muestran hacia la sanidad pública. Del análisis de los datos de las Encuestas Nacionales de Salud 2006 y 2011/12 se concluye que, en lo que respecta a los servicios no cubiertos –en particular las visitas al dentista–, la crisis está teniendo un efecto disuasorio en la utilización sanitaria de las capas sociales más desfavorecidas. Se recomienda definir mejor el papel que deben tener las aportaciones de los usuarios dentro del ámbito del Sistema Nacional de Salud, y prestar atención y medios a quienes más lo necesitan, para evitar que los colectivos con mejor situación socioeconómica capturen los servicios que quedan disponibles tras los recortes de fondos públicos.

  3. Solar Observations with the Atacama Large Millimeter/submillimeter Array (ALMA)

    Science.gov (United States)

    Bastian, Timothy S.

    2015-04-01

    The Atacama Large Millimeter/Submillimeter Array (ALMA) is a joint North American, European, and East Asian project that opens the mm-submm wavelength part of the electromagnetic spectrum for general astrophysical exploration, providing high-resolution imaging in frequency bands currently ranging from 84 GHz to 950 GHz (300 microns to 3 mm). Despite being a general purpose instrument, provisions have been made to enable solar observations with ALMA. Radiation emitted at ALMA wavelengths originates mostly from the chromosphere, which plays an important role in the transport of matter and energy, and the in heating the outer layers of the solar atmosphere. Despite decades of research, the solar chromosphere remains a significant challenge: both to observe, owing to the complicated formation mechanisms of currently available diagnostics; and to understand, as a result of the complex nature of the structure and dynamics of the chromosphere. ALMA has the potential to change the scene substantially as it serves as a nearly linear thermometer at high spatial and temporal resolution, enabling us to study the complex interaction of magnetic fields and shock waves and yet-to-be-discovered dynamical processes. Moreover, ALMA will play an important role in the study of energetic emissions associated with solar flares at sub-THz frequencies.In this paper we describe recent efforts to ensure that ALMA can be usefully exploited by the scientific community to address outstanding questions in solar physics. We summarize activities by the ALMA solar development team comprised of scientists from the East Asia, North America, and Europe. These activities include instrument testing, development of calibration and imaging strategies, software requirements development, and science simulations. Opportunities for the wider community to contribute to these efforts will be highlighted.

  4. Utilización de los recursos informáticos en la asignatura Fronteras de la Innovación Tecnológica

    OpenAIRE

    Gordaliza Escobar, Marina

    2010-01-01

    Se han conseguido y utilizado las herramientas informáticas relacionadas con este tema, englobadas en un entorno virtual, que permite a los estudiantes de las asignaturas incluídas en el proyecto, obtener la información más actual y realizar prácticas o seminarios de búsqueda o cálculo de parámetros y propiedades, realizar medidas y ejecutar modificaciones para conocer las características de los fármacos y aplicarlas en el diseño de otros nuevos. El empleo de estas herramienta ha facilitado l...

  5. Informe sobre la Situación Patológica de los Cacaotales en los Departamentos de Valle y Cauca.

    Directory of Open Access Journals (Sweden)

    Garcés O. Carlos

    1941-06-01

    Full Text Available Tengo a honor informar al señor Ministro de Economía Nacional sobre el resultado de la Comisión que se me confirió para estudiar las enfermedades del cacao en los Departamentos del Valle y del Cauca. Es natural que por el relativo corto tiempo de que dispuse, el reconocimiento de las enfermedades dichas no sea completo, pero sí es base para algunas importantes observaciones que espero sirvan para dar a conocer en parte la lamentable situación en que se encuentra un cultivo que debe ser todo un programa del desarrollo agrícola del país.

  6. Clasificación del Contenido de los Informes de Sostenibilidad de Empresas Premiadas por sus Prácticas de Responsabilidad Socioambiental

    Directory of Open Access Journals (Sweden)

    Magdalena Inglês da Costa

    2013-06-01

    Full Text Available Dada la importancia del informe de sostenibilidad – instrumento de gestión y de divulgación de informaciones acerca de la interacción de la empresa con el medio en que actúa –, el presente estudio tiene por objetivo analizar el contenido de la divulgación de informaciones acerca de las dimensiones de la sostenibilidad empresarial – económica, social y ambiental – en los informes de empresas premiadas por sus prácticas de responsabilidad socioambiental. Se trata de estudio descriptivo, de naturaleza cualitativa, haciendo uso de la pesquisa documental y del Análisis de Contenido. Los resultados apuntan la preponderancia de la dimensión social, especialmente de ámbito externo, y del disclosure cuantitativo no-monetario. Sugieren asimismo el efecto de la actividad en el medio ambiente y la estructura de propiedad del capital como factores indicativos de los niveles de evidenciación en los informes de sostenibilidad de las empresas pesquisadas, de entre aquellas premiadas por sus prácticas de responsabilidad socioambiental.

  7. ALMA reveals a chemically evolved submillimeter galaxy at z=4.76

    CERN Document Server

    Nagao, Tohru; De Breuck, Carlos; Caselli, Paola; Hatsukade, Bunyo; Saigo, Kazuya

    2012-01-01

    The chemical properties of high-z galaxies provide important information to constrain galaxy evolutionary scenarios. However, widely-used metallicity diagnostics based on rest-frame optical emission lines are not usable for heavily dust-enshrouded galaxies (such as Sub-Millimeter Galaxies; SMGs), especially at z>3. Here we focus on the flux ratio of the far-infrared fine-structure emission lines [NII]205um and [CII]158um to assess the metallicity of high-z SMGs. Through ALMA cycle 0 observations, we have detected the [NII]205um emission in a strongly [CII]-emitting SMG, LESS J033229.4-275619 at z=4.76. The velocity-integrated [NII]/[CII] flux ratio is 0.043 +/- 0.008. This is the first measurement of the [NII]/[CII] flux ratio in high-z galaxies, and the inferred flux ratio is similar to the ratio observed in the nearby universe (~0.02-0.07). The velocity-integrated flux ratio and photoionization models suggest that the metallicity in this SMG is consistent with solar, implying the chemical evolution has prog...

  8. GRB 110715A: The peculiar multiwavelength evolution of the first afterglow detected by ALMA

    CERN Document Server

    Sánchez-Ramírez, R; Jóhannesson, G; Murphy, Tara; Postigo, A de Ugarte; Gorosabel, J; Kann, D A; Krühler, T; Oates, S R; Japelj, J; Thöne, C C; Lundgren, A; Perley, D A; Malesani, D; Monsalvo, I de Gregorio; Castro-Tirado, A J; D'Elia, V; Fynbo, J P U; Garcia-Appadoo, D; Goldoni, P; Greiner, J; Hu, Y -D; Jelínek, M; Jeong, S; Kamble, A; Klose, S; Kuin, N P M; Llorente, A; Martín, S; Guelbenzu, A Nicuesa; Rossi, A; Schady, P; Sparre, M; Sudilovsky, V; Tello, J C; Updike, A; Wiersema, K; Zhang, B -B

    2016-01-01

    We present the extensive follow-up campaign on the afterglow of GRB 110715A at 17 different wavelengths, from X-ray to radio bands, starting 81 seconds after the burst and extending up to 74 days later. We performed for the first time a GRB afterglow observation with the ALMA observatory. We find that the afterglow of GRB 110715A is very bright at optical and radio wavelengths. We use optical and near infrared spectroscopy to provide further information about the progenitor's environment and its host galaxy. The spectrum shows weak absorption features at a redshift $z$ = 0.8225, which reveal a host galaxy environment with low ionization, column density and dynamical activity. Late deep imaging shows a very faint galaxy, consistent with the spectroscopic results. The broadband afterglow emission is modelled with synchrotron radiation using a numerical algorithm and we determine the best fit parameters using Bayesian inference in order to constrain the physical parameters of the jet and the medium in which the ...

  9. The Mysterious Morphology of MRC0943-242 as Revealed by ALMA and MUSE

    CERN Document Server

    Gullberg, Bitten; Lehnert, Matthew D; Vernet, Joel; Bacon, Roland; Drouart, Guillaume; Emonts, Bjorn; Galametz, Audrey; Ivison, Rob; Nesvadba, Nicole P H; Richard, Johan; Seymour, Nick; Stern, Daniel; Wylezalek, Dominika

    2015-01-01

    We present a pilot study of the z=2.923 radio galaxy MRC0943-242, where we for the first time combine information from ALMA and MUSE data cubes. Even with modest integration times, we disentangle an AGN and a starburst dominated set of components. These data reveal a highly complex morphology, as the AGN, starburst, and molecular gas components show up as widely separated sources in dust continuum, optical continuum and CO line emission observations. CO(1-0) and CO(8-7) line emission suggest that there is a molecular gas reservoir offset from both the dust and the optical continuum that is located ~90kpc from the AGN. The UV line emission has a complex structure in emission and absorption. The line emission is mostly due to i) a large scale ionisation cone energised by the AGN, ii) a Ly-alpha emitting bridge of gas between the radio galaxy and a heavily star-forming set of components. Strangely, the ionisation cone has no Ly-alpha emission. We find this is due to an optically thick layer of neutral gas with u...

  10. Health for All Now! Reviving the spirit of Alma Ata in the Twenty-first century: An Introduction to the Alma Ata Declaration

    Directory of Open Access Journals (Sweden)

    Fran Baum

    2007-01-01

    Full Text Available Abstract In 1978 two United Nations organizations, the World Health Organization and UNICEF, held a joint conference at Alma Ata in the Soviet Union at which health was described as a human right to which all people were entitled. The goal of achieving health for all by the end of the century was established. The Alma Ata Declaration on Primary Health Care emerged from this conference. It was endorsed on the 12th September 1978, and has inspired subsequent generations of health activists. It has become a common meeting ground where likeminded public health personnel can compare and discuss strategy and relate their discussion to a common document. The slogan “Health for All by the Year 2000”, while not achieved, has been a rallying call for progressive health workers and activists. The Declaration has also inspired the global people’s health movement and two global people’s health assemblies. The concept “primary health care” has been crucial to the improvement of many countries’ health systems and, while its meaning has been variously interpreted, the pursuit of the ideal of comprehensive primary health care still motivates health workers around the world who want to ensure a more people-centred, responsive and effective and efficient health care system for their community and country. Thus the Alma Ata Declaration is a quite remarkable document and has made an impact that few other before or since have had. This article describes the international context that enabled the drafting and adoption of the Alma Ata Declaration. It then describes the document and assesses the reasons for its importance. The struggles for the ideals and strategies of the Declaration through the progressively more hostile international climate of the 1980s and 1990s are discussed. Finally, the prospects for a revival of the spirit of Alma Ata are assessed.

  11. Información sobre las secuelas y futuros riesgos para los sobrevivientes de retinoblastoma Information on late effects and future risks for retinoblastoma survivors

    Directory of Open Access Journals (Sweden)

    Laura Schwartz

    2005-04-01

    Full Text Available Los índices de sobrevida de los pacientes con cáncer en la infancia han aumentado en las últimas décadas. Se observan secuelas como consecuencia de esta enfermedad y su tratamiento. Los sobrevivientes de retinoblastoma presentan efectos adversos como consecuencia de la cirugía, la radioterapia y la quimioterapia. Las formas bilaterales irradiadas presentan un riesgo aumentado de desarrollar un segundo cáncer. Tanto los casos que presentaron retinoblastoma unilateral o bilateral pueden transmitir esta enfermedad a su descendencia. El diagnóstico de este tumor es excepcional después de los 4 años de edad y no se sabe claramente qué conocimiento tienen estos sobrevivientes del diagnóstico, del tratamiento y de los futuros riesgos. El consentimiento informado y el posterior resumen de historia clínica no aclaran demasiado a los padres. Los pacientes curados de retinoblastoma se verían beneficiados con un seguimiento prolongado en las instituciones en que fueron tratados, ya que les permitiría recibir información acerca de lo padecido, del tratamiento, de los riesgos y se podrían identificar las consecuencias posteriores de la enfermedad y su tratamiento.The survival rates of childhood cancer have increased in the past few decades. Late consequences related to the cancer and the treatment are observed. The late effects in retinoblastoma survivors are related to the surgery, the radiotherapy and the chemotherapy. Patients with irradiated bilateral retinoblastoma are at high risk to develop a second cancer. Survivors of bilateral or unilateral forms could transmit this disease to their offspring. The diagnosis of retinoblastoma is exceptional after 4 years of age, and it is not clear whether these survivors have knowledge of their diagnosis, treatment and future risks. The informed consent and the summary of the clinical histories do not help to clarify the situation. It will be of great benefit for the patients cured of retinoblastoma

  12. Resolving the Planetesimal Belt of HR 8799 with ALMA

    CERN Document Server

    Booth, Mark; Casassus, Simon; Hales, Antonio S; Dent, William R F; Faramaz, Virginie; Matrà, Luca; Barkats, Denis; Brahm, Rafael; Cuadra, Jorge

    2016-01-01

    The star HR 8799 hosts one of the largest known debris discs and at least four giant planets. Previous observations have found evidence for a warm belt within the orbits of the planets, a cold planetesimal belt beyond their orbits and a halo of small grains. With the infrared data, it is hard to distinguish the planetesimal belt emission from that of the grains in the halo. With this in mind, the system has been observed with ALMA in band 6 (1.34 mm) using a compact array format. These observations allow the inner edge of the planetesimal belt to be resolved for the first time. A radial distribution of dust grains is fitted to the data using an MCMC method. The disc is best fit by a broad ring between $145^{+12}_{-12}$ AU and $429^{+37}_{-32}$ AU at an inclination of $40^{+5}_{-6}${\\deg} and a position angle of $51^{+8}_{-8}${\\deg}. A disc edge at ~145 AU is too far out to be explained simply by interactions with planet b, requiring either a more complicated dynamical history or an extra planet beyond the orb...

  13. Water around IRAS15398-3359 observed with ALMA

    CERN Document Server

    Bjerkeli, P; Bergin, E A; Frimann, S; Harsono, D; Jacobsen, S K; Lindberg, J E; Persson, M; Sakai, N; van Dishoeck, E F; Visser, R; Yamamoto, S

    2016-01-01

    How protostars accrete mass is one of the fundamental problems of star formation. High column densities and complex kinematical structures make direct observations challenging and they only provide a snapshot. Chemical tracers provide an interesting alternative to characterise the infall histories of protostars. Previous observations of H13CO+ towards the low-mass protostar IRAS15398-3359 showed a depression in the abundance. This is a sign of destruction of HCO+ by an enhanced presence of gaseous water in an extended region, possibly related to a recent burst in the accretion. Direct observations of water vapour can determine the exact extent of the emission and confirm the hypothesis that HCO+ is indeed a good tracer of the water snow-line. IRAS15398 was observed using ALMA at 0.5" resolution. Maps of HDO(101-000) and H218O(414-321) were taken simultaneously with observations of the CS(8-7) and N2H+(5-4) lines and continuum at 0.65 and 0.75 mm. The maps were interpreted using dust radiative transfer calcula...

  14. The 492 GHz emission of Sgr A* constrained by ALMA

    CERN Document Server

    Liu, Hauyu Baobab; Zhao, Jun-Hui; Mills, Elisabeth A C; Requena-Torres, Miguel A; Matsushita, Satoki; Martín, Sergio; Ott, Jürgen; Morris, Mark R; Longmore, Steven N; Brinkerink, Christiaan D; Falcke, Heino

    2016-01-01

    We report linearly polarized continuum emission properties of Sgr A* at $\\sim$492 GHz, based on the Atacama Large Millimeter Array (ALMA) observations. We used the observations of the likely unpolarized continuum emission of Titan, and the observations of C\\textsc{i} line emission, to gauge the degree of spurious polarization. The Stokes I flux of 3.6$\\pm$0.72 Jy during our run is consistent with extrapolations from the previous, lower frequency observations. We found that the continuum emission of Sgr A* at $\\sim$492 GHz shows large amplitude differences between the XX and the YY correlations. The observed intensity ratio between the XX and YY correlations as a function of parallactic angle may be explained by a constant polarization position angle of $\\sim$158$^{\\circ}$$\\pm$3$^{\\circ}$. The fitted polarization percentage of Sgr A* during our observational period is 14\\%$\\pm$1.2\\%. The calibrator quasar J1744-3116 we observed at the same night can be fitted to Stokes I = 252 mJy, with 7.9\\%$\\pm$0.9\\% polariz...

  15. Resolving the planetesimal belt of HR 8799 with ALMA

    Science.gov (United States)

    Booth, Mark; Jordán, Andrés; Casassus, Simon; Hales, Antonio S.; Dent, William R. F.; Faramaz, Virginie; Matrà, Luca; Barkats, Denis; Brahm, Rafael; Cuadra, Jorge

    2016-07-01

    The star HR 8799 hosts one of the largest known debris discs and at least four giant planets. Previous observations have found evidence for a warm belt within the orbits of the planets, a cold planetesimal belt beyond their orbits and a halo of small grains. With the infrared data, it is hard to distinguish the planetesimal belt emission from that of the grains in the halo. With this in mind, the system has been observed with ALMA in band 6 (1.34 mm) using a compact array format. These observations allow the inner edge of the planetesimal belt to be resolved for the first time. A radial distribution of dust grains is fitted to the data using an MCMC method. The disc is best fitted by a broad ring between 145^{+12}_{-12} au and 429^{+37}_{-32} au at an inclination of 40^{+5}_{-6}° and a position angle of 51^{+8}_{-8}°. A disc edge at ˜145 au is too far out to be explained simply by interactions with planet b, requiring either a more complicated dynamical history or an extra planet beyond the orbit of planet b.

  16. A code generation framework for the ALMA common software

    Science.gov (United States)

    Troncoso, Nicolás; von Brand, Horst H.; Ibsen, Jorge; Mora, Matias; Gonzalez, Victor; Chiozzi, Gianluca; Jeram, Bogdan; Sommer, Heiko; Zamora, Gabriel; Tejeda, Alexis

    2010-07-01

    Code generation helps in smoothing the learning curve of a complex application framework and in reducing the number of Lines Of Code (LOC) that a developer needs to craft. The ALMA Common Software (ACS) has adopted code generation in specific areas, but we are now exploiting the more comprehensive approach of Model Driven code generation to transform directly an UML Model into a full implementation in the ACS framework. This approach makes it easier for newcomers to grasp the principles of the framework. Moreover, a lower handcrafted LOC reduces the error rate. Additional benefits achieved by model driven code generation are: software reuse, implicit application of design patterns and automatic tests generation. A model driven approach to design makes it also possible using the same model with different frameworks, by generating for different targets. The generation framework presented in this paper uses openArchitectureWare1 as the model to text translator. OpenArchitectureWare provides a powerful functional language that makes this easier to implement the correct mapping of data types, the main difficulty encountered in the translation process. The output is an ACS application readily usable by the developer, including the necessary deployment configuration, thus minimizing any configuration burden during testing. The specific application code is implemented by extending generated classes. Therefore, generated and manually crafted code are kept apart, simplifying the code generation process and aiding the developers by keeping a clean logical separation between the two. Our first results show that code generation improves dramatically the code productivity.

  17. Further ALMA observations and detailed modeling of the Red Rectangle

    CERN Document Server

    Bujarrabal, V; Alcolea, J; Santander-Garcia, M; Van Winckel, H; Contreras, C Sanchez

    2016-01-01

    We present new high-quality ALMA observations of the Red Rectangle (a well known post-AGB object) in C17O J=6-5 and H13CN J=4-3 line emission and results from a new reduction of already published 13CO J=3-2 data. A detailed model fitting of all the molecular line data, including previous maps and single-dish spectra, was performed using a sophisticated code. These observations and the corresponding modeling allowed us to deepen the analysis of the nebular properties. We also stress the uncertainties in the model fitting. We confirm the presence of a rotating equatorial disk and an outflow, which is mainly formed of gas leaving the disk. The mass of the disk is ~ 0.01 Mo, and that of the CO-rich outflow is ~ 10 times smaller. High temperatures of ~ 100 K are derived for most components. From comparison of the mass values, we roughly estimate the lifetime of the rotating disk, which is found to be of about 10000 yr. Taking data of a few other post-AGB composite nebulae into account, we find that the lifetimes o...

  18. The Early ALMA View of the FU Ori Outburst System

    CERN Document Server

    Hales, A S; Dent, W R D; Andrews, S M; Eisner, J A; Cieza, L A

    2015-01-01

    We have obtained ALMA Band 7 observations of the FU Ori outburst system at 0.6"x0.5" resolution to measure the link between the inner disk instability and the outer disk through sub-mm continuum and molecular line observations. Our observations detect continuum emission which can be well modeled by two unresolved sources located at the position of each binary component. The interferometric observations recover the entire flux reported in previous single-dish studies, ruling out the presence of a large envelope. Assuming that the dust is optically thin, we derive disk dust masses of $2\\times 10^{-4}$M$_{\\odot}$ and $8\\times 10^{-5}$M$_{\\odot}$, for the north and south components respectively. We place limits on the disks' radii of $r<$45 AU. We report the detection of molecular emission from $^{12}$CO(3-2), HCO$^{+}$(4-3) and from HCN(4-3). The $^{12}$CO appears widespread across the two binary components, and is slightly more extended than the continuum emission. The denser gas tracer HCO$^{+}$ peaks close...

  19. Measuring Turbulence in TW Hya with ALMA: Methods and Limitations

    CERN Document Server

    Teague, Richard; Semenov, Dmitry; Henning, Thomas; Dutrey, Anne; Pietu, Vincent; Birnstiel, Tilman; Chapillon, Edwige; Hollenbach, David; Gorti, Uma

    2016-01-01

    We obtain high spatial and spectral resolution images of the CO J=2-1, CN N=2-1 and CS J=5-4 emission with ALMA in Cycle~2. The radial distribution of the turbulent broadening is derived with three approaches: two `direct' and one modelling. The first requires a single transition and derives \\Tex{} directly from the line profile, yielding a \\vturb{}. The second assumes two different molecules are co-spatial thus their relative linewidths allow for a calculation of \\Tkin{} and \\vturb{}. Finally we fit a parametric disk model where physical properties of the disk are described by power laws, to compare our `direct' methods with previous values. The two direct methods were limited to the outer $r > 40$~au disk due to beam smear. The direct method found \\vturb{} ranging from $\\approx$~\\vel{130} at 40~au, dropping to $\\approx$~\\vel{50} in the outer disk, qualitatively recovered with the parametric model fitting. This corresponds to roughly $0.2 - 0.4~c_s$. CN was found to exhibit strong non-LTE effects outside $r ...

  20. A sensitive ALMA Band 10 SIS receiver engineering model

    International Nuclear Information System (INIS)

    We have developed a single polarization engineering model of the Atacama Large Millimeter/Submillimeter Array (ALMA) Band 10 (0.78-0.95 THz) receivers. The front-end optics comprises a pair of ellipsoidal mirrors and a corrugated feed horn. A waveguide mixer block is attached to the feed horn in which an NbTiN-based superconductor-insulator-superconductor (SIS) mixer chip, which uses a quartz substrate, is mounted onto a WR-1.2 full-height waveguide. The SIS mixer employs two Nb/AlOx/Nb junctions and an NbTiN/SiO2/Al microstrip tuning circuit. A very wide intermediate frequency (IF) system with a bandwidth of 4-12 GHz is employed. The receiver demonstrated double-sideband (DSB) noise temperatures of below 240 K at local oscillator (LO) frequencies ranging from 792 to 945 GHz, without any correction for loss in front of the receiver. The lowest DSB receiver noise temperature, 179 K, was obtained at the center frequency of the designed band, which corresponds to about 4 quanta. These results represent state-of-the-art sensitivity for a receiver at an operating physical temperature of 4 K.

  1. Evidence for outflows in z ~ 6 galaxies with ALMA

    CERN Document Server

    Gallerani, S; Feruglio, C; Ferrara, A; Maiolino, R; Vallini, L; Riechers, D A

    2016-01-01

    We present the first attempt to detect outflows from galaxies approaching the Epoch of Reionization (EoR) using a sample of 9 star-forming (5 < SFR < 70 Msun/yr) z ~ 6 galaxies for which high-quality spectra of the [CII]158 micron line has been previously obtained with ALMA. We first fit each line with a Gaussian function and compute the residuals by subtracting the best fitting model from the data. We combine the residuals of all sample galaxies and find that the total signal is characterized by a flux excess that can be ascribed to broad wings of the [CII] line, which we interpret as a signature of starburst-driven outflows. The tentatively inferred outflow rate is dM/dt ~ 65 Msun/yr. Our interpretation is consistent with results from zoomed hydro- simulations of Dahlia, a z ~ 7 galaxy (SFR ~ 100 Msun/yr) whose feedback-regulated star formation results in an outflow rate dM/dt ~ 30 Msun/yr. These results suggest that starburst-driven outflows are in place in the EoR. Deeper observations of the [CII] l...

  2. ALMA Observations of HCN and its Isotopologues on Titan

    CERN Document Server

    Molter, Edward M; Cordiner, Martin A; Serigano, Joseph; Irwin, Patrick G J; Teanby, Nicholas A; Charnley, Steven B; Lindberg, Johan E

    2016-01-01

    We present sub-millimeter spectra of HCN isotopologues on Titan, derived from publicly available ALMA flux calibration observations of Titan taken in early 2014. We report the detection of a new HCN isotopologue on Titan, H$^{13}$C$^{15}$, and confirm an earlier report of detection of DCN. We model high signal-to-noise observations of HCN, H$^{13}$CN, HC$^{15}$N, DCN, and H$^{13}$C$^{15}$ to derive abundances and infer the following isotopic ratios: $^{12}$C/$^{13}$C = 89.8 $\\pm$ 2.8, $^{14}$N/$^{15}$N = 72.3 $\\pm$ 2.2, D/H = (2.5 $\\pm$ 0.2)$\\times$10$^{-4}$, and HCN/H$^{13}$C$^{15}$ = 5800 $\\pm$ 270 (1$\\sigma$ errors). The carbon and nitrogen ratios are consistent with and improve on the precision of previous results, confirming a factor of $\\sim$2.3 elevation in $^{14}$N/$^{15}$N in HCN compared to N$_2$ and a lack of fractionation in $^{12}$C/$^{13}$C from the protosolar value. This is the first published measurement of D/H in a nitrile species on Titan, and we find evidence for a factor of $\\sim$2 deuteri...

  3. Detection of CO and HCN in Pluto's atmosphere with ALMA

    CERN Document Server

    Lellouch, E; Butler, B; Fouchet, T; Lavvas, P; Strobel, D F; Sicardy, B; Moullet, A; Moreno, R; Bockelée-Morvan, D; Biver, N; Young, L; Lis, D; Stansberry, J; Stern, A; Weaver, H; Young, E; Zhu, X; Boissier, J

    2016-01-01

    Observations of the Pluto-Charon system, acquired with the ALMA interferometer on June 12-13, 2015, have yielded a detection of the CO(3-2) and HCN(4-3) rotational transitions from Pluto, providing a strong confirmation of the presence of CO, and the first observation of HCN, in Pluto's atmosphere. The CO and HCN lines probe Pluto's atmosphere up to ~450 km and ~900 km altitude, respectively. The CO detection yields (i) a much improved determination of the CO mole fraction, as 515+/-40 ppm for a 12 ubar surface pressure (ii) clear evidence for a well-marked temperature decrease (i.e., mesosphere) above the 30-50 km stratopause and a best-determined temperature of 70+/-2 K at 300 km, in agreement with recent inferences from New Horizons / Alice solar occultation data. The HCN line shape implies a high abundance of this species in the upper atmosphere, with a mole fraction >1.5x10-5 above 450 km and a value of 4x10-5 near 800 km. The large HCN abundance and the cold upper atmosphere imply supersaturation of HCN...

  4. ALMA - The March to Early Science and Beyond

    Science.gov (United States)

    Wootten, Alwyn

    2011-01-01

    The Atacama Large Millimeter/submillimeter Array is rapidly proceeding through its commissioning stages in Chile. Tests at the atmospherically superb 5050m Array Operations Site and readiness reviews held during the Fall of 2010 will result in a decision to issue a call for proposals to use the instrument during its 'Early Science' phase. At the beginning of Early Science, projected for later in 2011, 16 antennas of the final 66 will stand ready to produce the deepest integrations ever achieved in the cool thermal spectral region. The array will be equipped with at least three of its eventual complement of ten receivers operating over a decade of bandwidth from 3.6mm to 0.42mm. At this point, its sensitivity will be on the order of 0.5mJy in a minute's integration. Operating at this stage baselines of at least .25km, ALMA will provide a beam as small as 0".3 on the little-explored southern skies from its Chilean site near the Tropic of Capricorn. By one year later, the array will have grown to more than fifty antennas; at the second call for proposals the array will reach 0.2 mJy in a minute and baselines will extend to the full set of array configurations, effectively about 14 km. Observations which will be made possible by these transformative capabilities will be presented.

  5. ALMA: The March to Early Science and Beyond

    Science.gov (United States)

    Wootten, Al

    2010-05-01

    The Atacama Large Millimeter/submillimeter Array is rapidly proceeding through its commissioning stages in Chile. Within a short time, equipment from all over the world will be installed at the 5050m altitude Array Operations Site and a call will go out for proposals to use the instrument during its 'Early Science' phase. At the beginning of Early Science, a little over a year from now, 16 antennas of the final 66 will stand ready to produce the deepest images ever achieved in the cool thermal spectral region. The array will be equipped with at least three of its eventual complement of ten receivers; even now operating over a decade of bandwidth from 3.6mm to 0.42mm. At this point, its sensitivity will be on the order of 0.5mJy in a minute's integration. Operating at this stage baselines of at least .25km, ALMA will provide a beam as small as 0".3 on the little-explored southern skies from its Chilean site near the Tropic of Capricorn. By one year later, the array will have grown to more than fifty antennas; at the second call for proposals the array will reach 0.2 mJy in a minute and baselines will extend to the full set of array configurations, effectively about 14 km. Illustrative examples of observations which will be made possible by these transformative capabilities will be presented.

  6. Fast single-dish scans of the Sun using ALMA

    CERN Document Server

    Phillips, Neil; Bastian, Tim; Hudson, Hugh; Marson, Ralph; Wedemeyer, Sven

    2015-01-01

    We have implemented control and data-taking software that makes it possible to scan the beams of individual ALMA antennas to perform quite complex patterns while recording the signals at high rates. We conducted test observations of the Sun in September and December, 2014. The data returned have excellent quality; in particular they allow us to characterize the noise and signal fluctuations present in this kind of observation. The fast-scan experiments included both Lissajous patterns covering rectangular areas, and double-circle patterns of the whole disk of the Sun and smaller repeated maps of specific disk-shaped targets. With the latter we find that we can achieve roughly Nyquist sampling of the Band~6 (230~GHz) beam in 60~s over a region 300$"$ in diameter. These maps show a peak-to-peak brightness-temperature range of up to 1000~K, while the time-series variability at any given point appears to be of order 0.5 percent RMS over times of a few minutes. We thus expect to be able to separate the noise contr...

  7. New architectures support for ALMA common software: lessons learned

    Science.gov (United States)

    Menay, Camilo E.; Zamora, Gabriel A.; Tobar, Rodrigo J.; Avarias, Jorge A.; Dahl-skog, Kevin R.; von Brand, Horst H.; Chiozzi, Gianluca

    2010-07-01

    ALMA Common Software (ACS) is a distributed control framework based on CORBA that provides communication between distributed pieces of software. Because of its size and complexity it provides its own compilation system, a mix of several technologies. The current ACS compilation process depends on specific tools, compilers, code generation, and a strict dependency model induced by the large number of software components. This document presents a summary of several porting and compatibility attempts at using ACS on platforms other than the officially supported one. A porting of ACS to the Microsoft Windows Platform and to the ARM processor architecture were attempted, with different grades of success. Also, support for LINUX-PREEMPT (a set of real-time patches for the Linux kernel) using a new design for real-time services was implemented. These efforts were integrated with the ACS building and compilation system, while others were included in its design. Lessons learned in this process are presented, and a general approach is extracted from them.

  8. Ethyl cyanide on Titan: Spectroscopic detection and mapping using ALMA

    CERN Document Server

    Cordiner, M A; Nixon, C A; Irwin, P G J; Teanby, N A; Charnley, S B; Mumma, M J; Kisiel, Z; Serigano, J; Kuan, Y -J; Chuang, Y -L; Wang, K -S

    2014-01-01

    We report the first spectroscopic detection of ethyl cyanide (C$_2$H$_5$CN) in Titan's atmosphere, obtained using spectrally and spatially resolved observations of multiple emission lines with the Atacama Large Millimeter/submillimeter array (ALMA). The presence of C$_2$H$_5$CN in Titan's ionosphere was previously inferred from Cassini ion mass spectrometry measurements of C$_2$H$_5$CNH$^+$. Here we report the detection of 27 rotational lines from C$_2$H$_5$CN (in 19 separate emission features detected at $>3\\sigma$ confidence), in the frequency range 222-241 GHz. Simultaneous detections of multiple emission lines from HC$_3$N, CH$_3$CN and CH$_3$CCH were also obtained. In contrast to HC$_3$N, CH$_3$CN and CH$_3$CCH, which peak in Titan's northern (spring) hemisphere, the emission from C$_2$H$_5$CN is found to be concentrated in the southern (autumn) hemisphere, suggesting a distinctly different chemistry for this species, consistent with a relatively short chemical lifetime for C$_2$H$_5$CN. Radiative transf...

  9. ALMA Resolves the Nuclear Disks of Arp 220

    CERN Document Server

    Scoville, Nick; Walter, Fabian; Vlahakis, Catherine; Koda, Jin; Bout, Paul Vanden; Barnes, Joshua; Hernquist, Lars; Sheth, Kartik; Yun, Min; Sanders, David; Armus, Lee; Cox, Pierre; Thompson, Todd; Robertson, Brant; Zschaechner, Laura; Tacconi, Linda; Torrey, Paul; Hayward, Christopher C; Genzel, Reinhard; Hopkins, Phil; van der Werf, Paul; Decarli, Roberto

    2016-01-01

    We present 90 mas (37 pc) resolution ALMA imaging of Arp 220 in the CO (1-0) line and continuum at $\\lambda = 2.6$ mm. The internal gas distribution and kinematics of both galactic nuclei are well-resolved for the first time.In the more luminous West nucleus, the major gas and dust emission extends to 0.2\\arcsec radius (80 pc); the central resolution element shows a strong peak in the dust emission but a factor 3 dip in the CO line emission. In this nucleus, the dust is apparently optically thick ($\\tau_{\\rm 2.6mm} \\sim1$) at $\\lambda = 2.6$ mm with a dust emission brightness temperature $\\sim120$ K. The column of ISM at this nucleus is $\\rm N_{H2} \\geq 2\\times10^{26}$ cm$^{-2}$, corresponding to A$_V = 10^6$ mag and 1000 gr cm$^{-2}$. The East nucleus is somewhat more elongated with radial extent 0.3\\arcsec or $\\sim120$ pc. The derived kinematics of the nuclear disks provide a good fit to the line profiles sampled every 50 mas, yielding the emissivity distributions, the rotation curves and velocity dispersio...

  10. ALMA Finds Dew Drops in the Dusty Spider's Web

    CERN Document Server

    Gullberg, B; De Breuck, C; Branchu, S; Dannerbauer, H; Drouant, G; Emonts, B; Guillard, P; Hatch, N; Nesvadba, N P H; Omont, A; Seymour, N; Vernet, J

    2016-01-01

    We present 0."5 resolution ALMA detections of the observed 246GHz continuum, [CI]^3P_2-^3P_1 fine structure line ([CI]2-1), CO(7-6) and H2O lines in the z=2.161 radio galaxy MRC1138-262, the 'Spiderweb Galaxy'. We detect strong [CI]2-1 emission both at the position of the radio core, and in a second component ~4kpc away from it. The 1100km/s broad [CI]2-1 line in this latter component, combined with its H2 mass of 1.6x10^10Msun implies this emission must come from a compact region <60pc, possibly containing a second AGN. The combined H2 mass derived for both objects using the [CI]2-1 emission is 3.3x10^10Msun. The total CO(7-6)/[CI]2-1 line flux ratio of 0.2 suggests a low excitation molecular gas reservoir and/or enhanced atomic carbon in cosmic-ray dominated regions. We detect spatially-resolved H2O 2_{11}-2_{02} emission - for the first time in a high-z un-lensed galaxy - near the outer radio lobe to the east, and near the bend of the radio jet to the west of the radio galaxy. No underlying 246GHz conti...

  11. The Science Cases for Building a Band 1 Receiver Suite for ALMA

    CERN Document Server

    Di Francesco, J; Matthews, B C; Bartel, N; Bronfman, L; Casassus, S; Chitsazzadeh, S; Cunningham, M; Duchene, G; Geisbuesch, J; Hales, A; Ho, P T P; Houde, M; Iono, D; Kemper, F; Kepley, A; Koch, P M; Kohno, K; Kothes, R; Lai, S -P; Lin, K Y; Liu, S -Y; Mason, B; Maccarone, T J; Mizuno, N; Morata, O; Schieven, G; Scaife, A M M; Scott, D; Shang, H; Shimojo, M; Takakuwa, S; Wagg, J; Wootten, A; Yusef-Zadeh, F

    2013-01-01

    We present the various science cases for building Band 1 receivers as part of ALMA's ongoing Development Program. We describe the new frequency range for Band 1 of 35-52 GHz, a range chosen to maximize the receiver suite's scientific impact. We first describe two key science drivers: 1) the evolution of grains in protoplanetary disks and debris disks, and 2) molecular gas in galaxies during the era of re-ionization. Studies of these topics with Band 1 receivers will significantly expand ALMA's Level 1 Science Goals. In addition, we describe a host of other exciting continuum and line science cases that require ALMA's high sensitivity and angular resolution. For example, ALMA Band 1 continuum data will probe the Sunyaev-Zel'dovich Effect in galactic clusters, Very Small Grains and spinning dust, ionized jets from young stars, spatial and flaring studies of Sgr A*, the acceleration sites of solar flares, pulsar wind nebulae, radio supernovae, and X-ray binaries. Furthermore, ALMA Band 1 line data will probe che...

  12. The Database for Astronomical Spectroscopy - Updates, Additions and Plans for Splatalogue for Alma Full Science Operations

    Science.gov (United States)

    Remijan, Anthony; Seifert, Nathan A.; McGuire, Brett A.

    2016-06-01

    For the past 10 years, Splatalogue has been constantly updated, modified and enhanced in order to make molecular spectroscopy data readily available to the astronomical community. Splatalogue is fully integrated into the ALMA Observing Tool, the ALMA data reduction and analysis package (CASA) and several enhanced tools being developed through the ALMA development program including the next generation CASA viewer (CARTA) and the ALMA Data Mining Toolkit (ADMIT). In anticipation for ALMA full science operations, a number of improvements have taken place over the past year to the Splatalogue database including, but not limited too, additions to Splatalogue from the JPL and CDMS line lists, improvements and reconciliation of the Lovas/NIST Catalog assigning NRAO recommended rest frequencies to every astronomically detected transition, including recent astronomical surveys to the list of transitions detected in space and finally, improved search and display features as requested by the astronomical community. Splatalogue is planning for the next 10 years of development and welcomes any and all contributions to improving the data integrity and availability to the scientific community.

  13. Control de calidad en los cursos en línea de un programa en Ingeniería Informática

    Directory of Open Access Journals (Sweden)

    Gabriela Garita González

    2012-04-01

    Full Text Available Este artículo explica la experiencia obtenida, mediante el Programa Ingeniería informática de la Universidad Estatal a Distancia (Costa Rica, en la implementación de un proceso de control de calidad para evaluar y dar seguimiento a la mediación docente, el soporte técnico y al apoyo en los cursos en línea, que se ofrecen en los niveles de diplomado, bachillerato y licenciatura. Como elemento significativo del documento se pretende introducir modelos, estándares y mejores prácticas que ofrece el mercado como referencia para seleccionar y justificar los criterios de calidad que se desean alcanzar en los cursos de formación en línea. Se le ofrece al lector una serie de herramientas de implementación para un proceso de mejora en la calidad de los cursos en línea que se brinda al estudiante.

  14. The Cultural Implications of Primary Health Care and the Declaration of Alma-Ata: The Health District of Kedougou, Senegal

    Science.gov (United States)

    Blanas, Demetri A.

    2008-01-01

    In 1978, the World Health Organization (WHO) and the international health community convoked a conference in Alma-Ata, Kazakhstan, to address global inequalities in health. The conference resulted in the publication of the "Declaration of Alma-Ata," which made the ambitious call "for urgent action by all governments, all health and development…

  15. Reflexiones acerca de los sistemas de informacion universitarios ante los desafios y cambios generados por los procesos de evaluacion y acreditacion Some reflexions about informations systems for universities in the presence of challenges and changes produced by evaluation and acreditation processes

    Directory of Open Access Journals (Sweden)

    Santiago José Barcos

    2008-03-01

    Full Text Available Este artículo trata de la relevancia de los Sistemas de Información para universidades. Tales sistemas son esenciales para la gestión, para lograr enriquecer los resultados de la adopción de decisión y también para informar las acciones de las universidades a la sociedad. El artículo contiene algunas reflexiones respecto de los Sistemas de Informaciones en los Procesos de Evaluación y Acreditación y muestra los defectos detectados en Universidades Europeas y Latinoamericanas. Asimismo, se plantean requerimientos y funciones de este importante recurso y un especial énfasis en desarrollarlos adecuadamente para optimizar el funcionamiento y para impulsar la integración entre Instituciones Educativas en el contexto global.This article explains about the relevance that the Informations Systems have for universities, which are essential for management, to rich decision-making results, and also to report their actions to society. It contains some reflections about the necessity of Informations Systems in the Evaluation and Accreditation Processes, and expresses the faults detected in European and Latin American universities. Lastly, there is an enunciation of requirements and functions of this important resource, and a special emphasis on developing them properly to improve the integration between the Education Institutions in the global context.

  16. The European ALMA Regional Centre Network: A Geographically Distributed User Support Model

    CERN Document Server

    Hatziminaoglou, Evanthia; Andreani, Paola; Barta, Miroslav; Bertoldi, Frank; Brand, Jan; Gueth, Frederique; Hogerheijde, Michiel; Maercker, Matthias; Massardi, Marcella; Muehle, Stefanie; Muxlow, Thomas; Richards, Anita; Schilke, Peter; Tilanus, Remo; Vlemmings, Wouter; Afonso, Jose; Messias, Hugo

    2016-01-01

    In recent years there has been a paradigm shift from centralised to geographically distributed resources. Individual entities are no longer able to host or afford the necessary expertise in-house, and, as a consequence, society increasingly relies on widespread collaborations. Although such collaborations are now the norm for scientific projects, more technical structures providing support to a distributed scientific community without direct financial or other material benefits are scarce. The network of European ALMA Regional Centre (ARC) nodes is an example of such an internationally distributed user support network. It is an organised effort to provide the European ALMA user community with uniform expert support to enable optimal usage and scientific output of the ALMA facility. The network model for the European ARC nodes is described in terms of its organisation, communication strategies and user support.

  17. High-Angular-Resolution and High-Sensitivity Science Enabled by Beamformed ALMA

    CERN Document Server

    Fish, Vincent; Anderson, James; Asada, Keiichi; Baudry, Alain; Broderick, Avery; Carilli, Chris; Colomer, Francisco; Conway, John; Dexter, Jason; Doeleman, Sheperd; Eatough, Ralph; Falcke, Heino; Frey, Sándor; Gabányi, Krisztina; Gálvan-Madrid, Roberto; Gammie, Charles; Giroletti, Marcello; Goddi, Ciriaco; Gómez, Jose L; Hada, Kazuhiro; Hecht, Michael; Honma, Mareki; Humphreys, Elizabeth; Impellizzeri, Violette; Johannsen, Tim; Jorstad, Svetlana; Kino, Motoki; Körding, Elmar; Kramer, Michael; Krichbaum, Thomas; Kudryavtseva, Nadia; Laing, Robert; Lazio, Joseph; Loeb, Abraham; Lu, Ru-Sen; Maccarone, Thomas; Marscher, Alan; Mart'ı-Vidal, Iván; Martins, Carlos; Matthews, Lynn; Menten, Karl; Miller, Jon; Miller-Jones, James; Mirabel, Félix; Muller, Sebastien; Nagai, Hiroshi; Nagar, Neil; Nakamura, Masanori; Paragi, Zsolt; Pradel, Nicolas; Psaltis, Dimitrios; Ransom, Scott; Rodr'\\iguez, Luis; Rottmann, Helge; Rushton, Anthony; Shen, Zhi-Qiang; Smith, David; Stappers, Benjamin; Takahashi, Rohta; Tarchi, Andrea; Tilanus, Remo; Verbiest, Joris; Vlemmings, Wouter; Walker, R Craig; Wardle, John; Wiik, Kaj; Zackrisson, Erik; Zensus, J Anton

    2013-01-01

    An international consortium is presently constructing a beamformer for the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile that will be available as a facility instrument. The beamformer will aggregate the entire collecting area of the array into a single, very large aperture. The extraordinary sensitivity of phased ALMA, combined with the extremely fine angular resolution available on baselines to the Northern Hemisphere, will enable transformational new very long baseline interferometry (VLBI) observations in Bands 6 and 7 (1.3 and 0.8 mm) and provide substantial improvements to existing VLBI arrays in Bands 1 and 3 (7 and 3 mm). The ALMA beamformer will have impact on a variety of scientific topics, including accretion and outflow processes around black holes in active galactic nuclei (AGN), tests of general relativity near black holes, jet launch and collimation from AGN and microquasars, pulsar and magnetar emission processes, the chemical history of the universe and the evolution of fundame...

  18. Magnetic fields in protoplanetary disks: from MHD simulations to ALMA observations

    CERN Document Server

    Bertrang, Gesa H -M; Wolf, Sebastian

    2016-01-01

    Magnetic fields significantly influence the evolution of protoplanetary disks and the formation of planets, following the predictions of numerous magnetohydrodynamic (MHD) simulations. However, these predictions are yet observationally unconstrained. To validate the predictions on the influence of magnetic fields on protoplanetary disks, we apply 3D radiative transfer simulations of the polarized emission of aligned aspherical dust grains that directly link 3D global non-ideal MHD simulations to ALMA observations. Our simulations show that it is feasible to observe the predicted toroidal large-scale magnetic field structures, not only in the ideal observations but also with high-angular resolution ALMA observations. Our results show further that high angular resolution observations by ALMA are able to identify vortices embedded in outer magnetized disk regions.

  19. The ALMA Band 9 receiver - Design, construction, characterization, and first light

    CERN Document Server

    Baryshev, A M; Mena, F P; Klapwijk, T M; van Kempen, T A; Hogerheijde, M R; Jackson, B D; Adema, J; Gerlofsma, G J; Bekema, M E; Barkhof, J; de Haan-Stijkel, L H R; Bemt, M van den; Koops, A; Keizer, K; Pieters, C; Jagt, J Koops van het; Schaeffer, H H A; Zijlstra, T; Kroug, M; Lodewijk, C F J; Wielinga, K; Boland, W; de Graauw, M W M; van Dishoeck, E F; Jager, H; Wild, W

    2015-01-01

    We describe the design, construction, and characterization of the Band 9 heterodyne receivers (600-720 GHz) for the Atacama Large Millimeter / submillimeter Array (ALMA). The ALMA Band 9 receiver units ("cartridges"), which are installed in the telescope's front end, have been designed to detect and down-convert two orthogonal linear polarization components of the light collected by the ALMA antennas. The light entering the front end is refocused with a compact arrangement of mirrors, which is fully contained within the cartridge. The arrangement contains a grid to separate the polarizations and two beam splitters to combine each resulting beam with a local oscillator signal. The combined beams are fed into independent double-sideband mixers, each with a corrugated feedhorn coupling the radiation by way of a waveguide with backshort cavity into an impedance-tuned SIS junction that performs the heterodyne down-conversion. Finally, the generated intermediate frequency signals are amplified by cryogenic and room...

  20. ALMA service data analysis and level 2 quality assurance with CASA

    CERN Document Server

    Petry, Dirk; Villard, Eric; Komugi, Shinya; Schnee, Scott

    2014-01-01

    The Atacama Large mm and sub-mm Array (ALMA) radio observatory is one of the world's largest astronomical projects. After the very successful conclusion of the first observation cycles Early Science Cycles 0 and 1, the ALMA project can report many successes and lessons learned. The science data taken interleaved with commissioning tests for the still continuing addition of new capabilities has already resulted in numerous publications in high-profile journals. The increasing data volume and complexity are challenging but under control. The radio-astronomical data analysis package "Common Astronomy Software Applications" (CASA) has played a crucial role in this effort. This article describes the implementation of the ALMA data quality assurance system, in particular the level 2 which is based on CASA, and the lessons learned.

  1. ALMA service data analysis and level 2 quality assurance with CASA

    Science.gov (United States)

    Petry, Dirk; Vila-Vilaro, Baltasar; Villard, Eric; Komugi, Shinya; Schnee, Scott

    2014-07-01

    The Atacama Large mm and sub-mm Array (ALMA) radio observatory is one of the world's largest astronomical projects. After the very successful conclusion of the first observation cycles Early Science Cycles 0 and 1, the ALMA project can report many successes and lessons learned. The science data taken interleaved with commis- sioning tests for the still continuing addition of new capabilities has already resulted in numerous publications in high-profile journals. The increasing data volume and complexity are challenging but under control. The radio-astronomical data analysis package "Common Astronomy Software Applications" (CASA) has played a crucial role in this effort. This article describes the implementation of the ALMA data quality assurance system, in particular the level 2 which is based on CASA, and the lessons learned.

  2. Examining the Perils and Promises of an Informal Niche in a Global City: A Case Study of Mexican Immigrant Gardeners in Los Angeles

    OpenAIRE

    Huerta, Alvaro

    2011-01-01

    The domestic household service sector of contract gardening dominated by Mexican immigrants in Los Angeles constitutes an important and under-examined component of the city's informal economy. Mexican immigrant gardeners, like Latina domestic workers and Latino day laborers, represent an important and undervalued labor source in this global city and other U.S. cities and suburbs. While domestic help has historically been a privilege of the affluent, the middle-class, since the World War II er...

  3. ETHYL CYANIDE ON TITAN: SPECTROSCOPIC DETECTION AND MAPPING USING ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Cordiner, M. A.; Palmer, M. Y.; Nixon, C. A.; Charnley, S. B.; Mumma, M. J.; Serigano, J. [NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771 (United States); Irwin, P. G. J. [Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, University of Oxford, Parks Road, Oxford, OX1 3PU (United Kingdom); Teanby, N. A. [School of Earth Sciences, University of Bristol, Wills Memorial Building, Queen’s Road, Bristol, BS8 1RJ (United Kingdom); Kisiel, Z. [Institute of Physics, Polish Academy of Sciences, Al. Lotnikøw 32/46, 02-668 Warszawa (Poland); Kuan, Y.-J.; Chuang, Y.-L. [National Taiwan Normal University, Taipei 116, Taiwan (China); Wang, K.-S., E-mail: martin.cordiner@nasa.gov [Institute of Astronomy and Astrophysics, Academia Sinica, Taipei 106, Taiwan (China)

    2015-02-10

    We report the first spectroscopic detection of ethyl cyanide (C{sub 2}H{sub 5}CN) in Titan’s atmosphere, obtained using spectrally and spatially resolved observations of multiple emission lines with the Atacama Large Millimeter/submillimeter Array (ALMA). The presence of C{sub 2}H{sub 5}CN in Titan’s ionosphere was previously inferred from Cassini ion mass spectrometry measurements of C{sub 2}H{sub 5}CNH{sup +}. Here we report the detection of 27 rotational lines from C{sub 2}H{sub 5}CN (in 19 separate emission features detected at >3σ confidence) in the frequency range 222–241 GHz. Simultaneous detections of multiple emission lines from HC{sub 3}N, CH{sub 3}CN, and CH{sub 3}CCH were also obtained. In contrast to HC{sub 3}N, CH{sub 3}CN, and CH{sub 3}CCH, which peak in Titan’s northern (spring) hemisphere, the emission from C{sub 2}H{sub 5}CN is found to be concentrated in the southern (autumn) hemisphere, suggesting a distinctly different chemistry for this species, consistent with a relatively short chemical lifetime for C{sub 2}H{sub 5}CN. Radiative transfer models show that C{sub 2}H{sub 5}CN is most concentrated at altitudes ≳200 km, suggesting production predominantly in the stratosphere and above. Vertical column densities are found to be in the range (1–5) × 10{sup 14} cm{sup −2}.

  4. H-alpha features with hot onsets III. Fibrils in Lyman-alpha and with ALMA

    CERN Document Server

    Rutten, Robert J

    2016-01-01

    In H-alpha most of the solar surface is covered by a dense canopy of long opaque fibrils, but predictions for quiet-Sun observations with ALMA have ignored this fact. Comparison with Ly-alpha suggests that the large opacity of H-alpha fibrils is caused by hot precursor events. Application of a recipe that assumes momentary Saha-Boltzmann extinction during their hot onset to millimeter wavelengths suggests that ALMA will observe the H-alpha fibril canopy, not acoustic shocks underneath, and will yield data more interesting than if this canopy were transparent.

  5. SXDF-ALMA 2 arcmin$^2$ Deep Survey: 1.1-mm Number Counts

    OpenAIRE

    Hatsukade, Bunyo; Kohno, Kotaro; Umehata, Hideki; Aretxaga, Itziar; Caputi, Karina I.; Dunlop, James S.; Ikarashi, Soh; Iono, Daisuke; Ivison, Rob J.; Lee, Minju; Makiya, Ryu; Matsuda, Yuichi, Stott, John P; Motohara, Kentaro; Nakanishi, Kouichiro; Ohta, Kouji

    2016-01-01

    We report 1.1 mm number counts revealed with the Atacama Large Millimeter/submillimeter Array (ALMA) in the Subaru/XMM-Newton Deep Survey Field (SXDF). The advent of ALMA enables us to reveal millimeter-wavelength number counts down to the faint end without source confusion. However, previous studies are based on the ensemble of serendipitously-detected sources in fields originally targeting different sources and could be biased due to the clustering of sources around the targets. We derive n...

  6. Embriaguez e males da alma: entre a mania e a melancolia

    Directory of Open Access Journals (Sweden)

    Paulo José Carvalho da Silva

    2013-03-01

    Full Text Available Este artigo examina as relações estabelecidas no campo da medicina da alma entre a embriaguez e os males da alma. Parte da atitude ambivalente em relação ao vinho sustentada desde a Antiguidade para mostrar como no século XVIII explicações baseadas nas dinâmicas psicofisiológicas e tratamentos que faziam apelo à ordenação da razão com a vontade para o domínio dos apetites são substituídos por uma concepção propriamente patologizante do abuso da bebida.

  7. ALMA observations of Lyman-alpha Blob 1: halo sub-structure illuminated from within

    OpenAIRE

    Geach, J. E.; Narayanan, D.; Matsuda, Y.; Hayes, M.; Mas-Ribas, Ll.; Dijkstra, M.; Steidel, C.C.; Chapman, S. C.; Feldmann, R.; Avison, A.; Agertz, O.; Ao, Y.; Birkinshaw, M.; Bremer, M. N.; Clements, D. L.

    2016-01-01

    We present new Atacama Large Millimeter/Submillimeter Array (ALMA) 850um continuum observations of the original Lyman-alpha Blob (LAB) in the SSA22 field at z=3.1 (SSA22-LAB01). The ALMA map resolves the previously identified submillimeter source into three components with total flux density S_850 = 1.68+/-0.06 mJy, corresponding to a star formation rate of ~150 M_sun/yr. The submillimeter sources are associated with several faint (m~27 mag) rest-frame ultraviolet sources identified in Hubble...

  8. HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies

    Science.gov (United States)

    Bussmann, R. S.; Riechers, D.; Fialkov, A.; Scudder, J.; Hayward, C. C.; Cowley, W. I.; Bock, J.; Calanog, J.; Chapman, S. C.; Cooray, A.; De Bernardis, F.; Farrah, D.; Fu, Hai; Gavazzi, R.; Hopwood, R.; Ivison, R. J.; Jarvis, M.; Lacey, C.; Loeb, A.; Oliver, S. J.; Pérez-Fournon, I.; Rigopoulou, D.; Roseboom, I. G.; Scott, Douglas; Smith, A. J.; Vieira, J. D.; Wang, L.; Wardlow, J.

    2015-10-01

    The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-forming galaxies (DSFGs) over a wide range in redshift. A detailed understanding of these DSFGs is hampered by the limited spatial resolution of Herschel. We present 870 μm 0.″45 resolution imaging obtained with the Atacama Large Millimeter/submillimeter Array (ALMA) of a sample of 29 HerMES DSFGs that have far-infrared (FIR) flux densities that lie between the brightest of sources found by Herschel and fainter DSFGs found via ground-based surveys in the submillimeter region. The ALMA imaging reveals that these DSFGs comprise a total of 62 sources (down to the 5σ point-source sensitivity limit in our ALMA sample; σ ≈ 0.2 {mJy}). Optical or near-infrared imaging indicates that 36 of the ALMA sources experience a significant flux boost from gravitational lensing (μ \\gt 1.1), but only six are strongly lensed and show multiple images. We introduce and make use of uvmcmcfit, a general-purpose and publicly available Markov chain Monte Carlo visibility-plane analysis tool to analyze the source properties. Combined with our previous work on brighter Herschel sources, the lens models presented here tentatively favor intrinsic number counts for DSFGs with a break near 8 {mJy} at 880 μ {{m}} and a steep fall-off at higher flux densities. Nearly 70% of the Herschel sources break down into multiple ALMA counterparts, consistent with previous research indicating that the multiplicity rate is high in bright sources discovered in single-dish submillimeter or FIR surveys. The ALMA counterparts to our Herschel targets are located significantly closer to each other than ALMA counterparts to sources found in the LABOCA ECDFS Submillimeter Survey. Theoretical models underpredict the excess number of sources with small separations seen in our ALMA sample. The high multiplicity rate and small projected separations between sources seen in our sample argue in favor of interactions

  9. Informes realizados en 1760 para llevar a cabo los reparos de la iglesia parroquial de San Miguel en Peñaranda de Bracamonte (Salamanca

    Directory of Open Access Journals (Sweden)

    Muñoz González, María Jesús

    2003-09-01

    Full Text Available This article deals with the advice offered by four members of the Royal Academy of San Fernando in the eighteenth century upon being consulted concerning the restoration of the church of Peñaranda de Bracamonte (Salamanca, in a impending ruinous state. Through the reports submitted by Ventura Rodriguez, Alejandro González Velazquez, Jaime Marquet and Francisco Sabatini related to the plan, and the official report from the Dominican Friar Marcos de Santa Rosa, it is possible to discern the different approaches of the period to the restoration of old buildings.

    Este artículo trata de los informes que plantean cuatro miembros de la Real Academia de San Fernando en el siglo XVIII al ser consultados para dar su opinión sobre la restauración de la iglesia parroquial de Peñaranda de Bracamonte (Salamanca que amenazaba ruina. A través de los informes realizados por Ventura Rodríguez, Alejandro González Velázquez, Jaime Marquet y Francisco Sabatini sobre el plano e informe oficial del dominico Fray Marcos de Santa Rosa, podemos ver los distintos planteamientos que en la época se tenían sobre las restauraciones de edificios antiguos.

  10. Políticas de austeridad y cambios en las pautas de uso de los servicios sanitarios. Informe SESPAS 2014

    OpenAIRE

    Rosa Urbanos Garrido; Jaume Puig-Junoy

    2014-01-01

    Se analizan los principales cambios en los patrones de utilización sanitaria que se están produciendo en España como consecuencia de la crisis y de las medidas adoptadas frente a ella. Se examina el impacto de la reforma en el diseño del copago farmacéutico, que ofrece como resultado una importante reducción en el número de recetas dispensadas en las oficinas de farmacia, si bien sus efectos sobre la adherencia al tratamiento, el acceso a tratamientos necesarios y efectivos, y en última insta...

  11. La incorporación del cacao ecuatoriano al mercado mundial entre 1840 y 1925, según los informes consulares

    Directory of Open Access Journals (Sweden)

    Juan Maiguashca

    2012-07-01

    Full Text Available Este artículo ofrece una reinterpretación del proceso de incorporación del cacao ecuatoriano al mercado mundial, entre 1840 y 1925. Esta revisión se realiza a partir de los conceptos desarrollados por el economista italiano Giovanni Arrighi: incorporación nominal, incorporación periférica e incorporación no-periférica. Por medio de estos, el ensayo analiza la variedad de enlaces que se desarrollaron entre el centro y la periferia, y dentro la periferia misma. Se estudian especialmente dos momentos de este proceso: 1840-1890 y 1890-1910. El análisis de las articulaciones externas e internas que se dieron en cada una de estas fases y los factores de producción que los sustentaron permiten caracterizar al primer momento como ‘incorporación nominal’ y al segundo como ‘periférica’. Esta distinción permite una mejor comprensión del auge cacaotero ecuatoriano en el largo siglo XIX. El trabajo se basa en los informes consulares extranjeros, un tipo de documentación que no ha sido suficientemente estudiada todavía.

  12. Sistema informático para la gestión de los planes de ingreso a la educación media y superior en Cuba

    Directory of Open Access Journals (Sweden)

    Luis Ernesto Acosta Ortíz

    2012-12-01

    Full Text Available El objetivo del trabajo es presentar un sistema de gestión de los planes de ingreso a la educación media y superior en Cuba, el cual automatiza los procesos de recopilación de información, así como los algoritmos de asignación del ingreso que se desarrolla en el Departamento de Fuerza de Trabajo Calificada del Ministerio de Trabajo y Seguridad Social. Este departamento se encarga de gestionar los procesos de formación y empleo de la fuerza de trabajo calificada en el país; forma parte del Sistema Unificado de Gestión de Fuerza de Trabajo Calificada (GeForza, iniciado en 2009 en la Universidad de las Ciencias Informáticas (UCI, concebido a partir de la estrategia de actualizar el Estudio Integral para la Formación y Empleo de la Fuerza de Trabajo Calificada en Cuba. Para el desarrollo de la aplicación web se usó el marco de trabajo Sauxe, el lenguaje de programación PHP y la integración de otros marcos de trabajo como Zend Framework, Doctrine y ExtJS. Es una aplicación totalmente funcional que se encuentra en fase de despliegue.

  13. Revelation of the voluntary information about Human Capital in the Annual Reports Revelación de la información voluntaria sobre el capital humano en los informes anuales

    Directory of Open Access Journals (Sweden)

    Miguel Angel Villacorta

    2007-07-01

    Full Text Available The Financial Accounting impedes the registration on behalf of the information on the intangible of the different companies. To attenuate this situation, many companies offer voluntary data on them in the accounting documentation. This work analyzes the voluntary information of the Spanish companies about the intangible, impacting in the place that they occupy inside the Annual Report. The main conclusion of the investigation is that the companies offer the voluntary information that more it interests them for their own motivations and, however, the users of the Financial Accounting need a wider and more comparable information on the Human Capital.La normalización contable actual impide el registro de parte de la información sobre los intangibles de las diferentes empresas. Para atenuar esta situación, muchas empresas ofrecen datos voluntarios sobre ellos en la documentación contable que ofrecen a terceros. Este trabajo analiza la información voluntaria que exponen las empresas españolas cotizadas sobre los intangibles no reconocidos en el Balance, incidiendo en el lugar que ocupan dentro del Informe Anual. La principal conclusión de la investigación es que las empresas ofrecen la información voluntaria que más les interesa para sus propias motivaciones y, sin embargo, los usuarios de la Contabilidad Financiera necesitan una información más amplia y comparable sobre el Capital Humano.

  14. Errores algebraicos más comunes en los estudiantes de primer ingreso de las carreras de Informática, Administración y Turismo del Centro Universitario de los Valles de la Universidad de Guadalajara

    Directory of Open Access Journals (Sweden)

    Emilio Ramírez Mora

    2015-10-01

    Full Text Available En la presente investigación se analizan los errores algebraicos más comunes que cometen los estudiantes de primer ingreso de las licenciaturas de Informática, Administración y Turismo. La acotación del estudio a errores algebraicos se debe a que los conocimientos algebraicos básicos constituyen un conocimiento deseable antes de cursar las asignaturas de Matemáticas I y Precálculo. El test se aplicó a un total de 198 estudiantes, el cual consta de 15 reactivos de opción múltiple y se tiene un 51.31% de respuestas incorrectas, un 5.08% de respuestas sin contestar. El promedio general de los 198 estudiantes es de 43.60. Un estudiante no obtuvo ninguna respuesta correcta, así como ninguno los 15 reactivos correctamente. El error más común fue para el reactivo número 15 con el 69.19% de respuestas incorrectas; este reactivo serefiere a encontrar la solución de una ecuación cuadrática.  SummaryIn this research the most common algebraic errors committed by first semester students of Informatics, Administration and Tourism programs are analyzed. The idea of studying algebraic errors is due to the fact that basic algebraic knowledge constitutes a desirable knowledge before studying the subjects of Math I and Precalculus. The test was applied to 198 students. This test is formed by 15 reagents of multiple option and it had a 51,31% of incorrect answers, and 5,08% of noanswered questions. The general average of the 198 students is 43,60. A student did not obtain any correct answer, as well as none got the 15 reagents correctly. The most common error was for the reagent number 15 with the 69,19% of incorrect answers; this point refers to find the solution of a quadratic equation.

  15. Informe del estado de los ambientes y recursos marinos y costeros en Colombia: Año 2014

    OpenAIRE

    2014-01-01

    Balance anual sobre el estado del medio ambiente y los recursos naturales renovables, así como recomendaciones y alternativas para el logro de un desarrollo en armonía con la naturaleza, en las áreas geográficas y temáticas de competencia del INVEMAR.

  16. Informe del estado de los ambientes y recursos marinos y costeros en Colombia: Año 2013.

    OpenAIRE

    2014-01-01

    Balance anual sobre el estado del medio ambiente y los recursos naturales renovables, así como recomendaciones y alternativas para el logro de un desarrollo en armonía con la naturaleza, en las áreas geográficas y temáticas de competencia del INVEMAR.

  17. Informe del estado de los ambientes y recursos marinos y costeros en Colombia: Año 2012.

    OpenAIRE

    2013-01-01

    Balance anual sobre el estado del medio ambiente y los recursos naturales renovables, así como recomendaciones y alternativas para el logro de un desarrollo en armonía con la naturaleza, en las áreas geográficas y temáticas de competencia del INVEMAR.

  18. Subcontrataciones en sectores conocimiento-intensivos: el caso de los trabajos informático y bio-informático

    OpenAIRE

    Miguez, Pablo

    2012-01-01

    La subcontratación en sectores conocimiento-incentivos tiene efectos similares a los de todo proceso de tercerización con el agregado de que la naturaleza del producto muchas veces habilita su realización por razones técnicas y no necesariamente responde o esta ligado a trabajos de baja calificación. En estos proceso de trabajo complejos la subcontratación esta a la orden del día - cualquiera sea el tipo de producto que se realice- y genera los mismos problemas que en el sector industrial....

  19. El Aseguramiento de los Informes de Sostenibilidad: Diferencias Sustanciales con la Auditoría de Cuentas (Sustainability Reports Assurance: Substantial Differences with Financial Auditing

    Directory of Open Access Journals (Sweden)

    Amaia Zubiaurre

    2015-12-01

    Full Text Available Besides the growing interest of companies to communicate their commitment to sustainability, assurance of the information disclosed has increased, due to the interest of the stakeholders to know their reliability. Initially, we will explain the concept and benefits of sustainability reporting assurance. Subsequently, we will focus on the differences between the financial audit and sustainability reports assurance and the description of the main international report assurance statements. Finally, we will explain the main criticisms of assurance and some proposals for improvement. Junto al creciente interés de las empresas por comunicar su compromiso con la sostenibilidad, ha aumentado el aseguramiento de la información revelada, debido al interés de los grupos de interés por conocer su fiabilidad. Inicialmente, explicaremos el concepto y las ventajas del aseguramiento de los informes de sostenibilidad. Posteriormente, nos centraremos en las diferencias existentes entre la auditoría de cuentas y el aseguramiento de memorias de sostenibilidad y en la descripción de los principales estándares internacionales en materia de aseguramiento. Finalmente, expondremos las principales críticas al aseguramiento y algunas propuestas de mejora. DOWNLOAD THIS PAPER FROM SSRN: http://ssrn.com/abstract=2690158

  20. Sistema de clasificación del método en los informes de investigación en Psicología

    Directory of Open Access Journals (Sweden)

    Ignacio Montero

    2005-01-01

    Full Text Available En este trabajo se revisa y amplía un sistema de clasificación de las metodologías de investigación en Psicología previamente publicado por los autores en esta misma revista en el año 2002. Se argumentan las ventajas de su utilización y se advierte sobre los posibles inconvenientes. El sistema está basado en la clasificación del tipo de plan de investigación que se utiliza en cada caso. En un primer nivel, se compone de nueve grandes categorías: 1 estudios teóricos, 2 estudios descriptivos mediante observación, 3 estudios descriptivos mediante encuesta, 4 estudios cualitativos, 5 experimentos, 6 cuasi experimentos, 7 estudios «ex post facto», 8 experimentos de caso único y 9 estudios instrumentales. Se presentan las características más importantes de cada tipo de estudio y, dentro de cada tipo, las claves que permiten identificar cada una de sus posibles variantes –que constituyen las subcategorías del sistema de clasificación- ilustrando con investigaciones publicadas cada uno de los subtipos de investigación a los que da lugar el sistema. El sistema de clasificación aquí propuesto se utilizará como modelo para los informes de investigación que se envíen a esta revista.

  1. The mysterious morphology of MRC0943-242 as revealed by ALMA and MUSE

    Science.gov (United States)

    Gullberg, Bitten; De Breuck, Carlos; Lehnert, Matthew D.; Vernet, Joël; Bacon, Roland; Drouart, Guillaume; Emonts, Bjorn; Galametz, Audrey; Ivison, Rob; Nesvadba, Nicole P. H.; Richard, Johan; Seymour, Nick; Stern, Daniel; Wylezalek, Dominika

    2016-02-01

    We present a pilot study of the z = 2.923 radio galaxy MRC0943-242, where we combine information from ALMA and MUSE data cubes for the first time. Even with modest integration times, we disentangle the AGN and starburst dominated components. These data reveal a highly complex morphology as the AGN, starburst, and molecular gas components show up as widely separated sources in dust continuum, optical continuum, and CO line emission observations. CO(1-0) and CO(8-7) line emission suggest that there is a molecular gas reservoir offset from both the dust and the optical continuum that is located ~90 kpc from the AGN. The UV line emission has a complex structure in emission and absorption. The line emission is mostly due to a large scale ionisation cone energised by the AGN, and a Lyα emitting bridge of gas between the radio galaxy and a heavily star-forming set of components. Strangely, the ionisation cone has no Lyα emission. We find this is due to an optically thick layer of neutral gas with unity covering fraction spread out over a region of at least ~100 kpc from the AGN. Other less thick absorption components are associated with Lyα emitting gas within a few tens of kpc from the radio galaxy and are connected by a bridge of emission. We speculate that this linear structure of dust, Lyα and CO emission, and the redshifted absorption seen in the circum nuclear region may represent an accretion flow feeding gas into this massive AGN host galaxy.

  2. Water around IRAS 15398-3359 observed with ALMA

    Science.gov (United States)

    Bjerkeli, P.; Jørgensen, J. K.; Bergin, E. A.; Frimann, S.; Harsono, D.; Jacobsen, S. K.; Lindberg, J. E.; Persson, M.; Sakai, N.; van Dishoeck, E. F.; Visser, R.; Yamamoto, S.

    2016-10-01

    Context. Understanding how protostars accrete their mass is one of the fundamental problems of star formation. High dust column densities and complex kinematical structures make direct observations challenging. Moreover, direct observations only provide a snapshot. Chemical tracers provide an interesting alternative to characterise the infall histories of protostars. Aims: We aim to map the distribution and kinematics of gaseous water towards the low-mass embedded protostar IRAS 15398-3359. Previous observations of H13CO+ showed a depression in the abundance towards IRAS 15398-3359. This is a sign of destruction of HCO+ by an enhanced presence of gaseous water in an extended region, possibly related to a recent burst in the accretion. Direct observations of water vapour can determine the exact extent of the emission and confirm the hypothesis that HCO+ is indeed a good tracer of the water snow-line. Methods: IRAS 15398-3359 was observed using the Atacama Large Millimeter/submillimeter Array (ALMA) at 0.5″ resolution in two setups at 390 and 460 GHz. Maps of HDO (101-000) and were taken simultaneously with observations of the CS (8-7) and N2H+ (5-4) lines and continuum at 0.65 and 0.75 mm. The maps were interpreted using dust radiative transfer calculations of the protostellar infalling envelope with an outflow cavity. Results: HDO is clearly detected and extended over the scales of the H13CO+ depression, although it is displaced by 500 AU in the direction of the outflow. HO is tentatively detected towards the red-shifted outflow lobe, but otherwise it is absent from the mapped region, which suggests that temperatures are low. Although we cannot entirely exclude a shock origin, this indicates that another process is responsible for the water emission. Conclusions: Based on the temperature structure obtained from dust radiative transfer models, we conclude that the water was most likely released from the grains in an extended hour-glass configuration during a

  3. Multimolecule ALMA observations toward the Seyfert 1 galaxy NGC 1097

    Science.gov (United States)

    Martín, S.; Kohno, K.; Izumi, T.; Krips, M.; Meier, D. S.; Aladro, R.; Matsushita, S.; Takano, S.; Turner, J. L.; Espada, D.; Nakajima, T.; Terashima, Y.; Fathi, K.; Hsieh, P.-Y.; Imanishi, M.; Lundgren, A.; Nakai, N.; Schinnerer, E.; Sheth, K.; Wiklind, T.

    2015-01-01

    Context. The nearby Sy 1 galaxy NGC 1097 represents an ideal laboratory for exploring the molecular chemistry in the surroundings of an active galactic nucleus (AGN). Aims: Exploring the distribution of different molecular species allows us to understand the physical processes affecting the interstellar medium both in the AGN vicinity and in the outer star forming molecular ring. Methods: We carried out 3 mm ALMA observations that include seven different molecular species, namely HCN, HCO+, CCH, CS, HNCO, SiO, HC3N, and SO, as well as the 13C isotopologues of the first two. Spectra were extracted from selected positions and all species were imaged over the central 2 kpc (~30'') of the galaxy at a resolution of ~2.2'' × 1.5'' (150 pc × 100 pc). Results: HCO+ and CS appear to be slightly enhanced in the star forming ring. CCH shows the largest variations across NGC 1097 and is suggested to be a good tracer of both obscured and early stage star formation. HNCO, SiO, and HC3N are significantly enhanced in the inner circumnuclear disk surrounding the AGN. Conclusions: Differences in the molecular abundances are observed between the star forming ring and the inner circumnuclear disk. We conclude that the HCN/HCO+ and HCN/CS differences observed between AGN-dominated and starburst (SB) galaxies are not due to a HCN enhancement due to X-rays, but rather this enhancement is produced by shocked material at distances of 200 pc from the AGN. Additionally, we claim that lower HCN/CS is a combination of a small underabundance of CS in AGNs, together with excitation effects, where a high density gas component (~106 cm-3) may be more prominent in SB galaxies. However, the most promising are the differences found among the dense gas tracers that, at our modest spatial resolution, seem to outline the physical structure of the molecular disk around the AGN. In this picture, HNCO probes the well-shielded gas in the disk, surrounding the dense material moderately exposed to the X

  4. ALMA finds dew drops in the dusty spider's web

    Science.gov (United States)

    Gullberg, Bitten; Lehnert, Matthew D.; De Breuck, Carlos; Branchu, Steve; Dannerbauer, Helmut; Drouart, Guillaume; Emonts, Bjorn; Guillard, Pierre; Hatch, Nina; Nesvadba, Nicole P. H.; Omont, Alain; Seymour, Nick; Vernet, Joël

    2016-06-01

    We present 0.̋5 resolution ALMA detections of the observed 246 GHz continuum, [CI] 3P2→3P1 fine structure line ([CI]2-1), CO(7-6), and H2O lines in the z = 2.161 radio galaxy MRC1138-262, the so-called Spiderweb galaxy. We detect strong [CI]2-1 emission both at the position of the radio core, and in a second component ~4 kpc away from it. The 1100 km s-1 broad [CI]2-1 line in this latter component, combined with its H2 mass of 1.6 × 1010 M⊙, implies that this emission must come from a compact region <60 pc, possibly containing a second active galactic nucleus (AGN). The combined H2 mass derived for both objects, using the [CI]2-1 emission, is 3.3 × 1010 M⊙. The total CO(7-6)/[CI]2-1 line flux ratio of 0.2 suggests a low excitation molecular gas reservoir and/or enhanced atomic carbon in cosmic ray dominated regions. We detect spatially-resolved H2O 211-202 emission - for the first time in a high-z unlensed galaxy - near the outer radio lobe to the east, and near the bend of the radio jet to the west of the radio galaxy. No underlying 246 GHz continuum emission is seen at either position. We suggest that the H2O emission is excited in the cooling region behind slow (10-40 km s-1) shocks in dense molecular gas (103-5 cm-3). The extended water emission is likely evidence of the radio jet's impact on cooling and forming molecules in the post-shocked gas in the halo and inter-cluster gas, similar to what is seen in low-z clusters and other high-z radio galaxies. These observations imply that the passage of the radio jet in the interstellar and inter-cluster medium not only heats gas to high temperatures, as is commonly assumed or found in simulations, but also induces cooling and dissipation, which can lead to substantial amounts of cold dense molecular gas. The formation of molecules and strong dissipation in the halo gas of MRC1138-262 may explain both the extended diffuse molecular gas and the young stars observed around MRC1138-262. The reduced data cubes

  5. Measuring turbulence in TW Hydrae with ALMA: methods and limitations

    Science.gov (United States)

    Teague, R.; Guilloteau, S.; Semenov, D.; Henning, Th.; Dutrey, A.; Piétu, V.; Birnstiel, T.; Chapillon, E.; Hollenbach, D.; Gorti, U.

    2016-07-01

    Aims: We aim to obtain a spatially resolved measurement of velocity dispersions in the disk of TW Hya. Methods: We obtained images with high spatial and spectral resolution of the CO J = 2-1, CN N = 2-1 and CS J = 5-4 emission with ALMA in Cycle 2. The radial distribution of the turbulent broadening was derived with two direct methods and one modelling approach. The first method requires a single transition and derives Tex directly from the line profile, yielding a vturb. The second method assumes that two different molecules are co-spatial, which allows using their relative line widths for calculating Tkin and vturb. Finally we fitted a parametric disk model in which the physical properties of the disk are described by power laws, to compare our direct methods with previous values. Results: The two direct methods were limited to the outer r > 40 au disk because of beam smear. The direct method found vturb to range from ≈130 m s-1 at 40 au, and to drop to ≈50 m s-1 in the outer disk, which is qualitatively recovered with the parametric model fitting. This corresponds to roughly 0.2-0.4 cs. CN was found to exhibit strong non-local thermal equilibrium effects outside r ≈ 140 au, so that vturb was limited to within this radius. The assumption that CN and CS are co-spatial is consistent with observed line widths only within r ≲ 100 au, within which vturb was found to drop from 100 m s-1 (≈0.4 cs) to zero at 100 au. The parametric model yielded a nearly constant 50 m s-1 for CS (0.2-0.4 cs). We demonstrate that absolute flux calibration is and will be the limiting factor in all studies of turbulence using a single molecule. Conclusions: The magnitude of the dispersion is comparable with or below that predicted by the magneto-rotational instability theory. A more precise comparison would require reaching an absolute calibration precision of about 3%, or finding a suitable combination of light and heavy molecules that are co-located in the disk. The reduced

  6. Why complexity matters: using ALMaSS for risk assessment of wildlife

    DEFF Research Database (Denmark)

    Topping, Christopher John

    -sink dynamics are emergent properties and do not need to be imposed.ALMaSS is one such model system and is used here to exemplify aspects of complexity in population-level risk assessment for terrestrial mammals, birds, and arthropods exposed to pesticides. Results are used to argue for greater realism...

  7. ALMA imaging of the CO snowline of the HD 163296 disk with DCO

    NARCIS (Netherlands)

    Mathews, G. S.; Klaassen, P. D.; Juhasz, A.; Harsono, D.; Chapillon, E.; van Dishoeck, E. F.; Espada, D.; de Gregorio-Monsalvo, I.; Hales, A.; Hogerheijde, M. R.; Mottram, J. C.; Rawlings, M. G.; Takahashi, S.; Testi, L.

    2013-01-01

    Context. The high spatial resolution and line sensitivity of the Atacama Large Millimeter/submillimeter Array (ALMA) opens the possibility of resolving emission from molecules in large samples of circumstellar disks. With an understanding of the conditions under which these molecules can have high a

  8. MILLIMETER EMISSION STRUCTURE IN THE FIRST ALMA IMAGE OF THE AU Mic DEBRIS DISK

    NARCIS (Netherlands)

    MacGregor, Meredith A.; Wilner, David J.; Rosenfeld, Katherine A.; Andrews, Sean M.; Matthews, Brenda; Hughes, A. Meredith; Booth, Mark; Chiang, Eugene; Graham, James R.; Kalas, Paul; Kennedy, Grant; Sibthorpe, Bruce

    2013-01-01

    We present 1.3 mm ALMA Cycle 0 observations of the edge-on debris disk around the nearby, similar to 10 Myr old, M-type star AU Mic. These observations obtain 0 ''.6 (6 AU) resolution and reveal two distinct emission components: (1) the previously known dust belt that extends to a radius of 40 AU an

  9. SÓCRATES E O CUIDADO DE SI OU A TERAPÊUTICA DA ALMA

    Directory of Open Access Journals (Sweden)

    Raimundo Araújo dos Santos

    2008-03-01

    Full Text Available Esse artigo pretende ser uma abordagem simples, na verdade, um resumo, recolhido dostextos de Platão sobre o auto-conhecimento e o cuidado de si. Esses são os elementos queconstituem a base do saber ético iniciado por Sócrates e o ponto de partida do que chamamosterapêutica da alma.

  10. Improved design for low noise Nb SIS devices for Band 9 of ALMA (600 - 720 GHz)

    NARCIS (Netherlands)

    Lodewijk, C. F. J.; Kroug, M.; Klapwijk, T. M.; Mena, F. P.; Baryshev, A. M.; Wild, W.

    2005-01-01

    Superconducting-insulating-superconducting mixers incorporating a novel design were fabricated and evaluated for heterodyne detection in the frequency range of 600 to 720 GHz (ALMA Band 9). The improved design consists in tapering the corners of the RF transformer and a careful optimization of the d

  11. ALMA Temporal Phase Stability and the Effectiveness of Water Vapor Radiometer

    CERN Document Server

    Matsushita, S; Barkats, D; Hills, R E; Fomalont, E; Nikolic, B

    2012-01-01

    Atacama Large Millimeter/submillimeter Array (ALMA) will be the world largest mm/submm interferometer, and currently the Early Science is ongoing, together with the commissioning and science verification (CSV). Here we present a study of the temporal phase stability of the entire ALMA system from antennas to the correlator. We verified the temporal phase stability of ALMA using data, taken during the last two years of CSV activities. The data consist of integrations on strong point sources (i.e., bright quasars) at various frequency bands, and at various baseline lengths (up to 600 m). From the observations of strong quasars for a long time (from a few tens of minutes, up to an hour), we derived the 2-point Allan Standard Deviation after the atmospheric phase correction using the 183 GHz Water Vapor Radiometer (WVR) installed in each 12 m antenna, and confirmed that the phase stability of all the baselines reached the ALMA specification. Since we applied the WVR phase correction to all the data mentioned abov...

  12. Sideband separating mixer for 600-720 GHz for ALMA band 9 upgrade

    NARCIS (Netherlands)

    Khudchenko, Andrey; Hesper, Ronald; Baryshev, Andrey; Gerlofma, Gerrit; Barkhof, Jan; Adema, Joost; Mena, Patricio; Klapwijk, Teun; Spaans, Maarten

    2012-01-01

    For high-frequency observational bands like ALMA (Atacama Large Millimeter Array) Band 9 (600—720 GHz), which tend to be dominated by atmospheric noise, implementation of sideband-separating mixers can reduce, up to a factor of two, the integration time needed to reach a certain signal-to-noise rati

  13. Development of a 0.6 THz SIS Receiver for ALMA

    NARCIS (Netherlands)

    Baryshev, A. M.; van de Stadt, H.; Schaeffer, H.; Hesper, R.; Zijlstra, T.; Zuiddam, M.; Wild, W.; de Jong, L.

    2001-01-01

    The Atacama Large Millimeter Array (ALMA) requires low noise SIS receivers for frequencies from about 80 GHz to 950 GHz with very large IF bandwidth (4-12 GHz). Additional requirements for these receivers are high reliability, low cost and the possibility of series production. In this paper we repor

  14. Equilibrium chemical reaction of supersonic hydrogen-air jets (the ALMA computer program)

    Science.gov (United States)

    Elghobashi, S.

    1977-01-01

    The ALMA (axi-symmetrical lateral momentum analyzer) program is concerned with the computation of two dimensional coaxial jets with large lateral pressure gradients. The jets may be free or confined, laminar or turbulent, reacting or non-reacting. Reaction chemistry is equilibrium.

  15. Alma Reed: A Unique Bicultural Bridge between North American and Mexican Cultures in the Twentieth Century.

    Science.gov (United States)

    Finer, Neal

    Alma Reed, a Californian who became a noted figure in Mexican art history, was a bicultural individual who introduced famed Mexican muralists to the United States art world and who became a legendary figure in Mexican folklore from the 1920s through the 1960s. This paper traces her career. (JB)

  16. A detailed mass distribution of a high-density core in Taurus with ALMA

    CERN Document Server

    Tokuda, Kazuki; Matsumoto, Tomoaki; Saigo, Kazuya; Kawamura, Akiko; Fukui, Yasuo; Inutsuka, Shu-ichiro; Machida, Masahiro N; Tomida, Kengo; Tachihara, Kengo; André, Philippe

    2016-01-01

    We present the results of ALMA observations of dust continuum emission and molecular rotational lines, including the ALMA Compact Array, toward a dense core MC27 (a.k.a. L1521F) in Taurus, which is considered to be at very early stage of star formation. Detailed column density distribution with a size scale from a few tens AU to ~10000 AU scale are revealed by combining the ALMA data and the single-dish data. The high angular resolution observation at 0.87 mm reveals that a protostellar source, MMS-1, is still not spatially resolved without gas association and a starless high-density core, MMS-2, has substructures both in dust and molecular emission. The averaged radial column density distribution of the inner part (r < 3000 AU) is N_H2 ~r^-0.4, clearly flatter than that of the outer part, ~r^-1.0. We found the complex velocity/spatial structure obtained with previous ALMA observations is located inside the inner flatter region, which may reflect the dynamical status of the dense core.

  17. HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies

    CERN Document Server

    Bussmann, R S; Fialkov, A; Scudder, J; Hayward, C C; Cowley, W I; Bock, J; Calanog, J; Chapman, S C; Cooray, A; De Bernardis, F; Farrah, D; Fu, Hai; Gavazzi, R; Hopwood, R; Ivison, R J; Jarvis, M; Lacey, C; Loeb, A; Oliver, S J; Perez-Fournon, I; Rigopoulou, D; Roseboom, I G; Scott, Douglas; Smith, A J; Vieira, J D; Wang, L; Wardlow, J

    2015-01-01

    The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-forming galaxies (DSFGs) over a wide range in redshift. A detailed understanding of these DSFGs is hampered by the poor spatial resolution of Herschel. We present 870um 0.45" imaging obtained in Cycle 0 with the Atacama Large Millimeter/submillimeter Array (ALMA) of a sample of 29 HerMES DSFGs. The ALMA imaging reveals that these DSFGs comprise a total of 62 sources (down to the 5-sigma limit in our ALMA sample; sigma~0.2 mJy). Optical imaging indicates that 36 of the ALMA sources experience a significant flux boost from gravitational lensing (mu>1.1), but only 6 are strongly lensed and show multiple images. We introduce and make use of uvmcmcfit, a general purpose and publicly available Markov chain Monte Carlo visibility plane analysis tool to analyze the source properties. Combined with our previous work on brighter Herschel sources, the lens models presented here tentatively favor intrinsic number counts for...

  18. Generic Abstraction of Hardware Control Based on the ALMA Common Software

    Science.gov (United States)

    Jeram, B.; Chiozzi, G.; Ibsen, J.; Cirami, R.; Pokorny, M.; Muders, D.; Wischolek, D.

    2004-07-01

    The ALMA Common Software (ACS) is a CORBA-based framework that provides a common and homogeneous infrastructure for the whole ALMA software, from high-level data flow applications down to instrument control (Schwarz et al., 2004). This paper focuses on ACS support for the development of Control System applications. In this domain, ACS provides a generic abstraction of hardware control and monitor points that is independent of the software underneath. This abstraction layer is coupled to the hardware using the DevIO (Device Input/Output) interface, based on the Bridge design pattern. Application developers have to implement DevIO classes that handle the details of the communication with the hardware. ACS itself provides a default DevIO implementation which simply writes and reads into/from a memory location. Currently there are two other major DevIO implementations available: a CAN bus communication, used by ALMA, and a socket based implementation used by the Atacama Pathfinder EXperiment (APEX) project. In spite of using different hardware and control electronics, the DevIO abstraction allows the ALMA and APEX projects to have the same device architecture down to the level of the DevIO implementation.

  19. The Latin Grammys and the ALMAs: Awards Programs, Cultural Epideictic, and Intercultural Pedagogy.

    Science.gov (United States)

    Gonzalez, Alberto; Heuman, Amy N.

    2003-01-01

    Examines the Latin Grammy Awards and the ALMA Awards as media texts that can be used as course content on Latino people and cultures in an intercultural communication course. Outlines a critical reformulation of epideictic rhetoric, provides background on the two programs, and interprets their import as epideictic discourse. (Contains 25…

  20. The ALMA Data Mining Toolkit I: Archive Setup and User Usage

    Science.gov (United States)

    Teuben, P.; Pound, M.; Mundy, L.; Looney, L.; Friedel, D. N.

    2014-05-01

    We report on an ALMA development study and project where we employ a novel approach to add data and data descriptors to ALMA archive data and allowing further flexible data mining on retrieved data. We call our toolkit ADMIT (the ALMA Data Mining Toolkit) that works within the Python based CASA environment. What is described here is a design study, with some exiting toy code to prove the concept. After ingestion of science ready datacubes, ADMIT will compute a number of basic and advanced data products, and their descriptors. Examples of such data products are cube statistics, line identification tables, line cubes, moment maps, an integrated spectrum, overlap integrals and feature extraction tables. Together with a descriptive XML file, a small number of visual aids are added to a ZIP file that is deposited into the archive. Large datasets (such as line cubes) will have to be rederived by the user once they have also downloaded the actual ALMA Data Products, or via VO services if available. ADMIT enables the user to rederive all its products with different methods and parameters, and compare archive product with their own.

  1. Assembly, integration, and verification (AIV) in ALMA: series processing of array elements

    Science.gov (United States)

    Lopez, Bernhard; Jager, Rieks; Whyborn, Nicholas D.; Knee, Lewis B. G.; McMullin, Joseph P.

    2012-09-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) is a joint project between astronomical organizations in Europe, North America, and East Asia, in collaboration with the Republic of Chile. ALMA will consist of at least 54 twelve-meter antennas and 12 seven-meter antennas operating as an aperture synthesis array in the (sub)millimeter wavelength range. It is the responsibility of ALMA AIV to deliver the fully assembled, integrated, and verified antennas (array elements) to the telescope array. After an initial phase of infrastructure setup AIV activities began when the first ALMA antenna and subsystems became available in mid 2008. During the second semester of 2009 a project-wide effort was made to put in operation a first 3- antenna interferometer at the Array Operations Site (AOS). In 2010 the AIV focus was the transition from event-driven activities towards routine series production. Also, due to the ramp-up of operations activities, AIV underwent an organizational change from an autonomous department into a project within a strong matrix management structure. When the subsystem deliveries stabilized in early 2011, steady-state series processing could be achieved in an efficient and reliable manner. The challenge today is to maintain this production pace until completion towards the end of 2013. This paper describes the way ALMA AIV evolved successfully from the initial phase to the present steady-state of array element series processing. It elaborates on the different project phases and their relationships, presents processing statistics, illustrates the lessons learned and relevant best practices, and concludes with an outlook of the path towards completion.

  2. The ALMA common software: a developer-friendly CORBA-based framework

    Science.gov (United States)

    Chiozzi, Gianluca; Jeram, Bogdan; Sommer, Heiko; Caproni, Alessandro; Plesko, Mark; Sekoranja, Matej; Zagar, Klemen; Fugate, David W.; Di Marcantonio, Paolo; Cirami, Roberto

    2004-09-01

    The ALMA Common Software (ACS) is a set of application frameworks built on top of CORBA. It provides a common software infrastructure to all partners in the ALMA collaboration. The usage of ACS extends from high-level applications such as the Observation Preparation Tool [7] that will run on the desk of astronomers, down to the Control Software [6] domain. The purpose of ACS is twofold: from a system perspective, it provides the implementation of a coherent set of design patterns and services that will make the whole ALMA software [1] uniform and maintainable; from the perspective of an ALMA developer, it provides a friendly programming environment in which the complexity of the CORBA middleware and other libraries is hidden and coding is drastically reduced. The evolution of ACS is driven by a long term development plan, however on the 6-months release cycle the plan is adjusted based on incoming requests from ALMA subsystem development teams. ACS was presented at SPIE 2002[2]. In the two years since then, the core services provided by ACS have been extended, while the coverage of the application framework has been increased to satisfy the needs of high-level and data flow applications. ACS is available under the LGPL public license. The patterns implemented and the services provided can be of use also outside the astronomical community; several projects have already shown their interest in ACS. This paper presents the status of ACS and the progress over the last two years. Emphasis is placed on showing how requests from ACS users have driven the selection of new features.

  3. Bulk data transfer distributer: a high performance multicast model in ALMA ACS

    Science.gov (United States)

    Cirami, R.; Di Marcantonio, P.; Chiozzi, G.; Jeram, B.

    2006-06-01

    A high performance multicast model for the bulk data transfer mechanism in the ALMA (Atacama Large Millimeter Array) Common Software (ACS) is presented. The ALMA astronomical interferometer will consist of at least 50 12-m antennas operating at millimeter wavelength. The whole software infrastructure for ALMA is based on ACS, which is a set of application frameworks built on top of CORBA. To cope with the very strong requirements for the amount of data that needs to be transported by the software communication channels of the ALMA subsystems (a typical output data rate expected from the Correlator is of the order of 64 MB per second) and with the potential CORBA bottleneck due to parameter marshalling/de-marshalling, usage of IIOP protocol, etc., a transfer mechanism based on the ACE/TAO CORBA Audio/Video (A/V) Streaming Service has been developed. The ACS Bulk Data Transfer architecture bypasses the CORBA protocol with an out-of-bound connection for the data streams (transmitting data directly in TCP or UDP format), using at the same time CORBA for handshaking and leveraging the benefits of ACS middleware. Such a mechanism has proven to be capable of high performances, of the order of 800 Mbits per second on a 1Gbit Ethernet network. Besides a point-to-point communication model, the ACS Bulk Data Transfer provides a multicast model. Since the TCP protocol does not support multicasting and all the data must be correctly delivered to all ALMA subsystems, a distributer mechanism has been developed. This paper focuses on the ACS Bulk Data Distributer, which mimics a multicast behaviour managing data dispatching to all receivers willing to get data from the same sender.

  4. Development and testing of Band 10 receivers for the ALMA project

    Energy Technology Data Exchange (ETDEWEB)

    Uzawa, Y., E-mail: y.uzawa@nao.ac.jp [National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Fujii, Y.; Gonzalez, A.; Kaneko, K.; Kroug, M.; Kojima, T.; Kuroiwa, K.; Miyachi, A. [National Astronomical Observatory, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Saito, S.; Makise, K.; Wang, Z. [National Institute of Information and Telecommunications Technology, 588-2 Iwaoka, Iwaoka-cho, Kobe, Hyogo 651-2492 (Japan); Asayama, S. [Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura, Santiago (Chile)

    2013-11-15

    Highlights: •The ALMA Band 10 (787–950 GHz) SIS receivers have been developed. •The complex conductivity of NbTiN was measured by a THz-TDS for the mixer design. •Tens of Band 10 receivers have been produced and their performance was quite well. •The best achieved receiver noise temperature was 125 K corresponding to 3hf/k{sub B}. •Band 10 receiver installed in the ALMA antenna captured astronomical signals. -- Abstract: The production model of a dual polarization heterodyne receiver for the Atacama Large Millimeter/submillimteter Array (ALMA) telescope has been developed to operate in the 787–950 GHz frequency band. The receiver uses two double sideband (DSB) waveguide mixers with Nb/AlOx/Nb tunnel junctions and NbTiN/SiO{sub 2}/Al microstrip tuning circuits on quartz substrate. A terahertz time domain spectrometer was used to characterize our NbTiN film for the tuning circuit design, which revealed that the complex conductivity of the film is described by the Mattis-Bardeen theory including a finite scattering time of 15 fs and a superconducting gap with a gap ratio 2Δ/k{sub B}T{sub C} ∼ 4.0. Tens of these receivers (out of the total production number of 73) have been successfully produced, and their performance is well within the stringent ALMA requirements. The best achieved DSB receiver noise temperature is 125 K, corresponding to about 3hf/k{sub B} for 4 K operation. One of Band 10 receivers has successfully been installed in the ALMA antenna for a test observation.

  5. Utilización de recursos sociosanitarios y características del cuidado informal de los pacientes inmovilizados en atención domiciliaria

    Directory of Open Access Journals (Sweden)

    Francisco García Alcaraz

    2015-04-01

    Conclusiones: Las enfermedades del aparato locomotor constituyen los principales motivos de inmovilización en pacientes domiciliarios. La mayoría de los cuidadores informales son mujeres de edad avanzada. La duración e intensidad del cuidado son elevadas y los principales apoyos provienen de los profesionales sanitarios. Los pacientes hacen un uso reducido de recursos sociosanitarios.

  6. LA EDUCACIÓN AMBIENTAL FORMAL EN EL CONTEXTO SOCIAL DE LA EDUCACIÓN INFORMAL Y DE LOS MEDIOS DE COMUNICACIÓN

    Directory of Open Access Journals (Sweden)

    Luis Quintanar Medina

    2013-10-01

    Full Text Available En este trabajo se analiza la contradicción que hay entre la educación ambiental formal y los medios de comunicación potenciados actualmente por las tecnologías de información y comunicación, reflejo de la contradicción entre lo que debe promover este tipo de educación y lo que propugna la ideología dominante en gran parte de los países de América Latina. Lo anterior se fundamenta en la naturaleza política de la educación en general y de la educación ambiental en particular. Se muestra que la educación ambiental, sobre todo la formal, se ve fuertemente afectada por los medios de comunicación a través de la cada vez más importante fuente de socialización: la educación informal.

  7. Informe final. Monitoreo complementario de las mareas rojas en las regiones de Los Lagos, Aysén y Magallanes.

    OpenAIRE

    2013-01-01

    Se informa de los monitoreos de fitoplancton nocivo y toxinas marinas incluyendo variables oceanográficas y meteorológicas en el sur de Chile. En este contexto se entiende por un programa de monitoreo a una actividad sistemática en el espacio y tiempo, orientada a contar con información que permita conocer las tendencias naturales de determinadas variables que pueden ser utilizadas como indicadoras de cambio ambiental y eventualmente indicadoras de riesgo para la salud pública y las actividad...

  8. Solar ALMA: Observation-Based Simulations of the mm and sub-mm Emissions from Active Regions

    Science.gov (United States)

    Fleishman, G.; Loukitcheva, M.; Nita, G.

    2015-12-01

    We developed an efficient algorithm integrated in our 3D modeling tool, GX Simulator (Nita et al. 2015), allowing quick computation of the synthetic intensity and polarization maps of solar active regions (AR) in the ALMA spectral range.

  9. ALMA's view of the Sun's nearest neighbours: The submm/mm SEDs of the alpha Centauri binary and a new source

    CERN Document Server

    Liseau, R; O'Gorman, E; Bertone, E; Chavez, M; Tapia, F

    2016-01-01

    The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and other stars are at the focus of intense contemporary research. Observations at submm/mm wavelengths are particularly useful to obtain information about the run of the temperature in the upper atmosphere of Sun-like stars. We used ALMA to study the chromospheric emission of the aCen binary system in all six available frequency bands during Cycle2 in 2014/15. Since ALMA is an interferometer, the multi-telescope array is particularly suited for the observation of point sources. With its large collecting area, the sensitivity is high enough to allow the observation of nearby main-sequence stars at submm/mm wavelengths for the first time. The comparison of the observed spectral energy distributions with theoretical model computations provides the chromospheric structure in terms of temperature and density above the stellar photosphere and the quantitative understanding of the primary emission pro...

  10. Corporate Responsibilityon the Media Sector : Study on the Corporate Responsibility Perceptions of Alma Media’s Stakeholders

    OpenAIRE

    Poukka, Riikka

    2010-01-01

    Despite the globally growing interest in corporate responsibility (CR), there is little practical as wellas academic knowledge of CR practises in the media sector. The aim of this study is to make acontribution to the evolving understanding of what CR implies in the media sector by applying astakeholder approach to a case study, which is Alma Media, a Finnish media corporation. Firstly,from the corporate perspective, the objective of this study is to provide Alma Media with a CRagenda, based ...

  11. The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the sub-millimeter number counts

    CERN Document Server

    Simpson, James; Swinbank, Mark; Chapman, Scott; Geach, James; Ivison, Rob; Thomson, Alasdair; Aretxaga, Itziar; Blain, Andrew; Cowley, Will; Chen, Chian-Chou; Coppin, Kristen; Dunlop, Jim; Edge, Alastair; Farrah, Duncan; Ibar, Edo; Karim, Alex; Knudsen, Kirsten; Meijerink, Rowin; Michalowski, Michal; Scott, Douglas; Spanns, Marco; van der Werf, Paul

    2015-01-01

    We present high-resolution 870-um ALMA continuum maps of 30 bright sub-millimeter sources in the UKIDSS UDS field. These sources are selected from deep, 1-square degrees 850-um maps from the SCUBA--2 Cosmology Legacy Survey, and are representative of the brightest sources in the field (median SCUBA2 flux S_850=8.7+/-0.4 mJy). We detect 52 sub-millimeter galaxies (SMGs) at >4-sigma significance in our 30 ALMA maps. In 61+/-17% of the ALMA maps the single-dish source comprises a blend of >=2 SMGs, where the secondary SMGs are Ultra--Luminous Infrared Galaxies (ULIRGs) with L_IR>10^12 Lo. The brightest SMG contributes on average 80+/-4% of the single-dish flux density, and in the ALMA maps containing >=2 SMGs the secondary SMG contributes 25+/-3% of the integrated ALMA flux. We construct source counts and show that multiplicity boosts the apparent single-dish cumulative counts by 20% at S_870>7.5mJy, and by 60% at S_870>12mJy. We combine our sample with previous ALMA studies of fainter SMGs and show that the cou...

  12. Uso de información electrónica por los académicos de la Universidad de la República (Uruguay Electronic information as used by the academia at the State University in Uruguay

    Directory of Open Access Journals (Sweden)

    María Cristina Pérez Giffoni

    2003-12-01

    Full Text Available En el marco de un proyecto de investigación en la línea de los Estudios de Usuarios de la Información, se analiza el modo en el que los avances tecnológicos, materializados en redes de información electrónica, afectan el comportamiento de comunicación académica formal e informal, la búsqueda, el uso de la información y la generación de conocimiento de los investigadores universitarios. Mediante un estudio comprensivo de tratamiento básicamente cualitativo, se entrevistó a una muestra de 151 docentes investigadores, cubriendo todas las áreas y servicios que conforman la estructura de la Universidad de la República, se discutieron los resultados a la luz de los contextos reales y se visualizaron los posibles escenarios futuros.In a research project dealing with the study of information users, the way technological advances in the form of networks of electronic information is analyzed, as far as these advances affect behavior of formal and informal academic communication, search, use of information and the generation of knowledge by university researchers. Through an understanding study of a basically qualitative treatment, a sample of 151 research instructors were interviewed covering all fields and services within the structure of the State University (Universidad de la República, results on a real context basis were discussed and eventual future settings were viewed.

  13. Exploring Parenting: Information Sheets for Parents = Explorando El Arte de Ser Padres: Hojas informativas para los padres.

    Science.gov (United States)

    Administration for Children, Youth, and Families (DHHS), Washington, DC. Head Start Bureau.

    This document, provided here in separate English and Spanish versions, is a collection of informational and instructional sheets for parents of young children, divided into 20 thematic sections. Each of the sections includes information on the topic area, some learning activities, and questions for discussion. The sessions are: (1) "Getting…

  14. Spectators of Mockumentaries: Mockumentaries in the Information Society Espectadores de Falsos Documentales: Los falsos documentales en la Sociedad de la Información

    Directory of Open Access Journals (Sweden)

    Vicente Diaz Gandasegui

    2012-11-01

    Full Text Available

    The existence of a significant number of documentaries which are not intended to represent reality but to (recreate it has allowed that mockumentaries to become a subgenre halfway between reality and fiction. Mockdocumentaries aim to play with the status acquired over the years by the spectators of documentaries, parodying the conventions of the genre and criticizing certain cultural or social codes. Simultaneously, mockumentaries are a very useful tool to analyse the current social and cultural context of the image and the media in the society of information. Mockumentaries are therefore a significant product of the confusion between reality and unreality at a time when digital technology is able to simulate reality with absolute veracity.

    La existencia de un gran número de documentales que no tienen como objetivo representar la realidad sino (recrearla ha hecho que los falsos documentales se conviertan en un subgénero que se encuentra a medio camino entre la realidad y la ficción. Los falsos documentales pretenden jugar con el estatus adquirido durante años por el espectador de documentales, parodiar las convenciones existentes en el género o realizar una crítica de ciertos códigos culturales. La confusión entre realidad e irrealidad se encuentra pues en la base de los falsos documentales, pero debido a la amplitud que abarcan consiguen reflexionar, utilizando el humor, la sorpresa, el engaño o el terror, sobre aspectos de gran relevancia para analizar el actual contexto social, cultural y de los medios de comunicación en la sociedad de la información. Los falsos documentales son por lo tanto un producto significativo de una forma de jugar con la confusión que crean las imágenes en un momento en que la tecnología digital es capaz de simular la realidad con total veracidad.


  15. ALMA observations of the variable 12CO/13CO ratio around the asymptotic giant branch star R Sculptoris

    CERN Document Server

    Vlemmings, W H T; Lindqvist, M; Mohamed, S; Olofsson, H; Ramstedt, S; Brunner, M; Groenewegen, M A T; Kerschbaum, F; Wittkowski, M

    2013-01-01

    [abridged] The 12CO/13CO ratio is often used as a measure of the 12C/13C ratio in the circumstellar environment, carrying important information about the stellar nucleosynthesis. External processes can change the 12CO and 13CO abundances, and spatially resolved studies of the 12CO/13CO ratio are needed to quantify the effect of these processes on the globally determined values. Additionally, such studies provide important information on the conditions in the circumstellar environment. The detached-shell source R Scl, displaying CO emission from recent mass loss, in a binary-induced spiral structure as well as in a clumpy shell produced during a thermal pulse, provides a unique laboratory for studying the differences in CO isotope abundances throughout its recent evolution. We observed both the 12CO(J=3-2) and the 13CO(J=3-2) line using ALMA. We find significant variations in the 12CO/13CO intensity ratios and consequently in the abundance ratios. The average CO isotope abundance ratio is at least a factor thr...

  16. Pobres y pobreza en los testamentos (Reino de Chile, 1585-1641

    Directory of Open Access Journals (Sweden)

    Pablo Lacoste

    2014-12-01

    Full Text Available En el artículo se analiza a los pobres y la pobreza en testamentos de Santiago de Chile entre fines del siglo XVI y el primer tercio del XVII, a partir de un corpus documental de 300 testamentos. Se considera que el temor, las actitudes y las prácticas realizadas respecto a la pobreza y los pobres en este período, se relacionan con la muerte próxima y el juicio de Dios. Por eso es que los pobres aparecen como la oportunidad de practicar las enseñanzas cristianas, acumular méritos, y mejorar el futuro de las propias almas. El desafío consiste, entonces, en examinar los testamentos santiaguinos para identificar la presencia de los pobres y la pobreza, atendiendo a comprender el sentido de esos conceptos en la mentalidad de los testadores.

  17. ALMA observations of alpha Centauri: First detection of main-sequence stars at 3mm wavelength

    CERN Document Server

    Liseau, R; Bayo, A; Bertone, E; Black, J H; del Burgo, C; Chavez, M; Danchi, W; De la Luz, V; Eiroa, C; Ertel, S; Fridlund, M C W; Justtanont, K; Krivov, A; Marshall, J P; Mora, A; Montesinos, B; Nyman, L -A; Olofsson, G; Sanz-Forcada, J; Thebault, P; White, G J

    2014-01-01

    The precise mechanisms that provide the non-radiative energy for heating the chromosphere and the corona of the Sun and those of other stars constitute an active field of research. By studying stellar chromospheres one aims at identifying the relevant physical processes. Defining the permittable extent of the parameter space can also serve as a template for the Sun-as-a-star. Earlier observations with Herschel and APEX have revealed the temperature minimum of alpha Cen, but these were unable to spatially resolve the binary into individual components. With the data reported here, we aim at remedying this shortcoming. Furthermore, these earlier data were limited to the wavelength region between 100 and 870mu. In the present context, we intend to extend the spectral mapping to longer wavelengths, where the contrast between stellar photospheric and chromospheric emission becomes increasingly evident. ALMA is particularly suited to point sources, such as unresolved stars. ALMA provides the means to achieve our obj...

  18. ALMA observation of high-z extreme star-forming environments discovered by Planck/Herschel

    Science.gov (United States)

    Kneissl, R.

    2016-05-01

    The Comic Microwave Background satellite Planck with its High Frequency Instrument has surveyed the mm/sub-mm sky in six frequency channels from 100 to 900 GHz. A sample of 228 cold sources of the Cosmic Infrared Background was observed in follow-up with Herschel SPIRE. The majority of sources appear to be over-densities of star-forming galaxies matching the size of high-z proto-cluster regions, while a 3% fraction are individual bright, lensed galaxies. A large observing program is underway with the aim of resolving the regions into the constituent members of the Planck sources. First ALMA data have been received on one Planck/Herschel proto-cluster candidate, showing the expected large over-abundance of bright mm/sub-mm sources within the cluster region. ALMA long baseline data of the brightest lensed galaxy in the sample with > 1 Jy at 350 μm are also forthcoming.

  19. Transparent XML Binding using the ALMA Common Software (ACS) Container/Component Framework

    Science.gov (United States)

    Sommer, H.; Chiozzi, G.; Fugate, D.; Sekoranja, M.

    2004-07-01

    ALMA software, from high-level data flow applications down to instrument control, is built using the ACS framework. The common architecture and infrastructure used for the whole ALMA software is presented at this conference in (Schwarz, Farris, & Sommer 2004). ACS offers a CORBA-based container/component model and supports the exchange and persistence of XML data. For the Java programming language, the container integrates transparently the use of type-safe Java binding classes to let applications conveniently work with XML transfer objects without having to parse or serialize them. This paper will show how the ACS container/component architecture serves to pass complex data structures, such as observation meta-data, between heterogeneous applications.

  20. Spectral and morphological analysis of the remnant of Supernova 1987A with ALMA & ATCA

    CERN Document Server

    Zanardo, Giovanna; Indebetouw, Remy; Chevalier, Roger A; Matsuura, Mikako; Gaensler, Bryan M; Barlow, Michael J; Fransson, Claes; Manchester, Richard N; Baes, Maarten; Kamenetzky, Julia R; Lakicevic, Masha; Lundqvist, Peter; Marcaide, Jon M; Marti-Vidal, Ivan; Meixner, Margaret; Ng, C -Y; Park, Sangwook; Sonneborn, George; Spyromilio, Jason; van Loon, Jacco Th

    2014-01-01

    We present a comprehensive spectral and morphological analysis of the remnant of Supernova (SN) 1987A with the Australia Telescope Compact Array (ATCA) and the Atacama Large Millimeter/submillimeter Array (ALMA). The non-thermal and thermal components of the radio emission are investigated in images from 94 to 672 GHz ($\\lambda$ 3.2 mm to 450 $\\mu$m), with the assistance of a high-resolution 44 GHz synchrotron template from the ATCA, and a dust template from ALMA observations at 672 GHz. An analysis of the emission distribution over the equatorial ring in images from 44 to 345 GHz highlights a gradual decrease of the east-to-west asymmetry ratio with frequency. We attribute this to the shorter synchrotron lifetime at high frequencies. Across the transition from radio to far infrared, both the synchrotron/dust-subtracted images and the spectral energy distribution (SED) suggest additional emission beside the main synchrotron component ($S_{\

  1. Uuden median murros Alma Mediassa, Sanoma Oy:ssÀ ja Yleisradiossa 1994-2004

    OpenAIRE

    Lindblom, Tomi

    2009-01-01

    This is a qualitative and multimethodological comparative study, which consists of two main parts: examining the development of new media and analysing and comparing the new media strategies of the three companies studied (Alma Media, Sanoma and the Finnish Broadcasting Company Yleisradio). The study includes the first large-scale review in Finnish of the development of new media, paying attention to the birth of the Internet as well as to mobile media, web TV and any other element of ne...

  2. SXDF-UDS-CANDELS-ALMA 1.5 arcmin2 deep survey

    NARCIS (Netherlands)

    Kohno, Kotaro; Tamura, Yoichi; Yamaguchi, Yuki; Umehata, Hideki; Rujopakarn, Wiphu; Lee, Minju; Motohara, Kentaro; Makiya, Ryu; Izumi, Takuma; Ivison, Rob; Ikarashi, Soh; Tadaki, Ken-ichi; Kodama, Tadayuki; Hatsukade, Bunyo; Yabe, Kiyoto; Hayashi, Masao; Iono, Daisuke; Matsuda, Yuichi; Nakanishi, Kouichiro; Kawabe, Ryohei; Wilson, Grant; Yun, Min S.; Hughes, David; Caputi, Karina; Dunlop, James

    2015-01-01

    We have conducted 1.1 mm ALMA observations of a contiguous 105″ × 50″ or 1.5 arcmin2 window (achieved by 19 point mosaic) in the SXDF-UDS-CANDELS. We achieved a 5σ sensitivity of 0.28 mJy, giving a flat sensus of dusty star-forming galaxies with LIR ~6 × 1011 L⊙ (if Tdust = 40 K) or SFR ~100 M⊙ yr-1

  3. New Measurements of the Radio Photosphere of Mira based on Data from the JVLA and ALMA

    OpenAIRE

    Matthews, L. D.; Reid, M. J.; Menten, K. M.

    2015-01-01

    We present new measurements of the millimeter wavelength continuum emission from the long period variable Mira ($o$ Ceti) at frequencies of 46 GHz, 96 GHz, and 229 GHz ($\\lambda$~7 mm, 3 mm, and 1 mm) based on observations obtained with the Jansky Very Large Array (JVLA) and the Atacama Large Millimeter/submillimeter Array (ALMA). The measured millimeter flux densities are consistent with a radio photosphere model derived from previous observations, where flux density, $S_{\

  4. Compact Starbursts in z ∼ 3–6 Submillimeter Galaxies Revealed by ALMA

    NARCIS (Netherlands)

    Ikarashi, Soh; Ivison, R. J.; Caputi, Karina I.; Aretxaga, Itziar; Dunlop, James S.; Hatsukade, Bunyo; Hughes, David H.; Iono, Daisuke; Izumi, Takuma; Kawabe, Ryohei; Kohno, Kotaro; Lagos, Claudia D. P.; Motohara, Kentaro; Nakanishi, Kouichiro; Ohta, Kouji; Tamura, Yoichi; Umehata, Hideki; Wilson, Grant W.; Yabe, Kiyoto; Yun, Min S.

    2015-01-01

    We report the source size distribution, as measured by ALMA millimetric continuum imaging, of a sample of 13 AzTEC-selected submillimeter galaxies (SMGs) at {z}{phot}∼ 3–6. Their infrared luminosities and star formation rates (SFRs) are {L}{IR}∼ 2–6× {10}12 {L}ȯ and ∼200–600 {M}ȯ yr‑1, respectively.

  5. Poster 9: Isotopic Ratios of Carbon and Oxygen in Titan's CO using ALMA

    Science.gov (United States)

    Serigano, Joseph; Nixion, Conor A.; Cordiner, Martin A.; Irwin, Patrick G. J.; Teanby, Nick A.; Charnley, Steven B.; Lindberg, Johan E.

    2016-06-01

    The advent of the Atacama Large Millimeter/Submillimeter Array (ALMA) has provided a new and powerful facility for probing the atmospheres of solar system targets at long wavelengths (84-720 GHz) where the rotational lines of small, polar molecules are prominent. In the complex atmosphere of Titan, photochemical processes dissociate and ionize molecular nitrogen and methane in the upper atmosphere, creating a complex inventory of trace hydrocarbons and nitriles. Additionally, the existence of oxygen on Titan facilitates the synthesis of molecules of potential astrobiological importance. Utilization of ground-based submillimeter observations of Titan has proven to be a powerful tool to complement results from spacecraft observations. ALMA provides the ability to probe this region in greater detail with unprecedented spectral and spatial resolution at high sensitivity, allowing for the derivation of vertical mixing profiles, molecular detections, and observations of latitudinal and seasonal variations. Recent ALMA studies of Titan have presented spectrally and spatially-resolved maps of HNC and HC3N emission (Cordiner et al. 2014), as well as the first spectroscopic detection of ethyl cyanide (C2H5CN) in Titan's atmosphere (Cordiner et al. 2015). This poster will focus on ALMA observations of carbon monoxide (CO) and its isotopologues 13CO, C18O, and C 17O in Titan's atmosphere. Molecular abundances and the vertical atmospheric temperature profile were derived by modeling the observed emission line profiles using NEMESIS, a line-by-line radiative transfer code (Irwin et al. 2008). This study reports the first spectroscopic detection of 17O in the outer solar system with C17O detected at >8σ confidence. The abundances of these molecules and isotopic ratios of 12C/13C, 16O/18O, and 16O/17O will be presented. General implications for the history of Titan from these measurements will be discussed.

  6. Detection of Lensing Substructure Using ALMA Observations of the Dusty Galaxy SDP.81

    Science.gov (United States)

    Hezaveh, Yashar D.; Dalal, Neal; Marrone, Daniel P.; Mao, Yao-Yuan; Morningstar, Warren; Wen, Di; Blandford, Roger D.; Carlstrom, John E.; Fassnacht, Christopher D.; Holder, Gilbert P.; Kemball, Athol; Marshall, Philip J.; Murray, Norman; Perreault Levasseur, Laurence; Vieira, Joaquin D.; Wechsler, Risa H.

    2016-05-01

    We study the abundance of substructure in the matter density near galaxies using ALMA Science Verification observations of the strong lensing system SDP.81. We present a method to measure the abundance of subhalos around galaxies using interferometric observations of gravitational lenses. Using simulated ALMA observations we explore the effects of various systematics, including antenna phase errors and source priors, and show how such errors may be measured or marginalized. We apply our formalism to ALMA observations of SDP.81. We find evidence for the presence of a M = 108.96±0.12 M ⊙ subhalo near one of the images, with a significance of 6.9σ in a joint fit to data from bands 6 and 7; the effect of the subhalo is also detected in both bands individually. We also derive constraints on the abundance of dark matter (DM) subhalos down to M ˜ 2 × 107 M ⊙, pushing down to the mass regime of the smallest detected satellites in the Local Group, where there are significant discrepancies between the observed population of luminous galaxies and predicted DM subhalos. We find hints of additional substructure, warranting further study using the full SDP.81 data set (including, for example, the spectroscopic imaging of the lensed carbon monoxide emission). We compare the results of this search to the predictions of ΛCDM halos, and find that given current uncertainties in the host halo properties of SDP.81, our measurements of substructure are consistent with theoretical expectations. Observations of larger samples of gravitational lenses with ALMA should be able to improve the constraints on the abundance of galactic substructure.

  7. A dor da alma nas reflexões sobre a vaidade de Matias Aires (1952

    Directory of Open Access Journals (Sweden)

    Paulo José Carvalho da Silva

    2009-06-01

    Full Text Available Este artigo analisa as relações entre a vaidade e o sofrimento conforme a obra Reflexões sobre a vaidade dos homens, do filósofo paulista Matias Aires Ramos da Silva de Eça (1705-1763. Discutem-se algumas fontes de seu pensamento e conclui-se que o autor faz uma fina e ainda atual análise da alma humana.

  8. Optical Characterisation of Astronomical Submillimetre Receivers including ALMA Bands 5 and 9

    OpenAIRE

    Whale, Mark

    2010-01-01

    The primary concern of this thesis is the analysis of long wavelength quasioptical receiver systems operating within the Terahertz and submillimetre wavebands. Specific attention is paid to the front-end coupling optics of the Band 5 and Band 9 receiver channels of the Atacama Large Millimetre Array (ALMA). The theory of Gaussian Beam Mode Analysis (GBMA) is expanded and developed as the basic analytical tool for the work presented. This technique is utilised to model both clas...

  9. De Alma-Ata a Harry Potter : um testemunho pessoal

    OpenAIRE

    Sakellarides, Constantino

    2001-01-01

    RESUMO - Quando, finalmente, entendemos a importância dos cuidados de saúde primários, procuramos construí-los à maneira das antigas catedrais góticas dos velhos burgos medievais: desenhadas por poucos, construídas por alguns, frequentadas obrigatoriamente por todos os demais. Através de todo este esforço, aprendemos. Os cuidados de saúde primários acontecem todos os dias: quando as pessoas comuns aprendem ou fazem alguma coisa de útil à sua saúde e à dos que lhes estã...

  10. ALMA imaging of the CO snowline of the HD 163296 disk with DCO+

    CERN Document Server

    Mathews, G S; Juhasz, A; Harsono, D; Chapillon, E; van Dishoeck, E F; Espada, D; de Gregorio-Monsalvo, I; Hales, A; Hogerheijde, M R; Mottram, J C; Rawlings, M G; Takahashi, S; Testi, L

    2013-01-01

    The high spatial and line sensitivity of ALMA opens the possibility of resolving emission from molecules in circumstellar disks. With an understanding of physical conditions under which molecules have high abundance, they can be used as direct tracers of distinct physical regions. In particular, DCO+ is expected to have an enhanced abundance within a few Kelvin of the CO freezeout temperature of 19 K, making it a useful probe of the cold disk midplane. We compare ALMA line observations of HD 163296 to a grid of models. We vary the upper- and lower-limit temperatures of the region in which DCO+ is present as well as the abundance of DCO+ in order to fit channel maps of the DCO+ J=5-4 line. To determine the abundance enhancement compared to the general interstellar medium, we carry out similar fitting to HCO+ J=4-3 and H13CO+ J=4-3 observations. ALMA images show centrally peaked extended emission from HCO+ and H13CO+. DCO+ emission lies in a resolved ring from ~110 to 160 AU. The outer radius approximately corr...

  11. ALMA observations of the debris disk around the young Solar Analog HD 107146

    CERN Document Server

    Ricci, L; Fu, B; Hughes, A M; Corder, S; Isella, A

    2014-01-01

    We present ALMA continuum observations at a wavelength of 1.25 mm of the debris disk surrounding the $\\sim$ 100 Myr old solar analog HD 107146. The continuum emission extends from about 30 to 150 AU from the central star with a decrease in the surface brightness at intermediate radii. We analyze the ALMA interferometric visibilities using debris disk models with radial profiles for the dust surface density parametrized as i) a single power-law, ii) a single power-law with a gap, and iii) a double power-law. We find that models with a gap of radial width $\\sim 8$ AU at a distance of $\\sim 80$ AU from the central star, as well as double power-law models with a dip in the dust surface density at $\\sim 70$ AU provide significantly better fits to the ALMA data than single power-law models. We discuss possible scenarios for the origin of the HD 107146 debris disk using models of planetesimal belts in which the formation of Pluto-sized objects trigger disruptive collisions of large bodies, as well as models which co...

  12. The ALMA archive and its place in the astronomy of the future

    CERN Document Server

    Stoehr, Felix; Leon, Stéphane; Muller, Erik; Manning, Alisdair; Moins, Christophe; Jenkins, Dustin

    2015-01-01

    The Atacama Large Millimeter/submillimeter Array (ALMA), an international partnership of Europe, North America and East Asia in cooperation with the Republic of Chile, is the largest astronomical project in existence. While ALMA's capabilities are ramping up, Early Science observations have started. The ALMA Archive is at the center of the operations of the telescope array and is designed to manage the 200 TB of data that will be taken each year, once the observatory is in full operations. We briefly describe design principles. The second part of this paper focuses on how astronomy is likely to evolve as the amount and complexity of data taken grows. We argue that in the future observatories will compete for astronomers to work with their data, that observatories will have to reorient themselves to from providing good data only to providing an excellent end-to-end user-experience with all its implications, that science-grade data-reduction pipelines will become an integral part of the design of a new observat...

  13. SXDF-UDS-CANDELS-ALMA 1.5 arcmin$^2$ deep survey

    CERN Document Server

    Kohno, K; Tamura, Y; Tadaki, K; Hatsukade, B; Ikarashi, S; Caputi, K I; Rujopakarn, W; Ivison, R J; Dunlop, J S; Motohara, K; Umehata, H; Yabe, K; Wang, W -H; Kodama, T; Koyama, Y; Hayashi, M; Matsuda, Y; Hughes, D; Aretxaga, I; Wilson, G W; Yun, M S; Ohta, K; Akiyama, M; Kawabe, R; Iono, D; Nakanishi, K; Lee, M; Makiya, R

    2016-01-01

    We have conducted 1.1 mm ALMA observations of a contiguous $105'' \\times 50''$ or 1.5 arcmin$^2$ window in the SXDF-UDS-CANDELS. We achieved a 5$\\sigma$ sensitivity of 0.28 mJy, providing a flat sensus of dusty star-forming galaxies with $L_{\\rm IR} \\sim6\\times10^{11}$ $L_\\odot$ (for $T_{\\rm dust}$ =40K) up to $z\\sim10$ thanks to the negative K-correction at this wavelength. We detected 5 brightest sources (S/N$>$6) and 18 low-significance sources (5$>$S/N$>$4; these may contain spurious detections, though). One of the 5 brightest ALMA sources ($S_{\\rm 1.1mm} = 0.84 \\pm 0.09$ mJy) is extremely faint in the WFC3 and VLT/HAWK-I images, demonstrating that a contiguous ALMA imaging survey is able to uncover a faint dust-obscured population that is invisible in deep optical/near-infrared surveys. We found a possible [CII]-line emitter at $z=5.955$ or a low-$z$ CO emitting galaxy within the field, which may allow us to constrain the [CII] and/or the CO luminosity functions across the history of the universe.

  14. The serendipitous discovery of a possible new solar system object with ALMA

    CERN Document Server

    Vlemmings, W; Maercker, M; Davidsson, B

    2015-01-01

    The unprecedented sensitivity of the Atacama Large millimeter/submillimeter array (ALMA) is providing many new discoveries. Several of these are serendipitous to the original goal of the observations. We report the discovery of previously unknown continuum sources, or a single fast moving new source, in our ALMA observations. Here we aim to determine the nature of the detections. The detections, at $>5.8\\sigma$ in the image plane and $>14\\sigma$ in the $(u,v)-$plane, were made in two epochs of ALMA observations of a $25$ arc second region around the asymptotic giant branch star W Aql in the continuum around 345 GHz. At a third epoch, covering $50x50$ arcseconds, the source(s) were not seen. We have investigated if the detections could be spurious, if they could constitute a population of variable background sources, or if the observations revealed a fast moving single object. Based on our analysis, we conclude that a single object (with a flux of $\\sim3.0$ mJy) exhibiting a large proper motion ($\\sim87$ arcse...

  15. A detailed view of the gas shell around R Sculptoris with ALMA

    CERN Document Server

    Maercker, M; Brunner, M; De Beck, E; Humphreys, E M; Kerschbaum, F; Lindqvist, M; Olofsson, H; Ramstedt, S

    2016-01-01

    Thermal pulses are fundamental to the chemical evolution of AGB stars and their circumstellar envelopes. A further consequence of thermal pulses is the formation of detached shells of gas and dust around the star. We aim to determine the physical properties of the detached gas shell around R Sculptoris, in particular the shell mass and temperature, and to constrain the evolution of the mass-loss rate during and after a thermal pulse. We analyse CO(1-0), CO(2-1), and CO(3-2) emission, observed by. The spatial resolution of the ALMA data allows us to separate the detached shell emission from the extended emission inside the shell. We perform radiative transfer modelling of both components to determine the shell properties and the post-pulse mass-loss properties. The ALMA data show a gas shell with a radius of 19.5" expanding at 14.3km/s. The different scales probed by the ALMA Cycle 0 array show that the shell must be entirely filled with gas, contrary to the idea of a detached shell. The comparison to single-d...

  16. Development and testing of Band 10 receivers for the ALMA project

    Science.gov (United States)

    Uzawa, Y.; Fujii, Y.; Gonzalez, A.; Kaneko, K.; Kroug, M.; Kojima, T.; Kuroiwa, K.; Miyachi, A.; Saito, S.; Makise, K.; Wang, Z.; Asayama, S.

    2013-11-01

    The production model of a dual polarization heterodyne receiver for the Atacama Large Millimeter/submillimteter Array (ALMA) telescope has been developed to operate in the 787-950 GHz frequency band. The receiver uses two double sideband (DSB) waveguide mixers with Nb/AlOx/Nb tunnel junctions and NbTiN/SiO2/Al microstrip tuning circuits on quartz substrate. A terahertz time domain spectrometer was used to characterize our NbTiN film for the tuning circuit design, which revealed that the complex conductivity of the film is described by the Mattis-Bardeen theory including a finite scattering time of 15 fs and a superconducting gap with a gap ratio 2Δ/kBTC ∼ 4.0. Tens of these receivers (out of the total production number of 73) have been successfully produced, and their performance is well within the stringent ALMA requirements. The best achieved DSB receiver noise temperature is 125 K, corresponding to about 3hf/kB for 4 K operation. One of Band 10 receivers has successfully been installed in the ALMA antenna for a test observation.

  17. Reflections on the twenty-fifth anniversary of the Alma-Ata Declaration.

    Science.gov (United States)

    Banerji, Debabar

    2003-01-01

    The Alma-Ata Declaration on Primary Health Care of 1978-based on the World Health Assembly's resolution of 1977 on Health for All by the Year 2000--was a watershed in the concepts and practices of public health as a scientific discipline; it was endorsed by every country in the world, rich and poor. According to the Declaration, health is a fundamental right, to be guaranteed by the state; people should be the prime movers in shaping their health services, using and enlarging upon the capacities developed in their societies; health services should operate as an integral whole, with promotive, preventive, curative, and rehabilitative components; and any western medical technology used in non-western societies must conform to the cultural, social, economic, and epidemiological conditions of the individual countries. Since Alma-Ata, a syndicate of the rich countries and the ruling elites of the poor countries, aided by the WHO, World Bank, World Trade Organization, and other international institutions, has done much to overturn the Declaration's primary health care initiatives. The WHO's recent attempt to regain some credibility, its Commission on Macroeconomics and Health, ignored the primary health care principles of the Alma-Ata Declaration. A struggle for these principles will have to be part of the larger struggle, by like-minded individuals working in individual countries, for a just world order. PMID:14758860

  18. Blade Runner -What kind objects are there in the JVO ALMA Archive?-

    CERN Document Server

    Eguchi, Satoshi; Zapart, Christopher; Ohishi, Masatoshi; Mizumoto, Yoshihiko; Kawasaki, Wataru; Kobayashi, Tsuyoshi; Kosugi, George

    2015-01-01

    The JVO ALMA Archive provides users one of the easiest ways to access the ALMA archival data. The users can have a quick look at a 3 or 4-dimensional data cube without downloading multiple huge tarballs from a science portal of ALMA Regional Centers (ARCs). Since we just synchronize all datasets with those of ARCs, the metadata are identical to the upstream, including ``target name'' for each dataset. The name is not necessarily a common one like NGC numbers, but sometimes one of sequential numbers assigned in an observation proposal. Compilation of these artificial names into astronomical ones could provide users more flexible and powerful search interfaces; for instance, with the knowledge of the redshift for each source, the users can easily find the datasets which observed their interested emission/absorption lines at not the observer frame but the rest frame, fitting well with theoretical studies. To implement this functionality, cross-identification of all the sources in our archive with those in some o...

  19. Prototype Implementation of Web and Desktop Applications for ALMA Science Verification Data and the Lessons Learned

    Science.gov (United States)

    Eguchi, S.; Kawasaki, W.; Shirasaki, Y.; Komiya, Y.; Kosugi, G.; Ohishi, M.; Mizumoto, Y.

    2013-10-01

    ALMA is estimated to generate TB scale data during only one observation; astronomers need to identify which part of the data they are really interested in. We have been developing new GUI software for this purpose utilizing the VO interface: ALMA Web Quick Look System (ALMAWebQL) and ALMA Desktop Application (Vissage). The former is written in JavaScript and HTML5 generated from Java code by the Google Web Toolkit, and the latter is in pure Java. An essential point of our approach is how to reduce network traffic: we prepare, in advance, “compressed” FITS files of 2x2x1 (horizontal, vertical, and spectral directions, respectively) binning, 2 x 2 x 2 binning, 4 x 4 x 2 binning data, and so on. These files are hidden from users, and Web QL automatically chooses the proper one for each user operation. Through this work, we find that network traffic in our system is still a bottleneck towards TB scale data distribution. Hence we have to develop alternative data containers for much faster data processing. In this paper, we introduce our data analysis systems, and describe what we learned through the development.

  20. ALMA-resolved salt emission traces the chemical footprint and inner wind morphology of VY CMa

    CERN Document Server

    Decin, L; Millar, T J; Baudry, A; De Beck, E; Homan, W; Smith, N; Van de Sande, M; Walsh, C

    2016-01-01

    (abreviated) We aim to study the inner-wind structure (R<250 Rstar) of the well-known red supergiant VY CMa. We analyse high spatial resolution (~0".24x0".13) ALMA Science Verification (SV) data in band 7 in which four thermal emission lines of gaseous sodium chloride (NaCl) are present at high signal-to-noise ratio. For the first time, the NaCl emission in the inner wind region of VY CMa is spatially resolved. The ALMA observations reveal the contribution of up to four different spatial regions. The NaCl emission pattern is different compared to the dust continuum and TiO2 emission already analysed from the ALMA SV data. The emission can be reconciled with an axisymmetric geometry, where the lower density polar/rotation axis has a position angle of ~50 degrees measured from north to east. However, this picture can not capture the full morphological diversity, and discrete mass ejection events need to be invoked to explain localized higher-density regions. The velocity traced by the gaseous NaCl line profi...

  1. Detection of lensing substructure using ALMA observations of the dusty galaxy SDP.81

    CERN Document Server

    Hezaveh, Yashar D; Marrone, Daniel P; Mao, Yao-Yuan; Morningstar, Warren; Wen, Di; Blandford, Roger D; Carlstrom, John E; Fassnacht, Christopher D; Holder, Gilbert P; Kemball, Athol; Marshall, Philip J; Murray, Norman; Levasseur, Laurence Perreault; Vieira, Joaquin D; Wechsler, Risa H

    2016-01-01

    We study the abundance of substructure in the matter density near galaxies using ALMA Science Verification observations of the strong lensing system SDP.81. We present a method to measure the abundance of subhalos around galaxies using interferometric observations of gravitational lenses. Using simulated ALMA observations, we explore the effects of various systematics, including antenna phase errors and source priors, and show how such errors may be measured or marginalized. We apply our formalism to ALMA observations of SDP.81. We find evidence for the presence of a $M=10^{8.96\\pm 0.12} M_{\\odot}$ subhalo near one of the images, with a significance of $6.9\\sigma$ in a joint fit to data from bands 6 and 7; the effect of the subhalo is also detected in both bands individually. We also derive constraints on the abundance of dark matter subhalos down to $M\\sim 2\\times 10^7 M_{\\odot}$, pushing down to the mass regime of the smallest detected satellites in the Local Group, where there are significant discrepancies...

  2. ALMA continuum observations of a 30 Myr old gaseous debris disk around HD 21997

    CERN Document Server

    Moór, A; Kóspál, Á; Ábrahám, P; Apai, D; Csengeri, T; Grady, C; Henning, Th; Hughes, A M; Kiss, Cs; Pascucci, I; Schmalzl, M; Gabányi, K

    2013-01-01

    Circumstellar disks around stars older than 10 Myr are expected to be gas-poor. There are, however, two examples of old (30-40 Myr) debris-like disks containing a detectable amount of cold CO gas. Here we present ALMA and Herschel Space Observatory observations of one of these disks, around HD 21997, and study the distribution and origin of the dust and its connection to the gas. Our ALMA continuum images at 886um clearly resolve a broad ring of emission within a diameter of ~4.5 arcsec, adding HD 21997 to the dozen debris disks resolved at (sub)millimeter wavelengths. Modeling the morphology of the ALMA image with a radiative transfer code suggests inner and outer radii of ~55 and ~150 AU, and a dust mass of 0.09 M_Earth. Our data and modeling hints at an extended cold outskirt of the ring. Comparison with the morphology of the CO gas in the disk reveals an inner dust-free hole where gas nevertheless can be detected. Based on dust grain lifetimes, we propose that the dust content of this gaseous disk is of s...

  3. Observing the Circumstellar Environment of the Eruptive FUor/EXor Protostar V1647 Ori with ALMA

    Science.gov (United States)

    Principe, David; Cieza, Lucas A.; Zhu, Zhaohuan; Tobin, John J.; Prieto, Jose Luis

    2016-01-01

    Fu Ori (FUor) and EXor objects represent a short-lived stage of protostellar evolution characterized by intense mass accretion events which cause extreme variability in the form of outbursts. While it is well demonstrated that these objects exhibit sudden outbursts (ΔV~2-6), the mechanism causing such variability is not well understood. High spatial and spectral resolution observations of the circumstellar environment of these objects are essential to distinguish between different outbursting mechanisms. We present ALMA observations of the FUor/EXor object V1647 Ori as part of an ALMA campaign, which has observed a combined eight FUor and EXor type objects. Deeply embedded in the dark cloud LDN 1630 (L1630), V1647 Ori is one of a few FUor/EXor objects to have been extensively studied at multiple wavelengths before, during and after an outburst. We present preliminary results derived from ALMA 12CO, 13CO, C18O and continuum observations of the circumstellar environment of V1647 Ori. By measuring gas/dust masses and gas kinematics of the circumstellar disk, we investigate the potential mechanisms producing variability in these eruptive protostars during an essential, yet rarely observed, stage of pre-main sequence stellar evolution.

  4. ALMA observations of Lyman-alpha Blob 1: halo sub-structure illuminated from within

    CERN Document Server

    Geach, J E; Matsuda, Y; Hayes, M; Mas-Ribas, Ll; Dijkstra, M; Steidel, C C; Chapman, S C; Feldmann, R; Avison, A; Agertz, O; Ao, Y; Birkinshaw, M; Bremer, M N; Clements, D L; Dannerbauer, H; Farrah, D; Harrison, C M; Hine, N K; Kubo, M; Michalowski, M J; Scott, Douglas; Smith, D J B; Spaans, M; Simpson, J M; Swinbank, A M; Taniguchi, Y; van Kampen, E; van der Werf, P; Verma, A; Yamada, T

    2016-01-01

    We present new Atacama Large Millimeter/Submillimeter Array (ALMA) 850um continuum observations of the original Lyman-alpha Blob (LAB) in the SSA22 field at z=3.1 (SSA22-LAB01). The ALMA map resolves the previously identified submillimeter source into three components with total flux density S_850 = 1.68+/-0.06 mJy, corresponding to a star formation rate of ~150 M_sun/yr. The submillimeter sources are associated with several faint (m~27 mag) rest-frame ultraviolet sources identified in Hubble Space Telescope Imaging Spectrograph (STIS) clear filter imaging (~5850A). One of these companions is spectroscopically confirmed with Keck MOSFIRE to lie within 20 projected kpc and 250 km/s of one of the ALMA components. We postulate that some of these STIS sources represent a population of low-mass star-forming satellites surrounding the central submillimeter sources, potentially contributing to their growth and activity through accretion. Using a high resolution cosmological zoom simulation of a 10^13 M_sun halo at z...

  5. Información del conocimiento organizacional a través de los informes anuales publicados en las páginas web de las empresas

    Directory of Open Access Journals (Sweden)

    Tejedo Romero, Francisca

    2014-03-01

    Full Text Available Internet is a means of communication and transmission of information that has led companies to develop their business activities in knowledge-based economies. Knowledge has become the most important resource for creating competitive advantages, specifically the knowledge incorporated by companies into their processes, systems, culture, R&D, i.e., their organizational knowledge (Structural Capital. Therefore, Structural Capital disclosures by companies can improve their reputation. Thus, the objective of our work has focused on analysing the information on organizational knowledge supplied by companies in annual reports posted on their websites, as well as on its evolution over the years studied.Internet es un medio de comunicación y transmisión de información que ha dado lugar a que las empresas desarrollen su actividad en economías basadas en el conocimiento. El conocimiento se ha convertido en el recurso más importante para la creación de ventajas competitivas, en particular el conocimiento que las empresas han incorporado en sus procesos, sistemas, cultura, I+D, es decir, su conocimiento organizacional (Capital Estructural. Por ello, la publicación de información por parte de las empresas sobre su Capital Estructural puede mejorar la reputación de las mismas. Así, el objetivo de este trabajo se ha centrado en analizar la cantidad de información sobre el conocimiento organizacional que suministran las empresas en los informes anuales obtenidos de sus páginas web, así como la evolución sufrida en los años objeto de estudio.

  6. Malaria control in the African Region: perceptions and viewspoints on proceedings of the Africa Leaders Malaria Alliance (ALMA

    Directory of Open Access Journals (Sweden)

    Sambo Luis

    2011-06-01

    Full Text Available Abstract Background In 2009 a total of 153,408 malaria deaths were reported in Africa. Eleven countries showed a reduction of more than 50% in either confirmed malaria cases or malaria admissions and deaths in recent years. However, many African countries are not on track to achieve the malaria component of the Millennium Development Goal (MDG 6. The African Leaders Malaria Alliance (ALMA working session at the 15th African Union Summit discussed the bottlenecks to achieving MDG 6 (specifically halting and beginning to reverse the incidence of malaria by 2015, success factors, and what countries needed to do to accelerate achievement of the MDG. The purpose of this article is to reflect on the proceedings of the ALMA working session. Methods Working methods of the session included speeches and statements by invited speakers and high-level panel discussions. Discussion The main bottlenecks identified related to the capacity of the health systems to deliver quality care and accessibility issues; need for strong, decentralized malaria-control programmes with linkages with other health and development sectors, the civil society and private sector entities; benefits of co-implementation of malaria control programmes with child survival or other public health interventions; systematic application of integrated promotive, preventive, diagnostic and case management interventions with full community participation; adapting approaches to local political, socio-cultural and administrative environments. The following prerequisites for success were identified: a clear vision and effective leadership of national malaria control programmes; high level political commitment to ensure adequate capacity in expertise, skill mix and number of managers, technicians and service providers; national ownership, intersectoral collaboration and accountability, as well as strong civil society and private sector involvement; functional epidemiological surveillance systems

  7. Envidia, carcoma del alma: escorzo psico-literario

    Directory of Open Access Journals (Sweden)

    TERESA SÁNCHEZ SÁNCHEZ

    2004-01-01

    Full Text Available Desde Aristóteles hasta Castilla del Pino, desde Covarrubias hasta María Zambrano, desde el clasicismo grecolatino a la modernidad de los Simposiums de Psicología y Psicoanálisis, el tema de la envidia ha sido objeto de análisis. Tan sutiles matices provienen de la filosofía como de la psicología, de la literatura como de la clínica. La envidia es sometida a la mirada benevolente que exige su rango de emoción universal humana, derivada de la alteridad, la comparación y la autovaloración negativa, así como de la deficiente instalación narcisística y el anhelo de suplantación del otro idealizado. La envidia es antesala del odio y de un cortejo de expresiones interpersonales y sociales muy variadas y sibilinas. Anida, incluso, tras el choque de civilizaciones generador de los más atroces y destructivos episodios de fanatismo terrorista recientemente padecidos en nuestro mundo.

  8. Observaciones sobre chamanismo y el rito del bautismo entre los Ava-Katu-Ete

    Directory of Open Access Journals (Sweden)

    Hugo Florencio Centurion Mereles

    2013-05-01

    Full Text Available La cultura Ava-Katu-Ete, los menos estudiados en el Paraguay pero en contraste los que han logrado una mayor compenetración con la sociedad nacional, es una cultura de la palabra. Y como alma y palabra son la misma cosa, al ser producto del contacto con los Dioses, son palabras verdaderas, por eso en el ritual del bautismo es donde el chamán a través de la imposición del nombre del monte que realiza la unión del niño con la naturaleza y, pasa a tener su nombre-alma. En esta cultura centrada en la palabra, el chamán cumple un papel fundamental, al ser los elegidos por los Dioses para a través de los sueños recibir las palabras sagradas que indican el camino verdadero, el camino de la perfección, aspiración última Ava-Katu-Ete

  9. ¿Es posible comparar el empleo informal en los países de América del Sur? Análisis de su definición, clasificación y medición

    Directory of Open Access Journals (Sweden)

    Marisol E. Ruiz

    2015-01-01

    Conclusiones: Una definición precisa y adecuada de empleo informal permitirá contemplar los matices que incluye el concepto, lo que hará posible visibilizar las carencias que afrontan la mayoría de los trabajadores informales. La necesidad de incorporar indicadores comunes entre los sistemas de información es un aspecto clave para efectuar comparaciones válidas entre países, así como para determinar el impacto sobre la salud pública que sufre la población empleada informalmente.

  10. INFORME SOBRE LA SITUACIÓN DE LOS DERECHOS HUMANOS Y EL DERECHO INTERNACIONAL HUMANITARIO EN EL ORIENTE ANTIOQUEÑO

    Directory of Open Access Journals (Sweden)

    Mesa de derechos humanos y protección humanitaria del Oriente Antioqueño

    2008-12-01

    Full Text Available El presente informe sobre la situación de Derechos Humanos y Derecho Internacional Humanitario en el Oriente del Departamento de Antioquia (Colombia es el producto del trabajo de la Mesa de Derechos Humanos y Protección Humanitaria del Oriente Antioqueño. Acompañados en la fundamentación y presentación por el equipo de profesionales de los proyectos Unidad Móvil de Derechos Humanos y Observatorio de Paz del Oriente Antioqueño, como apoyo técnico y en terreno a su labor. Se promueve como evidencia del compromiso de la Mesa en la defensa y promoción de los Derechos Humanos y de su fortalecimiento como escenario de articulación interinstitucional. Confluyen en ella organismos de carácter gubernamental y ciudadano de orden local, departamental e internacional querealizan el seguimiento a una de las crisis humanitarias de mayor dimensión en la geografía nacional a través de actividades como sesiones permanentes de observación y análisis a la situación social y política de la región, jornadas de acompañamiento a comunidades vulneradas o en riesgo, seguimiento en situaciones de emergencia mediante misiones a terreno, asesoría jurídica a las víctimas y fortalecimiento a la institucionalidad pública.

  11. Herschel-ATLAS and ALMA: HATLAS J142935.3-002836, a lensed major merger at redshift 1.027

    CERN Document Server

    Messias, Hugo; Nagar, Neil; Orellana, Gustavo; Bussmann, R Shane; Calanog, Jae; Dannerbauer, Helmut; Fu, Hai; Ibar, Edo; Inohara, Andrew; Ivison, R J; Negrello, Mattia; Riechers, Dominik A; Sheen, Yun-Kyeong; Amber, Simon; Birkinshaw, Mark; Bourne, Nathan; Clements, Dave L; Cooray, Asantha; De Zotti, Gianfranco; Demarco, Ricardo; Dunne, Loretta; Eales, Stephen; Fleuren, Simone; Lupu, Roxana E; Maddox, Steve J; Michalowski, Michal J; Omont, Alain; Rowlands, Kate; Smith, Dan; Smith, Matt; Valiante, Elisabetta

    2014-01-01

    [Abridged] Aims: This work focuses on one lensed system, HATLAS J142935.3-002836 (H1429-0028), selected in the Herschel-ATLAS field. Gathering a rich, multi-wavelength dataset, we aim to confirm the lensing hypothesis and model the background source's morphology and dynamics, as well as to provide a full physical characterisation. Methods: Multi-wavelength high-resolution data is utilised to assess the nature of the system. A lensing-analysis algorithm which simultaneously fits different wavebands is adopted to characterise the lens. The background galaxy dynamical information is studied by reconstructing the 3-D source-plane of the ALMA CO(J:4-3) transition. Near-IR imaging from HST and Keck-AO allows to constrain rest-frame optical photometry independently for the foreground and background systems. Physical parameters (such as stellar and dust masses) are estimated via modelling of the spectral energy distribution taking into account source blending, foreground obscuration, and differential magnification. R...

  12. Deep ALMA imaging of the merger NGC1614 - Is CO tracing a massive inflow of non-starforming gas?

    CERN Document Server

    König, S; Muller, S; Gallagher, J S; Beswick, R J; Xu, C K; Evans, A

    2016-01-01

    Observations of the molecular gas over scales of ~0.5 to several kpc provide crucial information on how the gas moves through galaxies, especially in mergers and interacting systems, where it ultimately reaches the galaxy center, accumulates and feeds nuclear activity. To understand the processes involved in gas transport is one of the important steps forward to understand galaxy evolution. 12CO and 13CO1-0 high-sensitivity ALMA observations are used to assess properties of the large-scale molecular gas reservoir and its connection to the circumnuclear molecular ring in NGC1614. The role of excitation and abundances are studied in this context. Spatial distributions of the 12CO and 13CO 1-0 emission show significant differences. 12CO is tracing large-scale molecular gas reservoir associated with a dust lane associated with infalling gas and extends into the southern tidal tails. 13CO emission peaks at the connection between the dust lane and the circumnuclear molecular ring found in previous observations and ...

  13. An ALMA Early Science survey of molecular absorption lines toward PKS1830-211 -- Analysis of the absorption profiles

    CERN Document Server

    Muller, S; Guelin, M; Gerin, M; Aalto, S; Beelen, A; Black, J H; Curran, S J; Darling, J; Dinh-V-Trung,; Garcia-Burillo, S; Henkel, C; Horellou, C; Martin, S; Marti-Vidal, I; Menten, K M; Murphy, M T; Ott, J; Wiklind, T; Zwaan, M A

    2014-01-01

    We present the first results of an ALMA spectral survey of strong absorption lines for common interstellar species in the z=0.89 molecular absorber toward the lensed blazar PKS1830-211. The dataset brings essential information on the structure and composition of the absorbing gas in the foreground galaxy. In particular, we find absorption over large velocity intervals (gtrsim 100 km/s) toward both lensed images of the blazar. This suggests either that the galaxy inclination is intermediate and that we sample velocity gradients or streaming motions in the disk plane, that the molecular gas has a large vertical distribution or extraplanar components, or that the absorber is not a simple spiral galaxy but might be a merger system. The number of detected species is now reaching a total of 42 different species plus 14 different rare isotopologues toward the SW image, and 14 species toward the NE line-of-sight. The abundances of CH, H2O, HCO+, HCN, and NH3 relative to H2 are found to be comparable to those in the G...

  14. The ALMA Redshift 4 Survey (AR4S): I. The massive end of the z=4 main sequence of galaxies

    CERN Document Server

    Schreiber, C; Leiton, R; Elbaz, D; Wang, T; Okumura, K; Labbé, I

    2016-01-01

    We introduce the ALMA Redshift 4 Survey (AR4S), a systematic ALMA survey of all the known galaxies with stellar mass (M*) larger than 5e10 Msun at 3.5ALMA at 890um (180um rest-frame) with an on-source integration time of 1.3 min per galaxy. We detect 32% of the sample at more than 3 sigma significance. Using the stacked ALMA and Herschel photometry, we derive an average dust temperature of 40+/-2 K for the whole sample, and extrapolate the Lir and SFR for all our galaxies based on their ALMA flux. We then use a forward modeling approach to estimate their intrinsic sSFR distribution, deconvolved of measurement errors and selection effects: we find a linear relation between SFR and M*, with a median sSFR=2.8+/-0.8 Gyr and a dispersion around that relation of 0.28+/-0.13 dex. This latter value is consistent with that measured at lower redshifts, which is proof that the main ...

  15. Avaliação de modelos de estimativa da radiação solar incidente em Cruz das Almas, Bahia Evaluating models for estimation of incoming solar radiation in Cruz das Almas, Bahia, Brazil

    Directory of Open Access Journals (Sweden)

    Valéria P. Borges

    2010-01-01

    Full Text Available Em estudos agroambientais a radiação solar incidente (Rs é uma das mais importantes variáveis meteorológicas. Na ausência de dados observados de Rs é possível estimá-los mediante modelos. O objetivo deste estudo foi avaliar modelos baseados na temperatura do ar para estimativa diária de Rs nas condições do Recôncavo Sul da Bahia. Utilizaram-se dados de Rs do período de 2004 a 2006, medidos por uma estação meteorológica automática pertencente ao INMET, instalada em Cruz das Almas, Bahia. Como etapa preliminar, verificou-se a qualidade dos dados de Rs tomando-se como referência curvas de radiação esperada em dias claros. Os seguintes modelos foram avaliados: Hargreaves-Samani para regiões interiores e regiões costeiras, Thornton-Running e o de Weiss. O desempenho de cada método foi avaliado através dos seguintes indicadores: coeficiente de determinção (R², razão média (RM, erro absoluto médio (EAM, raiz quadrada do quadrado médio do erro (RQME e índice de concordância de Wilmott (dW. Os resultados obtidos recomendam o modelo de Hargreaves-Samani para regiões costeiras por apresentar o valor de RM mais próximo de 1 (1,01, menor EAM (2,54 MJ m-2 d-1, menor RQME (3,13 MJ m-2 d-1 e o maior dW (0,90.Solar radiation at the earth's surface (Rs is one of the essential weather variables for several agro-environmental studies. In the absence of measured Rs, it's possible to simulate them by models. Using three years of daily Rs data (2004-2006 collected by an INMET (Brazilian Meteorological Service automatic weather station installed in the municipality of Cruz das Almas, BA, three air temperature-based Rs simulation models were evaluated. As a preliminary step, data quality was investigated and, when needed, adjustments were made based on clear sky solar radiation envelopes. The following models were evaluated: Hargreaves-Samani for both interior and coastal regions, Thornton-Running, and the Weiss model. Linear

  16. Del ENIAC, hasta los andares

    OpenAIRE

    Molero Prieto, Xavier

    2014-01-01

    Si bien los computadores actuales, en todas sus variantes —portátiles, tabletas, teléfonos inteligentes—, resultan más pequeños, baratos y rápidos que los precedentes, no es menos cierto que el estudio minucioso de las viejas glorias de la historia de la informática nos puede facilitar la comprensión, no solo de algunos de los aspectos de la tecnología informática de aquel momento e incluso de la actual, sino también de los rasgos socioculturales propios del entorno científico y huma...

  17. Los Cactos

    Directory of Open Access Journals (Sweden)

    García Paredes Antonio

    1942-12-01

    Full Text Available El Cacto Cactus es uno de los géneros de plantas de la familia de las Cacteas Nopaleas que contiene muchas especies y variedades todas de formas extrañas, propias de la América intertropical y que habitan en los climas fríos y templados, en terrenos secos y estériles, desde el norte de Méjico hasta la Patagonia. Algunos cactos se cultivan por sus frutos que son sanosy sabrosos, otros como plantas ornamentales en los parques y jardines, otros como auxiliares para la industria, como los nopales en los que se cría la Cochinilla, insecto de la familia de los Hemípteros que produce la laca o carmín, materia colorante indispensable en la pintura al óleo y la acuarela, y por último, hoy están en moda y se cultivan con esmero una gran variedad de diminutos cactos exóticosque se mantienen sobre arena húmeda en pequeñas maceteras de porcelana, en los lugares más visibles de las habitaciones.

  18. Desvelando o cotidiano dos cuidadores informais de idosos Revelando el cotidiano de los cuidadores informales de ancianos Unveiling the routine of informal caregivers for the elderly

    Directory of Open Access Journals (Sweden)

    Michel Patrick Fonseca Rocha

    2008-12-01

    Full Text Available Este artigo objetivou descrever como os cuidadores informais de idosos interpretam e constroem o seu cotidiano. Estudo qualitativo, descritivo-exploratório, tendo como orientação teórico-metodológica, a dialética. O instrumento de coleta de dados foi a entrevista individual, com cinco cuidadores de idosos dependentes em domicílios de um Programa Saúde da Família, em Montes Claros Minas Gerais. Resultados evidenciaram situações adversas enfrentadas pelos cuidadores relacionadas ao sofrimento e sacrifícios na prestação dos cuidados e a falta de assistência para atender as necessidades do ser cuidado e do ser cuidador. Porém, exercem o cuidar com amor, carinho e dedicação, utilizando a fé e a espiritualidade como busca do equilíbrio biopsicossocial. Recomenda-se que esses profissionais tenham um olhar respeitoso e cooperativo ao trabalho desses cuidadores.El propósito del presente artículo ha sido describir cómo los cuidadores informales de ancianos interpretan y construyen su rutina. Se trata de un estudio cualitativo, descriptivo y exploratorio, con orientación teórico-metodológica. La recogida de datos se realizó mediante entrevistas individuales a cinco cuidadores de personas mayores dependientes que viven en domicilios incluidos en un Programa de Salud de la Familia de Montes Claros, Estado de Minas Gerais. Los resultados revelan que los cuidadores enfrentan situaciones hostiles que tienen que ver con sufrimiento y sacrificios en la prestación de los cuidados y con la falta de asistencia para atender a las necesidades del anciano y del cuidador. Pero, ejercen su tarea con amor, cariño y dedicación y, a través de la fe y de la espiritualidad, buscan su equilibrio biopsicosocial. Se aconseja que el trabajo de estos profesionales sea considerado com respecto y cooperación.This article intends to describe how the informal caregivers interpret and build their daily routine. It is a qualitative study using dialectics

  19. La educación informal de los medios de comunicación y la protección de los menores de la violencia en televisión: historia de un fracaso

    Directory of Open Access Journals (Sweden)

    Ángel Liceras Ruiz

    2014-01-01

    Full Text Available Recientes estudios muestran una preocupante complacencia de los niños y jóvenes con el uso de la violencia como práctica para obtener sus deseos. Salvando el debate y desacuerdo entre los investigadores sobre la naturaleza de la influencia de la televisión, asumimos la perspectiva de que, en todo caso, el tema de las repercusiones y el tratamiento de los contenidos televisivos es una cuestión cívica, no meramente científica. Sin duda la televisión, con sus formidables recursos pedagógicos, resulta un poderoso agente educativo, y los niños y adolescentes son grandes consumidores de este medio. Junto a esto, una trayectoria de reiteradas y persistentes vulneraciones por parte de las televisiones de sus autocompromisos y de la normativa vigente en materia de comunicación y protección de los menores respecto a la emisión de contenidos inapropiados para su formación en los horarios de protección infantil son factores que no parecen ajenos a este panorama. Una violencia televisiva que se presenta ausente de dolor y consecuencias, justificable y con rasgos atractivos favorece su imitación e influencia. Son viejas denuncias de cuestiones de enorme importancia formativa y social que no parecen merecer la necesaria atención de los agentes con responsabilidades en la protección y educación de los niños y adolescentes. Profesores, padres, asociaciones de telespectadores, empresas audiovisuales, poderes públicos y sociedad en general deben afrontar su compromiso desde sus parcelas de competencia.

  20. La microempresarialidad informal en México durante los años noventa: un análisis de la dinámica de flujos laborales

    Directory of Open Access Journals (Sweden)

    José G. Aguilar Barceló

    2012-01-01

    Full Text Available Con datos de la Encuesta nacional de empleo urbano se calculan aproximaciones a las probabilidades de transición entre las categorías ocupacionales relacionadas con la microempresarialidad en México, para el periodo 1987- 1999. Según una visión dualista, se encuentra que mucha de la microempresarialidad informal podría considerarse involuntaria, al surgir del desempleo y la inactividad. No obstante, un subconjunto pequeño de este grupo muestra un comportamiento inverso al optar por la empresarialidad, cuando la demanda del mercado de trabajo era alta, y se toma como voluntaria y afín con la visión legalista y de economía neoclásica. La vía para llegar a ser patrón formal fue el autoempleo informal. Durante los gobiernos de Carlos Salinas y Ernesto Zedillo el flujo hacia la formalización microempresarial fue bajo, en parte debido a las dificultades que para este sector provocaron las políticas de ajuste macroeconómico.

  1. El protestantismo en la España de la II República a la luz de los informes del Archivo Secreto Vaticano

    Directory of Open Access Journals (Sweden)

    Hernández Figueiredo, José Ramón

    2011-06-01

    Full Text Available On the eve of the Second Republic, an important worry of the Catholic Church is the condition and development of the Protestantism in Spain. Such worry comes directly from the Pope Pio XI that through the Minister asks the Nuncio Tedeschini an exact and complete report about the different Christian confessions in the Iberican Peninsula. About it, there are abundant unpublished information that comes from all the Spanish dioceses.

    En vísperas de la Segunda República, una preocupación importante de la Iglesia es el estado y desarrollo del protestantismo en España. Tal preocupación procede directamente del Papa Pío XI que por medio del Secretario de Estado pide al Nuncio Tedeschini un informe exacto y completo de las diversas confesiones cristianas en la Península. Al respecto, son abundantes los datos inéditos que proceden de todas las diócesis españolas.

  2. Métricas de riesgos para los proyectos productivos de la Universidad de las Ciencias Informáticas. Risk Metrics for the Productive Projects at the University of Informatics Sciences

    Directory of Open Access Journals (Sweden)

    Neysis Hernández Díaz

    2012-09-01

    Full Text Available En el presente trabajo se proponen métricas para disminuir el impacto negativo de los riesgos en los proyectos productivos de la Universidad de las Ciencias Informáticas, basado en el modelo CMMI. Las métricas pueden medir el avance del proyecto, así como contribuir a la prevención de los riesgos y en caso de ocurrir un riesgo, permite a los líderes tomar decisiones correctas ante los problemas presentados. Múltiples factores influyen en el desarrollo de software con calidad: los recursos humanos y materiales, uso adecuado de técnicas y metodologías, la selección correcta de la tecnología, la planificación del tiempo y los costos. Mediante este análisis se obtienen un conjunto de métricas que permiten determinar el impacto de los riesgos en los proyecto productivos de la Universidad.The present work proposes metrics to decrease the negative impact of risks in productive projects from the University of Informatics Sciences, based on the CMMI model. Metrics can measure the development of the project, as well as contribute to prevent risks, and in case it happens, they allow leaders to make the right decisions for the problems presented. Multiple factors influence on the development of the software with quality: human and material resources, correct use of techniques and methodologies, appropriate selection of technology, time planning and costs. However, it is important to make a detailed study of risks and apply rules and quality standards proposed worldwide, which consider, as an important area, risk management. Through this analysis it is obtained a set of metrics that allow determining the impact of risks in the productive projects of the University.

  3. Risk Metrics for the Productive Projects at the University of Informatics Sciences Métricas de riesgos para los proyectos productivos de la Universidad de las Ciencias Informáticas.

    Directory of Open Access Journals (Sweden)

    Rachel Rachel Seijó

    2012-09-01

    Full Text Available The present work proposes metrics to decrease the negative impact of risks in productive projects from the University of Informatics Sciences, based on the CMMI model. Metrics can measure the development of the project, as well as contribute to prevent risks, and in case it happens, they allow leaders to make the right decisions for the problems presented. Multiple factors influence on the development of the software with quality: human and material resources, correct use of techniques and methodologies, appropriate selection of technology, time planning and costs. However, it is important to make a detailed study of risks and apply rules and quality standards proposed worldwide, which consider, as an important area, risk management. Through this analysis it is obtained a set of metrics that allow determining the impact of risks in the productive projects of the University. En el presente trabajo se proponen métricas para disminuir el impacto negativo de los riesgos en los proyectos productivos de la Universidad de las Ciencias Informáticas, basado en el modelo CMMI. Las métricas pueden medir el avance del proyecto, así como contribuir a la prevención de los riesgos y en caso de ocurrir un riesgo, permite a los líderes tomar decisiones correctas ante los problemas presentados. Múltiples factores influyen en el desarrollo de software con calidad: los recursos humanos y materiales, uso adecuado de técnicas y metodologías, la selección correcta de la tecnología, la planificación del tiempo y los costos. Mediante este análisis se obtienen un conjunto de métricas que permiten determinar el impacto de los riesgos en los proyecto productivos de la Universidad.

  4. Destinos de la Herejía de los Padres Latinos a los Carolingios

    Directory of Open Access Journals (Sweden)

    Alfonso Hernandez

    2009-01-01

    Full Text Available El cristianismo tiene la particularidad de ser una religión salvífica en contraste con el paganismo que desconoce la idea de salvación del alma, entre otras cosas por desconocer también la idea de caída o pecado original. La preocupación por cómo salvarse llevó a la iglesia cristiana ya en la antigüedad a intentar definir con claridad cuáles eran las creencias fundamentales a través de las cuales los bautizados podían acceder a la salvación. La condición salvífica del cristianismo condujo al ...

  5. Destinos de la Herejía de los Padres Latinos a los Carolingios

    OpenAIRE

    Alfonso Hernandez

    2009-01-01

    El cristianismo tiene la particularidad de ser una religión salvífica en contraste con el paganismo que desconoce la idea de salvación del alma, entre otras cosas por desconocer también la idea de caída o pecado original. La preocupación por cómo salvarse llevó a la iglesia cristiana ya en la antigüedad a intentar definir con claridad cuáles eran las creencias fundamentales a través de las cuales los bautizados podían acceder a la salvación. La condición salvífica del cristianismo condujo al ...

  6. ALMA OBSERVATIONS OF THE DEBRIS DISK AROUND THE YOUNG SOLAR ANALOG HD 107146

    Energy Technology Data Exchange (ETDEWEB)

    Ricci, L.; Carpenter, J. M.; Fu, B. [Department of Astronomy, California Institute of Technology, MC 249-17, Pasadena, CA 91125 (United States); Hughes, A. M. [Department of Astronomy, Wesleyan University, Van Vleck Observatory, 96 Foss Hill Drive, Midletown, CT 06457 (United States); Corder, S. [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Isella, A., E-mail: lricci@astro.caltech.edu [Department of Physics and Astronomy, Rice University, 6100 South Main, Houston, TX 77521-1892 (United States)

    2015-01-10

    We present the Atacama Large Millimeter/submillimeter Array (ALMA) continuum observations at a wavelength of 1.25 mm of the debris disk surrounding the ∼100 Myr old solar analog HD 107146. The continuum emission extends from about 30 to 150 AU from the central star with a decrease in the surface brightness at intermediate radii. We analyze the ALMA interferometric visibilities using debris disk models with radial profiles for the dust surface density parameterized as (1) a single power law, (2) a single power law with a gap, and (3) a double power law. We find that models with a gap of radial width ∼8 AU at a distance of ∼80 AU from the central star, as well as double power-law models with a dip in the dust surface density at ∼70 AU provide significantly better fits to the ALMA data than single power-law models. We discuss possible scenarios for the origin of the HD 107146 debris disk using models of planetesimal belts in which the formation of Pluto-sized objects trigger disruptive collisions of large bodies, as well as models that consider the interaction of a planetary system with a planetesimal belt and spatial variation of the dust opacity across the disk. If future observations with higher angular resolution and sensitivity confirm the fully depleted gap structure discussed here, a planet with a mass of approximately a few Earth masses in a nearly circular orbit at ∼80 AU from the central star would be a possible explanation for the presence of the gap.

  7. El empleo informal en la frontera norte de México y el caso de Sonora: un análisis de expectativas en los ingresos

    Directory of Open Access Journals (Sweden)

    Luis Huesca Reynoso

    2010-01-01

    Full Text Available En el presente documento se muestra la distribución de los ingresos para trabajadores formales e informales en la frontera norte y en Sonora; se observó más participación de los jornaleros agrícolas informales y de quienes trabajan por cuenta propia. Con la base de datos de la Encuesta nacional de ocupación y empleo de 2006, se calculó un escenario contrafactual con la asunción de lo que pasaría con la distribución de los salarios si los informales se desempeñaran como empleados formales. Los resultados indican que los informales asalariados y por cuenta propia están en mejor situación, y es menos favorable la expectativa para los segundos en Sonora, así como para los jornaleros agrícolas en ambos lugares. Los informales por cuenta propia no cambian sustancialmente sus ingresos, si se ubican en la parte alta de la distribución en Sonora, y hay una polarización de las percepciones en los asalariados en la frontera.

  8. Cross-polarization in quasi-optical receivers: ALMA band 4 and 10

    Science.gov (United States)

    Gonzalez, A.; Uzawa, Y.

    2012-09-01

    A careful study about the influence of individual optical components on receiver cross-polarization has been performed. The basic mechanisms of generation of cross-polarization in ellipsoidal mirrors and dielectrics have been reviewed and characterized in terms of higher-order Gaussian beam modes. A simple model considering the phase differences of different Gaussian beam modes is proposed in order to calculate the final system cross-polarization pattern. This model has been successfully used to characterize the total cross-polarization in two cryogenically-cooled receivers for astronomy: ALMA band 4 and band 10.

  9. A dor de amor na medicina da alma da primeira modernidade

    Directory of Open Access Journals (Sweden)

    Paulo José Carvalho da Silva

    2008-09-01

    Full Text Available Este artigo discute o problema da dor de amor nos diferentes campos do saber que compunham a medicina da alma da primeira modernidade. Deu-se especial destaque às reflexões do médico francês Jacques Ferrand (1575-1623 sobre o caráter instável, ilusório e faltoso do amor. Conclui-se que a dor de amor exige pensar as relações entre os afetos e o corpo, além de desafiar as próprias categorias diagnósticas e os tratamentos tradicionais.

  10. ALMA view of the Galactic Center 50km/s molecular cloud

    CERN Document Server

    Uehara, Kenta; Kitamura, Yoshimi; Miyawaki, Ryosuke; Miyazaki, Atsushi

    2016-01-01

    We have observed the Galactic Center 50km/s molecular cloud (50MC) with ALMA to search for filamentary structures. In the CS J=2-1 emission line channel maps, we succeeded in identifying 27 molecular cloud filaments using the DisPerSE algorithm. This is the first attempt of "filament-finding" in the Galactic Center Region. These molecular cloud filaments strongly suggest that the molecular cloud filaments are also ubiquitous in the molecular clouds of the Galactic Center Region.

  11. Engineering within the assembly, verification, and integration (AIV) process in ALMA

    Science.gov (United States)

    Lopez, Bernhard; McMullin, Joseph P.; Whyborn, Nicholas D.; Duvall, Eugene

    2010-07-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) is a joint project between astronomical organizations in Europe, North America, and East Asia, in collaboration with the Republic of Chile. ALMA will consist of at least 54 twelve-meter antennas and 12 seven-meter antennas operating as an interferometer in the millimeter and sub-millimeter wavelength range. It will be located at an altitude above 5000m in the Chilean Atacama desert. As part of the ALMA construction phase the Assembly, Verification and Integration (AIV) team receives antennas and instrumentation from Integrated Product Teams (IPTs), verifies that the sub-systems perform as expected, performs the assembly and integration of the scientific instrumentation and verifies that functional and performance requirements are met. This paper aims to describe those aspects related to the AIV Engineering team, its role within the 4-station AIV process, the different phases the group underwent, lessons learned and potential space for improvement. AIV Engineering initially focused on the preparation of the necessary site infrastructure for AIV activities, on the purchase of tools and equipment and on the first ALMA system installations. With the first antennas arriving on site the team started to gather experience with AIV Station 1 beacon holography measurements for the assessment of the overall antenna surface quality, and with optical pointing to confirm the antenna pointing and tracking capabilities. With the arrival of the first receiver AIV Station 2 was developed which focuses on the installation of electrical and cryogenic systems and incrementally establishes the full connectivity of the antenna as an observing platform. Further antenna deliveries then allowed to refine the related procedures, develop staff expertise and to transition towards a more routine production process. Stations 3 and 4 deal with verification of the antenna with integrated electronics by the AIV Science Team and is not covered

  12. ALMA Observations of Orion Source I at 350 and 660 GHz

    CERN Document Server

    Plambeck, R L

    2016-01-01

    Orion Source I ('SrcI') is the protostar at the center of the Kleinmann-Low Nebula. ALMA observations of SrcI at 350 and 660 GHz failed to detect the H26$\\alpha$ and H21$\\alpha$ recombination lines, ruling out the possibility that SrcI is a hypercompact HII region. The deconvolved size of the continuum source is approximately 0.23 x 0.05" (100 x 20 AU); it is interpreted as a disk viewed almost edge-on. The continuum flux density is proportional to $\

  13. ALMA detection of the rotating molecular disk wind from the young star HD 163296

    OpenAIRE

    Klaassen, P. D.; Juhasz, A.; Mathews, G. S.; Mottram, J. C.; de Gregorio-Monsalvo, I.; van Dishoeck, E. F.; Takahashi, S.; Akiyama, E.; Chapillon, E.; Espada, D.; Hales, A.; Hogerheijde, M.R.; Rawlings, M.; Schmalzl, M.; Testi, L.

    2013-01-01

    Disk winds have been postulated as a mechanism for angular momentum release in protostellar systems for decades. HD 163296 is a Herbig Ae star surrounded by a disk and has been shown to host a series of HH knots (HH 409) with bow shocks associated with the farthest knots. Here we present ALMA Science Verification data of CO J=2-1 and J=3-2 emission which are spatially coincident with the blue shifted jet of HH knots, and offset from the disk by -18.6 km/s. The emission has a double corkscrew ...

  14. U.S. and European ALMA Partners Sign Agreement Green Light for World's Most Powerful Radio Observatory

    Science.gov (United States)

    2003-02-01

    Dr. Rita Colwell, director of the U.S. National Science Foundation (NSF), and Dr. Catherine Cesarsky, director general of the European Southern Observatory (ESO), today signed a historic agreement jointly to construct and operate ALMA, the Atacama Large Millimeter Array, the world's largest and most powerful radio telescope operating at millimeter and sub-millimeter wavelengths. "With this agreement, we usher in a new age of research in astronomy," said Dr. Colwell. "By working together in this truly global partnership, the international astronomy community will be able to ensure the research capabilities needed to meet the long-term demands of our scientific enterprise, and we will be able to study and understand our Universe in ways that have previously been beyond our vision." ALMA Array Artist's Conception of ALMA Array in Compact Configuration (Click on Image for Larger Version) Other Images Available: Artist's conception of the antennas for the Atacama Large Millimeter Array Moonrise over ALMA test equipment near Cerro Chajnantor, Chile VertexRSI antenna at the VLA test site Dr. Cesarsky also commented, "This agreement signifies the start of a great project of contemporary astronomy and astrophysics. Representing Europe, and in collaboration with many laboratories and institutes on this continent, we together look forward toward wonderful research projects. With ALMA, we may learn how the earliest galaxies in the Universe really looked like, to mention but one of the many eagerly awaited opportunities with this marvelous facility." When complete in 2011, ALMA will be an array of 64, 12-meter radio antennas that will work together as one telescope to study millimeter and sub-millimeter wavelength light from space. These wavelengths of the electromagnetic spectrum, which cross the critical boundary between infrared and microwave radiation, hold the key to understanding such processes as planet and star formation, the formation of early galaxies and galaxy

  15. ALMA detected overdensity of sub-mm sources around WISE/NVSS-selected z~2 dusty quasars

    CERN Document Server

    Silva, Andrea; Lonsdale, Carol; Lacy, Mark

    2015-01-01

    We study the environments of 49 WISE/NVSS-selected dusty, hyper-luminous, z~2 quasars using the Atacama Large Millimeter/Sub-millimeter Array (ALMA) 345GHz images. We find that 17 of the 49 WISE/NVSS sources show additional sub-mm galaxies within the ALMA primary beam, probing scales within ~150 kpc. We find a total of 23 additional sub-mm sources, four of which in the field of a single WISE/NVSS source. The measured 870 um source counts are ~10 times expectations for unbiased regions, suggesting such hyper-luminous dusty quasars are excellent at probing high-density peaks.

  16. ALMA-resolved salt emission traces the chemical footprint and inner wind morphology of VY Canis Majoris

    OpenAIRE

    Decin, L.; Richards, A. M. S.; Millar, T.J.; Baudry, A.; Beck, E.; Homan, W.; Smith, N; van der Sande, M.; Walsh, C

    2016-01-01

    (abreviated) We aim to study the inner-wind structure (R<250 Rstar) of the well-known red supergiant VY CMa. We analyse high spatial resolution (~0".24x0".13) ALMA Science Verification (SV) data in band 7 in which four thermal emission lines of gaseous sodium chloride (NaCl) are present at high signal-to-noise ratio. For the first time, the NaCl emission in the inner wind region of VY CMa is spatially resolved. The ALMA observations reveal the contribution of up to four different spatial r...

  17. los aprendizajes

    Directory of Open Access Journals (Sweden)

    Graciela Pérez Rivera

    2007-01-01

    Full Text Available En este documento se presentan algunos resultados, obtenidos hasta el momento, de un estudio sobre las prácticas de evaluación de profesores universitarios. El propósito del estudio es participar en la búsqueda de las relaciones existentes entre los conceptos y las prácticas educativas, en este caso de evaluación. Se identifican las principales tendencias en cuanto a la concepción de la evaluación del aprendizaje y las funciones que se le otorgan, los propósitos con los que se evalúa, los objetos o contenidos a evaluar, las formas en que se lleva a cabo la evaluación y el uso que se da a los resultados. Identificar cuáles son las tendencias de las prácticas de evaluación en nuestras aulas universitarias representa un paso que puede ayudar a cuidar que este proceso tan importante recobre su papel formativo para todos aquellos quienes participamos en los procesos educativos; además, representa la posibilidad de construir formas para lograr mejorar nuestra labor docente en general, y en particular, nuestra práctica evaluativa.

  18. ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Survey Description

    CERN Document Server

    Walter, Fabian; Aravena, Manuel; Carilli, Chris; Bouwens, Rychard; da Cunha, Elisabete; Daddi, Emanuele; Ivison, R J; Riechers, Dominik; Smail, Ian; Swinbank, Mark; Weiss, Axel; Anguita, Timo; Assef, Roberto; Bacon, Roland; Bauer, Franz; Bell, Eric F; Bertoldi, Frank; Chapman, Scott; Colina, Luis; Cortes, Paulo C; Cox, Pierre; Dickinson, Mark; Elbaz, David; Gónzalez-López, Jorge; Ibar, Edo; Inami, Hanae; Infante, Leopoldo; Hodge, Jacqueline; Karim, Alex; Fevre, Olivier Le; Magnelli, Benjamin; Neri, Roberto; Oesch, Pascal; Ota, Kazuaki; Popping, Gergö; Rix, Hans-Walter; Sargent, Mark; Sheth, Kartik; van der Wel, Arjen; van der Werf, Paul; Wagg, Jeff

    2016-01-01

    We present the rationale for and the observational description of ASPECS: The ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (UDF), the cosmological deep field that has the deepest multi-wavelength data available. Our overarching goal is to obtain an unbiased census of molecular gas and dust continuum emission in high-redshift (z$>$0.5) galaxies. The $\\sim$1$'$ region covered within the UDF was chosen to overlap with the deepest available imaging from HST. Our ALMA observations consist of full frequency scans in band 3 (84-115 GHz) and band 6 (212-272 GHz) at approximately uniform line sensitivity ($L'_{\\rm CO}\\sim$2$\\times$10$^{9}$ K km/s pc$^2$), and continuum noise levels of 3.8 $\\mu$Jy beam$^{-1}$ and 12.7 $\\mu$Jy beam$^{-1}$, respectively. The molecular surveys cover the different rotational transitions of the CO molecule, leading to essentially full redshift coverage. The [CII] emission line is also covered at redshifts $6.0

  19. ALMA Reveals a Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole

    Science.gov (United States)

    Tremblay, Grant

    2016-01-01

    A new ALMA observation of the cool core brightest cluster galaxy in Abell 2597 reveals that a supermassive black hole can act much like a mechanical pump in a water fountain, driving a convective flow of molecular gas that drains into the black hole accretion reservoir, only to be pushed outward again in a jet-driven outflow that then rains back toward the galaxy center from which it came. The ALMA data reveal "shadows" cast by giant molecular clouds falling on ballistic trajectories towards the black hole in the innermost 500 parsecs of the galaxy, manifesting as deep redshifted continuum absorption features. The black hole accretion reservoir, fueled by these infalling cold clouds, powers an AGN that drives a jet-driven molecular outflow in the form of a 10 kpc-scale, billion solar mass expanding molecular bubble or plume. The molecular shell is permeated with young stars, perhaps triggered in situ by the jet. Buoyant X-ray cavities excavated by the propagating radio source may further uplift the molecular filaments, which are observed to fall inward toward the center of the galaxy from which they came, presumably keeping the fountain long-lived. The results show that cold molecular gas can couple to black hole growth via both feedback and feeding, in alignment with "cold chaotic accretion" models for the regulation of star formation in galaxies.

  20. An ALMA Survey for Disks Orbiting Low-Mass Stars in the TW Hya Association

    CERN Document Server

    Rodriguez, David R; Kastner, Joel H; Schneider, Adam C; Faherty, Jacqueline K; Mardones, Diego; Mohanty, Subhanjoy; Principe, David

    2015-01-01

    We have carried out an ALMA survey of 15 confirmed or candidate low-mass (<0.2M$_\\odot$) members of the TW Hya Association (TWA) with the goal of detecting molecular gas in the form of CO emission, as well as providing constraints on continuum emission due to cold dust. Our targets have spectral types of M4-L0 and hence represent the extreme low end of the TWA's mass function. Our ALMA survey has yielded detections of 1.3mm continuum emission around 4 systems (TWA 30B, 32, 33, & 34), suggesting the presence of cold dust grains. All continuum sources are unresolved. TWA 34 further shows 12CO(2-1) emission whose velocity structure is indicative of Keplerian rotation. Among the sample of known ~7-10 Myr-old star/disk systems, TWA 34, which lies just ~50 pc from Earth, is the lowest mass star thus far identified as harboring cold molecular gas in an orbiting disk.

  1. An ALMA Constraint on the GSC 6214-210 B Circum-Substellar Accretion Disk Mass

    CERN Document Server

    Bowler, Brendan P; Kraus, Adam L; Ireland, Michael J; Herczeg, Gregory; Ricci, Luca; Carpenter, John; Brown, Michael E

    2015-01-01

    We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of GSC 6214-210 A and B, a solar-mass member of the 5-10 Myr Upper Scorpius association with a 15 $\\pm$ 2 Mjup companion orbiting at $\\approx$330 AU (2.2"). Previous photometry and spectroscopy spanning 0.3-5 $\\mu$m revealed optical and thermal excess as well as strong H$\\alpha$ and Pa~$\\beta$ emission originating from a circum-substellar accretion disk around GSC 6214-210 B, making it the lowest mass companion with unambiguous evidence of a subdisk. Despite ALMA's unprecedented sensitivity and angular resolution, neither component was detected in our 880 $\\mu$m (341 GHz) continuum observations down to a 3-$\\sigma$ limit of 0.22 mJy/beam. The corresponding constraints on the dust mass and total mass are <0.15 Mearth and <0.05 Mjup, respectively, or <0.003% and <0.3% of the mass of GSC 6214-210 B itself assuming a 100:1 gas-to-dust ratio and characteristic dust temperature of 10-20 K. If the host star possesses a putative c...

  2. Gaps, Rings, and Non-Axisymmetric Structures in Protoplanetary Disks - From Simulations to ALMA Observations

    CERN Document Server

    Flock, M; Dzyurkevich, N; Henning, Th; Klahr, H; Wolf, S

    2014-01-01

    Recent observations by the Atacama Large Millimeter/submillimeter Array (ALMA) of disks around young stars revealed distinct asymmetries in the dust continuum emission. In this work we want to study axisymmetric and non-axisymmetric structures, evocated by the magneto-rotational instability in the outer regions of protoplanetary disks. We combine the results of state-of-the-art numerical simulations with post-processing radiative transfer (RT) to generate synthetic maps and predictions for ALMA. We performed non-ideal global 3D MHD stratified simulations of the dead-zone outer edge using the FARGO MHD code PLUTO. The stellar and disk parameters are taken from a parameterized disk model applied for fitting high-angular resolution multi-wavelength observations of circumstellar disks. The 2D temperature and density profiles are calculated consistently from a given surface density profile and Monte-Carlo radiative transfer. The 2D Ohmic resistivity profile is calculated using a dust chemistry model. The magnetic ...

  3. SXDF-ALMA 2 arcmin$^2$ Deep Survey: 1.1-mm Number Counts

    CERN Document Server

    Hatsukade, Bunyo; Umehata, Hideki; Aretxaga, Itziar; Caputi, Karina I; Dunlop, James S; Ikarashi, Soh; Iono, Daisuke; Ivison, Rob J; Lee, Minju; Makiya, Ryu; Matsuda, Yuichi; Motohara, Kentaro; Nakanishi, Kouichiro; Ohta, Kouji; Tadaki, Ken-ich; Tamura, Yoichi; Wang, Wei-Hao; Wilson, Grant W; Yamaguchi, Yuki; Yun, Min S

    2016-01-01

    We report 1.1 mm number counts revealed with the Atacama Large Millimeter/submillimeter Array (ALMA) in the Subaru/XMM-Newton Deep Survey Field (SXDF). The advent of ALMA enables us to reveal millimeter-wavelength number counts down to the faint end without source confusion. However, previous studies are based on the ensemble of serendipitously-detected sources in fields originally targeting different sources and could be biased due to the clustering of sources around the targets. We derive number counts in the flux range of 0.2-2 mJy by using 23 (>=4sigma) sources detected in a continuous 2.0 arcmin$^2$ area of the SXDF. The number counts are consistent with previous results within errors, suggesting that the counts derived from serendipitously-detected sources are not significantly biased, although there could be field-to-field variation due to the small survey area. By using the best-fit function of the number counts, we find that ~40% of the extragalactic background light at 1.1 mm is resolved at S(1.1mm)...

  4. An ALMA Search for Substructure, Fragmentation, and Hidden Protostars in Starless Cores in Chamaeleon I

    CERN Document Server

    Dunham, Michael M; Pineda, Jaime E; Bourke, Tyler L; Tobin, John J; Arce, Héctor G; Chen, Xuepeng; Di Francesco, James; Johnstone, Doug; Lee, Katherine I; Myers, Philip C; Price, Daniel; Sadavoy, Sarah I; Schnee, Scott

    2016-01-01

    We present an Atacama Large Millimeter/submillimeter Array (ALMA) 106 GHz (Band 3) continuum survey of the complete population of dense cores in the Chamaeleon I molecular cloud. We detect a total of 24 continuum sources in 19 different target fields. All previously known Class 0 and Class I protostars in Chamaeleon I are detected, whereas all of the 56 starless cores in our sample are undetected. We show that the Spitzer+Herschel census of protostars in Chamaeleon I is complete, with the rate at which protostellar cores have been misclassified as starless cores calculated as <1/56, or < 2%. We use synthetic observations to show that starless cores collapsing following the turbulent fragmentation scenario are detectable by our ALMA observations when their central densities exceed ~10^8 cm^-3, with the exact density dependent on the viewing geometry. Bonnor-Ebert spheres, on the other hand, remain undetected to central densities at least as high as 10^10 cm^-3. Our starless core non-detections are used t...

  5. ALMA Science Verification Data: Millimeter Continuum Polarimetry of the Bright Radio Quasar 3C 286

    CERN Document Server

    Nagai, H; Paladino, R; Hull, C L H; Cortes, P; Moellenbrock, G; Fomalont, E; Asada, K; Hada, K

    2016-01-01

    We present full-polarization observations of the compact, steep-spectrum radio quasar 3C~286 made with the ALMA at 1.3~mm. These are the first full-polarization ALMA observations, which were obtained in the framework of Science Verification. A bright core and a south-west component are detected in the total intensity image, similar to previous centimeter images. Polarized emission is also detected toward both components. The fractional polarization of the core is about 17\\%, this is higher than the fractional polarization at centimeter wavelengths, suggesting that the magnetic field is even more ordered in the millimeter radio core than it is further downstream in the jet. The observed polarization position angle (or EVPA) in the core is $\\sim$\\,$39^{\\circ}$, which confirms the trend that the EVPA slowly increases from centimeter to millimeter wavelengths. With the aid of multi-frequency VLBI observations, we argue that this EVPA change is associated with the frequency-dependent core position. We also report ...

  6. A Measurement of the Black-Hole Mass in NGC 1097 using ALMA

    CERN Document Server

    Onishi, Kyoko; Sheth, Kartik; Kohno, Kotaro

    2015-01-01

    We present an estimate of the mass of the supermassive black hole (SMBH) in the nearby type-1 Seyfert galaxy \\object{NGC 1097} using Atacamma Large Millimeter/Submillimeter Array (ALMA) observations of dense gas kinematics. Dense molecular gas dynamics are traced with ${\\rm HCN} (J=1-0)$ and ${\\rm HCO^{+}} (J=1-0)$ emission lines. Assuming a host galaxy inclination of $46^{\\circ}$, we derive a SMBH mass, $M_{\\rm BH}=1.40^{+0.27}_{-0.32} \\times 10^{8}M_{\\odot}$, and an I-band mass to light ratio to be $5.14^{+0.03}_{-0.04}$, using ${\\rm HCN} (J=1-0)$. The estimated parameters are consistent between the two emission lines. The measured SMBH mass is in good agreement with the SMBH mass and bulge velocity dispersion relationship. Our result showcases ALMA's potential for deriving accurate SMBH masses, especially for nearby late-type galaxies. Larger samples and accurate SMBH masses will further elucidate the relationship between the black hole (BH) and host galaxy properties and constrain the coevolutionary growt...

  7. ALMA Imaging of Millimeter/Submillimeter Continuum Emission in Orion KL

    CERN Document Server

    Hirota, Tomoya; Kurono, Yasutaka; Honma, Mareki

    2015-01-01

    We have carried out high resolution observations with Atacama Large Millimeter/Submillimeter Array (ALMA) of continuum emission from Orion KL region. We identify 11 compact sources at ALMA band 6 (245 GHz) and band 7 (339 GHz), including Hot Core, Compact Ridge, SMA1, IRc4, IRc7, and a radio source I (Source I). Spectral energy distribution (SED) of each source is determined by using previous 3 mm continuum emission data. Physical properties such as size, mass, hydrogen number density and column density are discussed based on the dust graybody SED. Among 11 identified sources, Source I, a massive protostar candidate, is a dominant energy source in Orion KL. We extensively investigate its SED from centimeter to submillimeter wavelengths. The SED of Source I can be fitted with a single power-law index of 1.97 suggesting an optically thick emission. We employ the H$^{-}$ free-free emission as an opacity source of this optically thick emission. The temperature, density, and mass of the circumstellar disk associat...

  8. ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix cluster

    CERN Document Server

    Russell, H R; McNamara, B R; Fabian, A C; Nulsen, P E J; Bayliss, M B; Benson, B A; Brodwin, M; Carlstrom, J E; Edge, A C; Hlavacek-Larrondo, J; Marrone, D P; Reichardt, C L; Vieira, J D

    2016-01-01

    We report new ALMA observations of the CO(3-2) line emission from the $2.7\\pm0.4\\times10^{10}\\rm\\thinspace M_{\\odot}$ molecular gas reservoir in the central galaxy of the Phoenix cluster. The cold molecular gas is fuelling a vigorous starburst at a rate of $500-800\\rm\\thinspace M_{\\odot}\\rm\\; yr^{-1}$ and powerful black hole activity in the form of both intense quasar radiation and radio jets. The radio jets have inflated huge bubbles filled with relativistic plasma into the hot, X-ray atmospheres surrounding the host galaxy. The ALMA observations show that extended filaments of molecular gas, each $10-20\\rm\\; kpc$ long with a mass of several billion solar masses, are located along the peripheries of the radio bubbles. The smooth velocity gradients and narrow line widths along each filament reveal massive, ordered molecular gas flows around each bubble, which are inconsistent with gravitational free-fall. The molecular clouds have been lifted directly by the radio bubbles, or formed via thermal instabilities ...

  9. New Measurements of the Radio Photosphere of Mira Based on Data from the JVLA and ALMA

    Science.gov (United States)

    Matthews, L. D.; Reid, M. J.; Menten, K. M.

    2015-07-01

    We present new measurements of the millimeter wavelength continuum emission from the long period variable Mira (o Ceti) at frequencies of 46, 96, and 229 GHz (λ ≈ 7, 3, and 1 mm) based on observations obtained with the Jansky Very Large Array (JVLA) and the Atacama Large Millimeter/submillimeter Array (ALMA). The measured millimeter flux densities are consistent with a radio photosphere model derived from previous observations, where flux density {S}ν \\propto {ν }1.86. The stellar disk is resolved, and the measurements indicate a decrease in the size of the radio photosphere at higher frequencies, as expected if the opacity decreases at shorter wavelengths. The shape of the radio photosphere is found to be slightly elongated, with a flattening of ˜10%-20%. The data also reveal evidence for brightness non-uniformities on the surface of Mira at radio wavelengths. Mira’s hot companion, Mira B was detected at all three observed wavelengths, and we measure a radius for its radio-emitting surface of ≈ 2.0× {10}13 cm. The data presented here highlight the power of the JVLA and ALMA for the study of the atmospheres of evolved stars.

  10. ALMA observations of cool dust in a low-metallicity starburst, SBS0335-052

    CERN Document Server

    Hunt, L K; Casasola, V; Garcia-Burillo, S; Combes, F; Nikutta, R; Caselli, P; Henkel, C; Maiolino, R; Menten, K M; Sauvage, M; Weiss, A

    2013-01-01

    We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 0 Band 7 observations of an extremely metal-poor dwarf starburst galaxy in the Local Universe, SBS0335-052 (12+log(O/H)~7.2). With these observations, dust is detected at 870micron (ALMA Band 7), but 87% of the flux in this band is due to free-free emission from the starburst. We have compiled a spectral energy distribution (SED) of SBS0335-052 that spans almost 6 orders of magnitude in wavelength and fit it with a spherical dust shell heated by a single-age stellar population; the best-fit model gives a dust mass of (3.8+/-0.6)x10^4 Msun. We have also constructed a SED including Herschel archival data for IZw18, another low-metallicity dwarf starburst (12+log(O/H)=7.17), and fit it with a similar model to obtain a dust mass of (3.4+/-1.0)x10^2 Msun. Compared with their atomic gas mass, the dust mass of SBS0335-052 far exceeds the prediction of a linear trend of dust-to-gas mass ratio with metallicity, while IZw18 falls far below. We use gas...

  11. ALMA high spatial resolution observations of the dense molecular region of NGC 6302

    CERN Document Server

    Santander-García, M; Alcolea, J; Castro-Carrizo, A; Sánchez-Contreras, C; Quintana-Lacaci, G; Corradi, R L M; Neri, R

    2016-01-01

    The mechanism behind the shaping of bipolar planetary nebulae is still poorly understood. Accurately tracing the molecule-rich equatorial regions of post-AGB stars can give valuable insight into the ejection mechanisms at work. We investigate the physical conditions, structure and velocity field of the dense molecular region of the planetary nebula NGC 6302 by means of ALMA band 7 interferometric maps. The high spatial resolution of the $^{12}$CO and $^{13}$CO J=3-2 ALMA data allows for an analysis of the geometry of the ejecta in unprecedented detail. We built a spatio-kinematical model of the molecular region with the software SHAPE and performed detailed non-LTE calculations of excitation and radiative transfer with the SHAPEMOL plug-in. We find that the molecular region consists of a massive ring out of which a system of fragments of lobe walls emerge and enclose the base of the lobes visible in the optical. The general properties of this region are in agreement with previous works, although the much grea...

  12. Brown dwarf disks with ALMA: evidence for truncated dust disks in Ophiuchus

    CERN Document Server

    Testi, L; Scholz, A; Tazzari, M; Ricci, L; Monsalvo, I de Gregorio

    2016-01-01

    The study of the properties of disks around young brown dwarfs can provide important clues on the formation of these very low mass objects and on the possibility of forming planetary systems around them. The presence of warm dusty disks around brown dwarfs is well known, based on near- and mid-infrared studies. High angular resolution observations of the cold outer disk are limited, we used ALMA to attempt a first survey of young brown dwarfs in the rho-Ophiuchi star forming region with ALMA. All 17 young brown dwarfs in our sample were observed at 890 um in the continuum at ~0.5" angular resolution. The sensitivity of our observations was chosen to detect ~0.5 MEarth of dust. We detect continuum emission in 11 disks (65% of the total), the estimated mass of dust in the detected disks ranges from ~0.5 to ~6 MEarth. These disk masses imply that planet formation around brown dwarfs may be relatively rare and that the supra-Jupiter mass companions found around some brown dwarfs are probably the result of a binar...

  13. ALMA Science Verification Data: Millimeter Continuum Polarimetry of the Bright Radio Quasar 3C 286

    Science.gov (United States)

    Nagai, H.; Nakanishi, K.; Paladino, R.; Hull, C. L. H.; Cortes, P.; Moellenbrock, G.; Fomalont, E.; Asada, K.; Hada, K.

    2016-06-01

    We present full-polarization observations of the compact, steep-spectrum radio quasar 3C 286 made with the Atacama Large Millimeter and Submillimeter Array (ALMA) at 1.3 mm. These are the first full-polarization ALMA observations, which were obtained in the framework of Science Verification. A bright core and a south–west component are detected in the total intensity image, similar to previous centimeter images. Polarized emission is also detected toward both components. The fractional polarization of the core is about 17%; this is higher than the fractional polarization at centimeter wavelengths, suggesting that the magnetic field is even more ordered in the millimeter radio core than it is further downstream in the jet. The observed polarization position angle (or electric vector position angle (EVPA)) in the core is ˜39◦, which confirms the trend that the EVPA slowly increases from centimeter to millimeter wavelengths. With the aid of multi-frequency VLBI observations, we argue that this EVPA change is associated with the frequency-dependent core position. We also report a serendipitous detection of a sub-mJy source in the field of view, which is likely to be a submillimeter galaxy.

  14. ALMA observations of a misaligned binary protoplanetary disk system in Orion

    International Nuclear Information System (INIS)

    We present Atacama Large Millimeter/Submillimeter Array (ALMA) observations of a wide binary system in Orion, with projected separation 440 AU, in which we detect submillimeter emission from the protoplanetary disks around each star. Both disks appear moderately massive and have strong line emission in CO 3-2, HCO+ 4-3, and HCN 3-2. In addition, CS 7-6 is detected in one disk. The line-to-continuum ratios are similar for the two disks in each of the lines. From the resolved velocity gradients across each disk, we constrain the masses of the central stars, and show consistency with optical-infrared spectroscopy, both indicative of a high mass ratio ∼9. The small difference between the systemic velocities indicates that the binary orbital plane is close to face-on. The angle between the projected disk rotation axes is very high, ∼72°, showing that the system did not form from a single massive disk or a rigidly rotating cloud core. This finding, which adds to related evidence from disk geometries in other systems, protostellar outflows, stellar rotation, and similar recent ALMA results, demonstrates that turbulence or dynamical interactions act on small scales well below that of molecular cores during the early stages of star formation.

  15. ALMA Imaging of the CO(6-5) Line Emission in NGC 7130

    CERN Document Server

    Zhao, Yinghe; Xu, Kevin C; Gao, Yu; Barcos-Munoz, Loreto; Diaz-Santos, Tanio; Appleton, Philip; Charmandaris, Vassilis; Armus, Lee; van der Werf, Paul; Evans, Aaron; Cao, Chen; Inami, Hanae; Murphy, Eric

    2016-01-01

    In this paper, we report our high-resolution ($0^{\\prime\\prime}.20\\times0^{\\prime\\prime}.14$ or $\\sim$$70\\times49$ pc) observations of the CO(6-5) line emission, which probes warm and dense molecular gas, and the 434 $\\mu$m dust continuum in the nuclear region of NGC 7130, obtained with the Atacama Large Millimeter Array (ALMA). The CO line and dust continuum fluxes detected in our ALMA observations are $1230\\pm74$ Jy km s$^{-1}$ and $814\\pm52$ mJy, respectively, which account for 100% and 51% of their total respective fluxes. We find that the CO(6-5) and dust emissions are generally spatially correlated, but their brightest peaks show an offset of $\\sim$70 pc, suggesting that the gas and dust emissions may start decoupling at this physical scale. The brightest peak of the CO(6-5) emission does not spatially correspond to the radio continuum peak, which is likely dominated by an Active Galactic Nucleus (AGN). This, together with our additional quantitative analysis, suggests that the heating contribution of t...

  16. ALMA Imaging of the CO (6-5) Line Emission in NGC 7130*

    Science.gov (United States)

    Zhao, Yinghe; Lu, Nanyao; Xu, C. Kevin; Gao, Yu; Barcos-Munõz, Loreto; Díaz-Santos, Tanio; Appleton, Philip; Charmandaris, Vassilis; Armus, Lee; van der Werf, Paul; Evans, Aaron; Cao, Chen; Inami, Hanae; Murphy, Eric

    2016-04-01

    In this paper, we report our high-resolution (0.″20 × 0.″14 or ∼70 × 49 pc) observations of the CO(6-5) line emission, which probes warm and dense molecular gas, and the 434 μm dust continuum in the nuclear region of NGC 7130, obtained with the Atacama Large Millimeter Array (ALMA). The CO line and dust continuum fluxes detected in our ALMA observations are 1230 ± 74 Jy km s‑1 and 814 ± 52 mJy, respectively, which account for 100% and 51% of their total fluxes. We find that the CO(6-5) and dust emissions are generally spatially correlated, but their brightest peaks show an offset of ∼70 pc, suggesting that the gas and dust emissions may start decoupling at this physical scale. The brightest peak of the CO(6-5) emission does not spatially correspond to the radio continuum peak, which is likely dominated by an active galactic nucleus (AGN). This, together with our additional quantitative analysis, suggests that the heating contribution of the AGN to the CO(6-5) emission in NGC 7130 is negligible. The CO(6-5) and the extinction-corrected Pa-α maps display striking differences, suggestive of either a breakdown of the correlation between warm dense gas and star formation at linear scales of Universities, Inc.

  17. Kennicutt-Schmidt Law in the Central Region of NGC 4321 as Seen by ALMA

    Science.gov (United States)

    Azeez, Jazeel H.; Hwang, C.-Y.; Abidin, Zamri Z.; Ibrahim, Zainol A.

    2016-01-01

    We present the Atacama Large Millimeter/Sub-millimeter Array (ALMA) cycle-0 science verification data of the CO(1–0) line emission in the central region of NGC 4321 (also known as M100) at the distance of 17.1 Mpc and VLA, L-band data of HI of the same galaxy. We have drawn the center area of M100 in the 12CO(J = 1–0) line with the resolution of (3.87″ × 2.53″) as viewed by ALMA, along with HI and Spitzer 8 and 3.6 μm data. The relationship between the surface density of molecular gas mass ∑H2 and that of star formation rate ∑SFR has been investigated, in addition to the relationship between the surface density of the neutral atomic hydrogen mass and that of ∑SFR (Kennicutt–Schmidt law) in this galaxy with a high spatial resolution. The results indicate that a significant correlation exists between the SFR surface density and the molecular gas mass density in the ~2 kpc region. The power-law index has been determined for three regions: center, upper and lower arms. The value of this index in the center region is 1.13, which follows the traditional (K-S) law and indicates that the molecular gas is affected by star formation. PMID:27247251

  18. ALMA and VLA observations of the outflows in IRAS 16293-2422

    CERN Document Server

    Loinard, Laurent; Rodriguez, Luis F; Pech, Gerardo; Chandler, Claire J; Brogan, Crystal L; Wilner, David J; Ho, Paul T P; Parise, Berengere; Hartmann, Lee W; Zhu, Zhaohuan; Takahashi, Satoko; Trejo, Alfonso

    2012-01-01

    We present ALMA and VLA observations of the molecular and ionized gas at 0.1-0.3 arcsec resolution in the Class 0 protostellar system IRAS 16293-2422. These data clarify the origins of the protostellar outflows from the deeply embedded sources in this complex region. Source A2 is confirmed to be at the origin of the well known large scale north-east--south-west flow. The most recent VLA observations reveal a new ejection from that protostar, demonstrating that it drives an episodic jet. The central compact part of the other known large scale flow in the system, oriented roughly east-west, is well delineated by the CO(6-5) emission imaged with ALMA and is confirmed to be driven from within component A. Finally, a one-sided blueshifted bubble-like outflow structure is detected here for the first time from source B to the north-west of the system. Its very short dynamical timescale (~ 200 yr), low velocity, and moderate collimation support the idea that source B is the youngest object in the system, and possibly...

  19. High resolution ALMA observations of dense molecular medium in the central regions of active galaxies

    CERN Document Server

    Kohno, Kotaro; Taniguchi, Akio; Izumi, Takuma; Tosaki, Tomoka

    2016-01-01

    In the central regions of active galaxies, dense molecular medium are exposed to various types of radiation and energy injections, such as UV, X-ray, cosmic ray, and shock dissipation. With the rapid progress of chemical models and implementation of new-generation mm/submm interferometry, we are now able to use molecules as powerful diagnostics of the physical and chemical processes in galaxies. Here we give a brief overview on the recent ALMA results to demonstrate how molecules can reveal underlying physical and chemical processes in galaxies. First, new detections of Galactic molecular absorption systems with elevated HCO/H$^{13}$CO$^+$ column density ratios are reported, indicating that these molecular media are irradiated by intense UV fields. Second, we discuss the spatial distributions of various types of shock tracers including HNCO, CH$_3$OH and SiO in NGC 253 and NGC 1068. Lastly, we provide an overview of proposed diagnostic methods of nuclear energy sources using ALMA, with an emphasis on the syne...

  20. Dust properties across the CO snowline in the HD 163296 disk from ALMA and VLA observations

    CERN Document Server

    Guidi, G; Testi, L; de Gregorio-Monsalvo, I; Chandler, C J; Pérez, L; Isella, A; Natta, A; Ortolani, S; Hennings, Th; Corder, S; Linz, H; Andrews, S; Wilner, D; Ricci, L; Carpenter, J; Sargent, A; Mundy, L; Storm, S; Calvet, N; Dullemond, C; Greaves, J; Lazio, J; Deller, A; Kwon, W

    2016-01-01

    To characterize the mechanisms of planet formation it is crucial to investigate the properties and evolution of protoplanetary disks around young stars, where the initial conditions for the growth of planets are set. Our goal is to study grain growth in the disk of the young, intermediate mass star HD163296 where dust processing has already been observed, and to look for evidence of growth by ice condensation across the CO snowline, already identified in this disk with ALMA. Under the hypothesis of optically thin emission we compare images at different wavelengths from ALMA and VLA to measure the opacity spectral index across the disk and thus the maximum grain size. We also use a Bayesian tool based on a two-layer disk model to fit the observations and constrain the dust surface density. The measurements of the opacity spectral index indicate the presence of large grains and pebbles ($\\geq$1 cm) in the inner regions of the disk (inside $\\sim$50 AU) and smaller grains, consistent with ISM sizes, in the outer ...

  1. RESOLVED IMAGES OF THE PROTOPLANETARY DISK AROUND HD 100546 WITH ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Pineda, Jaime E.; Quanz, Sascha P.; Meru, Farzana; Meyer, Michael R.; Avenhaus, Henning [Institute for Astronomy, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich (Switzerland); Mulders, Gijs D. [Lunar and Planetary Laboratory, The University of Arizona, 1629 E. University Blvd., Tucson, AZ 85721 (United States); Panić, Olja, E-mail: pjaime@phys.ethz.ch [Institute of Astronomy, Madingley Road, Cambridge CB3 0HA (United Kingdom)

    2014-06-20

    The disk around the Herbig Ae/Be star HD 100546 has been extensively studied and it is one of the systems for which there are observational indications of ongoing and/or recent planet formation. However, up until now, no resolved image of the millimeter dust emission or the gas has been published. We present the first resolved images of the disk around HD 100546 obtained in Band 7 with the ALMA observatory. The CO (3-2) image reveals a gas disk that extends out to 350 au radius at the 3σ level. Surprisingly, the 870 μm dust continuum emission is compact (radius <60 au) and asymmetric. The dust emission is well matched by a truncated disk with an outer radius of ≈50 au. The lack of millimeter-sized particles outside 60 au is consistent with radial drift of particles of this size. The protoplanet candidate, identified in previous high-contrast NACO/VLT L' observations, could be related to the sharp outer edge of the millimeter-sized particles. Future higher angular resolution ALMA observations are needed to determine the detailed properties of the millimeter emission and the gas kinematics in the inner region (<2''). Such observations could also reveal the presence of a planet through the detection of circumplanetary disk material.

  2. O "imperscrutável vínculo": corpo e alma na medicina lusitana setecentista

    Directory of Open Access Journals (Sweden)

    Flavio Coelho Edler

    2013-08-01

    Full Text Available Este artigo discute a emergência do discurso médico sobre questões relativas ao comportamento transgressor no contexto intelectual lusitano do século XVIII, através das obras Dissertação sobre as paixões da alma (1753, de Antonio Ribeiro Sanches (1699-1783, e Medicina Theologica (1794, de Francisco de Melo Franco (1757-1823. Ambas escritas e publicadas durante as reformas ilustradas em Portugal, no período que se estende entre o consulado pombalino e o reinado mariano. Calcadas em referenciais filosóficos de matriz racional-empirista, os respectivos autores se utilizam de um vocabulário médico que se renovava através dos debates entre correntes vitalistas, animistas e mecanicistas, para interpelar os discursos tradicionais, sobretudo o Direito e a Teologia, e reivindicar a legitimidade do discurso médico para tratar da alma como um objeto próprio à sua jurisdição.

  3. ALMA observations of a misaligned binary protoplanetary disk system in Orion

    Energy Technology Data Exchange (ETDEWEB)

    Williams, Jonathan P. [Institute for Astronomy, University of Hawaii, Honolulu, HI 96816 (United States); Mann, Rita K.; Francesco, James Di; Johnstone, Doug; Matthews, Brenda [NRC Herzberg Astronomy and Astrophysics, 5071 West Saanich Road, Victoria, BC, V9E 2E7 (Canada); Andrews, Sean M.; Ricci, Luca [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Hughes, A. Meredith [Van Vleck Observatory, Astronomy Department, Wesleyan University, 96 Foss Hill Drive, Middletown, CT 06459 (United States); Bally, John, E-mail: jpw@ifa.hawaii.edu [CASA, University of Colorado, CB 389, Boulder, CO 80309 (United States)

    2014-12-01

    We present Atacama Large Millimeter/Submillimeter Array (ALMA) observations of a wide binary system in Orion, with projected separation 440 AU, in which we detect submillimeter emission from the protoplanetary disks around each star. Both disks appear moderately massive and have strong line emission in CO 3-2, HCO{sup +} 4-3, and HCN 3-2. In addition, CS 7-6 is detected in one disk. The line-to-continuum ratios are similar for the two disks in each of the lines. From the resolved velocity gradients across each disk, we constrain the masses of the central stars, and show consistency with optical-infrared spectroscopy, both indicative of a high mass ratio ∼9. The small difference between the systemic velocities indicates that the binary orbital plane is close to face-on. The angle between the projected disk rotation axes is very high, ∼72°, showing that the system did not form from a single massive disk or a rigidly rotating cloud core. This finding, which adds to related evidence from disk geometries in other systems, protostellar outflows, stellar rotation, and similar recent ALMA results, demonstrates that turbulence or dynamical interactions act on small scales well below that of molecular cores during the early stages of star formation.

  4. Development of the control system for the 40m OAN radiotelescope with the Alma Common Software

    Science.gov (United States)

    de Vicente, P.; Bolaño, R.; Barbas, L.

    2006-07-01

    The Observatorio Astronómico Nacional (OAN) is building a 40m radiotelescope in its facilities in Yebes (Spain) which will be delivered in summer 2006. The radiotelescope is an instrument composed of antenna, receivers, backends, and auxiliary equipment connected through a Local Area Network (LAN). The control system has to deal with a distributed environment which needs to be remotely controlled and monitored from external heterogeneous users (astronomers and engineers) and requires multiple processes simultaneously working and being synchronized. We have chosen the Alma Common Software (ACS) framework for the development of the control system. ACS provides an implementation of the component/container paradigm via Common Object Request Broker Architecture (CORBA) and also provides general purpose utility libraries, hiding the complexity of CORBA to the developer. ACS is supported by the European Southern Observatory (ESO) and the National Radioastronomy Observatory (NRAO) for the Atacama Large Millimeter Array (ALMA) with a lifetime similar to our radiotelescope. This is an important guarantee for the OAN with a very reduced software team. We present an overview of the planned software architecture of the radiotelescope and the current status of the development of the components.

  5. Linearly Polarized Millimeter and Submillimeter Continuum Emission of Sgr A* Constrained by ALMA

    CERN Document Server

    Liu, Hauyu Baobab; Zhao, Jun-Hui; Brinkerink, Christiaan D; Ho, Paul T P; Mills, Elisabeth A C; Martín, Sergio; Falcke, Heino; Matsushita, Satoki; Martí-Vidal, Ivan

    2016-01-01

    Our aim is to characterize the polarized continuum emission properties including intensity, polarization position angle, and polarization percentage of Sgr A* at $\\sim$100 (3.0 mm), $\\sim$230 (1.3 mm), $\\sim$345 (0.87 mm), $\\sim$500 (0.6 mm), and $\\sim$700 GHz (0.43 mm). We report continuum emission properties of Sgr A* at the above frequency bands, based on the Atacama Large Millimeter Array (ALMA) observations. We measured flux densities of Sgr A* from ALMA single pointing and mosaic observations. We performed sinusoidal fittings to the observed (XX-YY)/I intensity ratios, to derive the polarization position angles and polarization percentages. We successfully detect polarized continuum emission from all observed frequency bands. We observed lower Stokes I intensity at $\\sim$700 GHz than that at $\\sim$500 GHz, which suggests that emission at $\\gtrsim$500 GHz is from optically thin part of a synchrotron emission spectrum. Both the Stokes I intensity and the polarization position angle at our highest observin...

  6. Travessias discursivas: intertextualidade e interdisciplinaridade no romance Netto perde sua alma, de Tabajara Ruas

    Directory of Open Access Journals (Sweden)

    Marcelo de Andrade Duarte

    2016-03-01

    Full Text Available A partir de uma leitura crítica das relações intertextuais promovidas por Netto perde sua alma pretende-se analisar o romance, de Tabajara Ruas, não só em seu diálogo interdisciplinar com a historiografia, mas também nas relações que a obra suscita com outros textos literários. Nesse caminho, percebe-se que a historiografia tradicionalmente trata os homens que participaram de guerras como semideuses, configurando-os apenas por suas ações e participações heroicas em conflitos políticos. Enquanto o romance Netto perde sua alma, sem deixar de incorporar ações heroicas de seu protagonista, privilegia a configuração de uma dimensão humana e humanizadora de sua personagem histórica, pois a faz refletir e questionar profundamente sobre tais ações.  Dessa forma, destacamos nessa leitura o processo de humanização que o romance de Tabajara Ruas promove de um personagem relevante da história do Rio Grande do Sul, o General Antonio de Souza Netto.

  7. ALMA resolves extended star formation in high-z AGN host galaxies

    CERN Document Server

    Harrison, C M; Stanley, F; Alexander, D M; Daddi, E; Mullaney, J R; Pannella, M; Rosario, D J; Smail, Ian

    2015-01-01

    We present high-resolution Atacama Large Millimeter Array (ALMA) 870um imaging of five z~1.5-4.5 X-ray detected AGN (with luminosities of L(X)>10^42 erg/s). The sub-millimetre emission is extended on scales of FWHM~0.2"-0.5", corresponding to physical sizes of 1-3 kpc (median value of 1.8 kpc). These sizes are comparable to the majority of z=1-5 sub-millimetre galaxies (SMGs) with equivalent ALMA measurements. In combination with spectral energy distribution analyses, we attribute this rest-frame far-infrared (FIR) emission to dust heated by star formation. The implied star-formation rate surface densities are 20-200 Msol/yr/kpc^2, which are consistent with SMGs of comparable FIR luminosities (i.e., L(IR)~ [1-5]x10^12 Lsol). Although limited by a small sample of AGN, which all have high FIR luminosities, our study suggests that the kpc-scale spatial distribution and surface density of star formation in high-redshift star-forming galaxies is the same irrespective of the presence of X-ray detected AGN.

  8. Entre Napoleón y Jesucristo: las peripecias del “alma rusa” en la obra de Dostoievski / Between Napoleon and Jesus Christ: The adventures of the "Russian soul" in Dostoevsky's work

    Directory of Open Access Journals (Sweden)

    Tatiana Bubnova

    2011-11-01

    Full Text Available RESUMEN: Dos componentes del “alma rusa” que se destacan en la obra de Dostoievski – el napoleonismo y la cristología — resultan de la interacción de la cultura rusa con la historia y la civilización occidental. Paradójicamente, la evolución de las dos líneas en las novelas del gran escritor ruso conduce a una determinada, en algunos aspectos, de los dos tipos, en particular, en El idiota. La revisión del manoseado tópico del “alma rusa” a la luz de las recientes investigaciones de los especialistas rusos pone de manifiesto nuevasintertextualidades y abre la obra a un diálogo renovado acerca de la identidad. El trabajo se inspira en la antropología filosófica y la filosofía del lenguaje de M. M. Bajtín. ABSTRACT: This is an analysis of the two components of the “Russian soul” highlighted in the Dostoevsky’s novels: Napoleonism and Christology. The origins of both of them can be found in the Western history and civilization. There is a certain paradox in the fact that the evolution of these two lines in the oeuvre of the great Russian writer arrives to an approachof the two types, the Napoleonic one and that of the follower of Christ, especially in The Idiot. A revision of the “Russian soul” under the light of the most recent interpretations of Russian critics discovers new intertexts and opens Dostoevsky’s text to a renewed identity dialogue. This paper is influenced by Bakhtin’s philosophical anthropology and philosophy of language.

  9. La eliminación de la subjetividad de los fines: Platón y las matemáticas

    OpenAIRE

    Pérez Herranz, Fernando Miguel

    2007-01-01

    1. Planteamiento 2. Platón, cruce de caminos 3. La desconexión semántica y la teoría de las Ideas i) Concepto griego de número (arithmos) ii) Los objetos matemáticos iii) El modelo matemático de la filosofía 4. Las matemáticas, saber articulador entre los objetos sensibles e inteligibles i) Desconexión Cuerpo / Alma ii) Desconexión Lógica 5. La eliminación de la subjetividad de los fines 6. Final: «La sabiduría de Occidente».

  10. Los compadres

    Directory of Open Access Journals (Sweden)

    Luis Muñoz

    2010-03-01

    Full Text Available De lejos parecen ser personas muy silenciosas y cuando hablan lo hacen con una entonación diferente. Comienza un día hermoso en el que vamos a visitarlos y el humor es la disculpa más agradable para hacer alianzas. La señora va y viene del cuarto oscuro donde se encuentra el fogón, interviniendo a veces, con su presencia viva en la charla, aunque no lo parece. Un café, una taza de leche y roscones, un vaso de guarapo, una y otra vez. No sé como llamarlos; si cuenteros, poetas, hombres hablando. Los percibo como portadores de una tradición oral, compartiendo con nosotros sus pensamientos y creencias más profundos, en tomo a todos los matices de su realidad social. En la tradición oral se piensa el mundo de una manera integral mientras la cotidianidad está cada vez más condicionada por un mundo segmentado y especializado. Los cuentos innumerables que conocen han sido escuchados y modificados por niños, hombres y mujeres de todas las edades. Cualquier actividad diaria es buena para contar. Las noches en la caza de Luis son acogedoras, la señora Angelita prepara una sopa de maíz y tomamos hasta dos platos llenos para calentamos. La única esperma que ilumina la penumbra de la conversación se consume poco a poco. Los primeros días de mi visita sentí lo que llamaría miedos culturales, como mi obsesión por los insectos que imaginaba dentro de la casa, la cual se fue disipando en la medida en que afirmábamos nuestros lazos. Noches de tertulia, de diálogo, de cuentos. Generalmente Luis pasa esas horas escribiendo o leyendo, dedicado a su mayor afición que es la literatura, conversando con doña Angelita y escuchando cuando ella relata cuentos y anécdotas. Al joven escritor autodidacta lo cautivan las vivencias y fantasías humanas. Escribe sobre su gente y está interesado en las tradiciones literarias de la región. Trabaja como jornalero en fincas o haciendas, realizando varios oficios como la carpintería, la agricultura, la

  11. Informe de Amnesty Internacional. La pena de muerte en los Estados Unidos de América Una cuestión que atañe a los profesionales de la salud.

    Directory of Open Access Journals (Sweden)

    - Amnesty Internacional

    1987-01-01

    Full Text Available En los primeros nueve meses de 1986 fueron ejecutados dieciséis hombres en los EE.UU. Más de 1.700 reclusos están a la espera de la ejecución en 33 de los 37 Estados cuya legislación prevé la pena de muerte; algunos llevan hasta doce años en esta situación. A partir de la década de 1930, en que se dio la máxima frecuencia de la aplicación de la pena capital', hubo un descenso gradual de la misma hasta 1967, en que entró en vigor una moratoria para las ejecuciones, después de que se argumentara jurídicamente que la pena de muerte era una «pena cruel y excepcional» y, por tanto, inconstitucional. En 1972, el Tribunal Supremo de los EE.UU. declaró, por cinco votos a favor y cuatro en contra, la inconstitucionalidad de la pena de muerte en tres recursos interpuestos ante el mismo.

  12. Aproximación cultural y textual a los informes médico forenses en la traducción especializada francés/español

    OpenAIRE

    Françoise Olmo Cazevieille

    2015-01-01

    En el ámbito de la traducción judicial francés-español, los informes forenses se han estudiado muy poco por ser documentos confidenciales de acceso limitado. No obstante, su estudio resulta de gran interés para los profesionales de la traducción especializada pues están relacionados con varias disciplinas, entre otras, el derecho y la medicina. Para caracterizarlos mejor, estudiaremos el contexto cultural de estos documentos, comprobaremos las variaciones en cuanto a su denominación en las do...

  13. Productividad y Visibilidad Científica de los Profesores Funcionarios de las Universidades Públicas Españolas en el Área de Tecnologías Informáticas

    OpenAIRE

    Ibañez, Alfonso; Bielza, Concha; Larrañaga Múgica, Pedro

    2011-01-01

    Este informe describe y analiza de una manera estructurada, la productividad y visibilidad científica internacional de los profesores (Catedrático de Universidad (CU), Titular de Universidad (TU), Catedrático de Escuela Universitaria (CEU) y Titular de Escuela Universitaria (TEU)) de las universidades públicas españolas adscritos a las áreas de conocimiento de Arquitectura y Tecnología de los Computadores (ATC), Ciencia de la Computación e Inteligencia Artificial (CCIA), y Lenguajes y Sistema...

  14. The Sunyaev-Zel'dovich effect at 5″: RX J1347.5-1145 imaged by ALMA

    Science.gov (United States)

    Kitayama, Tetsu; Ueda, Shutaro; Takakuwa, Shigehisa; Tsutsumi, Takahiro; Komatsu, Eiichiro; Akahori, Takuya; Iono, Daisuke; Izumi, Takuma; Kawabe, Ryohei; Kohno, Kotaro; Matsuo, Hiroshi; Ota, Naomi; Suto, Yasushi; Takizawa, Motozaku; Yoshikawa, Kohji

    2016-10-01

    We present the first image of the thermal Sunyaev-Zel'dovich effect (SZE) obtained by the Atacama Large Millimeter/submillimeter Array (ALMA). Combining 7-m and 12-m arrays in Band 3, we create an SZE map toward a galaxy cluster RX J1347.5-1145 with 5″ resolution (corresponding to a physical size of 20 h-1 kpc), the highest angular and physical spatial resolutions achieved to-date for imaging the SZE, while retaining extended signals out to 40″. The 1 σ statistical sensitivity of the image is 0.017 mJy beam-1 or 0.12 mKCMB at the 5″ full width at half maximum. The SZE image shows a good agreement with an electron pressure map reconstructed independently from the X-ray data and offers a new probe of the small-scale structure of the intracluster medium. Our results demonstrate that ALMA is a powerful instrument for imaging the SZE in compact galaxy clusters with unprecedented angular resolution and sensitivity. As the first report on the detection of the SZE by ALMA, we present detailed analysis procedures including corrections for the missing flux, to provide guiding methods for analyzing and interpreting future SZE images obtained by ALMA.

  15. LOS SISTEMAS DE INFORMACIÓN GEOGRÁFICA (SIG, UNA GRAN HERRAMIENTA PARA LA SILVICULTURA URBANA GEOGRAPHICAL INFORMATION SYSTEMS (GIS, A GREAT TOOL FOR URBAN SYLVICULTURE

    Directory of Open Access Journals (Sweden)

    Leodán Andrés Otaya Burbano

    2006-06-01

    Full Text Available Como una fase piloto, para adquirir experiencia, definir metodologías y determinar las ventajas de los Sistemas de Información Geográfica (SIG al ser aplicados en la Silvicultura Urbana, se realizó el inventario, diagnóstico, propuesta de manejo y valoración económica del Bosque Urbano del barrio La Magnolia del Municipio de Envigado, Departamento de Antioquia, Colombia. Para el manejo y análisis de los registros recolectados en campo, se diseñó una base de datos en el software Microsoft Access®. Se ubicaron las especies inventariadas en mapas digitales y se analizó la condición de las mismas por medio de algunas herramientas y extensiones de la arquitectura tecnológica ArcGISÒ 8.3 en cuanto a: características, tratamientos silviculturales requeridos y conflictos con el entorno. Como resultado se determinó que el SIG del Bosque Urbano realizado para un barrio en particular se convierte en una herramienta que le permite a las autoridades ambientales y a investigadores interesados, tener acceso fácil y ágil de la información almacenada en él; permite realizar la programación de las actividades silviculturales requeridas, tener una visión general del Bosque Urbano de acuerdo a la infraestructura del barrio, apoyada con las fotografías del sector, para una mayor ilustración; permite además la inclusión o eliminación de información de una manera rápida y sencilla, facilitando así la toma de decisiones con relación al manejo del arbolado urbano y a la comparación con otros estudios similares.As a pilot phase, to acquire experience, define methodologies, and determine the advantages of Geographical Information Systems (GIS for applying to Urban Silviculture, an inventory, diagnosis, management plan and economic appraisal were made for the Urban Forest in the Magnolia neighborhood of the Envigado Municipality, Department of Antioquia, Colombia. For the management and analysis of the data collected in field, a database

  16. Los caminos del “alma rusa”: notas desde su historia flosófca, 1700-1861.

    Directory of Open Access Journals (Sweden)

    Richard Kalil Nieto

    2009-04-01

    Full Text Available This article is a project in hybridity that joins Russian philosophical history with a project on Russian national identity between 1700 and 1861. Based on the works of various Russian philosophical historians, and emphasizing, as the background, the preoccupation for developing a national identity within Russia’s arts, this text makes a novel suggestion: that Russian philosophical history should not only be read as an agglomeration of philosophical systems, but also as a science that contributes to the multishaped imaginary that is national identity. Like the biological fusion between two cells of different species to form a new one of mixed characteristics, the essay presents a interlaced hybrid that: (1 offers refections on the characteristics of the mother (Russian philosophical history; and (2 synthesizes refections on the features of the father (the project of national identity.

  17. La evaluación de software educativo en el escenario de la evolución de los paradigmas informáticos

    Directory of Open Access Journals (Sweden)

    María de los Ángeles MARTÍNEZ RUIZ

    2009-11-01

    Full Text Available RESUMEN: Progresivamente se incrementa el número de paquetes de software educativo disponibles y en las revistas se anuncia courseware para todas las áreas de conocimiento del ámbito educativo. El coste económico de los programas puede ser considerable por lo que la optimización de la toma de decisiones en las adquisiciones es uno de los nudos clave en el mundo de la enseñanza basada o asistida con ordenador. El problema con que se enfrentan los profesores en la selección del software no viene solucionado por las referencias, más o menos, subjetivas que aparecen en diversas revistas, es por ello que el diseño de un modelo de definición y evaluación de courseware responde a la necesidad de objetivización de las decisiones de elección de los programas informáticos más adecuados al contexto educativo. El objeto de este artículo es la propuesta de un modelo de definición y evaluación de software educativo que permita la comparación de paquetes y dé respuesta a las actuales necesidades del aula. El modelo incluye unas amplias categorías, que posteriormente se subdividen en apartados más concretos. Las áreas básicas se refieren a las características técnicas del material informático, al contexto, al diseño instruccional, a la tipología de la relación interactiva y a la configuración de la evaluación.ABSTRACT: The number of software packets available is increasing progressively and in journals courseware is announced for all áreas of knowledge in the educational range. The economic cost of the programs can be considerable; thus optimizing decision- making on acquisitions is one of the key problems in the world of computer based or assisted teaching. The problem teachers are faced with when selecting software is not solved by the more or less subjective references that appear in different  journals, henee the designing of a model for the definition and evaluation of courseware answers the need to objectify the decisions

  18. Evaluación de la práctica clínica del Consentimiento Informado en los ensayos clínicos Evaluation of the clinical practice of Informed Consent in clinical trials

    Directory of Open Access Journals (Sweden)

    J. Gost

    2003-04-01

    Full Text Available Sobre la base de las publicaciones existentes parece lícito suponer que en un ensayo clínico (EC, las dificultades inherentes al proceso de comunicación investigador-participante son en la práctica mayores que las deseadas. Se asume asimismo la hipótesis de que existen deficiencias en la legibilidad formal de los documentos de consentimiento informado. Se presentan los resultados de un estudio transversal realizado en una muestra aleatoria (n= 160 de los EC aprobados por el CEIC de Navarra durante los años 1995-1999. Los resultados encontrados (en el 69,7% de los casos el investigador archiva la documentación correspondiente al EC, el CI aparece firmado por el investigador en el 56,6% de los EC, y en más del 83% de los casos la información escrita presenta una deficiente legibilidad confirman la bondad de la hipótesis y detectan áreas de mejora a desarrollar.On the basis of existing publications it would seem legitimate to assume that in a clinical test (CT the difficulties inherent in the process of researcher-participant communication are in practice greater than desired. Similarly, the hypothesis is adopted that difficulties exist in the formal legibility of the documents of Informed Consent. We present the results of a transversal study made of a random sample (n=160 of the CTs approved by the Ethical Committee of Clinical Research (CEIC of Navarra during the years 1995-1999. The results found were: in 69.7% of the cases the researcher filed the documents corresponding to the CT, the Informed Consent appears signed by the researcher in 56.6% of the CTs, and in more than 83% of the cases the written information shows shortcomings in legibility, which confirms the correctness of the hypothesis and permits the detection of areas where improvements need to be developed.

  19. Informe de la comisión que estudió la organización de los servicios de la higiene municipal

    OpenAIRE

    Bejarano, Jorge; Aparicio, Julio

    2011-01-01

    EI señor Alcalde de la ciudad ha solicitado de la Corporación se le dé un concepto sobre la marcha y organización de los servicios de la Higiene Municipal, Con el fin de aprovecharlo para un posible mejoramiento de los mismos, dentro de las posibllidades del presupuesto. Muestra con ello el Jefe del Ejecutivo de Bogotá el decidido interés por la higiene pública y el acatamiento que le merecen las opiniones de esta Academia. Designados para formar la Comisión encargada de hacer los respectivos...

  20. La organización social en los barrios bajos

    Directory of Open Access Journals (Sweden)

    William Foote Whyte

    2010-07-01

    Full Text Available

    Por mucho tiempo, los sociólogos han estudiado los barrios bajos en términos de desorganización social. El interés en los mismos parece provenir de dos fuentes: una urgencia por promover reformas sociales y un esfuerzo para comprender el proceso de urbanización. Observando el quiebre de los controles del grupo primario en la vida de ciudad, algunos sociólogos han considerado analizar la situación resultante en términos del concepto de desorganización social. Los barrios bajos han sido caracterizados por ciertos sociólogos, como áreas de almas perdidas y misiones, áreas donde individuos y familias viven en intimidad forzada con personas a las cuales normalmente rechazan y evitan; áreas donde no se aprecian estándares de decencia o buena conducta excepto los impuestos por una autoridad externa. Según la opinión de otros sociólogos, los barrios bajos son un área de libertad e individualismo. Harvey Zorbaugh dice que la política en el distrito bajo no es como la política en el distrito de clase media. Como no se ajusta a los estándares de la clase media, no es más que un juego. Más aún, la preocupación con el estudio de la desorganización familiar ha conducido a algunos sociólogos a subestimar cualquier grado de organización que se pueda encontrar en los barrios bajos. 

  1. Quistes de los maxilares

    Directory of Open Access Journals (Sweden)

    Ivan Alberto Manotas Arevalo

    2013-12-01

    Full Text Available Los Grandes Quistes de los Maxilares han estado vinculados siempre a la humanidad, desde tiempos remotos, pues han sido halladas en restos de especimenes fosiles, han llamado la atencion de los clínicos, en torno a su etiologia, en la que se ha introducido la participacion de la genetica, (demostrada en el desarrollo de los queratoquistes maxilares, la fisiopatologia, caracteristicas histologicas (inmunohistoquimica, posibilidades diagnosticas por la imagen, (como la tomografia computarizada y la resonancia nuclear magnetica y otras pruebas. Además llaman la atención al estudio, por sus alternativas de manejo especialmente las formas radicales, y el analisis de asociaciones a otras patolo-gias benignas y malignas, y de la recurrencia muy alto de algunas de estas lesiones. Mucho se ha desarrollado para elucidar su naturaleza real, estadificar adecuadamente la lesion descartando asocia-ciones patologicas sindromicas, indicar un tratamiento apropiado, y realizar seguimientos a largo plazo. Este articulo pretende recaudar una information general que de parametros para abordar el estudio de los quistes maxilares a partir de la presentacion de un caso clinico.

  2. Necesidades de información de los usuarios de Atención Primaria desde la perspectiva de los profesionales sanitarios: Un estudio Delphi Information needs of patients in primary care from the perspective of health professionals: A Delphi study

    Directory of Open Access Journals (Sweden)

    José Ángel Maderuelo-Fernández

    2009-10-01

    Full Text Available Objetivos: Conocer las necesidades de información de los usuarios en relación a la oferta de servicios de Atención Primaria desde la perspectiva de los profesionales sanitarios. Métodos: Se ha utilizado la técnica Delphi como método de consenso. Se solicitó la participación de 70 expertos: 35 médicos de familia, 32 enfermeras y tres pediatras de centros de salud urbanos y rurales del Área de Salud de Salamanca, entre mayo y diciembre de 2006. Los cuestionarios estaban estructurados en seis apartados: conocimientos sobre su salud, oferta de su centro de salud, aspectos administrativos, medios de difusión, expectativas sobre información y barreras en la comunicación. Las respuestas priorizadas en el tercer cuestionario se puntuaron según una escala que otorga cinco puntos a la sentencia más importante y un punto a la seleccionada en quinto lugar. Resultados: Contestaron los tres cuestionarios 44 (62,8% expertos. Las necesidades de información más puntuadas fueron la información sobre su enfermedad (4,0 puntos, los aspectos relacionados con la responsabilidad sobre su salud (3,8 y los consejos preventivos (3,6, seguidos de aspectos relativos a la accesibilidad (4,2, urgencias (3,4, oferta de servicios de médico/a y enfermera/o (3,6 y sitios donde dirigirse para obtener información (4,0. La falta de coordinación entre niveles (4,1 y la burocratización (3,5 se consideraron barreras en la comunicación y la información. Conclusiones: Los factores identificados se centran en contenidos que permitan a los pacientes implicarse en su propio proceso y participar en la toma de decisiones que les incumben. También destacaron la información sobre los servicios y el acceso a éstos.Objective: To determine the information needed by patients in relation to the supply of primary care services from the perspective of health professionals. Methods: The Delphi technique was used as a consensus method. Seventy experts were asked to

  3. The ALMA Protostellar Interferometric Line Survey (PILS): First results from an unbiased submillimeter wavelength line survey of the Class 0 protostellar binary IRAS 16293-2422 with ALMA

    CERN Document Server

    Jørgensen, J K; Coutens, A; Lykke, J M; Müller, H S P; van Dishoeck, E F; Calcutt, H; Bjerkeli, P; Bourke, T L; Drozdovskaya, M N; Favre, C; Fayolle, E C; Garrod, R T; Jacobsen, S K; Öberg, K I; Persson, M V; Wampfler, S F

    2016-01-01

    The inner regions of the envelopes surrounding young protostars are characterised by a complex chemistry, with prebiotic molecules present on the scales where protoplanetary disks eventually may form. This paper introduces a systematic survey, "Protostellar Interferometric Line Survey (PILS)" of the Class 0 protostellar binary IRAS 16293-2422 using the Atacama Large Millimeter/submillimeter Array (ALMA). The survey covers the full frequency range from 329 to 363 GHz (0.8 mm) with additional targeted observations at 3.0 and 1.3 mm. More than 10,000 features are detected toward one component in the protostellar binary. Glycolaldehyde, its isomers, methyl formate and acetic acid, and its reduced alcohol, ethylene glycol, are clearly detected. For ethylene glycol both lowest state conformers, aGg' and gGg', are detected, the latter for the first time in the ISM. The abundance of glycolaldehyde is comparable to or slightly larger than that of ethylene glycol. In comparison to the Galactic Center, these two species...

  4. Resolving the extended atmosphere and the inner wind of Mira (o Ceti) with long ALMA baselines

    Science.gov (United States)

    Wong, K. T.; Kamiński, T.; Menten, K. M.; Wyrowski, F.

    2016-05-01

    Context. High angular resolution (sub)millimetre observations of asymptotic giant branch (AGB) stars, now possible with the Atacama Large Millimeter/submillimeter Array (ALMA), allow direct imaging of these objects' photospheres. The physical properties of the molecular material around these regions, which until now has only been studied by imaging of maser emission and spatially unresolved absorption spectroscopy, can be probed with radiative transfer modelling and compared to hydrodynamical model predictions. The prototypical Mira variable, o Cet (Mira), was observed as a Science Verification target in the 2014 ALMA Long Baseline Campaign, offering the first opportunity to study these physical conditions in detail. Aims: With the longest baseline of 15 km, ALMA produces clearly resolved images of the continuum and molecular line emission/absorption at an angular resolution of ~30 mas at 220 GHz. Models are constructed for Mira's extended atmosphere to investigate the physics and molecular abundances therein. Methods: We imaged the data of 28SiO ν= 0, 2J = 5-4 and H2O v2 = 1JKa,Kc = 55,0-64,3 transitions and extracted spectra from various lines of sight towards Mira's extended atmosphere. In the course of imaging the emission/absorption, we encountered ambiguities in the resulting images and spectra that appear to be related to the performance of the CLEAN algorithm when applied to a combination of extended emission, and compact emission and absorption. We addressed these issues by a series of tests and simulations. We derived the gas density, kinetic temperature, molecular abundance, and outflow/infall velocities in Mira's extended atmosphere by modelling the SiO and H2O lines. Results: We resolve Mira's millimetre continuum emission and our data are consistent with a radio photosphere with a brightness temperature of 2611 ± 51 K. In agreement with recent results obtained with the Very Large Array, we do not confirm the existence of a compact region (physical

  5. Informed consent document in gastrointestinal endoscopy: understanding and acceptance by patients Estudio del grado de entendimiento y aceptación por nuestros pacientes de los consentimientos informados utilizados para endoscopia

    Directory of Open Access Journals (Sweden)

    J. J. Vila

    2006-02-01

    Full Text Available Objective: we wanted to know if patients read and understand the informed consent (IC document used for endoscopic procedures, and to evaluate the readability of IC. Method: during two months we gave patients studied in our endoscopy unit an anonymous questionnaire with different items concerning reading degree, knowledge of the technique, complications, sedation used, and information received. We evaluated IC readability using the Flesch index. Results: 309 patients were included (mean age: 53 years, 55% males, 86% outpatients, 50% with basic education; 85% of patients read the IC, 96% considered they understood the exploration technique, 22% were not aware of severe complications, and 82% knew which kind of sedation would be used; 88% of patients received additional information from their doctors. Outpatients read the IC in a greater percentage versus inpatients (p Objetivo: conocer si los pacientes estudiados en nuestra unidad de endoscopia leen y comprenden el documento de consentimiento informado. Conocer la legibilidad de dichos consentimientos informados. Método: entregamos a los pacientes estudiados endoscopicamente en nuestra unidad un cuestionario acerca del grado de lectura del consentimiento informado, conocimiento de la técnica endoscópica, complicaciones, sedación utilizada e información recibida. Valoramos la legibilidad de nuestros consentimientos informados mediante el índice de Flesch. Resultados: 309 pacientes fueron incluidos (edad media: 53 años, 55% varones. El 85% de los pacientes se había leído el consentimiento informado, el 96% conocían la técnica endoscópica, 15,2% no conocían el riesgo de complicaciones graves durante la exploración. El 82% sabía qué tipo de sedación iba a recibir. El 88% recibieron información adicional por sus médicos. Los pacientes con estudios básicos tendieron a desconocer la posibilidad de complicaciones (p < 0,05. Los médicos aportaron más información a los pacientes de

  6. Las nuevas herramientas de productividad informática aplicadas a la resolución de los modelos de previsión de estados contables

    OpenAIRE

    Bernal García, Juan Jesús; Sánchez García, Juan Francisco.

    2000-01-01

    Si el gestor empresarial no desea verse desbordado ante la ocurrencia de acontecimientos inesperados, debe recurrir a una planificación eficaz, de forma que pueda prever las nuevas situaciones y acometer, con la debida agilidad, los cambios pertinentes, teniendo especial importancia los modelos de planificación financiera, la cual utiliza, habitualmente, la programación lineal. No obstante, con frecuencia, la no linealidad y la variabilidad aleatoria de las funciones que interv...

  7. Los Alamos National Security, LLC Request for Information from industrial entities that desire to commercialize Laboratory-developed Extremely Low Resource Optical Identifier (ELROI) tech

    Energy Technology Data Exchange (ETDEWEB)

    Erickson, Michael Charles [Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

    2015-11-10

    Los Alamos National Security, LLC (LANS) is the manager and operator of the Los Alamos National Laboratory for the U.S. Department of Energy National Nuclear Security Administration under contract DE-AC52-06NA25396. LANS is a mission-centric Federally Funded Research and Development Center focused on solving the most critical national security challenges through science and engineering for both government and private customers.

  8. Uso de los sistemas de información documental en la educación superior: estado del arte Use of the Documental Information Systems in Higher Education: State of the Art

    Directory of Open Access Journals (Sweden)

    Edilma Naranjo Vélez

    2010-06-01

    Full Text Available Considerando que los Sistemas de Información Documental (SID cumplen un papel mediador en los procesos de enseñanza y de aprendizaje en la educación superior, se presenta el estado del arte que da cuenta de la necesidad de abordar este tema a partir de la relación entre la didáctica y la bibliotecología, para encontrar fuentes bibliográficas que permitan sustentar teóricamente una estrategia didáctica para enseñar a usar los SID a los profesores, y así estos los utilicen y puedan enseñar datos e información generando conocimiento, superando la memorización y repetición en los estudiantes. A partir de un enfoque hermenéutico que posibilita mostrar el avance y las tendencias del tema en diferentes países, se acude al proceso de búsqueda, recuperación, selección y evaluación de los documentos disponibles en bases de datos, bibliotecas, sitios Web, buscadores y repositorios, etc. Con los documentos seleccionados, se realiza el análisis, comprensión, interpretación y una posterior síntesis, que se presenta en este artículo, de manera concreta resaltando la metodología empleada y los resultados obtenidos; pues se comprueba que los SID con la connotación que se le da en este escrito, apenas comienzan a ser tratados como medios y espacio didáctico, ya que en gran parte al aludir al uso de la información, se centran en las Tecnologías de Información y Comunicación -TIC- con énfasis en Internet y los buscadores.Taking into account that the Documental Information Systems (DIS have a role of mediator in the teaching and learning processes in higher education, a state of the art that shows the need to talk about this topic is presented here starting from the relation between the didactics and the library science in order to find bibliographic sources that allow to theoretically support an strategy to teach professors how to use the DIS, so that they can effectively use them and teach data and information, generating

  9. Contrafuegos o el resurgimiento de los núcleos agrarios. (Reflexiones a propósito del V informe de Gobierno - Región Valle de Bravo

    Directory of Open Access Journals (Sweden)

    Sergio Zamorano Camiro

    2005-01-01

    Full Text Available La precarización de la vida campesina en los núcleos agrarios de la región Valle de Bravo puede ser remontada reactivando su estructura legal de organización. Esta constituye un importante activo de los actores colectivos que ha sido olvidado por los gobiernos y que debe ser movilizado como capital social para fomentar el desarrollo local. El núcleo agrario de Bosencheve, en el municipio de Villa de Allende fue la sede elegida por el Lic. Arturo Montiel Rojas para informar de los efectos de su gestión gubernamental en la región Valle de Bravo, que comprende a los municipios de Amanalco, Donato Guerra, Ixtapan del Oro, Otzoloapan, Santo Tomás, Valle de Bravo, Villa de Allende, Villa Victoria y Zacazonapan. Esta elección singular de la sede (un núcleo agrario, relacionada con el dato de COESPO-INEGI (2000 acerca del elevado grado de marginación (1.35 que padecen los habitantes de la región Valle de Bravo nos sugiere hacer con nuestros lectores las reflexiones que siguen.

  10. Calidad de los sistemas de información de mortalidad por violencias en Argentina y Brasil - 1990-2010 The quality of information systems on violence-related deaths in Argentina and Brazil between 1990 and 2010

    Directory of Open Access Journals (Sweden)

    Marcio Alazraqui

    2012-12-01

    Full Text Available Las muertes por violencias son un problema de salud pública por la magnitud de su impacto social y en los servicios de salud. Se realizó un estudio descriptivo de tendencia temporal a partir de los sistemas de información oficiales nacionales de mortalidad por violencias en Argentina y Brasil en el periodo 1990-2010. Se elaboraron indicadores de la calidad de la información según sexo, edad y causa de defunción. Los resultados muestran una tendencia temporal a la mejoría de calidad en los sistemas de información. Esta tendencia se repite cuando analizamos las muertes por violencias en particular, con una disminución de los registros por muertes por violencias de intencionalidad ignorada; y un porcentaje alto de muertes por armas de fuego de intencionalidad ignorada en Argentina. El análisis de la calidad de los sistemas de información de mortalidad por violencias permite detectar problemas y orientar acciones para obtener información de mayor calidad a fin de orientar políticas públicas preventivas.Violence-related deaths are a public health issue by virtue of the magnitude of their impact on society and on the health services. A study of the descriptive temporal trend was conducted using the official national information systems of violence-related mortality in Argentina and Brazil for the period from 1990 to 2010. Indicators were created to evaluate information quality by sex, age, and cause of death. The results demonstrate a temporal trend of improvement in the quality of the information systems. This trend is repeated especially when violence-related deaths are analyzed, with a decrease in the number of records for violence-related death of undetermined intent; as well as a high percentage of firearm-related deaths of undetermined intent in Argentina. The analysis of the quality of information systems regarding violence-related deaths makes it possible to detect problems and orient actions in order to obtain better quality

  11. EL JUICIO DE LOS TRANSGÉNICOS

    OpenAIRE

    Antonio F. Díaz García

    2015-01-01

    Se plantea la incertidumbre con la cual se autoriza el empleo de los transgénicos, se hace una relación de causas por las cuales no existen pruebas absolutas de la bondad de los transgénicos y se analiza la necesidad de dotar a los estudios de posible riesgo y a los informes sobre resultados de diversas pruebas de los OGMs (organismos genéticamente modificados) de un grado de credibilidad mayor. Se propone el establecimiento de sanciones mayores para los especialistas que faltan a la verdad u...

  12. Evaluación experimental de los factores de amortiguamiento en muros de concreto para vivienda

    OpenAIRE

    CARRILLO, JULIÁN; Alcocer, Sergio M.; GONZÁLEZ, GIOVANNI

    2012-01-01

    En viviendas de concreto de baja altura se emplean usualmente muros delgados con baja resistencia del concreto, cuantías mínimas de refuerzo y mallas de alambre soldado para refuerzo a cortante en el alma. Con base en la respuesta sísmica medida durante el ensayo en mesa vibratoria de seis muros de concreto de baja altura se evalúa el factor de amortiguamiento que se utiliza usualmente en el análisis dinámico especificado en los reglamentos. Las variables estudiadas fueron el tipo de concreto...

  13. ALMA OBSERVATIONS OF THE MASSIVE MOLECULAR OUTFLOW G331.512-0.103

    Energy Technology Data Exchange (ETDEWEB)

    Merello, Manuel; Bronfman, Leonardo; Garay, Guido; Lo, Nadia [Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago (Chile); Evans, Neal J. II [Department of Astronomy, University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, TX 78712-1205 (United States); Nyman, Lars-Ake; Cortes, Juan R. [Joint ALMA Observatory (JAO), Alonso de Cordova 3107, Vitacura, Santiago (Chile); Cunningham, Maria R. [School of Physics, University of New South Wales, Sydney, NSW 2052 (Australia)

    2013-09-01

    The object of this study is one of the most energetic and luminous molecular outflows known in the Galaxy, G331.512-0.103. Observations with ALMA Band 7 (350 GHz; 0.86 mm) reveal a very compact, extremely young bipolar outflow and a more symmetric outflowing shocked shell surrounding a very small region of ionized gas. The velocities of the bipolar outflow are about 70 km s{sup -1} on either side of the systemic velocity. The expansion velocity of the shocked shell is {approx}24 km s{sup -1}, implying a crossing time of about 2000 yr. Along the symmetry axis of the outflow, there is a velocity feature, which could be a molecular ''bullet'' of high-velocity dense material. The source is one of the youngest examples of massive molecular outflow found associated with a high-mass star.

  14. ALMA observations of the massive molecular outflow G331.512-0.103

    CERN Document Server

    Merello, Manuel; Garay, Guido; Lo, Nadia; Evans, Neal J; Nyman, Lars-Ake; Cortés, Juan R; Cunningham, Maria R

    2013-01-01

    The object of this study is one of the most energetic and luminous molecular outflows known in the Galaxy, G331.512-0.103. Observations with ALMA Band 7 (350 GHz; 0.86 mm) reveal a very compact, extremely young bipolar outflow and a more symmetric outflowing shocked shell surrounding a very small region of ionized gas. The velocities of the bipolar outflow are about 70 km s^{-1} on either side of the systemic velocity. The expansion velocity of the shocked shell is ~24 km s^{-1}, implying a crossing time of about 2000 yrs. Along the symmetry axis of the outflow, there is a velocity feature, which could be a molecular "bullet" of high-velocity dense material. The source is one of the youngest examples of massive molecular outflow found associated with a high-mass star.

  15. VLT/SPHERE- and ALMA-based shape reconstruction of asteroid (3) Juno

    Science.gov (United States)

    Viikinkoski, M.; Kaasalainen, M.; Ďurech, J.; Carry, B.; Marsset, M.; Fusco, T.; Dumas, C.; Merline, W. J.; Yang, B.; Berthier, J.; Kervella, P.; Vernazza, P.

    2015-09-01

    We use the recently released Atacama Large Millimeter Array (ALMA) and VLT/SPHERE science verification data, together with earlier adaptive-optics images, stellar occultation, and lightcurve data to model the 3D shape and spin of the large asteroid (3) Juno with the all-data asteroid modelling (ADAM) procedure. These data set limits on the plausible range of shape models, yielding reconstructions suggesting that, despite its large size, Juno has sizable unrounded features moulded by non-gravitational processes such as impacts. Based on observations collected at the European Southern Observatory, Paranal, Chile (prog. ID: 60.A-9379, 086.C-0785), and at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation.

  16. From Alma Ata to the Global Fund: The history of international health policy

    Directory of Open Access Journals (Sweden)

    Italian Global Health Watch

    2008-01-01

    Full Text Available “Global Funds are like stars in the sky, you can see them, admire them, appreciate their abundance… but fail to touch them.” - Ministry of Health Official, Malawi Abstract The paper traces the evolution of international health policies and international health institutions, starting from the birth of the World Health Organization, the setting up of the Health for All target at the Alma Ata conference in 1978 and the rise of neo-liberal policies promoted by international financial institutions from 1980 to the present. The paper looks at different issues surrounding public-private partnerships and the setting up of the Global Fund to fight AIDS, Tuberculosis and Malaria and the influence of these institutions on the health systems in poor countries.

  17. A bela alma e a estética goethiana do símbolo

    Directory of Open Access Journals (Sweden)

    Wilma Patricia Maas

    2011-08-01

    Full Text Available Pretende-se acompanhar o desenvolvimento do pensamento estético de Goethe entre os anos de 1780 e 1790 paralelamente a sua expressão no livro VI do romance Os anos de aprendizado de Wilhelm Meister (1795-1796, no qual se narra a trajetória da Bela Alma em direção ao progressivo abandono dos símbolos religiosos como suporte sensível da fé. Entende-se que a convivência de Goethe com Karl Philipp Moritz foi decisiva para a concepção dos ensaios “Sobre os objetos das artes plásticas” (1797 e “Imitação simples, maneira, estilo” (1789, fundamentais para a constituição do pensamento estético de Goethe à época.

  18. Platão e a cidade justa: poetas ilusionistas e potências da alma

    Directory of Open Access Journals (Sweden)

    Rachel Gazolla

    2007-12-01

    Full Text Available A censura que Platão faz à poesia na República apresenta dois ângulos que serão investigados neste texto: de um lado, a relação com a mímesis, considerada como necessária para o conhecimento pela via da phantasía; de outro, a relação do gênero epithymético da alma, com a crítica mais específica exposta no livro X.The censorship Plato directs against poetry in the Republic is investigated from two points of view in this article: on one hand, the perspective of mimesis, which is seen as necessary to achieve knowledge, through phantasía; on the other, the issue of the epithymetic genre of soul, which is part of the more specific criticism developed in book X.

  19. Constraining turbulence mixing strength in transitional discs with planets using SPHERE and ALMA

    Science.gov (United States)

    de Juan Ovelar, M.; Pinilla, P.; Min, M.; Dominik, C.; Birnstiel, T.

    2016-06-01

    We investigate the effect that the turbulent mixing strength parameter αturb plays on near-infrared polarimetric and sub-millimetre interferometric imaging observations of transitional discs (TDs) with a gap carved by a planet. We generate synthetic observations of these objects with ALMA and VLT/SPHERE-ZIMPOL by combining hydrodynamical, dust evolution, radiative transfer and instrument models for values of α _{turb}=[10^{-4}, 10^{-3}, 10^{-2}]. We find that, through a combination of effects on the viscosity of the gas, the turbulent mixing and dust evolution processes, αturb strongly affects the morphology of the dust distribution that can be traced with these observations. We constrain the value of αturb to be within an order of magnitude of 10-3 in TD sources that show cavities in sub-mm continuum images while featuring continuous distribution of dust or smaller cavities in NIR-polarimetric images.

  20. ALMA and CARMA observations of Brown Dwarfs disks: testing the models of dust evolution

    CERN Document Server

    Ricci, L; Natta, A; Scholz, A; de Gregorio-Monsalvo, I; Isella, A; Carpenter, J M

    2013-01-01

    The first steps toward planet formation involve the coagulation of small microscopic grains into larger and larger pebbles and rocks in gas-rich disks around young stars and brown dwarfs. Observations in the sub-millimeter can trace mm/cm-sized pebbles in the outer disks, and investigate the mechanisms of coagulation/fragmentation and radial migration of these solids. These represent key, yet not fully understood ingredients for our understanding of the formation of planetesimals, the building blocks of planets. Here we present the first results from an observational program using the ALMA and CARMA sub-mm/mm interferometers aimed at characterizing the dust properties and disk structure of young disks around brown dwarfs and very low mass stars. Given the physical conditions expected for these disks, they represent critical test beds for the models of the early stages of planet formation in proto-planetary disks.

  1. ¿Es posible comparar el empleo informal en los países de América del Sur? Análisis de su definición, clasificación y medición

    OpenAIRE

    Marisol E. Ruiz; Gemma Tarafa Orpinell; Pere Jódar Martínez; Joan Benach

    2015-01-01

    Objetivo: Caracterizar y analizar la situación del empleo informal respecto a su definición, medición y clasificación, en los países de América del Sur. Métodos: A través de una scoping review se realizó una revisión bibliográfica a partir de cuatro bases de datos y de literatura gris, considerando informes de organismos internacionales de los 12 países de América del Sur. Se analizó la información, valorando su contenido y se establecieron similitudes entre países. Resultados: A partir...

  2. The corporative information systems and their application in the SICORP of Comision Federal de Electricidad; Los sistemas de informacion corporativa y su aplicacion en el SICORP de la Comision Federal de Electricidad

    Energy Technology Data Exchange (ETDEWEB)

    Mejia Lavalle, Manuel; Gonzalez Sustaeta, Jorge [Instituto de Investigaciones Electricas, Temixco, Morelos (Mexico); Miranda Miranda, Oscar [Comision Federal de Electricidad (Mexico)

    2000-07-01

    To be well informed sometimes is a difficult goal to reach, mainly when the companies are developed and grown at the present times rate. It is from this necessity that the Corporative Information Systems (SIC) arise. In this article a real application of a SIC in the Comision Federal de Electricidad (CFE) is presented, in whose conceptualization and implementation, personnel of the Instituto de Investigaciones Electricas (IIE) is participating. [Spanish] Estar bien informado a veces resulta una meta dificil de alcanzar, sobre todo cuando las empresas se desarrollan y crecen al ritmo de los tiempos actuales. Es a partir de esta necesidad que surgen los Sistemas de Informacion Corporativa (SIC). En este articulo se presenta una aplicacion real de un SIC en la Comision Federal de Electricidad (CFE), en cuya conceptualizacion e implantacion esta participando personal del Instituto de Investigaciones Electricas (IIE).

  3. Spectral and morphological analysis of the remnant of supernova 1987A with ALMA and ATCA

    Energy Technology Data Exchange (ETDEWEB)

    Zanardo, Giovanna; Staveley-Smith, Lister [International Centre for Radio Astronomy Research (ICRAR), M468, University of Western Australia, Crawley, WA 6009 (Australia); Indebetouw, Remy; Chevalier, Roger A. [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904 (United States); Matsuura, Mikako; Barlow, Michael J. [Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT (United Kingdom); Gaensler, Bryan M. [Australian Research Council, Centre of Excellence for All-sky Astrophysics (CAASTRO) (Australia); Fransson, Claes; Lundqvist, Peter [Department of Astronomy, Oskar Klein Center, Stockholm University, AlbaNova, SE-106 91 Stockholm (Sweden); Manchester, Richard N. [CSIRO Astronomy and Space Science, Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710 (Australia); Baes, Maarten [Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281 S9, B-9000 Gent (Belgium); Kamenetzky, Julia R. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721-0065 (United States); Lakićević, Maša [Institute for the Environment, Physical Sciences and Applied Mathematics, Lennard-Jones Laboratories, Keele University, Staffordshire ST5 5BG (United Kingdom); Marcaide, Jon M. [Departamento de Astronomía, Universidad de Valencia, C/Dr. Moliner 50, E-46100 Burjassot (Spain); Martí-Vidal, Ivan [Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala (Sweden); Meixner, Margaret [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Ng, C.-Y. [Department of Physics, University of Hong Kong, Pokfulam Road, Hong Kong (China); Park, Sangwook, E-mail: giovanna.zanardo@gmail.com [Department of Physics, University of Texas at Arlington, 108 Science Hall, Box 19059, Arlington, TX 76019 (United States); and others

    2014-12-01

    We present a comprehensive spectral and morphological analysis of the remnant of supernova (SN) 1987A with the Australia Telescope Compact Array (ATCA) and the Atacama Large Millimeter/submillimeter Array (ALMA). The non-thermal and thermal components of the radio emission are investigated in images from 94 to 672 GHz (λ 3.2 mm to 450 μm), with the assistance of a high-resolution 44 GHz synchrotron template from the ATCA, and a dust template from ALMA observations at 672 GHz. An analysis of the emission distribution over the equatorial ring in images from 44 to 345 GHz highlights a gradual decrease of the east-to-west asymmetry ratio with frequency. We attribute this to the shorter synchrotron lifetime at high frequencies. Across the transition from radio to far infrared, both the synchrotron/dust-subtracted images and the spectral energy distribution (SED) suggest additional emission beside the main synchrotron component (S {sub ν}∝ν{sup –0.73}) and the thermal component originating from dust grains at T ∼ 22 K. This excess could be due to free-free flux or emission from grains of colder dust. However, a second flat-spectrum synchrotron component appears to better fit the SED, implying that the emission could be attributed to a pulsar wind nebula (PWN). The residual emission is mainly localized west of the SN site, as the spectral analysis yields –0.4 ≲ α ≲ –0.1 across the western regions, with α ∼ 0 around the central region. If there is a PWN in the remnant interior, these data suggest that the pulsar may be offset westward from the SN position.

  4. MILLIMETER EMISSION STRUCTURE IN THE FIRST ALMA IMAGE OF THE AU Mic DEBRIS DISK

    Energy Technology Data Exchange (ETDEWEB)

    MacGregor, Meredith A.; Wilner, David J.; Rosenfeld, Katherine A.; Andrews, Sean M. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Matthews, Brenda; Booth, Mark [Herzberg Institute of Astrophysics, 5072 West Saanich Road, Victoria, BC V9E 2E7 (Canada); Hughes, A. Meredith; Chiang, Eugene; Graham, James R.; Kalas, Paul [Department of Astronomy, 601 Campbell Hall, University of California, Berkeley, CA 94720 (United States); Kennedy, Grant [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Sibthorpe, Bruce [SRON Netherlands Institute for Space Research, NL-9747 AD Groningen (Netherlands)

    2013-01-10

    We present 1.3 mm ALMA Cycle 0 observations of the edge-on debris disk around the nearby, {approx}10 Myr old, M-type star AU Mic. These observations obtain 0.''6 (6 AU) resolution and reveal two distinct emission components: (1) the previously known dust belt that extends to a radius of 40 AU and (2) a newly recognized central peak that remains unresolved. The cold dust belt of mass {approx}1 M{sub Moon} is resolved in the radial direction with a rising emission profile that peaks sharply at the location of the outer edge of the 'birth ring' of planetesimals hypothesized to explain the midplane scattered light gradients. No significant asymmetries are discerned in the structure or position of this dust belt. The central peak identified in the ALMA image is {approx}6 times brighter than the stellar photosphere, which indicates an additional emission process in the inner regions of the system. Emission from a stellar corona or activity may contribute, but the observations show no signs of temporal variations characteristic of radio-wave flares. We suggest that this central component may be dominated by dust emission from an inner planetesimal belt of mass {approx}0.01 M{sub Moon}, consistent with a lack of emission shortward of 25 {mu}m and a location {approx}<3 AU from the star. Future millimeter observations can test this assertion, as an inner dust belt should be readily separated from the central star at higher angular resolution.

  5. Integrating a university team in the ALMA software development process: a successful model for distributed collaborations

    Science.gov (United States)

    Mora, Matias; Ibsen, Jorge; Chiozzi, Gianluca; Troncoso, Nicolás; Tobar, Rodrigo; Araya, Mauricio; Avarias, Jorge; Hoffstadt, Arturo

    2010-07-01

    Observatories are not all about exciting new technologies and scientific progress. Some time has to be dedicated to the future engineers' generations who are going to be on the front line in a few years from now. Over the past six years, ALMA Computing has been helping to build up and collaborating with a well-organized engineering students' group at Universidad Técnica Federico Santa Maria in Chile. The Computer Systems Research Group (CSRG) currently has wide collaborations with national and international organizations, mainly in the astronomical observations field. The overall coordination and technical work is done primarily by students, working side-by-side with professional engineers. This implies not only using high engineering standards, but also advanced organization techniques. This paper aims to present the way this collaboration has built up an own identity, independently of individuals, starting from its origins: summer internships at international observatories, the open-source community, and the short and busy student's life. The organizational model and collaboration approaches are presented, which have been evolving along with the years and the growth of the group. This model is being adopted by other university groups, and is also catching the attention of other areas inside the ALMA project, as it has produced an interesting training process for astronomical facilities. Many lessons have been learned by all participants in this initiative. The results that have been achieved at this point include a large number of projects, funds sources, publications, collaboration agreements, and a growing history of new engineers, educated under this model.

  6. ALMA observations of warm molecular gas and cold dust in NGC 34

    International Nuclear Information System (INIS)

    We present Atacama Large Millimeter Array (ALMA) Cycle-0 observations of the CO (6-5) line emission (rest-frame frequency = 691.473 GHz) and of the 435 μm dust continuum emission in the nuclear region of NGC 34, a local luminous infrared galaxy at a distance of 84 Mpc (1'' = 407 pc) which contains a Seyfert 2 active galactic nucleus (AGN) and a nuclear starburst. The CO emission is well resolved by the ALMA beam (0.''26 × 0.''23), with an integrated flux of f CO(6-5) = 1004 (± 151) Jy km s–1. Both the morphology and kinematics of the CO (6-5) emission are rather regular, consistent with a compact rotating disk with a size of 200 pc. A significant emission feature is detected on the redshifted wing of the line profile at the frequency of the H13CN (8-7) line, with an integrated flux of 17.7 ± 2.1(random) ± 2.7(systematic) Jy km s–1. However, it cannot be ruled out that the feature is due to an outflow of warm dense gas with a mean velocity of 400 km s–1. The continuum is resolved into an elongated configuration, and the observed flux corresponds to a dust mass of M dust = 106.97±0.13 M ☉. An unresolved central core (radius ≅ 50 pc) contributes 28% of the continuum flux and 19% of the CO (6-5) flux, consistent with insignificant contributions of the AGN to both emissions. Both the CO (6-5) and continuum spatial distributions suggest a very high gas column density (≳ 104 M ☉ pc–2) in the nuclear region at radius ≲ 100 pc.

  7. ALMA observations of warm molecular gas and cold dust in NGC 34

    Energy Technology Data Exchange (ETDEWEB)

    Xu, C. K.; Cao, C.; Lu, N.; Mazzarella, J. M.; Diaz-Santos, T.; Zhao, Y.-H.; Appleton, P.; Armus, L.; Lord, S.; Murphy, E. J.; Schulz, B. [Infrared Processing and Analysis Center, MS 100-22, California Institute of Technology, Pasadena, CA 91125 (United States); Gao, Y. [Purple Mountain Observatory, Chinese Academy of Sciences, 2 West Beijing Road, Nanjing 210008 (China); Van der Werf, P.; Meijerink, R. [Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA Leiden (Netherlands); Evans, A. S.; Stierwalt, S. [Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904 (United States); Chu, J.; Sanders, D. B. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96816 (United States); Haan, S. [CSIRO Astronomy and Space Science, ATNF, P.O. Box 76, Epping 1710 (Australia); Charmandaris, V., E-mail: caochen@sdu.edu.cn [Department of Physics, University of Crete, GR-71003, Heraklion (Greece)

    2014-05-20

    We present Atacama Large Millimeter Array (ALMA) Cycle-0 observations of the CO (6-5) line emission (rest-frame frequency = 691.473 GHz) and of the 435 μm dust continuum emission in the nuclear region of NGC 34, a local luminous infrared galaxy at a distance of 84 Mpc (1'' = 407 pc) which contains a Seyfert 2 active galactic nucleus (AGN) and a nuclear starburst. The CO emission is well resolved by the ALMA beam (0.''26 × 0.''23), with an integrated flux of f {sub CO(6-5)} = 1004 (± 151) Jy km s{sup –1}. Both the morphology and kinematics of the CO (6-5) emission are rather regular, consistent with a compact rotating disk with a size of 200 pc. A significant emission feature is detected on the redshifted wing of the line profile at the frequency of the H{sup 13}CN (8-7) line, with an integrated flux of 17.7 ± 2.1(random) ± 2.7(systematic) Jy km s{sup –1}. However, it cannot be ruled out that the feature is due to an outflow of warm dense gas with a mean velocity of 400 km s{sup –1}. The continuum is resolved into an elongated configuration, and the observed flux corresponds to a dust mass of M {sub dust} = 10{sup 6.97±0.13} M {sub ☉}. An unresolved central core (radius ≅ 50 pc) contributes 28% of the continuum flux and 19% of the CO (6-5) flux, consistent with insignificant contributions of the AGN to both emissions. Both the CO (6-5) and continuum spatial distributions suggest a very high gas column density (≳ 10{sup 4} M {sub ☉} pc{sup –2}) in the nuclear region at radius ≲ 100 pc.

  8. Detection of the Simplest Sugar, Glycolaldehyde, in a Solar-type Protostar with ALMA

    Science.gov (United States)

    Jørgensen, Jes K.; Favre, Cécile; Bisschop, Suzanne E.; Bourke, Tyler L.; van Dishoeck, Ewine F.; Schmalzl, Markus

    2012-09-01

    Glycolaldehyde (HCOCH2OH) is the simplest sugar and an important intermediate in the path toward forming more complex biologically relevant molecules. In this Letter we present the first detection of 13 transitions of glycolaldehyde around a solar-type young star, through Atacama Large Millimeter Array (ALMA) observations of the Class 0 protostellar binary IRAS 16293-2422 at 220 GHz (6 transitions) and 690 GHz (7 transitions). The glycolaldehyde lines have their origin in warm (200-300 K) gas close to the individual components of the binary. Glycolaldehyde co-exists with its isomer, methyl formate (HCOOCH3), which is a factor 10-15 more abundant toward the two sources. The data also show a tentative detection of ethylene glycol, the reduced alcohol of glycolaldehyde. In the 690 GHz data, the seven transitions predicted to have the highest optical depths based on modeling of the 220 GHz lines all show redshifted absorption profiles toward one of the components in the binary (IRAS 16293B) indicative of infall and emission at the systemic velocity offset from this by about 0farcs2 (25 AU). We discuss the constraints on the chemical formation of glycolaldehyde and other organic species—in particular, in the context of laboratory experiments of photochemistry of methanol-containing ices. The relative abundances appear to be consistent with UV photochemistry of a CH3OH-CO mixed ice that has undergone mild heating. The order of magnitude increase in line density in these early ALMA data illustrates its huge potential to reveal the full chemical complexity associated with the formation of solar system analogs.

  9. Selection of new drill sites using a Geographic Information System (GIS) at Los Azufres, Mexico; Seleccion de nuevos sitios de perforacion empleando un Sistema de Informacion Geografica (SIG) en Los Azufres, Mexico

    Energy Technology Data Exchange (ETDEWEB)

    Garcia-Estrada, G.H [Comision Federal de Electricidad, Morelia, Michoacan (Mexico)]. E-mail: gerardo.garcia04@cfe.gob.mx; Lopez-Hernandez, A [Facultad de Ingenieria Civil, Universidad Michoacana de San Nicolas de Hidalgo, Morelia (Mexico); Quijano Leon, J.L Cuauhtemoc [Comision Federal de Electricidad, Morelia, Michoacan (Mexico)

    2008-07-15

    GIS technology is used to study the effects of distance between producing wells and superficial-thermal features and faults. It is used to interpret topographic lineaments and linear-resistivity interfaces at depth to identify hidden faults. Finally, a geothermal interpretation is conducted by applying a Multi-Criteria Evaluation Method (MCE) on a comprehensive data set, including geology, geophysics, and well production data. Visual comparisons of exploratory and drilling-data maps, with thermal discharge measured from wells, were used to select variables and data ranges that could be more directly associated with energy-production levels. Relative weights assigned by visual inspection are used to extend this knowledge to the whole exploration area. Criteria are compared to calculate a geothermal index representing the geothermal-production suitability for each cell into which the study area is divided. Considering the geometry of fault planes at depths from 700 to 2000 m below the surface, and a 250 m exclusion zone around productive wells, we choose areas from the normalized-geothermal index to propose new drill sites with different levels of risk, ranging from production (low risk) to exploration (high risk) boreholes. [Spanish] Se empleo la tecnologia de Sistemas de Informacion Geografica (SIG) para estudiar el efecto de la distancia de los pozos productores a las manifestaciones termales superficiales y a las fallas, y para interpretar los lineamientos topograficos y las interfaces lineales de resistividad a profundidad para identificar fallas ocultas. Finalmente, se realizo una interpretacion geotermica aplicando un Metodo Multi-Criterio de Evaluacion (MCE) a un conjunto completo de datos que incluye geologia, geofisica y datos de produccion de pozos. Se utilizo una comparacion visual de mapas de datos de exploracion y perforacion con descargas termicas medidas en pozos, a fin de seleccionar variables y rangos de datos que podrian asociarse mas directamente

  10. SXDF-ALMA 1.5 arcmin2 Deep Survey: A Compact Dusty Star-forming Galaxy at z = 2.5

    NARCIS (Netherlands)

    Tadaki, Ken-ichi; Kohno, Kotaro; Kodama, Tadayuki; Ikarashi, Soh; Aretxaga, Itziar; Berta, Stefano; Caputi, Karina I.; Dunlop, James S.; Hatsukade, Bunyo; Hayashi, Masao; Hughes, David H.; Ivison, Rob; Izumi, Takuma; Koyama, Yusei; Lutz, Dieter; Makiya, Ryu; Matsuda, Yuichi; Nakanishi, Kouichiro; Rujopakarn, Wiphu; Tamura, Yoichi; Umehata, Hideki; Wang, Wei-Hao; Wilson, Grant W.; Wuyts, Stijn; Yamaguchi, Yuki; Yun, Min S.

    2015-01-01

    We present the first results from the SXDF-Atacama Large Millimeter/submillimeter Array (ALMA) 1.5 arcmin2 deep survey at 1.1 mm using ALMA. The map reaches a 1σ depth of 55 μJy/beam and covers 12 Hα-selected star-forming galaxies (SFGs) at z = 2.19 or z = 2.53. We have detected continuum emission f

  11. Mejorar las recomendaciones contenidas en los informes elaborados por consultores. La optimización del discurso (To improve the embedded recommendations from the consultants' detailed reports. The discourse and its enhancement

    Directory of Open Access Journals (Sweden)

    Estrella Montolío Durán

    2010-06-01

    Full Text Available El trabajo se plantea cuatro objetivos: (i caracterizar desde el punto de vista lingüístico y pragmático el género textual del informe que elaboran los profesionales de la Consultoría, género que se encuentra en pleno proceso de transformación; (ii describir las fases de las que se compone el proceso de asesoramiento de un lingüista en la optimización de este tipo de informe; (iii analizar algunos mecanismos lingüísticos y discursivos característicos de este género, así como la dificultad de su elaboración para los profesionales, y (iv reivindicar la necesidad de una línea de investigación lingüística que se imbrique con los resultados empíricos de la mejora de los intercambios comunicativos producidos en los contextos profesionales (estudios de optimización del discurso. (The present study has four principal aims. First, to offer a linguistic and pragmatic characterization of a genre under a transformation process: consultancy report. Second, to describe phases of the counseling process that linguists provide to optimize this kind of report. Third, to analyze some linguistic and discourse mechanisms, distinctive of this gender, as well as the difficulty of its elaboration for professionals. Finally, to argue for the need of a linguistic research line overlapped with the empirical results of the improvement of the communicative exchanges produced in professional settings (studies of discourse optimization.

  12. El mercado del suelo informal en favelas y la movilidad residencial de los pobres en las grandes metrópolis: un objeto de estudio para América Latina

    Directory of Open Access Journals (Sweden)

    Pedro Abramo

    2008-01-01

    Full Text Available Existe un gran vacío en los estudios urbanos, en particular de economía urbana, sobre el mercado informal de terrenos en las ciudades. La importancia actual de ese mercado y las perspectivas de su crecimiento futuro relacionadas con la evidente reducción de la ocupación (invasión de tierras urbanas, imponen la urgencia de plantearlo como un objeto de estudio prioritario. El primer esfuerzo de investigación debe ser la construcción de bancos de datos e informaciones dinámicas sobre el mercado informal de tierras y de la movilidad residencial de los pobres. La pregunta que se debe formular sobre este mercado tiene que ver con sus similitudes y diferencias con respecto al mercado formal. Nuestra respuesta a este desafío se da en dos planos. El primero, a partir de un levantamiento empírico en las favelas de la ciudad de Río de Janeiro; el segundo tomando el mercado informal de tierras y la movilidad de los pobres urbanos como un objeto conceptual que permita re-problematizar temas tradicionales de la economía urbana ortodoxa (neoclásica.

  13. Los dos cuerpos mayas: Esbozo de una antropología elemental indígena The two Maya bodies: An outline for an indigenous elemental Anthropology

    Directory of Open Access Journals (Sweden)

    Pedro Pitarch

    2011-01-01

    Full Text Available El propósito de este artículo es llamar la atención sobre la distinción indígena maya de dos clases de cuerpos humanos: uno carnal compartido con los animales y uno fenoménico específico de los seres humanos. Esta distinción resulta a su vez análoga a las dos clases de almas indígenas: una con la forma del cuerpo y otra con figura no humana, generalmente de algún animal. Semejante paralelismo entre cuerpos y almas me lleva a proponer una reorganización del concepto de persona en términos de un modelo cuaternario. Éste, sin dejar de ser fundamentalmente binario (cuerpo/alma, debe permitir integrar elementos que, como los dos cuerpos por una parte, y las dos almas por otra, se distinguen tanto como se requieren mutuamente para llegar a constituir la persona.The purpose of this paper is to draw attention to the indigenous Maya distinction between two types of human bodies: a carnal body, shared with animals, and a specifically human phenomenic body. This distinction, in turn, is equivalent to the indigenous distinction between two souls: a soul in a human shape and a soul in a non-human shape, generally of an animal species. The parallelism between bodies and souls leads me to propose a reorganization of the Mesoamerican concept of person in terms of a quaternary model which remains essentially binary (body/soul, yet permits the integration of elements which are different to each other, like the two bodies and the two souls, and yet mutually necessary to make up the person.

  14. Los inmigrados

    Directory of Open Access Journals (Sweden)

    Lojze Kovačič

    2007-12-01

    Full Text Available Lojze Kovačič nació el 9 de noviembre de 1928 en Basilea, Suiza, en una familia de emigrantes, de madre alemana y padre esloveno. En 1938, cuando las autoridades suizas expulsaron del país a todos los emigrantes que no tenían ciudadanía suiza, se fue a vivir con su familia a Eslovenia, primero a Novo mesto, luego a Ljubljana donde frecuentó la escuela primaria, secundaria y la academia de pedagogía. Vivió en Ljubljana donde trabajó primero como periodista y luego como pedagogo. Murió el 1 de mayo de 2004 en la capital eslovena. Escribió obras autobiográficas y de ficción: Ljubljanske razglednice / Postales de Ljubljana (1956, Ključi mesta / Las llaves de la ciudad (1967, Deček in smrt / El niño y la muerte (1968, Sporočila v spanju – Resničnost / Mensajes en el sueño – Realidad (1972, Pet fragmentov / Cinco fragmentos (1981, Pri{leki / Los inmigrados (trilogía 1983–85, Basel / Basilea (1986, Prah / Polvo (1988, Kristalni čas / Tiempo de cristal (1990, Zgodbe s panjskih končnic / Relatos de las tablas de la colmena (1992, Knji`evna delavnica – {ola pisanja / Taller de literatura – escuela de la escritura (1997. A continuación se presentan dos fragmentos de la primera parte de la trilogía Pri{leki / Los inmigrados, una historia marcadamente autobiográfica del retorno a Eslovenia de una familia desalojada de Basilea, narrada a través de la voz de un niño de diez años, traducida al castellano por Xavier Farré y publicada por la editorial Siruela de Madrid en 2007.

  15. Informe: Los hospitales de día intramuros para enfermos mentales en Francia Day-care hospitals for mental patients in France.

    Directory of Open Access Journals (Sweden)

    R Martínez

    1991-01-01

    Full Text Available Los hospitales de día intramuros ocupan un lugar predominante en el abanico de la asistencia psiquiátrica en Francia.
    Fueron concebidos como estructuras intermedias encaminadas a favorecer la desactivación de ese proceso inexorable, que es la cronificación de los pacientes en psiquiatría.
    Su misión primordial es la de preparar y favorecer la reinserción de los pacientes psiquiátricos procedentes del hospital, sin olvidar la dependencia adquirida por el enfermo respecto a la institución durante sus, a menudo, largas estancias en el medio psiquiátrico.

  16. Informe de los anillamientos de aves de la Estación Ornitológica de San Sebastián. Periodo 1997-2000

    Directory of Open Access Journals (Sweden)

    RIOFRIO AIZPURUA, J.

    2001-01-01

    Full Text Available En la presente publicación se resumen los anillamientos y recuperaciones de las aves anilladas por la Estación Ornitológica de San Sebastián entre los años 1997 y 2000. En este lapso de tiempo han sido anilladas 9.423 aves pertenecientes a 125 especies y subespecies diferentes. 1.459 fueron anilladas como pollos y las 7.964 restantes como volanderos. Además se detallan por especie las 152.488 aves anilladas durante los 52 años de existencia de la Estación Ornitológica de San Sebastián pertenecientes a 230 especies.

  17. Estrategia de diseño y aspectos a considerar en los planes de EEEStudios de Grado en Ingeniería Informática

    OpenAIRE

    Sánchez Carracedo, Fermín; García Almiñana, Jordi; Díaz Fondón, María Ángeles; Riesco Albizu, Miguel; Pérez Pérez, Juan Ramón; Juan Fuente, Aquilino Adolfo

    2008-01-01

    La implantación de los títulos de Grado y Postgrado en el marco del Espacio Europeo de Educación superior (EEES) supone el rediseño de todos los planes de estudios de todas las universidades europeas. De la estrategia de desarrollo utilizada para su diseño dependerá en buena parte la calidad curricular que estos títulos ofrezcan. En estos momentos, en España, sólo se han dado los primeros pasos con el diseño de una pequeña cantidad de títulos de Grado y Máster y con algunas experiencia...

  18. Programas e intervenciones de apoyo a los cuidadores informales en España Supporting programs and interventions for informal care providers in Spain

    Directory of Open Access Journals (Sweden)

    Mª Pilar Torres Egea

    2008-03-01

    Full Text Available Cuidar a personas con dependencia es una responsabilidad que implica a los familiares más directos. El cuidado individualizado suele recaer en una persona a quien se identifica como el cuidador principal. La sobrecarga que genera el cuidado continuado hace preciso que este cuidador reciba un soporte de los profesionales del ámbito sanitario y/o social. Desde el sector formal se realizan diversos programas e intervenciones, individuales o grupales, para dar soporte a los cuidadores de personas con dependencia. El presente trabajo analiza las publicaciones científicas, aparecidas en los últimos diez años, que tratan sobre diferentes programas e intervenciones de soporte a los cuidadores informales, y que surgen de la preocupación de diferentes profesionales por la calidad de vida y la salud de los cuidadores.Taking care of dependent people is a task the performance of which involves the family members. Individualized care burden is normally borne on only one person, who is identified as the main caregiver. The burden that these care activities generate makes necessary that care provider receives professional assistance from healthcare and social experts. From the formal area some programs and interventions, from both individuals and groups, are conducted to support care providers for dependent people. This work analyzes scientific publications, appeared in the last ten years, which focus on some programs and interventions to support non-professional caregivers and which arise out of some professionals worries for care providers health and quality of life.

  19. ¿Cómo manejan información los estudiantes de educación superior?: El caso de la Universidad de La Sabana, Colombia How Students of Higher Education Handle Information?

    Directory of Open Access Journals (Sweden)

    Patricia Jaramillo

    2011-12-01

    Full Text Available Esta investigación identificó las competencias en manejo de información (CMI de un grupo de estudiantes universitarios con miras a mejorar los programas de formación. Como referente teórico y de análisis se tomó el estándar propuesto por Association of College and Research Libraries. Para la recolección de datos se utilizó un cuestionario constituido por tres partes, la primera da cuenta de la percepción de los estudiantes sobre sus CMI, la segunda plantea un ejercicio que requiere poner en práctica estas competencias y tiene como resultado la producción de un texto y la tercera es la reflexión de los estudiantes sobre su desempeño en el ejercicio. Los textos fueron parte de los datos de investigación. Adicionalmente se realizaron entrevistas semi-estructuradas para profundizar en el proceso de manejo de información. Los hallazgos dan cuenta de que los participantes tienen bajo nivel de CMI, por lo que se proponen algunos lineamientos para intervenir con mayor fuerza en el fomento de estas competencias, que pueden ser considerados en otros contextos.This study identified the Information Management Competencies (CMI of university students to enhance those skills in training programs. As a theoretical reference we took the standard proposed by the Association of College and Research Libraries. For data collection we used a questionnaire consisting of three parts. The first part is related to the perception of the students about their CMI, the second part has an exercise that requires to put into practice those skills and its result is a text production, and the third part is the reflection of the students on its performance in the exercise. The texts produced were part of the research data. In addition, semi-structured interviews were done to deepen in the process of information handling. Findings shows that participants have a low CMI level, so some guidelines to strengthen the promotion of that competency are provided and can be

  20. Tecnología Informática en los procesos de enseñanza y aprendizaje semipresenciales y a distancia

    OpenAIRE

    Madoz, María Cristina; Gorga, Gladys; Sanz, Cecilia Verónica; Lanzarini, Laura Cristina; Champredonde, Raúl; De Giusti, Armando Eduardo; Pereira, Hernán; Feierherd, Guillermo Eugenio; Depetris, Beatriz O.

    2004-01-01

    En esta línea de investigación se vienen realizando estudios y trabajos experimentales relacionados con los procesos de enseñanza y de aprendizaje en modalidad semipresencial y a distancia. Entre ellos, se analiza la transformación de cursos presenciales en semipresenciales y a distancia, se evalúa a través de métricas dicha transformación, analizando luego los resultados. También se estudia el impacto de algunos ambientes de simulación y entornos de aprendizaje virtual sobre el proceso de ap...

  1. Experiencia en informática: uso del portafolio como herramienta para la mejora de la motivación en el aprendizaje de los alumnos

    OpenAIRE

    Segrelles Quilis, José Damián; Sentieri Omarrementeria, Carla; Salido, Miguel Ángel

    2013-01-01

    El rediseño de las guías docentes para su adecuación a la filosofía del Espacio Europeo de Educación Superior (EEES), ha tenido como consecuencia el aumento del empleo de metodologías activas y nuevas estrategias basadas en Evaluaciones Continuas Formativas (ECF) en los procesos de enseñanzaaprendizaje. En este marco, el uso del portafolio y las ECF son habituales en las nuevas guías docentes. El portafolio docente permite al profesor evaluar los esfuerzos realizado...

  2. Los enemigos del alma y los amigos del corazón: crónica de un exilio en femenino

    Directory of Open Access Journals (Sweden)

    Carmen Corral

    2003-01-01

    Full Text Available The main aim of these lines is to rescue from oblivion the voice and the writing of Carmen Laforet. She won the Nadal Prize in 1944, and since then silence and forgetfulness have covered her life and her work until our days. However, she is alive and we can know some details of her chosen exile through the reading of her correspondence with Ramón J. Sender from 1965 until 1975. In these letters, we find literary suggestions, philosophical thoughts and everyday incidents expressed with the sincerity of a genuine friendship. Two exiles, one of them feminine, and two passions: memory and literature.

  3. La auditoría: proceso y resultado. Análisis de los informes de auditoría depositados en el Registro Mercantil de la Región de Murcia en el periodo 1995-1998

    OpenAIRE

    Villa Sanz, Domingo de la

    2001-01-01

    Se analiza, en primer lugar, las características, metodología, contenido y fases del proceso auditor hasta llegar a su conclusión o producto final: el informe de auditoría. Posteriormente se revisan desde el punto de vista técnico los informes de auditoría depositados en el R.Mercantil de Murcia durante el periodo 1995-1998 para determinar en que medidad se adaptan a lo establecido en la normativa correspondiente, tanto desde el punto de vista formal como desde las perspectiva de su contenido...

  4. Los cuerpos del deseo: potencias y acciones colectivas

    OpenAIRE

    Ana María Fernández

    2013-01-01

    Se genealogiza aquí el binarismo alma/cuerpo y se transversaliza la problemática, abriendo la dimensión social, histórica y política de la producción de los cuerpos, y se elucidan las dimensiones deseantes de las corporalidades al valorar la noción de deseo como potencia. Su aporte es la metodología de problematización recursiva, específica para un campo de problemas de la subjetividad. Finalmente, se afirma que la elucidación, genealogización y deconstrucción de la invisibilización de las co...

  5. Los cuerpos del deseo: potencias y acciones colectivas

    Directory of Open Access Journals (Sweden)

    Ana María Fernández

    2013-10-01

    Full Text Available Se genealogiza aquí el binarismo alma/cuerpo y se transversaliza la problemática, abriendo la dimensión social, histórica y política de la producción de los cuerpos, y se elucidan las dimensiones deseantes de las corporalidades al valorar la noción de deseo como potencia. Su aporte es la metodología de problematización recursiva, específica para un campo de problemas de la subjetividad. Finalmente, se afirma que la elucidación, genealogización y deconstrucción de la invisibilización de las corporalidades crea condiciones de posibilidad para realizar la experiencia de pensar lo impensado.

  6. LOS SISTEMAS DE INFORMACIÓN GEOGRÁFICA COMO HERRAMIENTA DE APOYO EN LOS ESTUDIOS HIDROGEOLÓGICOS DOS CASOS DE ESTUDIO EN AMÉRICA LATINA: TWO CASE STUDIES IN LATIN AMERICA GEOGRAPHIC INFORMATION SYSTEMS AS A SUPPORTING TOOL IN HYDRO-GEOLOGICAL STUDIES

    Directory of Open Access Journals (Sweden)

    Mauricio Quiroz

    2007-07-01

    Full Text Available En los estudios de aguas subterráneas, se genera y recopila gran cantidad de datos, que necesariamente deben ser procesados y analizados de manera conjunta, buscando encontrar relaciones y/o patrones con los que se definen modelos conceptuales y numéricos adecuados para explicar de forma coherente el funcionamiento hidrogeológico de una zona específica. Acorde con lo anterior, los Sistemas de Información Geográfica (SIG, se plantean como una de las herramientas básicas del hidrogeólogo, ya que permiten de una manera fácil y dinámica, almacenar, analizar y visualizar datos e información, así como el análisis de su comportamiento en las dimensiones espacial y temporal. No obstante, la utilización de los SIG en los proyectos hidrogeológicos se ha limitado, en muchos casos, a la elaboración de la cartografía de las diferentes unidades hidrogeológicas incluidas dentro del área de estudio y la ubicación de diferentes mediciones y parámetros relacionados con el recurso hídrico subterráneo, en detrimento de sus capacidades para el análisis de fenómenos espaciales complejos en los cuales intervienen múltiples variables. El presente trabajo presenta dos ejemplos de aplicación en Latinoamérica en los que los sistemas de información geográfica han ayudado en la modelación y preprocesamiento de los fenómenos y variables involucradas, además de la tradicional identificación de las características esenciales de los acuíferos.In underground water studies, a big amount of data is generated and compiled: these data should be jointly processed, correlated, and analyzed in order to look for relations and /or patterns through which appropriate conceptual and numerical models are defined for explaining, in a coherent way, hydro-geological functioning in a specific zone. Geographic Information Systems (GIS must be considered as one of the basic tools of hydro-geologists, because they allow storing, analyzing, and visualizing data

  7. ALMA DETECTED OVERDENSITY OF SUB-MILLIMETER SOURCES AROUND WISE/NVSS-SELECTED z ∼ 2 DUSTY QUASARS

    Energy Technology Data Exchange (ETDEWEB)

    Silva, Andrea; Sajina, Anna [Department of Physics and Astronomy, Tufts University, Medford, MA 02155 (United States); Lonsdale, Carol; Lacy, Mark [National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States)

    2015-06-20

    We study the environments of 49 WISE/NVSS-selected dusty, hyper-luminous, z ∼ 2 quasars using the Atacama Large Millimeter/Sub-millimeter Array (ALMA) 345 GHz images. We find that 17 of the 49 WISE/NVSS sources show additional sub-millimeter galaxies within the ALMA primary beam, probing scales within ∼150 kpc. We find a total of 23 additional sub-millimeter sources, four of which are in the field of a single WISE/NVSS source. The measured 870 μm source counts are ∼10× what is expected for unbiased regions, suggesting such hyper-luminous dusty quasars are excellent at probing high-density peaks.

  8. Analysis of antenna position measurements and weather station network data during the ALMA Long Baseline Campaign of 2015

    CERN Document Server

    Hunter, Todd R; Broguiere, Dominique; Fomalont, Ed B; Dent, William R F; Phillips, Neil; Rabanus, David; Vlahakis, Catherine

    2016-01-01

    In a radio interferometer, the determination of geometrical antenna positions relies on accurate calibration of the dry and wet delay of the atmosphere above each antenna. For the Atacama Large Millimeter/Submillimeter Array (ALMA), which has baseline lengths up to 16 kilometers, the geography of the site forces the height above mean sea level of the more distant antenna pads to be significantly lower than the central array. Thus, both the ground level meteorological values and the total water column can be quite different between antennas in the extended configurations. During 2015, a network of six additional weather stations was installed to monitor pressure, temperature, relative humidity and wind velocity, in order to test whether inclusion of these parameters could improve the repeatability of antenna position determinations in these configurations. We present an analysis of the data obtained during the ALMA Long Baseline Campaign of Oct. through Nov. 2015. The repeatability of antenna position measurem...

  9. Diagnóstico del grado de alfabetización informacional en los profesionales del Centro Tecnologías para la Formación de la Universidad de las Ciencias Informáticas

    Directory of Open Access Journals (Sweden)

    Tamayo-Rueda, Deymis

    2012-06-01

    Full Text Available The increase in information curren tly available as a result of the evolution of the Internet has brought about socio-cultural phenomena such as the «infoxication» of informational service users. So much information on any single subject, together with the ease of publishing even further on the same topic, makes it confusing, and even diffi cult, to know what to look for and what is best suited to the information need in question. One way to address this phenomenon is through information literacy, thus providing mechanisms, strategies and criteria for searching and retrieving information available on the web. The mission statements of some information institutions emphasize the importance of offering information literacy programs for the benefi t of their users. From this premise the Information and Knowledge Management Group (GIC of the Technologies Training Center (FORTES at the University of Informatics Sciences (UCI, which researches and develops software products related to educational technologies, has developed products and services for improving information literacy among its users. The group has carried out the current research in order to diagnose the state of information literacy among the GIC’s users at FORTES.

    El auge informacional disponible en la actualidad a partir de la evolución de Internet, ha traído consigo fenómenos socioculturales, como la denominada infoxicación de los usuarios de los servicios informacionales. Existe tanta información sobre un mismo tema, y la posibilidad además de publicar otras sobre la misma problemática, que ya resulta confuso y hasta complejo saber qué buscar y qué es lo más idóneo para la necesidad informativa en cuestión. Una de las vías para resolver este fenómeno, es la Alfabetización Informacional, capaz de brindar mecanismos, estrategias y criterios de búsqueda y recuperación de la información disponible en la web. Algunas instituciones de información incluyen

  10. Informe: Taller de descripción de las diferencias entre Aynokas y parcela privada y muestreo preliminar de suelos para caracterizar los tipos de suelos

    OpenAIRE

    Baylon, C.; Cóndor, Pedro

    2008-01-01

    La investigación tuvo como objetivos diferenciar los tipos de suelos según su manejo (parcela privada y aynokas) utilizando indicadores mas relevantes y muestrear suelos de la aynoka más representa de la comunidad. LTRA-4 (Practices and Strategies for Vulnerable Agro-Ecosystems)

  11. Some considerations on professional ethics in information and bibliotecology Algunas reflexiones sobre la ética de los profesionales de la información y la bibliotecología

    Directory of Open Access Journals (Sweden)

    Dayanay Collado Almeida

    2011-04-01

    Full Text Available This article develops some considerations on ethics, moral and professional ethics particularly in reference to the ethics of Bibliotecology , the sciences of information and their relation with the impetuous advances in the development of Communication and Information Technology. Thus the paper defines the application of the ethical principles in the development the functions, decision taking, actions, prestige and competence in the social environment of the services of the Health Information Management. Ethics is analyzed from the standpoint of behavior, which is an essential aspect for the optimum practice of the profession in any institution of information in which the professionals of this field work. A group of professional ethic codes for Information and Bibliotecology are approached and the guidelines for each of them are also identified in this search.En este artículo se realizan algunas reflexiones sobre ética, moral y ética profesional, en particular se hace referencia a la ética en la bibliotecología, las ciencias de la información y su relación con el desarrollo impetuoso de las tecnologías de la información y las comunicaciones. Se define la aplicación de los principios éticos en el desempeño de las funciones, la toma de decisiones, acciones, prestigio y competencia en el contexto social de los servicios de gestión de información en salud. Se analiza la ética desde el punto de vista del comportamiento, el cual es un aspecto esencial para el adecuado ejercicio de la profesión en cualquier institución de información en la que se labora. Se aborda un conjunto de códigos de ética del profesional de la información y la bibliotecología y se identifican los lineamientos contemplados en cada uno de ellos.

  12. Oferta sanitaria y crisis: financiamos los bienes y servicios según su valor o caemos en la insolvencia. Informe SESPAS 2014

    Directory of Open Access Journals (Sweden)

    Enrique Bernal-Delgado

    2014-06-01

    Full Text Available La reacción de la política sanitaria a la crisis financiera ha puesto excesivo énfasis en medidas orientadas a disminuir precios unitarios, aumentar barreras (lista de espera o cerrar dispositivos. Aún es pronto para saber con fundamento científico si estos cambios en la oferta tienen correlato en la equidad de acceso o en la calidad y la seguridad de los servicios, y a la postre en la salud de los pacientes y la población. En cualquier caso, la urgencia en conseguir la estabilización fiscal ha movido el foco hacia la resolución de los problemas de liquidez presupuestaria, y ha relegado a un segundo plano medidas de mayor calado orientadas a decidir, con trazo fino, qué debe financiarse y cómo. En este trabajo se aboga por una política fundamentada en la financiación selectiva de las prestaciones sobre la base de su valor. Las experiencias de otros países pueden servirnos de orientación: métodos robustos para identificar tecnologías (o sus usos de valor cuestionable, criterios de priorización y una cuidadosa consideración de las limitaciones asociadas a la eliminación de una cierta prestación, en especial si afecta a los valores esenciales del sistema. España cuenta con los mimbres necesarios: regulación, legislación y organismos con capacidad técnica para identificar tecnologías de bajo valor, guiar las decisiones y evaluar oportunamente los efectos de estas últimas. Los obstáculos son numerosos, pero mantener el statu quo es la peor opción, dado el coste de oportunidad en pérdidas de efectividad y seguridad, equidad y eficiencia económica del Sistema Nacional de Salud, y su eventual traducción en el empeoramiento del estado de salud de la población.

  13. Evolución de los riesgos ambientales en el contexto de la crisis económica. Informe SESPAS 2014

    Directory of Open Access Journals (Sweden)

    Ferran Ballester

    2014-06-01

    Full Text Available Nuestro objetivo es analizar el impacto de la crisis económica-financiera en los determinantes ambientales de la salud. La Organización Mundial de la Salud estima que entre un 13% y un 27% de la carga de enfermedad de los países podría prevenirse mejorando el medio ambiente. Los efectos son de mayor magnitud en poblaciones más vulnerables, en especial entre los más pobres. En la última década, la contaminación atmosférica exterior (el riesgo ambiental más relevante, en términos de salud, para la mayoría de los países europeos se ha reducido moderadamente, sobre todo por las políticas europeas de reducción de emisiones y por la disminución de la actividad con la crisis económica. En los últimos años esta mejora de la calidad del aire ha sido simultánea a una reducción en las inversiones en protección ambiental, por lo que, a medio plazo, podría verse contrarrestada. La tendencia al incremento de las temperaturas en España y Europa no se ha visto reducida con la crisis económica, ya que el cambio climático es un fenómeno global que no se relaciona directamente con las emisiones locales. Para reducir el riesgo de un incremento del impacto sobre la salud de los factores ambientales existen aspectos fundamentales que deben ser considerados, como la necesidad de mantener o desarrollar sistemas de vigilancia y control adecuados y la oportunidad de aplicar políticas que ayuden a mejorar la calidad ambiental y a reducir la vulnerabilidad de diferentes grupos de la población, en un marco de trabajo intersectorial, de transparencia y de participación de la ciudadanía.

  14. Los unos y los otros

    OpenAIRE

    Victoriano, Marta Irurozqui

    2015-01-01

    La etapa de gobierno de los partidos conservadores bolivianos -Constitucional, Demócrata y Conservador- cubre el período histórico que va desde la retirada de Bolivia de la Guerra del Pacífico (1880), que enfrentó a la alianza peruana-boliviana contra Chile, hasta el estallido de la Guerra Federal de 1899 entre conservadores y liberales bolivianos. Este período de entre-guerras encierra la génesis de la implantación del régimen de partidos políticos en Bolivia. Una vez que quedó establecida u...

  15. Leibniz acerca de almas, corpos, agregados e substâncias na discussão com Fardella (1690)

    OpenAIRE

    Edgar Marques

    2010-01-01

    Defendo neste artigo, contra a interpretação de Robert Adams, a tese de que, na discussão com Fardella (1690), Leibniz adota uma ontologia realista, segundo a qual seres vivos, e não almas, são substâncias.In this article, I sustain, against Robert Adam's interpretation, the thesis that Leibniz, in the discussion with Fardella (1690), adopts a realistic ontology, according to which live beings, instead of souls, are substances.

  16. VizieR Online Data Catalog: ALMA 870um obs. of HerMES galaxies (Bussmann+, 2015)

    Science.gov (United States)

    Bussmann, R. S.; Riechers, D.; Fialkov, A.; Scudder, J.; Hayward, C. C.; Cowley, W. I.; Bock, J.; Calanog, J.; Chapman, S. C.; Cooray, A.; de Bernardis, F.; Farrah, D.; Fu, H.; Gavazzi, R.; Hopwood, R.; Ivison, R. J.; Jarvis, M.; Lacey, C.; Loeb, A.; Oliver, S. J.; Perez-Fournon, I.; Rigopoulou, D.; Roseboom, I. G.; Scott, D.; Smith, A. J.; Vieira, J. D.; Wang, L.; Wardlow, J.

    2016-02-01

    ALMA 870um data were obtained during Cycle 0 from 2012 June to December (Program 2011.0.00539.S; PI: D. Riechers). Optical imaging observations (ugriz) using the Gemini Multi-Object Spectrograph-South (GMOS-S) were conducted in queue mode during the 2013B semester as part of program GS-2013B-Q-77 (PI: R. S. Bussmann). (3 data files).

  17. Los enemigos naturales de los pulgones

    OpenAIRE

    Miñarro, Marcos

    2011-01-01

    Los pulgones se alimentan de la mayoría de los cultivos agrícolas y forestales, aunque gracias a la acción de los enemigos naturales sólo en casos puntuales se convierten en verdaderas plagas. Conocer, reconocer y facilitar la presencia de los agentes que atacan a los pulgones es el primer paso para lograr unos cultivos más sanos y libres de residuos pesticidas.

  18. Band-9 ALMA observations of the [NII] 122 micron line and FIR continuum in two high-z galaxies

    CERN Document Server

    Ferkinhoff, Carl; Nikola, Thomas; Stacey, Gordon J; Sheth, Kartik; Hailey-Dunsheath, Steve; Falgarone, Edith

    2015-01-01

    We present Atacama Large Millimeter Array (ALMA) observations of two high-redshift systems (SMMJ02399-0136 and the Cloverleaf QSO) in their rest-frame 122 micron continuum (~650 GHz or ~450 micron on-sky) and [NII] 122 micron line emission. The continuum observations with a synthesized beam of ~0.25" resolve both sources and recover the expected flux. The Cloverleaf is resolved into a partial Einstein ring, while the SMMJ02399-0136 is unambiguously separated into two components; an AGN associated point source and an extend region at the location of a previously identified dusty starburst. We detect the [NII] line in both systems, though significantly weaker than our previous detections made with the 1st generation z(Redshift) and Early Universe Spectrometer. We show that this discrepancy is mostly explained if the line flux is resolved out due to significantly more extended emission and longer ALMA baselines than expected. Based on the ALMA observations we determine that greater than 75% of the total [NII] li...

  19. Toward Precision Black Hole Masses with ALMA: NGC 1332 as a Case Study in Molecular Disk Dynamics

    CERN Document Server

    Barth, A J; Baker, A J; Boizelle, B D; Buote, D A; Ho, L C; Walsh, J L

    2016-01-01

    We present first results from a program of Atacama Large Millimeter/submillimeter Array (ALMA) CO(2-1) observations of circumnuclear gas disks in early-type galaxies. The program was designed with the goal of detecting gas within the gravitational sphere of influence of the central black holes. In NGC 1332, the 0.3"-resolution ALMA data reveal CO emission from the highly inclined (i~ 83 degrees) circumnuclear disk, spatially coincident with the dust disk seen in Hubble Space Telescope images. The disk exhibits a central upturn in maximum line-of-sight velocity reaching +-500 km/s relative to the systemic velocity, consistent with the expected signature of rapid rotation around a supermassive black hole. Rotational broadening and beam smearing produce complex and asymmetric line profiles near the disk center. We constructed dynamical models for the rotating disk and fitted the modeled CO line profiles directly to the ALMA data cube. Degeneracy between rotation and turbulent velocity dispersion in the inner dis...

  20. A low-mass protostar's disk-envelope interface: disk-shadowing evidence from ALMA DCO+ observations of VLA1623

    CERN Document Server

    Murillo, Nadia M; van Dishoeck, Ewine F; Walsh, Catherine; Harsono, Daniel; Lai, Shih-Ping; Fuchs, Christian M

    2015-01-01

    Due to instrumental limitations and a lack of disk detections, the structure between the envelope and the rotationally supported disk has been poorly studied. This is now possible with ALMA through observations of CO isotopologs and tracers of freezeout. Class 0 sources are ideal for such studies given their almost intact envelope and young disk. The structure of the disk-envelope interface of the prototypical Class 0 source, VLA1623A which has a confirmed Keplerian disk, is constrained from ALMA observations of DCO+ 3-2 and C18O 2-1. The physical structure of VLA1623 is obtained from the large-scale SED and continuum radiative transfer. An analytic model using a simple network coupled with radial density and temperature profiles is used as input for a 2D line radiative transfer calculation for comparison with the ALMA Cycle 0 12m array and Cycle 2 ACA observations of VLA1623. DCO+ emission shows a clumpy structure bordering VLA1623A's Keplerian disk, suggesting a cold ring-like structure at the disk-envelope...

  1. The Sunyaev-Zel'dovich Effect at Five Arc-seconds: RXJ1347.5-1145 Imaged by ALMA

    CERN Document Server

    Kitayama, T; Takakuwa, S; Tsutsumi, T; Komatsu, E; Akahori, T; Iono, D; Izumi, T; Kawabe, R; Kohno, K; Matsuo, H; Ota, N; Suto, Y; Takizawa, M; Yoshikawa, K

    2016-01-01

    We present the first image of the thermal Sunyaev-Zel'dovich effect (SZE) obtained by the Atacama Large Millimeter/submillimeter Array (ALMA). Combining 7-m and 12-m arrays in Band 3, we create an SZE map toward a galaxy cluster RXJ1347.5-1145 with 5 arc-second resolution (corresponding to the physical size of 20 kpc/h), the highest angular and physical spatial resolutions achieved to date for imaging the SZE, while retaining extended signals out to 40 arc-seconds. The 1-sigma statistical sensitivity of the image is 0.017 mJy/beam or 0.12 mK_CMB at the 5 arc-second full width at half maximum. The SZE image shows a good agreement with an electron pressure map reconstructed independently from the X-ray data and offers a new probe of the small-scale structure of the intracluster medium. Our results demonstrate that ALMA is a powerful instrument for imaging the SZE in compact galaxy clusters with unprecedented angular resolution and sensitivity. As the first report on the detection of the SZE by ALMA, we present ...

  2. ALMA-SZ Detection of a Galaxy Cluster Merger Shock at Half the Age of the Universe

    Science.gov (United States)

    Basu, K.; Sommer, M.; Erler, J.; Eckert, D.; Vazza, F.; Magnelli, B.; Bertoldi, F.; Tozzi, P.

    2016-10-01

    We present ALMA measurements of a merger shock using the thermal Sunyaev-Zel’dovich (SZ) effect signal, at the location of a radio relic in the famous El Gordo galaxy cluster at z≈ 0.9. Multi-wavelength analysis in combination with the archival Chandra data and a high-resolution radio image provides a consistent picture of the thermal and non-thermal signal variation across the shock front and helps to put robust constraints on the shock Mach number as well as the relic magnetic field. We employ a Bayesian analysis technique for modeling the SZ and X-ray data self-consistently, illustrating respective parameter degeneracies. Combined results indicate a shock with Mach number { M }={2.4}-0.6+1.3, which in turn suggests a high value of the magnetic field (of the order of 4-10 μ {{G}}) to account for the observed relic width at 2 GHz. At roughly half the current age of the universe, this is the highest-redshift direct detection of a cluster shock to date, and one of the first instances of an ALMA-SZ observation in a galaxy cluster. It shows the tremendous potential for future ALMA-SZ observations to detect merger shocks and other cluster substructures out to the highest redshifts.

  3. Measurement of the Black Hole Mass in NGC 1332 from ALMA Observations at 0.044 Arcsecond Resolution

    CERN Document Server

    Barth, Aaron J; Darling, Jeremy; Baker, Andrew J; Buote, David A; Ho, Luis C; Walsh, Jonelle L

    2016-01-01

    We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 3 observations of CO(2-1) emission from the circumnuclear disk in the E/S0 galaxy NGC 1332 at 0.044" resolution. The disk exhibits regular rotational kinematics and central high-velocity emission (+/-500 km/s) consistent with the presence of a compact central mass. We construct models for a thin, dynamically cold disk in the gravitational potential of the host galaxy and black hole, and fit the beam-smeared model line profiles directly to the ALMA data cube. Model fits successfully reproduce the disk kinematics out to r=200 pc. Fitting models just to spatial pixels within projected r=50 pc of the nucleus (two times larger than the black hole's gravitational radius of influence), we find M_BH=6.64(-0.63,+0.65)*10^8 solar masses. This observation demonstrates ALMA's powerful capability to determine the masses of supermassive black holes by resolving gas kinematics on small angular scales in galaxy nuclei.

  4. Aproximación cultural y textual a los informes médico forenses en la traducción especializada francés/español

    Directory of Open Access Journals (Sweden)

    Françoise Olmo Cazevieille

    2015-12-01

    Full Text Available En el ámbito de la traducción judicial francés-español, los informes forenses se han estudiado muy poco por ser documentos confidenciales de acceso limitado. No obstante, su estudio resulta de gran interés para los profesionales de la traducción especializada pues están relacionados con varias disciplinas, entre otras, el derecho y la medicina. Para caracterizarlos mejor, estudiaremos el contexto cultural de estos documentos, comprobaremos las variaciones en cuanto a su denominación en las dos lenguas y analizaremos su macroestructura mediante un estudio contrastivo de documentos originales para aportar datos que caractericen este género textual y su tipología en Francia y en España.

  5. TRINCO: una estrategia para la transformación de la información en conocimiento con el uso de los SID TRINCO: A Strategy for the Transformation of Knowledge Information with the Use of the SID

    Directory of Open Access Journals (Sweden)

    Edilma Naranjo Vélez

    2012-12-01

    Full Text Available Presenta una estrategia didáctica, fundamentada teórica y metodológicamente que permita a los profesores como usuarios de la información acercarse a los sistemas de información documental, para que sean ellos quienes enseñen a los estudiantes de la educación superior a utilizarlos a fin de que les faciliten resolver sus necesidades de información y transformar la información en conocimiento, es el objetivo central de la tesis doctoral denominada Los sistemas de información documental -SID- como medios didácticos: de la información al conocimiento, de la cual se socializan algunos de sus resultados en este artículo. Este se organiza a partir de una serie de preguntas que se responden desde la reflexión teórica, como qué es una estrategia didáctica y la metodología empleada para el diseño de la misma; se explica la estructura de la estrategia didáctica TRINCO que se diseñó desde la reflexión metodológica, y se presentan además las consideraciones finales que surgen luego de esta labor investigativa.This article presents an instructional strategy theoretically and methodologically founded in order to allow professors, as users of the information, to approach to the documental information systems to teach their higher education students how to use those systems, making easier for them to solve their information needs and transform the information into knowledge. This is the main objective of the Ph.D. dissertation, The Documental Information Systems -DIS- as instructional media: from information to knowledge, and some of its results are shared in this article as well. It is organized from a set of questions answered from the theoretical reflection as what an instructional strategy is and the methodology used for its design; the structure of the instructional strategy TRINCO designed from the methodological reflection is also explained, and final considerations arising after this research work are presented.

  6. Modeling the thermal emission from asteroid 3 Juno using ALMA observations and the KRC thermal model

    Science.gov (United States)

    Titus, Timothy N.; Li, Jian-Yang; Moullet, Arielle; Sykes, Mark V.

    2015-11-01

    Asteroid 3 Juno (hereafter referred to as Juno), discovered 1 September 1804, is the 11th largest asteroid in the Main Asteroid Belt (MAB). Containing approximately 1% of the mass in the MAB [1], Juno is the second largest S-type [2].As part of the observations acquired from Atacama Large Millimeter/submillimeter Array (ALMA) [3], 10 reconstructed images at ~60km/pixel resolution were acquired of Juno [4] that showed significant deviations from the Standard Thermal Model (STM) [5]. These deviations could be a result of surface topography, albedo variations, emissivity variations, thermal inertia variations, or any combination.The KRC thermal model [6, 7], which has been extensively used for Mars [e.g. 8, 9] and has been applied to Vesta [10] and Ceres [11], will be used to compare model thermal emission to that observed by ALMA at a wavelength of 1.33 mm [4]. The 10 images, acquired over a four hour period, captured ~55% of Juno’s 7.21 hour rotation. Variations in temperature as a function of local time will be used to constrain the source of the thermal emission deviations from the STM.This work is supported by the NASA Solar System Observations Program.References:[1] Pitjeva, E. V. (2005) Solar System Research 39(3), 176. [2] Baer, J. and S. R. Chesley (2008) Celestial Mechanics and Dynamical Astronomy, 100, 27-42. [3] Wootten A. et al. (2015) IAU General Assembly, Meeting #29, #2237199 [4] arXiv:1503.02650 [astro-ph.EP] doi: 10.1088/2041-8205/808/1/L2 [5] Lebofsky, L.A. eta al. (1986) Icarus, 68, 239-251. [6] Kieffer, H. H., et al. (1977) J. Geophys. Res., 82, 4249-4291. [7] Kieffer, Hugh H., (2013) Journal of Geophysical Research: Planets, Volume 118, Issue 3, pp. 451-470 [8] Titus, T. N., H. H. Kieffer, and P. N. Christensen (2003) Science, 299, 1048-1051. [9] Fergason, R. L. et al. (2012) Space Sci. Rev, 170, 739-773, doi:10.1007/s11214-012-9891-3. [10] Titus, T. N. et al. (2012) 43rd LPSC, held March 19-23, 2012 at The Woodlands, Texas. LPI Contribution No

  7. Terahertz Desorption Emission Spectroscopy (THz DES) – ‘ALMA in the Lab’

    Science.gov (United States)

    Emile Auriacombe, Olivier Bruno Jacques; Fraser, Helen; Ellison, Brian; Ioppolo, Sergio; Rea, Simon

    2016-06-01

    ALMA is revolutionising our scope to identify and locate molecules that have been desorbed from ices, particularly complex organic molecules (COMS), which provide a vital link between interstellar and prebiotic chemistry. Explaining the existence of these molecules in star-forming regions relies on an empirical understanding of the chemistry that underpins their formation:- do COMS form predominantly in the solid-phase and then desorb to the gas phase, or do only “smaller” species, radials or ions desorb and then undergo gas-phase chemical reactions to generate larger COMS?-are the rotational state populations in COMS only attributable to equilibrium chemistry, or could their formation mechanisms and desorption processes affect the rotational state occupancy of these molecules, thereby directly tying certain species to solid-state origins?We have developed a novel laboratory method - THz Desorption Emission Spectroscopy (THz-DES) that combines “traditional” laboratory astrophysics high-vacuum ice experiments with a sensitive high-spectral-resolution terahertz total-power heterodyne radiometer 1,2, partially mirroring the spectral range of ALMA band 7 (275– 373 GHz). Ices are grown in situ on a cold-plate, situated in a vacuum cell, then (thermally) desorbed. The sub-mm emission spectra of the resultant gas-phase molecules are detected as a function of time, temperature, or distance from the surface. Our first THz DES results will be shown for pure and binary ice systems including H2O, N2O and CH3OH. They show good correlation with established methods e.g. TPD, with the advantage of exploiting the molecular spectroscopy to unravel surface dynamics, state-occupancy, and unequivocal molecular identification, as well as concurrently measuring desorption barriers and molecular yields. We will extend our technique to a broader frequency range, enabling us to detect radical and ion desorption, to differentiate between A and E populations of CH3OH or ortho

  8. Peri physeos psyches: sobre a natureza da alma no Fedro de Platão

    Directory of Open Access Journals (Sweden)

    Maria Aparecida de Paiva Montenegro

    2010-12-01

    Full Text Available No passo 245c do Fedro de Platão, no contexto do segundo discurso de Sócrates (no qual ele compõe sua palinodia dirigida a Eros, o filósofo chama atenção para a importância de "se tornar explícita a natureza da alma, dos seus estados e atos, assim como indagar se esta natureza é humana ou divina". Pretendo mostrar que Platão, nesse diálogo, tenta fundamentar a natureza mista da alma: em parte racional em parte passional. Essa ambiguidade constitutiva mostra-se diretamente correlacionada àquelas referentes às formas de Amor, Loucura e Retórica abordadas ao longo do diálogo, à medida que estas podem ser tanto perniciosas quanto prodigiosas, a depender do modo como se as conduz. Nessa perspectiva, meu propósito é defender a presença, na filosofia pensada por Platão, de elementos passionais imprescindíveis ao sucesso de sua atividade, cabendo ao filósofo alcançar, por meio de uma formação apropriada, a maestria para reverter aquilo que pode mergulhá-lo na ignorância e, consequentemente, na escravidão e na infelicidade, naquilo que justamente irá conduzi-lo na direção oposta: a do amor à Sabedoria.In Plato's Phaedrus 245-c, when Socrates delivers his second speech (in which he composes his palinodia addressed to Eros, the philosopher calls attention to the importance of "first understanding the truth about the nature of the soul, divine or human, by examining what it does and what is done to it". I intend to point out that in this dialogue, Plato tries to found the mixed composition of the soul: partly rational, partly passionate. This constitutive ambiguity seems to be directly related to those different kinds of Love, Madness and Rhetoric examined in the dialogue, inasmuch as they could be either beneficial or harmful, depending on the way they are managed. Therefore, my purpose is to point that regarding philosophy as conceived by Plato, the appealing of passionate elements are quite indispensable for its successful

  9. Thermal structure and minor species distribution of Venus mesosphere by ALMA submm observations

    Science.gov (United States)

    Piccialli, Arianna; Moreno, Raphael; Encrenaz, Therese; Fouchet, Thierry; Lellouch, Emmanuel; Moullet, Arielle; Widemann, Thomas

    2015-11-01

    Venus upper atmosphere (70-150 km altitude) is a transition region characterized by a complex dynamics: strong retrograde zonal winds dominate the lower mesosphere while a solar-to-antisolar circulation is observed in the upper mesosphere/lower thermosphere. In addition, photochemical processes play an important role at these altitudes and affect the thermal structure and chemical stability of the entire atmosphere. Sulfur dioxide and water vapor are key species in the photochemical cycles taking place in the troposphere and mesosphere of Venus. They are carried by convective transport, together with the Hadley circulation, up to about 60 km where SO2 is photodissociated and oxydated, leading to the formation of H2SO4 which condenses in the clouds enshrouding the planet. Previous observations obtained by several instruments on board Venus Express and during ground-based campaigns have shown evidence of strong temporal variations, both on day-to-day as well as longer timescales, of density, temperature and SO2 abundance. Such strong variability is still not well understood.Submillimeter observations obtained with the Atacama Large Millimeter Array (ALMA) offer the possibility of probing Venus upper mesosphere and of monitoring minor species, winds and the thermal structure. A first set of observations was obtained on November 14, 15, 26 and 27, 2011 during the first ALMA Early Science observation cycle. These observations targeted SO2, SO, HDO and CO transitions around 345 GHz during four sequences of 30 minutes each. The Venus’ disk was about 11” with an illumination factor of 90%, so that mostly the dayside of the planet was mapped.Assuming nominal night-time and dayside CO abundance profiles from Clancy et al. 2013, we retrieved vertical temperature profiles over the entire disk as a function of latitude and local time for the four days of observation. Temperature profiles were later used to derive the abundances of minor species (HDO, SO, SO2) in each pixel

  10. LA EDUCACIÓN AMBIENTAL FORMAL EN EL CONTEXTO SOCIAL DE LA EDUCACIÓN INFORMAL Y DE LOS MEDIOS DE COMUNICACIÓN

    OpenAIRE

    Luis Quintanar Medina

    2013-01-01

    En este trabajo se analiza la contradicción que hay entre la educación ambiental formal y los medios de comunicación potenciados actualmente por las tecnologías de información y comunicación, reflejo de la contradicción entre lo que debe promover este tipo de educación y lo que propugna la ideología dominante en gran parte de los países de América Latina. Lo anterior se fundamenta en la naturaleza política de la educación en general y de la educación ambiental en particular. Se muestra que la...

  11. El acceso a la información de la administración pública en los Estados Unidos Mexicanos: la regulación del principio de libre información Access to Public Administration Information in Mexico: regulation of the Free Information Principle

    Directory of Open Access Journals (Sweden)

    Genaro Luis García López

    2007-12-01

    Full Text Available Análisis de la Ley de Acceso a la Información Pública del Estado de Sinaloa y la Ley Federal de Transparencia y Acceso a la Información Pública Gubernamental en el marco de la sociedad del conocimiento, el desarrollo de las tecnologías de la información y la comunicación, la lucha contra la corrupción y el desarrollo de la administración y el gobierno electrónicos en México. Se analizan los principios generales de derecho que son de aplicación (derecho de acceso a la información pública, privacidad de los datos personales y protección de la información privada y confidencial, se define información pública y documento, se establecen criterios para clasificar la información, se detallan los organismos afectados, se especifican criterios para establecer costos de acceso y se especifican distintos procedimientos para el desarrollo de las leyes. Se hace un estudio del posterior desarrollo normativo y la creación de organismos para cumplir los preceptos legislativos. Se concluye señalando las limitaciones que se observan en el desarrollo del libre acceso a la información y el desinterés de muchos ciudadanos, y se plantean los retos del nuevo marco para los profesionales de la documentación.The Law of Access to Public Information in the State of Sinaloa, and the Federal Law of Transparency and Access to Public Governmental Information are analysed within the framework of the knowledge society, the development of information and communication technologies, the fight against corruption and the development of e-Government and e-Administration in Mexico. General principles of law such as the right of access to public information, privacy of personal data and protection of private and confidential data are analysed; "public information" and "public document" are defined; criteria for the classification of information are established; the government bodies affected are specified, and also the criteria for establishing the cost of

  12. Witnessing the birth of the red sequence: ALMA high-resolution imaging of [CII] and dust in two interacting ultra-red starbursts at z = 4.425

    CERN Document Server

    Oteo, I; Dunne, L; Smail, I; Swinbank, M; Zhang, Z-Y; Lewis, A; Maddox, S; Riechers, D; Serjeant, S; Van der Werf, P; Bremer, M; Cigan, P; Clements, D L; Cooray, A; Dannerbauer, H; Eales, S; Ibar, E; Messias, H; Michałowski, M J; Pérez-Fournon, I; van Kampen, E

    2016-01-01

    Exploiting the sensitivity and spatial resolution of the Atacama Large Millimeter/submillimeter Array (ALMA), we have studied the morphology and the physical scale of the interstellar medium - both gas and dust - in SGP38326, an unlensed pair of interacting starbursts at $z= 4.425$. SGP38326 is the most luminous star bursting system known at $z > 4$ with an IR-derived ${\\rm SFR \\sim 4300 \\,} M_\\odot \\, {\\rm yr}^{-1}$. SGP38326 also contains a molecular gas reservoir among the most massive ever found in the early Universe, and it is the likely progenitor of a massive, red-and-dead elliptical galaxy at $z \\sim 3$. Probing scales of $\\sim 0.1"$ or $\\sim 800 \\, {\\rm pc}$ we find that the smooth distribution of the continuum emission from cool dust grains contrasts with the more irregular morphology of the gas, as traced by the [CII] fine structure emission. The gas is also extended over larger physical scales than the dust. The velocity information provided by the resolved [CII] emission reveals that the dynamics...

  13. Análisis del Informe de la Comisión Bicameral Investigadora de las Violaciones de los Derechos Humanos en la provincia de Tucumán (1974-1983

    Directory of Open Access Journals (Sweden)

    Rubén Kotler

    2007-12-01

    Full Text Available El informe de la CONADEP sostiene que a "la provincia de Tucumán le cupo el siniestro privilegio de haber inaugurado la institución centro clandestino de detención.". El presente trabajo se propone analizar el Informe elaborado por la Comisión Bicameral Investigadora de las Violaciones de los Derechos Humanos en la provincia de Tucumán, que da cuenta de cómo la represión ilegal en el "Jardín de la República" comenzó mucho antes de producirse el golpe de Estado el 24 de marzo de 1976. Un informe que no ha sido lo suficientemente difundido y que arroja datos fundamentales para saber qué ha sucedido en dicha provincia.

  14. The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud

    CERN Document Server

    Groenewegen, M A T; Marigo, P; Sloan, G C; Decin, L; Feast, M W; Goldman, S R; Justtanont, K; Kerschbaum, F; Matsuura, M; McDonald, I; Olofsson, H; Sahai, R; van Loon, J Th; Wood, P R; Zijlstra, A A; Bernard-Salas, J; Boyer, M L; Guzman-Ramirez, L; Jones, O C; Lagadec, E; Meixner, M; Rawlings, M G; Srinivasan, S

    2016-01-01

    Context: Low- and intermediate-mass stars lose most of their stellar mass at the end of their lives on the asymptotic giant branch (AGB). Determining gas and dust mass-loss rates (MLRs) is important in quantifying the contribution of evolved stars to the enrichment of the interstellar medium. Aims: Attempt to, for the first time, spectrally resolve CO thermal line emission in a small sample of AGB stars in the Large Magellanic Cloud. Methods: ALMA was used to observe 2 OH/IR stars and 4 carbon stars in the LMC in the CO J= 2-1 line. Results: We present the first measurement of expansion velocities in extragalactic carbon stars. All four C-stars are detected and wind expansion velocities and stellar velocities are directly measured. Mass-loss rates are derived from modelling the spectral energy distribution and Spitzer/IRS spectrum with the DUSTY code. Gas-to-dust ratios are derived that make the predicted velocities agree with the observed ones. The expansion velocities and MLRs are compared to a Galactic sam...

  15. ALMA observations of TiO$_2$ around VY Canis Majoris

    CERN Document Server

    De Beck, E; Muller, S; Black, J H; O'Gorman, E; Richards, A M S; Baudry, A; Maercker, M; Decin, L; Humphreys, E M

    2015-01-01

    Titanium dioxide, TiO$_2$, is a refractory species that could play a crucial role in the dust-condensation sequence around oxygen-rich evolved stars. To date, gas phase TiO$_2$ has been detected only in the complex environment of the red supergiant VY CMa. We aim to constrain the distribution and excitation of TiO$_2$ around VY CMa in order to clarify its role in dust formation. We analyse spectra and channel maps for TiO$_2$ extracted from ALMA science verification data. We detect 15 transitions of TiO$_2$, and spatially resolve the emission for the first time. The maps demonstrate a highly clumpy, anisotropic outflow in which the TiO$_2$ emission likely traces gas exposed to the stellar radiation field. A roughly east-west oriented, accelerating bipolar-like structure is found, of which the blue component runs into and breaks up around a solid continuum component. A distinct tail to the south-west is seen for some transitions, consistent with features seen in the optical and near-infrared. We find that a si...

  16. ALMA detection of the rotating molecular disk wind drom the young star HD 163296

    CERN Document Server

    Klaassen, P D; Mathews, G S; De Gregorio-Monsalvo, J C Mottram I; van Dishoeck, E F; Takahashi, S; Akiyama, E; Chapillon, E; Espada, D; Hales, A; Hogerheijde, M R; Rawlings, M; Schmalzl, M; Testi, L

    2013-01-01

    Disk winds have been postulated as a mechanism for angular momentum release in protostellar systems for decades. HD 163296 is a Herbig Ae star surrounded by a disk and has been shown to host a series of HH knots (HH 409) with bow shocks associated with the farthest knots. Here we present ALMA Science Verification data of CO J=2-1 and J=3-2 emission which are spatially coincident with the blue shifted jet of HH knots, and offset from the disk by -18.6 km/s. The emission has a double corkscrew morphology and extends more than 10" from the disk with embedded emission clumps coincident with jet knots. We interpret this double corkscrew as emission from material in a molecular disk wind, and that the compact emission near the jet knots is being heated by the jet which is moving at much higher velocities. We show that the J=3-2 emission is likely heavily filtered by the interferometer, but the J=2-1 emission suffers less due to the larger beam and measurable angular scales. Excitation analysis suggests temperatures...

  17. ALMA CO J=6-5 observations of IRAS16293-2422: Shocks and entrainment

    CERN Document Server

    Kristensen, L E; Mottram, J C; Schmalzl, M; Hogerheijde, M R

    2012-01-01

    Observations of higher-excited transitions of abundant molecules such as CO are important for determining where energy in the form of shocks is fed back into the parental envelope of forming stars. The nearby prototypical and protobinary low-mass hot core, IRAS16293-2422 (I16293) is ideal for such a study. The source was targeted with ALMA for science verification purposes in band 9, which includes CO J=6-5 (E_up/k_B ~ 116 K), at an unprecedented spatial resolution (~0.2", 25 AU). I16293 itself is composed of two sources, A and B, with a projected distance of 5". CO J=6-5 emission is detected throughout the region, particularly in small, arcsecond-sized hotspots, where the outflow interacts with the envelope. The observations only recover a fraction of the emission in the line wings when compared to data from single-dish telescopes, with a higher fraction of emission recovered at higher velocities. The very high angular resolution of these new data reveal that a bow shock from source A coincides, in the plane...

  18. Unveiling the gas and dust disk structure in HD 163296 using ALMA observations

    CERN Document Server

    de Gregorio-Monsalvo, I; Dent, W; Pinte, C; López, C; Klaassen, P; Hales, A; Cortés, P; Rawlings, M G; Tachihara, K; Testi, L; Takahashi, S; Chapillon, E; Mathews, G; Juhasz, A; Akiyama, E; Higuchi, A E; Saito, M; Nyman, L - Å; Phillips, N; Rodń, J; Corder, S; Van Kempen, T

    2013-01-01

    Aims: The aim of this work is to study the structure of the protoplanetary disk surrounding the Herbig Ae star HD 163296. Methods: We have used high-resolution and high-sensitivity ALMA observations of the CO(3-2) emission line and the continuum at 850 microns, as well as the 3- dimensional radiative transfer code MCFOST to model the data presented in this work. Results: The CO(3-2) emission unveils for the first time at sub-millimeter frequencies the vertical structure details of a gaseous disk in Keplerian rotation, showing the back- and the front-side of a flared disk. Continuum emission at 850 microns reveals a compact dust disk with a 240 AU outer radius and a surface brightness profile that shows a very steep decline at radius larger than 125 AU. The gaseous disk is more than two times larger than the dust disk, with a similar critical radius but with a shallower radial profile. Radiative transfer models of the continuum data confirms the need for a sharp outer edge to the dust disk. The models for the ...

  19. The Molecular Wind in the Nearest Seyfert Galaxy Circinus Revealed by ALMA

    CERN Document Server

    Zschaechner, Laura K; Bolatto, Alberto; Farina, Emanuele P; Kruijssen, J M Diederik; Leroy, Adam; Meier, David S; Ott, Jürgen; Veilleux, Sylvain

    2016-01-01

    We present ALMA observations of the inner 1' (1.2 kpc) of the Circinus galaxy, the nearest Seyfert. We target CO (1-0) in the region associated with a well-known multiphase outflow driven by the central active galactic nucleus (AGN). While the geometry of Circinus and its outflow make disentangling the latter difficult, we see indications of outflowing molecular gas at velocities consistent with the ionized outflow. We constrain the mass of the outflowing molecular gas to be 1.5e5 -5.1e6 solar masses, yielding a molecular outflow rate of 0.35-12.3 solar masses per year. The values within this range are comparable to the star formation rate in Circinus, indicating that the outflow indeed regulates star formation to some degree. The molecular outflow in Circinus is considerably lower in mass and energetics than previously-studied AGN-driven outflows, especially given its high ratio of AGN luminosity to bolometric luminosity. The molecular outflow in Circinus is, however, consistent with some trends put forth in...

  20. Constraining turbulence mixing strength in transitional discs with planets using SPHERE and ALMA

    CERN Document Server

    Ovelar, M de Juan; Min, M; Dominik, C; Birnstiel, T

    2016-01-01

    We investigate the effect that the turbulent mixing strength parameter $\\alpha_{\\rm{turb}}$ plays on near-infrared polarimetric and sub-millimetre interferometric imaging observations of transitional discs (TDs) with a gap carved by a planet. We generate synthetic observations of these objects with ALMA and VLT/SPHERE-ZIMPOL by combining hydrodynamical, dust evolution, radiative transfer and instrument models for values of $\\alpha_{\\rm{turb}}=[10^{-4}, 10^{-3}, 10^{-2}]$. We find that, through a combination of effects on the viscosity of the gas, the turbulent mixing and dust evolution processes, $\\alpha_{\\rm{turb}}$ strongly affects the morphology of the dust distribution that can be traced with these observations. We constrain the value of $\\alpha_{\\rm{turb}}$ to be within an order of magnitude of $10^{-3}$ in TD sources that show cavities in sub-mm continuum images while featuring continuous distribution of dust or smaller cavities in NIR-polarimetric images.

  1. Three-dimensional mapping of the water cycle and D/H on Mars with ALMA

    Science.gov (United States)

    Villanueva, Geronimo Luis; Mumma, Michael J.; Novak, Robert E.; Gurwell, Mark A.; Clarke, John T.; Tokunaga, Alan T.; Khayat, Alain; Hecht, Michael; Fisher, David Andrew

    2016-10-01

    Using ALMA, we mapped the vertical distribution of the water D/H across a broad range of terrains and times of days and local seasons on Mars. The observations were done in March/2016 and targeted four lines of isotopic water (H2O, HDO, H218O, H217O), and one line of isotopic carbon monoxide (C17O) used for establishing the thermal structure. The observations allowed us to investigate and separate how the D/H evolves on the planet, since fractionation processes induced by cloud formation would lead to notable variations of D/H along the column.Isotopic measurements are per-se excellent tracers of water loss/evolution on Mars (Villanueva et al. 2015), yet some of the recently observed variations are striking and reveal a far more complex scenario for the processes acting on the Martian water cycle. They are perhaps indicative of sub-surface water reservoirs interacting with the atmosphere, but the IR measurements did not resolve the vertical structure, limiting the untangling of climatological effects (e.g., cloud formation, Rayleigh distillation).We will present 3D maps of water and D/H and will discuss possible scenarios to explain the observations, in particular, in the context of the upper-atmosphere D/H MAVEN measurements.Villanueva, G. L., Mumma, M. J., Novak, R. E., et al. 2015, Science, 348, 218

  2. High resolution observations of the outer disk around T Cha: the view from ALMA

    CERN Document Server

    Huelamo, N; Macias, E; Pinte, C; Ireland, M; Tuthill, P; Lacour, S

    2015-01-01

    T Cha is a young star surrounded by a transitional disk with signatures of planet formation. We have obtained high-resolution and high-sensitivity ALMA observations of T Cha in the ${\\rm CO}(3$--$2)$, ${\\rm ^{13}CO}(3$--$2)$, and ${\\rm CS}(7$--$6)$ emission lines to reveal the spatial distribution of the gaseous disk around the star. In order to study the dust within the disk we have also obtained continuum images at 850$\\mu$m from the line-free channels. We have spatially resolved the outer disk around T Cha. Using the CO(3-2) emission we derive a radius of $\\sim$230 AU. We also report the detection of the $^{13}$CO(3-2) and the CS(7-8) molecular emissions, which show smaller radii than the CO(3-2) detection. The continuum observations at 850$\\mu$m allow the spatial resolution of the dusty disk, which shows two emission bumps separated by $\\sim$40AU, consistent with the presence of a dust gap in the inner regions of the disk, and an outer radius of $\\sim$80AU. Therefore, T Cha is surrounded by a compact dust...

  3. ALMA Reveals Weak [NII] Emission in "Typical" Galaxies and Intense Starbursts at z=5-6

    CERN Document Server

    Pavesi, Riccardo; Capak, Peter L; Carilli, Christopher L; Sharon, Chelsea E; Stacey, Gordon J; Karim, Alexander; Scoville, Nicholas Z; Smolcic, Vernesa

    2016-01-01

    We report interferometric measurements of [NII] 205 um fine-structure line emission from a representative sample of three galaxies at z=5-6 using the Atacama Large (sub)Millimeter Array (ALMA). These galaxies were previously detected in [CII] and far-infrared continuum emission and span almost two orders of magnitude in star formation rate (SFR). Our results show at least two different regimes of ionized inter-stellar medium properties for galaxies in the first billion years of cosmic time, separated by their L_[CII]/L_[NII] ratio. We find extremely low [NII] emission compared to [CII] (L_ [CII]/L_[NII]=68 [+200/-28]) from a "typical" L*_UV star-forming galaxy, likely directly or indirectly (by its effect on the radiation field) related to low dust abundance and low metallicity. The infrared-luminous modestly star-forming Lyman Break Galaxy (LBG) in our sample is characterized by an ionized-gas fraction (L_[CII]/L_[NII]<=20) typical of local star-forming galaxies and shows evidence for spatial variations i...

  4. Merger-induced Shocks in the Nearby LIRG VV 114 through Methanol Observations with ALMA

    CERN Document Server

    Saito, Toshiki; Espada, Daniel; Nakanishi, Kouichiro; Ueda, Junko; Sugai, Hajime; Takano, Shuro; Yun, Min S; Imanishi, Masatoshi; Ohashi, Satoshi; Lee, Minju; Hagiwara, Yoshiaki; Motohara, Kentaro; Kawabe, Ryohei

    2016-01-01

    We report the detection of two CH$_3$OH lines (J$_K$ = 2$_K$-1$_K$ and 3$_K$-2$_K$) between the progenitor's disks ("Overlap") of the mid-stage merging galaxy VV 114 obtained using the Atacama Large Millimeter/submillimeter Array (ALMA) Band 3 and Band 4. The detected CH$_3$OH emission show an extended filamentary structure (~ 3 kpc) across the progenitor's disks with relatively large velocity width (FWZI ~ 150 km/s). The emission is only significant in the "overlap" and not detected in the two merging nuclei. Assuming optically-thin emission and local thermodynamic equilibrium (LTE), we found the CH$_3$OH column density relative to H$_2$ ($X_{\\rm CH_3OH}$) peaks at the "Overlap" (~ 8 $\\times$ 10$^{-9}$), which is almost an order of magnitude larger than that at the eastern nucleus. We suggest that kpc-scale shocks driven by galaxy-galaxy collision may play an important role to enhance the CH$_3$OH abundance at the "Overlap". This scenario is consistent with that shock-induced large velocity dispersion compon...

  5. The ALMA Patchy Deep Survey: A blind search for [CII] emitters at z~4.5

    CERN Document Server

    Matsuda, Y; Iono, D; Hatsukade, B; Kohno, K; Tamura, Y; Yamaguchi, Y; Shimizu, I

    2015-01-01

    We present a result of a blind search for [CII] 158 $\\mu$m emitters at $z\\sim 4.5$ using ALMA Cycle~0 archival data. We collected extra-galactic data covering at 330-360 GHz (band~7) from 8 Cycle~0 projects from which initial results have been already published. The total number of fields is 243 and the total on-source exposure time is 19.2 hours. We searched for line emitters in continuum-subtracted data cubes with spectral resolutions of 50, 100, 300 and 500 km/s. We could not detect any new line emitters above a 6-$\\sigma$ significance level. This result provides upper limits to the [CII] luminosity function at $z\\sim 4.5$ over $L_{\\rm [CII]} \\sim 10^8 - 10^{10} L_{\\odot}$ or star formation rate, SFR $\\sim$ 10-1000 M$_{^\\odot}$/yr. These limits are at least 2 orders of magnitude larger than the [CII] luminosity functions expected from the $z \\sim 4$ UV luminosity function or from numerical simulation. However, this study demonstrates that we would be able to better constrain the [CII] luminosity function a...

  6. Pre-ALMA observations of GRBs in the mm/submm range

    CERN Document Server

    Postigo, A de Ugarte; Martín, S; Garcia-Appadoo, D; Monsalvo, I de Gregorio; Michałowski, M J; Thöne, C C; Campana, S; Gorosabel, J; Tanvir, N R; Wiersema, K; Castro-Tirado, A J; Schulze, S; De Breuck, C; Petitpas, G; Hjorth, J; Jakobsson, P; Covino, S; Fynbo, J P U; Winters, J M; Bremer, M; Levan, A J; Salvaterra, R

    2011-01-01

    It is well known that GRBs generate an afterglow emission that can be detected from radio to X-rays during days, or even weeks after the initial explosion. The peak of this emission crosses the mm/submm range during the first hours to days, making their study in this range crucial for constraining the models. Observations have been limited until now due to the low sensitivity of the observatories in this range. We present observations of 10 GRB afterglows obtained from APEX and SMA at 230 and 345GHz and put them into context with a catalogue of all the observations that have been published until now in the spectral range that will be covered by ALMA. The catalogue of mm/submm observations collected here is the largest to date and is composed of 77 GRBs, of which 65 had afterglow observations, whereas the rest are host galaxy searches. With our programmes, we contributed with data of 10 GRBs and the discovery of 2 submm counterparts. In total, the full sample, including data from the literature, has 19 aftergl...

  7. Protoplanetary Disks in the Orion OMC1 Region Imaged with ALMA

    CERN Document Server

    Eisner, J A; Ginsburg, A; Sheehan, P D

    2016-01-01

    We present ALMA observations of the Orion Nebula that cover the OMC1 outflow region. Our focus in this paper is on compact emission from protoplanetary disks. We mosaicked a field containing $\\sim 600$ near-IR-identified young stars, around which we can search for sub-mm emission tracing dusty disks. Approximately 100 sources are known proplyds identified with HST. We detect continuum emission at 1 mm wavelengths towards $\\sim 20\\%$ of the proplyd sample, and $\\sim 8\\%$ of the larger sample of near-IR objects. The noise in our maps allows 4$\\sigma$ detection of objects brighter than $\\sim 1.5$ mJy, corresponding to protoplanetary disk masses larger than 1.5 M$_{\\rm J}$ (using standard assumptions about dust opacities and gas-to-dust ratios). None of these disks are detected in contemporaneous CO(2-1) or C$^{18}$O(2-1) observations, suggesting that the gas-to-dust ratios may be substantially smaller than the canonical value of 100. Furthermore, since dust grains may already be sequestered in large bodies in ON...

  8. Isotopic Ratios of Carbon and Oxygen in Titan's CO using ALMA

    CERN Document Server

    Serigano, Joseph; Cordiner, Martin A; Irwin, Patrick G J; Teanby, Nicholas A; Charnley, Steven B; Lindberg, Johan E

    2016-01-01

    We report interferometric observations of carbon monoxide (CO) and its isotopologues in Titan's atmosphere using the Atacama Large Millimeter/submillimeter Array (ALMA). The following transitions were detected: CO (J = 1-0, 2-1, 3-2, 6-5), $^{13}$CO (J = 2-1, 3-2, 6-5), C$^{18}$O (J = 2-1, 3-2), and C$^{17}$O (J = 3-2). Molecular abundances and the vertical atmospheric temperature profile were derived by modeling the observed emission line profiles using NEMESIS, a line-by-line radiative transfer code. We present the first spectroscopic detection of $^{17}$O in the outer solar system with C$^{17}$O detected at > 8$\\sigma$ confidence. The abundance of CO was determined to be 49.6 ${\\pm}$ 1.8 ppm, assumed to be constant with altitude, with isotopic ratios $^{12}$C/$^{13}$C = 89.9 ${\\pm}$ 3.4, $^{16}$O/$^{18}$O = 486 ${\\pm}$ 22, and $^{16}$O/$^{17}$O = 2917${\\pm}$359. The measurements of $^{12}$C/$^{13}$C and $^{16}$O/$^{18}$O ratios are the most precise values obtained in Titan's atmospheric CO to date. Our res...

  9. Galactic Center Mini-spiral by ALMA - Possible Origin of the Central Cluster

    CERN Document Server

    Tsuboi, Masato; Miyoshi, Makoto; Uehara, Kenta; Tsutsumi, Takahiro; Miyazaki, Atsushi

    2016-01-01

    We present continuum images of the "Galactic Center Mini-spiral" of 100, 250, and 340 GHz bands with the analysis of the Cy.0 data acquired from the Atacama Large Millimeter/submillimeter Array (ALMA) archive. Pretty good UV coverage of the data and the "self-calibration" method give us an opportunity to obtain dynamic ranges of over 2x10^4 in the resultant maps of the 250 and 340 GHz bands. In particular the image of the 340 GHz band has high dynamic ranges unprecedented in sub-millimeter wave. The angular resolutions attain to 1.57"x1.33" in the 100 GHz band, 0.63"x0.53" in the 250 GHz band, and 0.44"x0.38" in the 340 GHz band, respectively. The continuum images clearly depict the "Mini-spiral", which is an ionized gas stream in the vicinity of Sgr A*. We found the tight correlation between the dust emission peaks and the OB/WR stars in the Northern-arm of the "Mini-spiral". The core mass function of the dust core identified by the clumpfind algorithm would obey the flat power-law dN/dM=aM^-1.5+/-0.4 on the...

  10. ALMA observations of the supergiant B[e] star Wd1-9

    CERN Document Server

    Fenech, D; Prinja, R K; Morford, J C; Dougherty, S; Blomme, R

    2016-01-01

    Mass-loss in massive stars plays a critical role in their evolution, although the precise mechanism(s) responsible - radiatively driven winds, impulsive ejection and/or binary interaction -remain uncertain. In this paper we present ALMA line and continuum observations of the supergiant B[e] star Wd1-9, a massive post-Main Sequence object located within the starburst cluster Westerlund 1. We find it to be one of the brightest stellar point sources in the sky at millimetre wavelengths, with (serendipitously identified) emission in the H41alpha radio recombination line. We attribute these properties to a low velocity (~100 km/s) ionised wind, with an extreme mass-loss rate 6.4x10^-5(d/5kpc)^1.5 Msol/yr. External to this is an extended aspherical ejection nebula indicative of a prior phase of significant mass-loss. Taken together, the millimetre properties of Wd1-9 show a remarkable similarity to those of the highly luminous stellar source MWC349A.We conclude that these objects are interacting binaries evolving a...

  11. ALMA View of the Galactic Center Mini-spiral: Ionized Gas Flows around Sagittarius A*

    CERN Document Server

    Tsuboi, Masato; Uehara, Kenta; Miyawaki, Ryosuke; Tsutsumi, Takahiro; Miyazaki, Atsushi; Miyoshi, Makoto

    2016-01-01

    We have performed the observation of the "Galactic Center Mini-spiral(GCMS)" in H42alpha recombination line as a part of the first large-scale mosaic observation in the Sagittarius A complex using Atacama Millimeter/sub-millimeter Array (ALMA). We revealed the kinematics of the ionized gas streamers of the GCMS. Especially we found that the streamer corresponding to the Bar of the GCMS has a Keplerian orbit with high eccentricity which is independent from the Keplerian orbits of the other streamers of the GCMS. The periastron is probably located within the Bondi accretion radius derived from X-ray observation. In addition, we estimated the LTE electron temperature in the sub-structures of the GCMS from the line-continuum flux density ratio. The electron temperatures are in the range of T* e=(6-13)x10^3 K. We confirmed the previously claimed tendency that the electron temperatures increase toward Sgr A*. We also found that the electron temperature at the positive velocity end of the Bar is twice as high as tha...

  12. Measuring the Distribution and Excitation of Cometary CH3OH Using ALMA

    CERN Document Server

    Cordiner, M A; Mumma, M J; Bockelée-Morvan, D; Biver, N; Villanueva, G; Paganini, L; Milam, S N; Remijan, A J; Lis, D C; Crovisier, J; Boissier, J; Kuan, Y -J; Coulson, I M

    2016-01-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) was used to obtain measurements of spatially and spectrally resolved CH$_3$OH emission from comet C/2012 K1 (PanSTARRS) on 28-29 June 2014. Detection of 12-14 emission lines of CH$_3$OH on each day permitted the derivation of spatially-resolved rotational temperature profiles (averaged along the line of sight), for the innermost 5000 km of the coma. On each day, the CH$_3$OH distribution was centrally peaked and approximately consistent with spherically symmetric, uniform outflow. The azimuthally-averaged CH$_3$OH rotational temperature ($T_{rot}$) as a function of sky-projected nucleocentric distance ($\\rho$), fell by about 40 K between $\\rho=0$ and 2500 km on 28 June, whereas on 29 June, $T_{rot}$ fell by about 50 K between $\\rho=$0 km and 1500 km. A remarkable ($\\sim50$ K) rise in $T_{rot}$ at $\\rho=$1500-2500 km on 29 June was not present on 28 June. The observed variations in CH$_3$OH rotational temperature are interpreted primarily as a result of v...

  13. Multi-molecule ALMA observations towards the Seyfert 1 galaxy NGC 1097

    CERN Document Server

    Martin, S; Izumi, T; Krips, M; Meier, D S; Aladro, R; Matsushita, S; Takano, S; Turner, J L; Espada, D; Nakajima, T; Terashima, Y; Fathi, K; Hsieh, P -Y; Imanishi, M; Lundgren, A; Nakai, N; Schinnerer, E; Sheth, K; Wiklind, T

    2014-01-01

    The nearby Sy 1 galaxy NGC 1097 represents an ideal laboratory to explore the molecular chemistry in the presence and surroundings of an active galactic nucleus. Exploring the distribution of different molecular species allows us to understand the physical processes affecting the ISM both in the AGN vicinity as well as in the outer star forming molecular ring. We carried out 3 mm ALMA observations of HCN, HCO+, CCH, CS, HNCO, SiO, HC3N, and SO as well as the 13C isotopologues. All species were imaged over the central 2 kpc (~30") of the galaxy at a resolution of ~2.2"x1.5 (150 pc x 100 pc). HCO+ and CS appear to be slightly enhanced in the star forming ring. CCH, showing the largest variations across NGC 1097, is suggested to be a good tracer of both obscured and early stage star formation. HNCO, SiO and HC3N are significantly enhanced in the inner circumnuclear disk surrounding the AGN. Differences in the molecular abundances are observed between the star forming ring and the inner circumnuclear disk. We con...

  14. Measures of galaxy dust and gas mass with Herschel photometry and prospects for ALMA

    CERN Document Server

    Berta, S; Genzel, R; Foerster-Schreiber, N M; Tacconi, L J

    2015-01-01

    (Abridged) Combining the deepest Herschel extragalactic surveys (PEP, GOODS-H, HerMES), and Monte Carlo mock catalogs, we explore the robustness of dust mass estimates based on modeling of broad band spectral energy distributions (SEDs) with two popular approaches: Draine & Li (2007, DL07) and a modified black body (MBB). As long as the observed SED extends to at least 160-200 micron in the rest frame, M(dust) can be recovered with a >3 sigma significance and without the occurrence of systematics. An average offset of a factor ~1.5 exists between DL07- and MBB-based dust masses, based on consistent dust properties. At the depth of the deepest Herschel surveys (in the GOODS-S field) it is possible to retrieve dust masses with a S/N>=3 for galaxies on the main sequence of star formation (MS) down to M(stars)~1e10 [M(sun)] up to z~1. At higher redshift (z1, the delta(GDR) dependence on metallicity is consistent with the local relation. We combine far-IR Herschel data and sub-mm ALMA expected fluxes to study ...

  15. CO gas inside the protoplanetary disk cavity in HD 142527: disk structure from ALMA

    CERN Document Server

    Perez, Sebastian; Ménard, F; Roman, P; van der Plas, G; Cieza, L; Pinte, C; Christiaens, V; Hales, A S

    2014-01-01

    Inner cavities and annular gaps in circumstellar disks are possible signposts of giant planet formation. The young star HD 142527 hosts a massive protoplanetary disk with a large cavity that extends up to 140 au from the central star, as seen in continuum images at infrared and millimeter wavelengths. Estimates of the survival of gas inside disk cavities are needed to discriminate between clearing scenarios. We present a spatially and spectrally resolved carbon monoxide isotopologue observations of the gas-rich disk HD 142527, in the J=2-1 line of 12CO, 13CO and C18O, obtained with the Atacama Large Millimeter Array (ALMA). We detect emission coming from inside the dust-depleted cavity in all three isotopologues. Based on our analysis of the gas in the dust cavity, the 12CO emission is optically thick, while 13CO and C18O emission are both optically thin. The total mass of residual gas inside the cavity is about 1.5-2 Jupiter masses. We model the gas with an axisymmetric disk model. Our best fit model shows t...

  16. Chemical complexity in protoplanetary disks in the era of ALMA and Rosetta

    CERN Document Server

    Walsh, Catherine

    2016-01-01

    Comets provide a unique insight into the molecular composition and complexity of the material in the primordial solar nebula. Recent results from the Rosetta mission, currently monitoring comet 67P/Churyumov-Gerasimenko in situ, and ALMA (the Atacama Large Millimeter/submillimeter Array), have demonstrated a tantalising link between the chemical complexity now confirmed in disks (via the detection of gas-phase CH3CN; Oberg et al. 2015) and that confirmed on the surface of 67P (Goesmann et al. 2015), raising questions concerning the chemical origin of such species (cloud or inheritance versus disk synthesis). Results from an astrochemical model of a protoplanetary disk are presented in which complex chemistry is included and in which it is assumed that simple ices only are inherited from the parent molecular cloud. The model results show good agreement with the abundances of several COMs observed on the surface of 67P with Philae/COSAC. Cosmic-ray and X-ray-induced photoprocessing of predominantly simple ices ...

  17. An ALMA Disk Mass for the Candidate Protoplanetary Companion to FW Tau

    CERN Document Server

    Kraus, Adam L; Bowler, Brendan P; Herczeg, Gregory; Ireland, Michael J; Liu, Michael C; Metchev, Stanimir; Cruz, Kelle L

    2014-01-01

    We present ALMA observations of the FW Tau system, a close binary pair of M5 stars with a wide-orbit (300 AU projected separation) substellar companion. The companion is extremely faint and red in the optical and near-infrared, but boasts a weak far-infrared excess and optical/near-infrared emission lines indicative of a primordial accretion disk of gas and dust. The component-resolved 1.3 mm continuum emission is found to be associated only with the companion, with a flux (1.78 +/- 0.03 mJy) that indicates a dust mass of 1-2 M_Earth. While this mass reservoir is insufficient to form a giant planet, it is more than sufficient to produce an analog of the Kepler-42 exoplanetary system or the Galilean satellites. The mass and geometry of the disk-bearing FW Tau companion remains unclear. Near-infrared spectroscopy shows deep water bands that indicate a spectral type later than M5, but substantial veiling prevents a more accurate determination of the effective temperature (and hence mass). Both a disk-bearing "pl...

  18. ALMA Imaging of HCN, CS and dust in Arp 220 and NGC 6240

    CERN Document Server

    Scoville, Nick; Walter, Fabian; Manohar, Swarnima; Zschaechner, Laura; Yun, Min; Koda, Jin; Sanders, David; Murchikova, Lena; Thompson, Todd; Robertson, Brant; Genzel, Reinhard; Hernquist, Lars; Tacconi, Linda; Brown, Robert; Narayanan, Desika; Hayward, Christopher C; Barnes, Joshua; Kartaltepe, Jeyhan; Davies, Richard; van der Werf, Paul; Fomalont, Edward

    2014-01-01

    We report ALMA Band 7 (350 GHz) imaging at 0.4 - 0.6arcsec resolution and Band 9 (696 GHz) at ~0.25arcsec resolution of the luminous IR galaxies Arp 220 and NGC 6240. The long wavelength dust continuum is used to estimate ISM masses for Arp 220 East, West and NGC 6240 of 1.9, 4.2 and 1.6x10^9 msun within radii of 69, 65 and 190 pc. The HCN emission was modeled to derive the emissivity distribution as a function of radius and the kinematics of each nuclear disk, yielding dynamical masses consistent with the masses and sizes derived from the dust emission. In Arp 220, the major dust and gas concentrations are at radii less than 50 pc in both counter-rotating nuclear disks. The thickness of the disks in Arp 220estimated from the velocity dispersion and rotation velocities are 10-20 pc and the mean gas densities are n_H2 ~10^5 cm^-3 at R < 50 pc. We develop an analytic treatment for the molecular excitation (including photon trapping), yielding volume densities for both the HCN and CS emission with n_H2 ~2x10^...

  19. VLA and ALMA Imaging of Intense, Galaxy-Wide Star Formation in z ~ 2 Galaxies

    CERN Document Server

    Rujopakarn, W; Rieke, G H; Ivison, R J; Cibinel, A; Nyland, K; Jagannathan, P; Silverman, J D; Alexander, D M; Biggs, A D; Bhatnagar, S; Ballantyne, D R; Dickinson, M; Elbaz, D; Geach, J E; Hayward, C C; Kirkpatrick, A; McLure, R J; Michalowski, M J; Miller, N A; Narayanan, D; Owen, F N; Pannella, M; Papovich, C; Pope, A; Rau, U; Robertson, B E; Scott, D; Swinbank, A M; van der Werf, P; van Kampen, E; Windhorst, R A

    2016-01-01

    We present $\\simeq$0$.\\!\\!^{\\prime\\prime}4$-resolution extinction-independent distributions of star formation and dust in 11 star-forming galaxies (SFGs) at $z = 1.3-3.0$. These galaxies are selected from sensitive, blank-field surveys of the $2' \\times 2'$ Hubble Ultra-Deep Field at $\\lambda = 5$ cm and 1.3 mm using the Karl G. Jansky Very Large Array (VLA) and Atacama Large Millimeter/submillimeter Array (ALMA). They have star-formation rates (SFRs), stellar masses, and dust properties representative of massive main-sequence SFGs at $z \\sim 2$. Morphological classification performed on spatially-resolved stellar mass maps indicates a mixture of disk and morphologically disturbed systems; half of the sample harbor X-ray active galactic nuclei (AGN), thereby representing a diversity of $z \\sim 2$ SFGs undergoing vigorous mass assembly. We find that their intense star formation most frequently occurs at the location of stellar-mass concentration and extends over an area comparable to their stellar-mass distrib...

  20. ALMA Imaging of Gas and Dust in a Galaxy Protocluster at Redshift 5.3

    CERN Document Server

    Riechers, Dominik A; Capak, Peter L; Scoville, Nicholas Z; Smolcic, Vernesa; Schinnerer, Eva; Yun, Min; Cox, Pierre; Bertoldi, Frank; Karim, Alexander; Yan, Lin

    2014-01-01

    We report interferometric imaging of [CII] and OH emission toward the center of the galaxy protocluster associated with the z=5.3 submillimeter galaxy (SMG) AzTEC-3, using the Atacama Large (sub)Millimeter Array (ALMA). We detect strong [CII], OH, and rest-frame 157.7 um continuum emission toward the SMG. The [CII] emission is distributed over a scale of 3.9 kpc, implying a dynamical mass of 9.7 x 10^10 Msun, and a star formation rate (SFR) surface density of Sigma_SFR = 530 Msun/yr/kpc2. This suggests that AzTEC-3 forms stars at Sigma_SFR approaching the Eddington limit for radiation pressure supported disks. We find that the OH emission is slightly blueshifted relative to the [CII] line, which may indicate a molecular outflow associated with the peak phase of the starburst. We also detect and dynamically resolve [CII] emission over a scale of 7.5 kpc toward a triplet of Lyman-break galaxies with moderate UV-based SFRs in the protocluster at ~95kpc projected distance from the SMG. These galaxies are not dete...