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Sample records for alma ata declaration

  1. 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…

  2. The Declaration of Alma Ata on its 30th anniversary: relevance for family medicine today.

    Science.gov (United States)

    Hixon, Allen L; Maskarinec, Gregory G

    2008-09-01

    The Declaration of Alma Ata, issued on September 12, 1978, provides a moral vision for primary care that remains valuable today at a time of transformation of the specialty of family medicine. The Declaration asserts a comprehensive definition of health that recognizes health as a fundamental human right, argues persuasively that gross inequalities in health status are politically, socially, and economically unacceptable, and identifies primary health care as the key to improving health and reducing health status inequalities. The values of Alma Ata can guide the specialty of family medicine to lead positive health system change through renewed collaboration, addressing inequalities, efficient use of resources and appropriate technology, and advocacy in the spirit of social justice.

  3. The enduring legacy of Alma Ata: 30 years on.

    Science.gov (United States)

    Exworthy, Mark

    2008-01-01

    The 1978 Alma Ata conference and declaration was a landmark in defining and providing a direction for primary healthcare. Despite the initial enthusiasm for Alma Ata, its impact appeared to have declined in the 1990s. However, in recent years, there has been a revitalisation of primary healthcare. This article reviews the Alma Ata conference and declaration, assesses its waxing and waning, and examines its recent revival. The paper draws conclusions about the relevance of Alma Ata, 30 years on.

  4. Primary health care development: where is Nepal after 30 years of Alma Ata Declaration?

    Science.gov (United States)

    Karkee, R; Jha, N

    2010-01-01

    The year 2008 has witnessed the global conversation to return to tenets of Alma-Ata and to review its 30 years of journey. We reviewed Nepal's journey on Primary Health Care development: policy formulation, structure development, progress and constraints. Though Nepal has institutionalised the PHC approach in health policy, strategy and health care delivery system, this has not been effectively translated into actions, and the results are mixed. Nepal has gained impressive achievements in selective primary health care markers: 45.43% maternal mortality and 62.34% child mortality reduction during 1990-2005. But gain in comprehensive health care markers is not impressive: 18.7% Skilled Birth Attendant (4% in poorest quintile and 45% in richest quintile), 39% having access to improved sanitation and 55.7% of females are literate as compared to males. Socio-political environment until recently was not favourable for comprehensive primary health care, allowing limited health sector decentralisation and community empowerment. Health activities were focussed more on selective health care strategy in the form of disease control, immunisation, vitamin A supplementation, oral rehydration solution use and contraceptive use. Nepal's rural hilly geography posed great challenge on logistic supply, communication and retention of health workers rendering public health centres of low quality with negative perceptions of consumers. Nepal is on the pathway to build equitable comprehensive primary health care.

  5. Kan strategien for primaer sundhedstjeneste genoplives 30 år efter Alma-Ata?

    DEFF Research Database (Denmark)

    Lund, Stine; Probst, Helene Bilsted; Bygbjerg, Ib

    2010-01-01

    Thirty years ago the Alma-Ata declaration on primary health care was developed. Implementation has been compounded by inadequate financing, changing disease patterns and immature health systems, and there is an ongoing discussion between selective and comprehensive primary health care supporters...

  6. Primary health care in the Eastern Mediterranean Region: from Alma-Ata to Doha.

    Science.gov (United States)

    Shawky, S

    2012-12-04

    The celebration in Doha of the 30th anniversary of the Alma-Ata Declaration at the International Conference on Primary Health Care renewed the commitment of the Eastern Mediterranean Region to primary health care as the tool for better health. The principles agreed at Alma-Ata in 1978 apply as much now as they did before. The event provided an opportunity for the Eastern Mediterranean countries to define future directions to steer the health systems to integrate primary health care and harness the intersectoral approach.

  7. Kan strategien for primær sundhedstjeneste genoplives 30 år efter Alma-Ata?

    DEFF Research Database (Denmark)

    Lund, Stine; Probst, Helene Bilsted; Bygbjerg, Ib Christian

    2010-01-01

    Thirty years ago the Alma-Ata declaration on primary health care was developed. Implementation has been compounded by inadequate financing, changing disease patterns and immature health systems, and there is an ongoing discussion between selective and comprehensive primary health care supporters...

  8. Primary health care and England: the coming of age of Alma Ata?

    Science.gov (United States)

    Green, Andrew; Ross, Duncan; Mirzoev, Tolib

    2007-01-01

    The Alma Ata Declaration is now 28 years old. This article uses its framework to assess the changes that have occurred in recent years in the English health system. It summarises the health reform changes that have occurred internationally and those in the English health system in two eras, pre- and post-1997 - when the Labour Party came to power. It concludes that linked forces of managerialism and consumerism have had an impact on the health system which has undergone a number of structural changes in recent years. It suggests that the original Alma Ata focus on equity is being modified by the concept of choice. The tensions between central priorities, often reflected in targets, and local accountability and needs are explored. There appears to be a greater interest in seeking genuine health (rather than solely health care) change, with attendant public health and partnership policies, however the gap between policy and practice still needs to be bridged, and questions as to the appropriate locus and leadership for health promotion activities addressed. However there have been numerous institutional changes which carry the danger of distracting from the purpose of achieving health change, and which continue to raise questions as to the appropriateness of a market model for health. Finally the paper argues that the PHC framework of Alma Ata remains a useful framework for assessing health systems, but needs to be tailored to, and prioritised within, a political dynamic.

  9. [Can strategy for primary health care be revitalized 30 years after Alma-Ata?].

    Science.gov (United States)

    Lund, Stine; Probst, Helene Bilsted; Bygbjerg, Ib Christian

    2010-12-06

    Thirty years ago the Alma-Ata declaration on primary health care was developed. Implementation has been compounded by inadequate financing, changing disease patterns and immature health systems, and there is an ongoing discussion between selective and comprehensive primary health care supporters. Globally, child mortality for under-five-year-olds has been reduced by 50%, but there are still large regional differences. This year the WHO development report is about revitalisation of the primary health care strategy. Recognition of this strategy may be the best instrument to improve health globally.

  10. [Alma Ata 30 years on. Evolution and perspectives of primary health care].

    Science.gov (United States)

    Maciocco, G

    2008-01-01

    The Alma Ata Declaration (September 1978) was a turning point in the definition of "Primary Health Care". The traditional bio-medical model was based on a paternalistic approach and on the treatment of the individual episodes of disease. The new bio-psycho-social model was based on prevention, continuity of care, integrated health care teams and on a direct role of patients in managing their health. Thirty years on, this approach is still relevant. Actually, it is the only adequate one to answer effectively to the current challenges: epidemiological changes (increasing prevalence of chronic diseases), social changes (increased social inequalities in health), cultural changes (increased patients demand for information and autonomy).

  11. Alma-Ata 30 years on: revolutionary, relevant, and time to revitalise.

    Science.gov (United States)

    Lawn, Joy E; Rohde, Jon; Rifkin, Susan; Were, Miriam; Paul, Vinod K; Chopra, Mickey

    2008-09-13

    In this paper, we revisit the revolutionary principles-equity, social justice, and health for all; community participation; health promotion; appropriate use of resources; and intersectoral action-raised by the 1978 Alma-Ata Declaration, a historic event for health and primary health care. Old health challenges remain and new priorities have emerged (eg, HIV/AIDS, chronic diseases, and mental health), ensuring that the tenets of Alma-Ata remain relevant. We examine 30 years of changes in global policy to identify the lessons learned that are of relevance today, particularly for accelerated scale-up of primary health-care services necessary to achieve the Millennium Development Goals, the modern iteration of the "health for all" goals. Health has moved from under-investment, to single disease focus, and now to increased funding and multiple new initiatives. For primary health care, the debate of the past two decades focused on selective (or vertical) versus comprehensive (horizontal) delivery, but is now shifting towards combining the strengths of both approaches in health systems. Debates of community versus facility-based health care are starting to shift towards building integrated health systems. Achievement of high and equitable coverage of integrated primary health-care services requires consistent political and financial commitment, incremental implementation based on local epidemiology, use of data to direct priorities and assess progress, especially at district level, and effective linkages with communities and non-health sectors. Community participation and intersectoral engagement seem to be the weakest strands in primary health care. Burgeoning task lists for primary health-care workers require long-term human resource planning and better training and supportive supervision. Essential drugs policies have made an important contribution to primary health care, but other appropriate technology lags behind. Revitalisng Alma-Ata and learning from three

  12. Primary health care: making Alma-Ata a reality.

    Science.gov (United States)

    Walley, John; Lawn, Joy E; Tinker, Anne; de Francisco, Andres; Chopra, Mickey; Rudan, Igor; Bhutta, Zulfiqar A; Black, Robert E

    2008-09-13

    The principles agreed at Alma-Ata 30 years ago apply just as much now as they did then. "Health for all" by the year 2000 was not achieved, and the Millennium Development Goals (MDGs) for 2015 will not be met in most low-income countries without substantial acceleration of primary health care. Factors have included insufficient political prioritisation of health, structural adjustment policies, poor governance, population growth, inadequate health systems, and scarce research and assessment on primary health care. We propose the following priorities for revitalising primary health care. Health-service infrastructure, including human resources and essential drugs, needs strengthening, and user fees should be removed for primary health-care services to improve use. A continuum of care for maternal, newborn, and child health services, including family planning, is needed. Evidence-based, integrated packages of community and primary curative and preventive care should be adapted to country contexts, assessed, and scaled up. Community participation and community health workers linked to strengthened primary-care facilities and first-referral services are needed. Furthermore, intersectoral action linking health and development is necessary, including that for better water, sanitation, nutrition, food security, and HIV control. Chronic diseases, mental health, and child development should be addressed. Progress should be measured and accountability assured. We prioritise research questions and suggest actions and measures for stakeholders both locally and globally, which are required to revitalise primary health care.

  13. Thirty years of Alma Ata pledges: is devolution in Pakistan an opportunity for rekindling primary health care?

    Science.gov (United States)

    Shaikh, Babar T; Kadir, Muhammad Masood; Pappas, Gregory

    2007-05-01

    The 1978 Alma Ata Conference presented the manifesto to attain global health for the next century by providing basic health care aimed at the urban and rural poor of the developing world. While the goals of Alma Ata were noble, they were untenable. Today, developing countries face serious issues of equity in health care delivery and fairness in health care management with even a greater need to transform the management systems and practice. Primary health care remains a cornerstone of building the capacity of health systems. Devolution in health sector in Pakistan seems like a chance to re-exert Alma Ata agenda. To achieve the millennium development goals by 2015, revitalization and effective implementation of primary health care will be a vital reform.

  14. 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.

  15. Healthcare for the poor and dispossessed: from Alma-Ata to the Millennium Development Goals.

    Science.gov (United States)

    Maharaj, S R

    2011-07-01

    Healthcare models which recognize the equity principle have had to confront the challenge of providing healthcare for the poor and dispossessed. Healthcare premised on "human rights" strives to remove/ reduce barriers to access by a complete waiver of all fees in the public sector or various other subsidies to make healthcare more affordable. Social welfare programmes are held hostage to the vagaries of the economy and resource scarcity. The Alma-Ata's primary healthcare is inherently a health development strategy which embraces a wholistic approach to health and wellness. This strategy, by refocussing on the Millennium Development Goals, can therefore accommodate the innovations required to overcome the challenges posed by technological, financial, cultural and geographical factors to provide a better quality of life for all, but moreso for the poor and dispossessed.

  16. 30 years after Alma-Ata: has primary health care worked in countries?

    Science.gov (United States)

    Rohde, Jon; Cousens, Simon; Chopra, Mickey; Tangcharoensathien, Viroj; Black, Robert; Bhutta, Zulfiqar A; Lawn, Joy E

    2008-09-13

    We assessed progress for primary health care in countries since Alma-Ata. First we analysed life expectancy relative to national income and HIV prevalence to identify overachieving and underachieving countries. Then we focused on the 30 low-income and middle-income countries with the highest average yearly reduction of mortality among children less than 5 years of age, describing coverage and equity of primary health care as well as non-health sector actions. These 30 countries have scaled up selective primary health care (eg, immunisation, family planning), and 14 have progressed to comprehensive primary health care, marked by high coverage of skilled attendance at birth. Good governance and progress in non-health sectors are seen in almost all of the 14 countries identified with a comprehensive primary health care system. However, these 30 countries include those that are making progress despite very low income per person, political instability, and high HIV/AIDS prevalence. Thailand has the highest average yearly reduction in mortality among children less than 5 years of age (8.5%) and has achieved universal coverage of immunisation and skilled birth attendance, with low inequity. Lessons learned from all these countries include the need for a nationally agreed package of prioritised and phased primary health care that all stakeholders are committed to implementing, attention to district management systems, and consistent investment in primary health-care extension workers linked to the health system. More detailed analysis and evaluation within and across countries would be invaluable in guiding investments for primary health care, and expediting progress towards the Millennium Development Goals and "health for all".

  17. Thirty years after Alma-Ata: a systematic review of the impact of community health workers delivering curative interventions against malaria, pneumonia and diarrhoea on child mortality and morbidity in sub-Saharan Africa

    Directory of Open Access Journals (Sweden)

    Lewin Simon

    2011-10-01

    Full Text Available Abstract Background Over thirty years have passed since the Alma-Ata Declaration on primary health care in 1978. Many governments in the first decade following the declaration responded by developing national programmes of community health workers (CHWs, but evaluations of these often demonstrated poor outcomes. As many CHW programmes have responded to the HIV/AIDS pandemic, international interest in them has returned and their role in the response to other diseases should be examined carefully so that lessons can be applied to their new roles. Over half of the deaths in African children under five years of age are due to malaria, diarrhoea and pneumonia - a situation which could be addressed through the use of cheap and effective interventions delivered by CHWs. However, to date there is very little evidence from randomised controlled trials of the impacts of CHW programmes on child mortality in Africa. Evidence from non-randomised controlled studies has not previously been reviewed systematically. Methods We searched databases of published and unpublished studies for RCTs and non-randomised studies evaluating CHW programmes delivering curative treatments, with or without preventive components, for malaria, diarrhoea or pneumonia, in children in sub-Saharan Africa from 1987 to 2007. The impact of these programmes on morbidity or mortality in children under six years of age was reviewed. A descriptive analysis of interventional and contextual factors associated with these impacts was attempted. Results The review identified seven studies evaluating CHWs, delivering a range of interventions. Limited descriptive data on programmes, contexts or process outcomes for these CHW programmes were available. CHWs in national programmes achieved large mortality reductions of 63% and 36% respectively, when insecticide-treated nets and anti-malarial chemoprophylaxis were delivered, in addition to curative interventions. Conclusions CHW programmes could

  18. ATA50 TELESCOPE: HARDWARE

    Directory of Open Access Journals (Sweden)

    C. Yesilyaprak

    2014-01-01

    Full Text Available El telescopio ATA50 es un nuevo telescopio de 50cm de di ́amet ro con ́optica RC. Fue apoyado por el Proyecto de Investigaci ́on Cient ́ıfica de la Universidad de Atat ̈urk (2 010 y establecido a 2000 m.s.n.m. en Erzurum, Turqu ́ıa en 2012. Las observaciones empezaron en 2013 bajo la direcci ́on y control de el centro de aplicaciones e investi- gaci ́ones astrof ́ısicas de la Universidad de Atat ̈urk (ATA SAM. Las propiedades t ́ecnicas e infraestructuras del Telescopio ATA50 son presentadas y al igual que el trabajo en la automatizaci ́on rob ́otica del telescopio tanto en hardware como software para ser un candidato disponible par a redes de telescopios nacionales e internacionales.

  19. The state of the ionosphere above Alma Ata

    Science.gov (United States)

    Rudina, M. P.; Solonitsyna, N. F.

    1972-01-01

    The basic patterns are described in the behavior of critical frequencies and minimum effective heights of the ionosphere's reflecting E, F1, and F2 layers, according to ionospheric recorder measurements from 1943 to 1967. The variations of critical frequencies and virtual heights are compared with the relative sunspot numbers and the flux of the sun's radio emission at 10.7 cm.

  20. ATA50 TELESCOPE: SOFTWARE

    Directory of Open Access Journals (Sweden)

    B. B. Gücsav

    2014-01-01

    Full Text Available Buscamos implementar una estructura de observatorio completamente aut ́onomo para el telescopio ATA50. T o d o s l o s c o m p o n e n t e s d e l o b s e r v a t o r i o e s t ́ a n a c t u a l m e n t e c o n t r o l a d o s m a n u a l m e n t e p o r a p l i c a c i o n e s d e M S W i n d o w s . U n s i s t e m a O C S b i e n d i s e ̃ n a d o , c o m o R T S 2 , p u e d e p r o v e e r n o s u n a s o l u c i ́ o n r ́ a p i d a . G N U / L i n u x e s nuestro sistema operativo predilecto al considerar la filosof ́ıa c ́odigo abierto y el desarrollo de RTS2 (Kubanek et al. 2006. Como era de esperarse, hemos encontrado problemas con drivers ausentes/dolorosos para nuestro equipo. Aceptar estas condiciones ha hecho que codificar los drivers de componentes f ́ısicos constituya un enorme y complejo OCS.

  1. ATA injector-gun calculations

    Energy Technology Data Exchange (ETDEWEB)

    Paul, A.C.

    1981-08-03

    ATA is a pulsed, 50 ns 10 KA, 50 MeV linear induction electron accelerator at LLNL. The ETA could be used as an injector for ATA. However the possibility of building a new injector gun for ATA, raised the question as to what changes from the ETA gun in electrode dimensions or potentials, if any, should be considered. In this report the EBQ code results for the four electrode configurations are reviewed and an attempt is made to determine the geometrical scaling laws appropriate to these ETA type gun geometries. Comparison of these scaling laws will be made to ETA operation. The characteristic operating curves for these geometries will also be presented and the effect of washer position determined. It will be shown that emittance growth will impose a limitation on beam current for a given anode potential before the virtual cathode limit is reached.

  2. 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.

  3. 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.

  4. Declarative Networking

    CERN Document Server

    Loo, Boon Thau

    2012-01-01

    Declarative Networking is a programming methodology that enables developers to concisely specify network protocols and services, which are directly compiled to a dataflow framework that executes the specifications. Declarative networking proposes the use of a declarative query language for specifying and implementing network protocols, and employs a dataflow framework at runtime for communication and maintenance of network state. The primary goal of declarative networking is to greatly simplify the process of specifying, implementing, deploying and evolving a network design. In addition, decla

  5. 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.

  6. Diagnostics for the ATA beam propagation experiments

    Energy Technology Data Exchange (ETDEWEB)

    Fessenden, T.J.; Atchison, W.L.; Barletta, W.A.

    1981-11-01

    This report contains a discussion of the diagnostics required for the beam propagation experiment to be done with the ATA accelerator. Included are a list of the diagnostics needed; a description of the ATA experimental environment; the status of beam diagnostics available at Livermore including recent developments, and a prioritized list of accelerator and propagation diagnostics under consideration or in various stages of development.

  7. 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

  8. FEMA Disaster Declarations Summary

    Data.gov (United States)

    Department of Homeland Security — The FEMA Disaster Declarations Summary is a summarized dataset describing all federally declared disasters, starting with the first disaster declaration in 1953,...

  9. 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.

  10. 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.

  11. Solar ALMA predictions: tutorial

    CERN Document Server

    Rutten, Robert J

    2016-01-01

    I have proposed that long Halpha fibrils are caused by heating events of which the tracks are afterwards outlined by contrails of cooling gas with extraordinary Halpha opacity and yet larger opacity at the ALMA wavelengths. Here I detail the radiative transfer background.

  12. 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.

  13. 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.

  14. 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.

  15. Is the Alma Ata vision of comprehensive primary health care viable? Findings from an international project

    Directory of Open Access Journals (Sweden)

    Ronald Labonté

    2014-08-01

    Full Text Available Background: The 4-year (2007–2011 Revitalizing Health for All international research program (http://www.globalhealthequity.ca/projects/proj_revitalizing/index.shtml supported 20 research teams located in 15 low- and middle-income countries to explore the strengths and weaknesses of comprehensive primary health care (CPHC initiatives at their local or national levels. Teams were organized in a triad comprised of a senior researcher, a new researcher, and a ‘research user’ from government, health services, or other organizations with the authority or capacity to apply the research findings. Multiple regional and global team capacity-enhancement meetings were organized to refine methods and to discuss and assess cross-case findings. Objective: Most research projects used mixed methods, incorporating analyses of qualitative data (interviews and focus groups, secondary data, and key policy and program documents. Some incorporated historical case study analyses, and a few undertook new surveys. The synthesis of findings in this report was derived through qualitative analysis of final project reports undertaken by three different reviewers. Results: Evidence of comprehensiveness (defined in this research program as efforts to improve equity in access, community empowerment and participation, social and environmental health determinants, and intersectoral action was found in many of the cases. Conclusions: Despite the important contextual differences amongst the different country studies, the similarity of many of their findings, often generated using mixed methods, attests to certain transferable health systems characteristics to create and sustain CPHC practices. These include: 1. Well-trained and supported community health workers (CHWs able to work effectively with marginalized communities 2. Effective mechanisms for community participation, both informal (through participation in projects and programs, and meaningful consultation and formal (though program management structures 3.Co-partnership models in program and policy development (in which financial and knowledge supports from governments or institutions are provided to communities, which retain decision-making powers in program design and implementation 4. Support for community advocacy and engagement in health and social systems decision making These characteristics, in turn, require a political context that supports state responsibilities for redistributive health and social protection measures.

  16. Learning from Alma Ata: the medical home and comprehensive primary health care.

    Science.gov (United States)

    Gottlieb, Laura M

    2009-01-01

    The patient-centered medical home (PCMH) recently has received much attention in health systems literature. The PCMH holds considerable promise for improving health outcomes and re-establishing a role for family medicine in a fragmented health care system. Despite its philosophical approach to comprehensive health care reform, the PCMH fails to offer concrete recommendations to address the social determinants of health, which include health and social policy. Political engagement to promote health is part of both primary health care and specifically family medicine's history; the absence of practical, adaptable ways to implement this engagement may undermine the PCMH's ultimate goals of improving individual and population health.

  17. Lessons from community participation in health programmes: a review of the post Alma-Ata experience.

    Science.gov (United States)

    Rifkin, Susan B

    2009-09-01

    The year 2008 marked the 30 year anniversary of Primary Health Care, the health policy of all member nations of the WHO. Community participation was one of the key principles of this policy. This article reviews the experiences of and lessons learned by policy makers, planners and programme managers in attempting to integrate community participation into their health programmes. The lessons, identified in an earlier article by the author, are still relevant today. They help to identify three reasons why integrating community participation into health programmes is so difficult. These reasons are: (1) the dominance of the bio-medical paradigm as the main planning tool for programmes, leading to the view of community participation as an intervention; (2) the lack of in-depth analysis of the perceptions of community members regarding the use of community health workers; and (3) the propensity to use a framework that limits investigation into what works, why and how in community participation in health programmes. Despite these challenges, evidence suggests that community participation has contributed to health improvements at the local level, particularly in poor communities, and will continue to be relevant to programme professionals.

  18. Lupus Alma Disk Survey

    Science.gov (United States)

    Ansdell, Megan

    2016-07-01

    We present the first unbiased ALMA survey of both dust and gas in a large sample of protoplanetary disks. We surveyed 100 sources in the nearby (150-200 pc), young (1-2 Myr) Lupus region to constrain M_dust to 2 M_Mars and M_gas to 1 M_Jup. Most disks have masses < MMSN and gas-to-dust ratios < ISM. Such rapid gas depletion may explain the prevalence of super-Earths in the exoplanet population.

  19. 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.

  20. The ALMA Frontier Fields

    Science.gov (United States)

    Bauer, Franz E.; Gonzalez-Lopez, Jorge; Laporte, Nicolas; Muñoz Arancibia, Alejandra; Villard, Eric; Kneissl, Ruediger; Kim, Sam; ALMA Frontier Fields Team

    2017-01-01

    The Frontier Fields Legacy Program targets six strong lensing clusters with deep HST and Spitzer imaging to detect and characterize the faint background galaxy population, particularly the first galaxies at z~6-10. We initiated an ALMA survey to produce “shallow” ~2'x2' maps of the Frontier Field cluster fields at 1.1mm to study intrinsically faint dusty star-forming galaxies (DSFGs) and place constraints on the star formation from a variety of interesting extragalactic source populations. Five of the six clusters have now been completed, yielding relatively uniform maps that pinpoint cool dust emission from powerful DSFGs at z>1. I will present a census of the detected objects thus far, as well as some stacking constraints on the average emission from undetected source populations.

  1. From Virgil to Alma Mater

    Science.gov (United States)

    Spitz, Ellen Handler

    2007-01-01

    For a college to become an alma mater in the hearts of its students, it must show, true to the Latin meaning, the wisdom and comfort of a good foster mother. Since "alma mater" is Latin, and since the study of Latin has waned on all educational levels in both pious and secular milieus, the author wonders whether folks who use that term really know…

  2. ALMA telescope reaches new heights

    Science.gov (United States)

    2009-09-01

    The ALMA (Atacama Large Millimeter/submillimeter Array) astronomical observatory has taken another step forward - and upwards. One of its state-of-the-art antennas was carried for the first time to the 5000m plateau of Chajnantor, in the Chilean Andes, on the back of a custom-built giant transporter. The antenna, which weighs about 100 tons and has a diameter of 12 metres, was transported up to the high-altitude Array Operations Site, where the extremely dry and rarefied air is ideal for ALMA's observations of the Universe. The conditions at the Array Operations Site on Chajnantor, while excellent for astronomy, are also very harsh. Only 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 2900 m altitude of the ALMA Operations Support Facility. It was from this relatively hospitable base camp that the ALMA antenna began its journey to the high Chajnantor site. "This is an important moment for ALMA. We are very happy that the first transport of an antenna to the high site went flawlessly. This achievement was only possible through contributions from all international ALMA partners: this particular antenna is provided by Japan, the heavy-lift transporter by Europe, and the receiving electronics inside the antenna by North America, Europe, and Asia", said Wolfgang Wild, European ALMA Project Manager. The trip began when one of the two ALMA transporters, named Otto, lifted the antenna onto its back. It then carried its heavy load along the 28 km road from the Operations Support Facility up to the Array Operations Site. While the transporter is capable of speeds of up to 12 km/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 are the most advanced submillimetre-wavelength antennas ever made. They are designed to operate fully exposed in the harsh conditions

  3. Advanced techniques for actinide spectroscopy (ATAS 2012). Abstract book

    Energy Technology Data Exchange (ETDEWEB)

    Foerstendorf, Harald; Mueller, Katharina; Steudtner, Robin (eds.)

    2012-07-01

    The abstract book of the International workshop on advanced techniques for actinide spectroscopy (ATAS 2012) include contributions concerning the following issues: environmental applications, NMR spectroscopy, vibrational spectroscopy, X-ray spectroscopy and theory, technical application: separation processes, emission spectroscopy.

  4. O livro da alma

    Directory of Open Access Journals (Sweden)

    Oliver Tolle

    2016-12-01

    Full Text Available Trata-se de compreender os pressupostos da filosofia concreta pretendida por Johann Gottfried Herder (1744-1803 em uma série de textos redigidos durante as décadas de 1760-70. Se, por um lado, Herder demonstra afinidade com a mesma harmonia preestabelecida que está na base de leibnizianos como Gottsched e Baumgarten, por outro, ele aprofunda a discussão sobre a origem do conhecimento humano ao reduzir a importância de juízos de valor universal e acentuar a necessidade de uma aproximação constante das sensações que se agitam obscuramente no fundo da alma. Disso resulta uma concepção inusitada de sabedoria, a qual depende de uma renúncia à posse confortável de conhecimentos abstratos e da aceitação da natureza cambiante e apenas parcialmente perscrutável daquilo que nos move. Se com isso perde-se a certeza, abre-se em contrapartida uma dimensão essencialmente ativa e sensível de realização no mundo.

  5. 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...

  6. Declarative programming in PROLOG

    Directory of Open Access Journals (Sweden)

    Felician ALECU

    2014-03-01

    Full Text Available The declarative programming by declarative languages is clearly the best option a programmer can have for a completely readable, flexible and extensible code. Today, the economics of programming is clearly focused on the declarative paradigm while most imperative languages are trying to become cost effective by using new added declarative features for productivity and ease of use, like the Java 8. This paper tries to demonstrate a declarative language like PROLOG is perfectly suitable to be used to solve even common programming issue, like deciding an element is part of an array or not.

  7. 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.

  8. TV-acquired optical diagnostics systems on ATA

    Energy Technology Data Exchange (ETDEWEB)

    Kalibjian, R.; Chong, Y.P.; Cornish, J.P.; Jackson, C.H.; Fessenden, T.J.

    1984-06-01

    The purpose of this paper is to report on optical system developments on the ATA and their applications to ATA beam characterization. Television (TV)-acquired optical diagnostics data provide spatial and temporal properties of the ATA beam that complements recorded information from other types of sensors, such as, beam-wall current monitors, x-ray probes, and rf probes. The ATA beam operates: (1) in the normal mode at 50-MeV, 10-kA at a 1-Hz rate; and (2) in the 1-KHz burst mode (for 10-pulses) at a 0.5 Hz rate. The beam has a 70-ns pulse width in vacuum propagation; however, beam-head erosion will occur in atmospheric propagation, thus limiting the pulse width to less than 50-ns. Various optical systems are used for ATA diagnostics. Optical-imaging provides a convenient measurement in a single pulse of the 2-dimensional profile of the beam intensity. It can also provide multiple 2-D framing in a single pulse. In some studies it may be desirable to study optical events with temporal resolution less than 100-ps with 1-dimensional streak cameras. Spatially integrated data from phototube cameras can also be used for background measurement applications as well as for single pixel monitoring. The optical line-of-sight (LOS) configurations have been made versatile to accommodate a large number of options for the various optical systems.

  9. 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.

  10. Permasalahan Iman : Kritik Atas Iman Dalam Filsafat Barat dan Tawaran Jawaban

    Directory of Open Access Journals (Sweden)

    Setyo Wibowo

    2013-06-01

    Full Text Available Abstract : Faith becomes problematic in our modern world. In the age of secularization and emancipation man masters the Nature with his growing reason and ever developing technology. This new situation brings with itself a discredit toward faith and religion. Without refusing the existence of God, Immanuel Kant declares that theology is a paralogism (a fallacious reasoning. Auguste Comte corners the religion in the realm of infantile age to be overcomed by the progress of science. Meanwhile Friedrich Nietzsche, from his own view, analyses that the phenomenon of fanatism in religion hides the uncontrallble “need to believe” typically found among the weaks.The central critique of Martin Heidegger toward ontotheological metaphysics shows that theology defined as science does not think. Man of faith has already all the answer before a question is posed, therefore he cannot truly pariticipate in the question of Being. This article tries to consider these objections against faith. As an answer, this article offers to acknowledge “the act of believe” as an universal disposition in man. Much wider than his need to possess knowledge, man is driven by a desire for the infinite. Faith resumes this human desire for infinite.Keywords : Emancipation, theology, metaphysics, faith, knowledge, way of belief, act of belief, passivity, infinite horizon, anthropological disposision.Abstrak : Iman menjadi problem di dunia modern. Gerak sekularisasi dan emansipasi manusia berkat perkembangan rasionya, yang tampak dalam penguasaan manusia atas alam lewat teknologi, membuat keyakinan pada Tuhan dianggap ketinggalan roh jaman. Meskipun tidak menolak Tuhan, Immanuel Kant menganggap bahwa teologi adalah sebuah paralogisme. Auguste Comte tegas-tegas mengatakan bahwa jaman teologi dan agama adalah era kekanak-kanakan yang harus dilampaui demi kemajuan jaman. Friedrich Nietzsche memperingatkan bahwa fanatisme dalam agama adalah tanda besarnya kebutuhan manusia

  11. A Look Inside Hurricane Alma

    Science.gov (United States)

    2002-01-01

    Hurricane season in the eastern Pacific started off with a whimper late last month as Alma, a Category 2 hurricane, slowly made its way up the coast of Baja California, packing sustained winds of 110 miles per hour and gusts of 135 miles per hour. The above image of the hurricane was acquired on May 29, 2002, and displays the rainfall rates occurring within the storm. Click the image above to see an animated data visualization (3.8 MB) of the interior of Hurricane Alma. The images of the clouds seen at the beginning of the movie were retrieved from the National Oceanic and Atmospheric Association's (NOAA's) Geostationary Orbiting Environmental Satellite (GOES) network. As the movie continues, the clouds are peeled away to reveal an image of rainfall levels in the hurricane. The rainfall data were obtained by the Precipitation Radar aboard NASA's Tropical Rainfall Measuring Mission (TRMM) satellite. The Precipitation Radar bounces radio waves off of clouds to retrieve a reading of the number of large, rain-sized droplets within the clouds. Using these data, scientists can tell how much precipitation is occurring within and beneath a hurricane. In the movie, yellow denotes areas where 0.5 inches of rain is falling per hour, green denotes 1 inch per hour, and red denotes over 2 inches per hour. (Please note that high resolution still images of Hurricane Alma are available in the NASA Visible Earth in TIFF format.) Image and animation courtesy Lori Perkins, NASA Goddard Space Flight Center Scientific Visualization Studio

  12. Magnetic switching, final chapter, Book I: the ATA upgrade prototype

    Energy Technology Data Exchange (ETDEWEB)

    Birx, D.; Cook, E.; Hawkins, S.; Poor, S.; Reginato, L.; Schmidt, J.; Smith, M.W.

    1983-03-22

    Efforts directed at finding a 10 kHz switch to replace the current 1 kHz gas blown spark gap have culminated in a prototype for an upgrade of ATA. The design and performance of this prototype as well as possible options and recommendations concerning an eventual upgrade are described. 4 references, 9 figures.

  13. EC declaration of conformity.

    Science.gov (United States)

    Donawa, M E

    1996-05-01

    The CE-marking procedure requires that manufacturers draw up a written declaration of conformity before placing their products on the market. However, some companies do not realize that this is a requirement for all devices. Also, there is no detailed information concerning the contents and format of the EC declaration of conformity in the medical device Directives or in EC guidance documentation. This article will discuss some important aspects of the EC declaration of conformity and some of the guidance that is available on its contents and format.

  14. 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

  15. 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

  16. Aspek Hukum Pengalihan Hak Atas Saham Pada Perseroan Tertutup.

    OpenAIRE

    Siregar, Ragil Muhammad

    2015-01-01

    Pengalihan hak atas saham merupakan bagian dari pengalihan tentang hak kebendaan. Tentang kebendaan merupakan bagian dari penjelasan tentang status saham yang memilik sifat kebendaan tidak bergerak yang menjelaskan isi tentang kepemilikan saham beserta hak dan kewajiban nya. Saham yang merupakan bagian dari pendirian Perseroan Terbatas menjadi bagian yang disebut dengan Modal utama dari pendirian perseroan terbatas tersebut. Penelitian dalam penulisan skripsi ini diarahkan kepada penelit...

  17. Probing Cometary Chemistry with ALMA

    Science.gov (United States)

    Milam, Stefanie N.

    2010-01-01

    Comets are considered to bear the record of the primitive Solar nebula as remnants of planetesimals that formed the outer planets. To date there are just over two dozen known cometary species compared to the >150 known interstellar molecules. This is likely due to the challenges posed when attempting to measure the composition of these small bodies. With the significant improvement in sensitivity, ALMA will likely enable the detection of new molecules to help us gain better understanding of the chemical complexity found in comets. This advancement in sensitivity will also assist in the measurement of isotope ratios in various species. These values are imperative for determining the conditions during cometary formation as well as provide insight into ongoing speculations of parent species, the possible delivery of H2O to Earth, and a direct comparison to protostellar disk chemistry. The high angular resolution obtained with ALMA will be capable of resolving any compact distributions or density enhancements in the more extended distribution that may lead to a better understanding of the formation of these species in the outer coma. By studying comet compositions we gain insight into the composition of the early Solar System as well as their astrobiological implications.

  18. Declaration and Announcement

    Institute of Scientific and Technical Information of China (English)

    2000-01-01

    Declaration To meet the needs of the national information development and widen the academic exchange channel of the authors, we declare that the journal, PEDOSPHERF,, has joined the databases of Chinese Academic Journal (CD), China Journal Net, and Chinainfo Digital Periodicals. If an author does not agree to include his article in the databases,please make a declaration at the time of contribution. Announcement Since the year 2001, the domestic distributor of PEDOSPHERE will change to the Beijing Bureau for Distribution of Newspapers and Journals, China. The domestic post office distribution No. of PEDOSPHERE is 2-576. For domestic subscribers to PEDOSPHERE,please send your orders to the local post offices in China.

  19. 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.

  20. Retreat from Alma Ata? The WHO's report on Task Shifting to community health workers for AIDS care in poor countries.

    Science.gov (United States)

    Campbell, C; Scott, K

    2011-01-01

    This paper examines the potential of community health worker (CHW) programmes, as proposed by the 2008 World Health Organisation (WHO) document Task Shifting to tackle health worker shortages, to contribute to HIV/AIDS prevention and treatment and various Millennium Development Goals in low-income countries. It examines the WHO proposal through a literature review of factors that have facilitated the success of previous CHW experiences. The WHO has taken account of five key lessons learnt from past CHW programmes (the need for strong management, appropriate selection, suitable training, adequate retention structures and good relationships with other healthcare workers). It has, however, neglected to emphasise the importance of a sixth lesson, the 'community embeddedness' of CHWs, found to be of critical importance to the success of past CHW programmes. We have no doubt that the WHO plans will increase the number of workers able to perform medically oriented tasks. However, we argue that without community embeddedness, CHWs will be unable to successfully perform the socially oriented tasks assigned to them by the WHO, such as health education and counselling. We locate the WHO's neglect of community embeddedness within the context of a broader global public health trend away from community-focused primary healthcare towards biomedically focused selective healthcare.

  1. [What a primary health care is: some considerations after almost thirty five years of Alma-Ata].

    Science.gov (United States)

    Tejada de Rivero, David A

    2013-04-01

    Primary health care was conceived in the 70s as a comprehensive, joint and inclusive strategy to achieve the goal of "Health for Everyone". It was the result of important social, political and economic changes which occurred at global level back in those years and which persist until now. Due to an unfortunate combination of words, Primary Healthcare has been mistakenly understood by many as "healthcare at the basic level" or the "provision of basic, and hence insufficient services to the poorest", wrong concepts that contribute to the current social and health inequalities. This article explains what primary healthcare is and what it is not in order to address the subject in its real context.

  2. First two ALMA antennas successfully linked

    Science.gov (United States)

    2009-05-01

    Scientists and engineers working on the world's largest ground-based astronomical project, the Atacama Large Millimeter/submillimeter Array (ALMA), have achieved another milestone -- the successful linking of two ALMA astronomical antennas, synchronised with a precision of one millionth of a millionth of a second -- to observe the planet Mars. ALMA is under construction by an international partnership in the Chilean Andes. ESO PR Photo 18a/09 The two ALMA antennas On 30 April, the team observed the first "interferometric fringes" of an astronomical source by linking two 12-metre diameter ALMA antennas, together with the other critical parts of the system. Mars was chosen as a suitable target for the observations, which demonstrate ALMA's full hardware functionality and connectivity. This important milestone was achieved at the ALMA Operations Support Facility, high in Chile's Atacama region, at an altitude of 2900 metres. "We're very proud and excited to have made this crucial observation, as it proves that the various hardware components work smoothly together. This brings us another step closer to full operations for ALMA as an astronomical observatory," says Wolfgang Wild, the European ALMA Project Manager. The two antennas used in this test will be part of ALMA's array of 66 giant 12-metre and 7-metre diameter antennas that will observe in unison as a single giant telescope, under construction on the Chajnantor plateau above the Operations Support Facility, at an altitude of 5000 metres. ALMA will operate as an interferometer, capturing millimetre and submillimetre wavelength signals from the sky with multiple antennas, and combining them to create extremely high resolution images, similar to those that would be obtained by a single, giant antenna with a diameter equal to the distance between the antennas used. "This can only be achieved with the perfect synchronisation of the antennas and the electronic equipment: a precision much better than one millionth of

  3. ALMA quality assurance: concepts, procedures, and tools

    Science.gov (United States)

    Chavan, A. M.; Tanne, S. L.; Akiyama, E.; Kurowski, R.; Randall, S.; Vila Vilaro, B.; Villard, E.

    2016-07-01

    Data produced by ALMA for the community undergoes a rigorous quality assurance (QA) process, from the initial observation ("QA0") to the final science-ready data products ("QA2"), to the QA feedback given by the Principal Investigators (PIs) when they receive the data products ("QA3"). Calibration data is analyzed to measure the performance of the observatory and predict the trend of its evolution ("QA1"). The procedure develops over different steps and involves several actors across all ALMA locations; it is made possible by the support given by dedicated software tools and a complex database of science data, meta-data and operational parameters. The life-cycle of each involved entity is well-defined, and it prevents for instance that "bad" data (that is, data not meeting the minimum quality standards) is ever processed by the ALMA pipeline. This paper describes ALMA's quality assurance concepts and procedures, including the main enabling software components.

  4. 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.

  5. Two years of ALMA bibliography: lessons learned

    Science.gov (United States)

    Meankins, Silvia; Grothkopf, Uta; Bishop, Marsha J.; Stoehr, Felix; Tatematsu, Ken

    2014-08-01

    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. 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.

  7. The essential guide to Serial ATA and SATA express

    CERN Document Server

    Deming, David A

    2014-01-01

    Used in laptop and desktop computers, low-end servers, and mobile devices, Serial ATA (Advance Technology Attachment), or SATA, is the pervasive disk storage technology in use today. SATA has also penetrated the enterprise computing environment by adding hardware components for fail-over, extending command processing capabilities, and increasing device performance and link speeds. If you work in a data center or manage your company's storage resources, you will likely encounter storage solutions that require SATA software or hardware.In this book, leading storage networking technologist David

  8. Darwin and the Declaration.

    Science.gov (United States)

    Seagrave, S Adam

    2011-01-01

    Does the prima facie contradiction between the Declaration of Independence's description of the separate and unique "creation" of human beings and Darwin's evolutionary account indicate a broader contradiction between theories of human rights and Darwinian evolution? While similar troubling questions have been raised and answered in the affirmative since Darwin's time, this article renews, updates and significantly fortifies such answers with original arguments. If a "distilled" formulation of the Declaration's central claims, shorn of complicating entanglements with both theology and comprehensive philosophical doctrines, may still be in contradiction with Darwinian evolutionary theory, this should be cause for substantial concern on the part of all normative political theorists, from Straussians to Rawlsians. Despite the notable recent efforts of a few political theorists, evolutionary ethicists and sociobiologists to establish the compatibility of Darwinian evolutionary theory with moral norms such as the idea of natural or human rights, I argue that significant obstacles remain.

  9. Declarative Programming in Java

    Directory of Open Access Journals (Sweden)

    Razvan DINA

    2014-03-01

    Full Text Available Despite the code is rarely self-explanatory, the imperative programming languages are the most commonly used in our days by the programmers all over the world and Java is definitely the lead language in popularity. This paper tries to conclude if there are any chances to use the most popular programming language of the moment in a declarative manner, even if Java itself is an intrinsic imperative language.

  10. Logic and declarative language

    CERN Document Server

    Downward, M

    2004-01-01

    Logic has acquired a reputation for difficulty, perhaps because many of the approaches adopted have been more suitable for mathematicians than computer scientists. This book shows that the subject is not inherently difficult and that the connections between logic and declarative language are straightforward. Many exercises have been included in the hope that these will lead to a much greater confidence in manual proofs, therefore leading to a greater confidence in automated proofs.

  11. 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...

  12. 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.

  13. FEMA Historical Disaster Declarations - shp

    Data.gov (United States)

    Department of Homeland Security — The Historical Disaster Declarations provides geospatial view to the Robert T. Stafford Disaster Relief and Emergency Assistance Act (referred to as the Stafford...

  14. FEMA Disaster Declaration Summary -shp

    Data.gov (United States)

    Department of Homeland Security — This dataset lists all official FEMA Disaster Declarations. This is raw, unedited data from FEMA's National Emergency Management Information System (NEMIS) and as...

  15. FEMA Disaster Declaration Summary - API

    Data.gov (United States)

    Department of Homeland Security — This dataset lists all official FEMA Disaster Declarations. This is raw, unedited data from FEMA's National Emergency Management Information System (NEMIS) and as...

  16. ALMA Polarization Science Verification: 3C 286

    Science.gov (United States)

    Nagai, H.; Nakanishi, K.; Paladino, R.; Moellenbrock, G.; Fomalont, E.; Amigano, A.; Vlahakis, C.; Remijan, A.; ALMA Polarization Team

    2015-12-01

    The ALMA polarization science verification results on 3C 286 are presented. The measured polarization percentage and polarization position angle of the continuum emission at 1.3 mm are about 16% and 39 degrees, respectively. They are quite similar to those at longer wavelength, but seem to increase slightly. Similar trends were also found in the previous measurement using the IRAM 30-m telescope (Agudo et al. 2012). The final image rms on the polarization image is better than 0.1% of the total intensity, demonstrating the very high polarization sensitivity of ALMA.

  17. 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

  18. Serendipitous ALMA detections of faint submm galaxies in SERVS

    Science.gov (United States)

    Patil, Pallavi; Lacy, Mark; Nyland, Kristina

    2017-01-01

    We present a preliminary ALMA study of faint (ALMA observations. The high sensitivity, spatial resolution, and positional accuracy of ALMA have enabled us to probe the nature of the sub-mJy population by resolving their spatial extents and improving constraints on their SEDS and photometric redshifts. We are building a catalog of sources by searching the ALMA archive for moderate to deep observations in the area covered by SERVS. This study will help us begin to understand the contribution of obscured star formation to the total star formation rate at high redshift and guide future wide-area surveys of submm galaxies with ALMA.

  19. 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.

  20. Advanced techniques in actinide spectroscopy (ATAS 2014). Abstract book

    Energy Technology Data Exchange (ETDEWEB)

    Foerstendorf, Harald; Mueller, Katharina; Steudtner, Robin (eds.)

    2014-07-01

    In 2012, The Institute of Resource Ecology at the Helmholtz-Zentrum Dresden Rossendorf organized the first international workshop of Advanced Techniques in Actinide Spectroscopy (ATAS). A very positive feedback and the wish for a continuation of the workshop were communicated from several participants to the scientific committee during the workshop and beyond. Today, the ATAS workshop has been obviously established as an international forum for the exchange of progress and new experiences on advanced spectroscopic techniques for international actinide and lanthanide research. In comparison to already established workshops and conferences on the field of radioecology, one main focus of ATAS is to generate synergistic effects and to improve the scientific discussion between spectroscopic experimentalists and theoreticians. The exchange of ideas in particular between experimental and theoretical applications in spectroscopy and the presentation of new analytical techniques are of special interest for many research institutions working on the improvement of transport models of toxic elements in the environment and the food chain as well as on reprocessing technologies of nuclear and non-nuclear waste. Spectroscopic studies in combination with theoretical modelling comprise the exploration of molecular mechanisms of complexation processes in aqueous or organic phases and of sorption reactions of the contaminants on mineral surfaces to obtain better process understanding on a molecular level. As a consequence, predictions of contaminant's migration behaviour will become more reliable and precise. This can improve the monitoring and removal of hazardous elements from the environment and hence, will assist strategies for remediation technologies and risk assessment. Particular emphasis is placed on the results of the first inter-laboratory Round-Robin test on actinide spectroscopy (RRT). The main goal of RRT is the comprehensive molecular analysis of the actinide

  1. Night Sky Quality Measurements at the ATA50 Telescope

    Science.gov (United States)

    Er, Hüseyin; Nasiroglu, Ilham; Guney, Yavuz

    2016-07-01

    One of the most important factor affecting the quality of the sky in astronomy is the light pollution (luminance of the night sky). Light pollution, also affects humans and wildlife in many ways. This effect occurs by using the light source of outdoor lighting in the wrong way. Light pollution can be reduced by lighting only what is actually needed, when and where it is needed. In generally, SQM (Sky Quality Meter- Clear Sky Detector) is used to measure this light effect. In this work we present night sky brightness measurements performed at the Atatürk University Astrophysics Research Telescope (ATA50) and the surrounding area, Erzurum, TURKEY. We also discussed the physical impacts of light pollution on science, humans and wildlife.

  2. Advanced Test Accelerator (ATA) pulse power technology development

    Energy Technology Data Exchange (ETDEWEB)

    Reginato, L.L.; Branum, D.; Cook, E.

    1981-03-09

    The Advanced Test Accelerator (ATA) is a pulsed linear induction accelerator with the following design parameters: 50 MeV, 10 kA, 70 ns, and 1 kHz in a ten-pulse burst. Acceleration is accomplished by means of 190 ferrite-loaded cells, each capable of maintaining a 250 kV voltage pulse for 70 ns across a 1-inch gap. The unique characteristic of this machine is its 1 kHz burst mode capability at very high currents. This paper dscribes the pulse power development program which used the Experimental Test Accelerator (ETA) technology as a starting base. Considerable changes have been made both electrically and mechanically in the pulse power components with special consideration being given to the design to achieve higher reliability. A prototype module which incorporates all the pulse power components has been built and tested for millions of shots. Prototype components and test results are described.

  3. 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

  4. 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

  5. ALMA - the Atacama Large Millimeter Array

    NARCIS (Netherlands)

    Wild, W.; Cunningham, C.

    2002-01-01

    The Atacama Large Millimeter Array (ALMA) is a major ground based project for millimeter and submillimeter astronomy to be realized during this decade. It comprises an array of 64 telescopes of 12 meter diameter, each equipped with 10 receivers bands covering the atmospheric windows from 30 GHz to 9

  6. 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…

  7. The Brussels Declaration

    DEFF Research Database (Denmark)

    Holgate, S; Bisgaard, H; Bjermer, L

    2008-01-01

    Asthma is a highly prevalent condition across Europe and numerous guidelines have been developed to optimise management. However, asthma can be neither cured nor prevented, treatment choices are limited and many patients have poorly controlled or uncontrolled asthma. The Brussels Declaration...... and action on the following points: the systemic inflammatory component of asthma should be better understood and considered in assessments of treatment efficacy; current research must be communicated and responded to quickly; the European Medicines Agency guidance note on asthma should be updated; "real...... world" studies should be funded and results used to inform guidelines; variations in care across Europe should be addressed; people with asthma should participate in their own care; the impact of environmental factors should be understood; and targets should be set for improvement. The present paper...

  8. 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.

  9. "Tell Me, Nana": The Image of the Grandmother in the Works of Ama Ata Aidoo.

    Science.gov (United States)

    Hill-Lubin, Mildred A.

    1988-01-01

    Analyzes the role of the grandmother in the African extended family as portrayed in the work of Ghanian author and playwright, Ama Ata Aidoo. Discusses her functions as foster parent, babysitter, psychologist, teacher, and confidante. (FMW)

  10. Concurrency & Asynchrony in Declarative Workflows

    DEFF Research Database (Denmark)

    Debois, Søren; Hildebrandt, Thomas; Slaats, Tijs

    2015-01-01

    Declarative or constraint-based business process and workflow notations have received increasing interest in the last decade as possible means of addressing the challenge of supporting at the same time flexibility in execution, adaptability and compliance. However, the definition of concurrent...... of concurrency in DCR Graphs admits asynchronous execution of declarative workflows both conceptually and by reporting on a prototype implementation of a distributed declarative workflow engine. Both the theoretical development and the implementation is supported by an extended example; moreover, the theoretical...

  11. Wake potentials and impedances for the ATA (Advanced Test Accelerator) induction cell

    Energy Technology Data Exchange (ETDEWEB)

    Craig, G.D.

    1990-09-04

    The AMOS Wakefield Code is used to calculate the impedances of the induction cell used in the Advanced Test Accelerator (ATA) at Livermore. We present the wakefields and impedances for multipoles m = 0, 1 and 2. The ATA cell is calculated to have a maximum transverse impedance of approximately 1000 {Omega}/m at 875 MHz with a quality factor Q = 5. The sensitivity of the impedance spectra to modeling variations is discussed.

  12. FEMA Current Disaster Declarations -shp

    Data.gov (United States)

    Department of Homeland Security — This dataset lists the current Disaster Declarations in Shapefile. This data was compiled and distributed by FEMA Mapping and Analysis Center (MAC). Metadata file...

  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. 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.

  16. Alma M. Karlin – in private

    Directory of Open Access Journals (Sweden)

    Maja Šučur

    2014-06-01

    Full Text Available The article presents the Slovenian writer and traveler, Alma M. Karlin, from two perspectives—the public and the private. The author begins with a summary of the most well-known facts of Alma Karlin's life: She describes her journey around the world, her motivation for writing literary works and travel logs, she places herself into the linguistic and political milieu and uncovers her contribution to the deconstruction of the role a woman was expected to perform in the early 20th century. In this text, the author exposes the previously secret or intentionally hidden elements of Karlin's privacy, for example her relationships with love and the physical. She also brings to light Karlin's relationships with men. However, the author focuses especially on the relationship between Alma Karlin and Thea Gamelin and the related speculations about Karlin's lesbianism, offering a new insight through the concept of the romantic friendship. The article raises the question whether the researching that ignores all the possible interpretations of Karlin’s life and identity has also become an act of heteronormativity.

  17. The Tbilisi Declaration.

    Science.gov (United States)

    1991-05-01

    The Tbilisi Declaration of 13 October 1990 approved by participants at an international conference supported by UNFPA, WHO/Europe, PPF/Europe, and the Zhordania Institute is printed in its entirety. The original conference document was altered inspite of IPPF Europe Regions' protestations and final approval that the conference document remain intact. In dispute was the last sentence in the "contraception reduces abortion" section, which originally left out the modifiers and stated that with appropriate backup, simple safe inexpensive ... procedures exist for use in PHC settings. ILPPF urged government agencies to change participant's views; a position expressed and agreed with in Tbilisi. The document itself is concerned with the right to reproductive health, a major public health problem, contraception reduces abortion, and the impact of legislation. The UNFPA formal position on abortion is stated as "not a means of family planning;" government support does not imply endorsement of national policy. UNFPA is concerned with increases in the availability of family planning. Participants agreed that couples and individuals have the right to decide freely, responsibly and without coercion the number and spacing of children, the right to reproductive health, self-determination, and that every child should be a wanted child. Recognition was given to unwanted pregnancy and unsafe abortion as major public health and social problems. Also, it was recognized that abortion rates are highest in countries with weak education in FP and sexuality and constraints on women. Criminal sanctions have no impact on the abortion or birth rates, but are associated with unsafe abortion. Abortion can be reduced through family planning. There is need for 1) high quality reproductive health services that respect women's autonomy and dignity; 2) early sex education; 3) lifestyle changes to place responsibility also on men for contraception, family formation, and rearing; 4) increased

  18. The Atacama Large Millimeter Array (ALMA)

    Science.gov (United States)

    1999-06-01

    The Atacama Large Millimeter Array (ALMA) is the new name [2] for a giant millimeter-wavelength telescope project. As described in the accompanying joint press release by ESO and the U.S. National Science Foundation , the present design and development phase is now a Europe-U.S. collaboration, and may soon include Japan. ALMA may become the largest ground-based astronomy project of the next decade after VLT/VLTI, and one of the major new facilities for world astronomy. ALMA will make it possible to study the origins of galaxies, stars and planets. As presently envisaged, ALMA will be comprised of up to 64 12-meter diameter antennas distributed over an area 10 km across. ESO PR Photo 24a/99 shows an artist's concept of a portion of the array in a compact configuration. ESO PR Video Clip 03/99 illustrates how all the antennas will move in unison to point to a single astronomical object and follow it as it traverses the sky. In this way the combined telescope will produce astronomical images of great sharpness and sensitivity [3]. An exceptional site For such observations to be possible the atmosphere above the telescope must be transparent at millimeter and submillimeter wavelengths. This requires a site that is high and dry, and a high plateau in the Atacama desert of Chile, probably the world's driest, is ideal - the next best thing to outer space for these observations. ESO PR Photo 24b/99 shows the location of the chosen site at Chajnantor, at 5000 meters altitude and 60 kilometers east of the village of San Pedro de Atacama, as seen from the Space Shuttle during a servicing mission of the Hubble Space Telescope. ESO PR Photo 24c/99 and ESO PR Photo 24d/99 show a satellite image of the immediate vicinity and the site marked on a map of northern Chile. ALMA will be the highest continuously operated observatory in the world. The stark nature of this extreme site is well illustrated by the panoramic view in ESO PR Photo 24e/99. High sensitivity and sharp images ALMA

  19. From the Hawaii Declaration to the Declaration of Madrid.

    Science.gov (United States)

    Helmchen, H; Okasha, A

    2000-01-01

    The Declaration of Hawaii, adopted by the World Psychiatric Association (WPA) in 1977, was a significant event. But the needs and new ethical dilemmas of the 1990s led WPA to develop new recommendations on the duties of psychiatrists resulting in the Declaration of Madrid, adopted by WPA in 1996. It outlines the framework of ethical conduct of psychiatrists, formulates seven general guidelines with an increased emphasis on research and resource allocation, and gives five specific guidelines on euthanasia, torture, the death penalty, selection of sex, and organ transplantation.

  20. 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...

  1. Tingkat Pelayanan Fasilitas Pendidikan Sekolah Menengah Tingkat Atas di Kabupaten Sidoarjo

    Directory of Open Access Journals (Sweden)

    Sisca Henlita

    2013-09-01

    Full Text Available Fasilitas pendidikan Sekolah Menengah Tingkat Atas (SMA dan SMK termasuk dalam fasilitas sosial yang merupakan salah satu kebutuhan pokok penduduk di suatu wilayah. Permasalahan penyediaan fasilitas Sekolah Menengah Tingkat Atas yang kurang memadai di Kabupaten Sidoarjo ditandai dengan ketersediaan fasilitas SMA dan SMK di masing-masing wilayah yang tidak mampu melayani kebutuhan penduduknya. Oleh karena itu, penelitian ini bertujuan untuk mengetahui sejauh mana tingkat pelayanan fasilitas Sekolah Menengah Tingkat Atas di Kabupaten Sidoarjo. Metode analisis yang digunakan yaitu analisis daya tampung dan analisis kebutuhan fasilitas dengan teknik analisis statistik deskriptif. Teknik analisis overlay pada ArcGIS digunakan untuk menganalisis tingkat ketersediaan terhadap tingkat kebutuhan fasilitas. Hasil studi menunjukan bahwa tingkat pelayanan Sekolah Menengah Tingkat Atas di sebagian wilayah masih tergolong very overdemand dan overdemand, artinya tingkat pelayanan fasilitas Sekolah Menengah Tingkat Atas di sebagian wilayah belum mampu memenuhi kebutuhan tingkat pelayanan fasilitas berdasarkan jumlah usia 16-19 tahun dan kepadatan permukiman. Hal ini dikarenakan ketersediaan fasilitas masih belum memenuhi kebutuhan penduduknya.

  2. The ALMA Snooping Project Interface (SnooPI)

    Science.gov (United States)

    Halevin, Alexandros; Hatziminaoglou, Evanthia; Chavan, A. M.

    2016-07-01

    In order to provide ALMA users with a comprehensive view of their observing projects, we developed the ALMA Snooping Project Interface (SnooPI) application. The simple and intuitive interface allows scientists to follow the status of their projects, broken down into observing unit sets and scheduling blocks. The application itself contains two separate parts: a Java back-end server and a JavaScript front-end client application. The application interacts with REST interfaces of other ALMA software components to get the necessary project reports, certain details describing the observations and to access statistics of the user's ALMA Helpdesk tickets. All this information allows to successfully trace all stages of observations, processing and delivery of the ALMA science projects.

  3. Temporomandibular disorders and declarative memory.

    Science.gov (United States)

    Yang, Dongmei; Ye, Ling

    2011-05-01

    Temporomandibular disorder (TMD) is a somatic manifestation of stress. Previous researches suggested hypothalamic-pituitary-adrenal (HPA) axis hyperactivity in TMD, through which TMD patients exhibited abnormalities of the stress response hormone - causing additional cortisol release. Increased cortisol, the principal circulating glucocorticoid in humans, would impair memory retrieval of declarative material. This effect on memory retrieval may in particular be due to glucocorticoid receptors (GR) in the hippocampus. The hypothesis we proposed is that TMD might result in declarative memory impairment by increasing the cortisol.

  4. La tragedia Ataúlfo de Montiano y el concordato de 1753

    Directory of Open Access Journals (Sweden)

    Berbel Rodríguez, José Juan

    2001-06-01

    Full Text Available Agustín de Montiano y Luyando didn't write Virginia (1750 and Ataúlfo (1753, the first Spanish neoclassical tragedies, how «playing theatre», but «reading theatre». Both tragedies were read in selected intellectual and artistic circles, because atmosphere of Spanish theatre didn't accept the neoclassical tragic method that Montiano proposed. Ataúlfo isn't an antiabsolutist tragedy wrote against the establishment of the Spanish monarchy. Ataúlfo explains disillusionment and disappointment of Montiano about political intrigues of Marqués de la Ensenada and Rávago, when Fernando VI Government signed the concordat with the Pope Benedicto XIV in 1753.Agustín de Montiano y Luyando no compuso Virginia (1750 y Ataúlfo (1753, las primeras tragedias neoclásicas españolas, como «teatro representable», sino como «teatro leído». Ambas tragedias fueron leídas en selectos y minoritarios círculos intelectuales y artísticos, porque el ambiente teatral español no hubiera aceptado el método trágico neoclásico que Montiano proponía. Ataúlfo no es una tragedia antiabsolutista escrita contra el orden establecido en la monarquía española. Ataúlfo expresa la desilusión y el desengaño de Montiano hacia las intrigas políticas del marqués de la Ensenada y de Rávago, cuando el gobierno de Fernando VI firmó el concordato con el papa Benedicto XIV en 1753.

  5. Concurrency & Asynchrony in Declarative Workflows

    DEFF Research Database (Denmark)

    Debois, Søren; Hildebrandt, Thomas; Slaats, Tijs

    2015-01-01

    Declarative or constraint-based business process and workflow notations have received increasing interest in the last decade as possible means of addressing the challenge of supporting at the same time flexibility in execution, adaptability and compliance. However, the definition of concurrent se...... development has been verified correct in the Isabelle-HOL interactive theorem prover....

  6. Thyroid nodule sizes influence the diagnostic performance of TIRADS and ultrasound patterns of 2015 ATA guidelines: a multicenter retrospective study

    Science.gov (United States)

    Xu, Ting; Gu, Jing-yu; Ye, Xin-hua; Xu, Shu-hang; Wu, Yang; Shao, Xin-yu; Liu, De-zhen; Lu, Wei-ping; Hua, Fei; Shi, Bi-min; Liang, Jun; Xu, Lan; Tang, Wei; Liu, Chao; Wu, Xiao-hong

    2017-01-01

    To evaluate the impact of thyroid nodule sizes on the diagnostic performance of thyroid imaging reporting and data system (TIRADS) and ultrasound patterns of 2015 American Thyroid Association (ATA) guidelines. Total 734 patients with 962 thyroid nodules were recruited in this retrospective study. All nodules were divided into three groups according to the maximal diameter (d  20 mm). The ultrasound images were categorized based on TIRADS and ATA ultrasound patterns, respectively. A total of 931 (96.8%) and 906 (94.2%) patterns met the criteria for TIRADS and ATA ultrasound patterns. The AUC (0.849) and sensitivity (85.3%) of TIRADS were highest in d = 10–20 mm group. However, ATA had highest AUC (0.839) and specificity (89.8%) in d > 20 mm group. ATA ultrasound patterns had higher specificity (P = 0.04), while TI-RADS had higher sensitivity (P = 0.02). In nodules d > 20 mm, the specificity of ATA patterns was higher than TIRADS (P = 0.003). Our results indicated that nodule sizes may influence the diagnostic performance of TIRADS and ATA ultrasound patterns. The ATA patterns may yield higher specificity than TIRADS, especially in nodules larger than 20 mm. PMID:28233806

  7. 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, ...

  8. 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).

  9. Kırgız Atasözlerinin Cümle Yapısı Üzerinde Bazı Gözlemler Some Observations On The Sentence Structures of The Kirghiz Proverbs

    Directory of Open Access Journals (Sweden)

    Mevlüt GÜLTEKİN

    2013-03-01

    Full Text Available Kirghiz Turks have a rich treasure of folklore. Their proverbs, the numbers of which are given in some litery works over ten thousands, build an essential part of this treasure. We explore 97 Kirghiz proverbs,most of them chosen from Bir Miñ Kırgız Eliniñ Makal-Lakaptarı (BM,published in Kirghizstan and Kırgız Atasözleri (KA, published inTurkey, regarding their sentence structure in our article. Kirghizproverbs are classified according to their sentence structure: 1. simple,2. complex: a. coordinated, b. proverbs presenting a subordinatedsentence structure having infinitive verb forms such as infinitives,participials or gerundial forms, c. conditional, d. proverbs presentingcomplex sentence structures with a direct quote and 3. proverbs havinga mixed sentence structure. Simple sentences (1-10 are classifiedaccording to their meaning as: declarative sentences and imperativesentences. Coordinated sentences (11-25 are also studied according totheir word order as sentences presenting regular turkic word order withpredicates placed at the end of the sentence in question and sentenceswith diversed word order. Conditional clauses (26-44 are examinedaccording to their functions as adverbials, subject clauses, concessiveclauses etc. Direct quote (45-55 embedded in main sentences arestudied regarding their functions as object clauses or relative clausesbuilded by degen. We study subordinated clauses formed by infinitiveverb forms such as infinitives, participials or gerundials (56-78 and tryto determine their functions in the main sentences they take part in.Sentences comprising two or more independent clauses, at least one ofwhich has one conditional clause or a clause builded by infinitive verbforms mentioned above are definited as mixed sentences (79-97. Kırgız Türkleri zengin bir folklor hazinesine sahiptir. Bu hazinenin önemli bir bölümünü de bazı çalışmalarda sayısı on bini aşan atasözleri oluşturmaktadır. Biz bu

  10. 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

  11. Fewer Cancer Reoperations for Medullary Thyroid Cancer After Initial Surgery According to ATA Guidelines

    NARCIS (Netherlands)

    Verbeek, Hans H. G.; Meijer, Johannes A. A.; Zandee, Wouter T.; Kramp, Kelvin H.; Sluiter, Willem; Smit, Johannes W.; Kievit, Job; Links, Thera P.; Plukker, John Th M.

    2015-01-01

    Surgery is still the only curative treatment for medullary thyroid cancer (MTC). We evaluated clinical outcome in patients with locoregional MTC with regard to adequacy of treatment following ATA guidelines and number of sessions to first intended curative surgery in different hospitals. We reviewed

  12. Fewer cancer reoperations for medullary thyroid cancer after initial surgery according to ATA guidelines

    NARCIS (Netherlands)

    Verbeek, H.H.; Meijer, J.A.M.; Zandee, W.T.; Kramp, K.H.; Sluiter, W.J.; Smit, J.W.A.; Kievit, J.; Links, T.P.; Plukker, J.T.

    2015-01-01

    BACKGROUND: Surgery is still the only curative treatment for medullary thyroid cancer (MTC). We evaluated clinical outcome in patients with locoregional MTC with regard to adequacy of treatment following ATA guidelines and number of sessions to first intended curative surgery in different hospitals.

  13. Sistem Rekomendasi Pemilihan Sekolah Menengah Tingkat Atas Menggunakan Metode Naive Bayes

    Directory of Open Access Journals (Sweden)

    Triana Dewi Salma

    2016-12-01

    Full Text Available Setiap tahun pendidikan di Indonesia semakin maju dan berkembang seiring dengan semakin bertambahnya jumlah sekolah atau lembaga pendidikan. Sementara itu berdasarkan data dari Dinas Pendidikan Kabupaten Sragen, bertambahnya jumlah sekolah yang berdiri juga diimbangi dengan jumlah siswa yang semakin meningkat pada tiap tahunnya. Sekolah-sekolah ini tidak jarang didirikan dalam jarak yang berdekatan dalam satu wilayah seperti halnya dengan sekolah menengah atas sederajat di kota Sragen. Dewasa ini, sekolah tersebut tidak hanya bersaing dalam hal akademik melalui prestasi sekolah maupun akreditasi, namun juga bersaing dalam mutu pendidikan yang baik untuk menarik minat calon siswa. Namun, permasalahan yang sering dihadapi yaitu banyak faktor-faktor yang akhirnya melatarbelakangi siswa untuk memilih sebuah calon sekolah baik faktor eksternal sekolah maupun internal. Sehingga siswa dituntut cerdas dalam menentukancalon sekolah terbaik dan sesuai dengan kriterianya. Penelitian ini dilakukan dalam rangka membantu siswa  untuk memilih calon sekolah menengah tingkat atas terbaik sesuai dengan kriteria-kriteria yang diinginkan. Penerapan metode Naïve Bayes digunakan dalam penelitian ini untuk merekomendasikan calon sekolah terbaik bagi siswa dengan memanfaatkan data sekolah menengah atas di Kota Sragen. Metode Naïve Bayes diterapkan untuk mencari probabilitas terbesar dari semua instance pada atribut target seperti jarak, biaya SPP, akreditasi, tingkat kelulusan dan nilai rata-rata minimal UAN. Hasil dari penelitian ini yaitu sebuah sistem rekomendasi yang dapat membantu menyajikan informasi sekolah-sekolah menengah atas yang sesuai dengan kriteria. Sehingga dapat menjadi pertimbangan bagi siswa untuk memilih calon sekolah menengah atas yang terbaik sesuai dengan kriteria yang diajukan.

  14. 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...

  15. Declaration of income for 2005

    CERN Multimedia

    HR Department

    2006-01-01

    Information from the Legal Service and the HR Department Information for members of the personnel residing in France Following the introduction of the internal taxation of salaries and emoluments of members of the CERN personnel on 1st January 2005 (cf. Bulletin No. 48-49/2005), the French Finance Ministry has communicated the following information on the procedure for completing the 2005 declaration of income form, which must be returned by 31 May 2006 at the latest. All members of the personnel*) residing in France, whether or not they are of French nationality, are required to complete a declaration of income for 2005 according to the following instructions and to return a signed copy to their local tax office by 31 May 2006 at the latest. Members of the personnel should receive an income declaration form for 2005 at the beginning of May. Those who do not receive a form directly should obtain one from their local 'Centre des Impôts', Trésorerie' or 'Mairie', or download one from the Finance Ministry...

  16. Probing Sagittarius A* accretion with ALMA

    Science.gov (United States)

    Murchikova, Elena

    2017-01-01

    The submm Hydrogen recombination line technique can be used as a probe of the Galactic Center. We present the results of our H30α observations of ionized gas from within 0.015 pc around SgrA*. The observations were obtained on ALMA in cycle 3. The line was not detected, but we were able to set a limit on the mass of the cool gas (T~ 104 K) at 2 × 10-3 M ⊙. This is the unique probe of gas cooler than T ~106 K traced by X-ray emission. The total amount of gas near SgrA* gives us clues to understanding the accretion rate of SgrA*.

  17. Astrochemical Modeling In the ALMA Era

    Science.gov (United States)

    Charnley, Steven

    2009-01-01

    Interstellar chemistry provides a natural laboratory for studying exotic species and processes at densities, temperatures, and reaction rates, that are difficult or impractical to address in the laboratory. Thus, many chemical reactions considered too slow by the standards of terrestrial chemistry, can be observed' and modeled. Various proposals concerning the nature and chemistry of complex interstellar organic molecules will be described. Catalytic reactions on grain surfaces can, in principle, lead to a large variety of species and this has motivated many laboratory and theoretical studies. Gas phase processes may also build large species in molecular clouds. Future laboratory data and computational tools needed to construct accurate chemical models of various sources to be observed by ALMA will be outlined.

  18. Artificial calibration source for ALMA radio interferometer

    Science.gov (United States)

    Kiuchi, Hitoshi; Hills, Richard; Whyborn, Nicholas D.; Asayama, Shinichiro; Sakamoto, Seiichi; Iguchi, Satoru; Corder, Stuartt A.

    2016-07-01

    The ALMA (Atacama Large Millimeter/submillimeter Array) radio interferometer has some different types of antennas which have a variation of gain and leakages across the primary beam of an individual antenna. We have been developing an artificial calibration source which is used for compensation of individual difference of antennas. In a high-frequency antenna, using astronomical sources to do calibration measurement would be extremely time consuming, whereas with the artificial calibration source becomes a realistic possibility. Photonic techniques are considered to be superior to conventional techniques based on electronic devices in terms of wide bandwidth and high-frequency signals. Conversion from an optical signal to a millimeter/sub-millimeter wave signal is done by a photo-mixer.

  19. ALMA and RATIR observations of GRB 131030A

    Science.gov (United States)

    Huang, Kuiyun; Urata, Yuji; Takahashi, Satoko; Im, Myungshin; Yu, Po-Chieh; Choi, Changsu; Butler, Nathaniel; Watson, Alan M.; Kutyrev, Alexander; Lee, William H.; Klein, Chris; Fox, Ori D.; Littlejohns, Owen; Cucchiara, Nino; Troja, Eleonora; González, Jesús; Richer, Michael G.; Román-Zúñiga, Carlos; Bloom, Josh; Prochaska, J. Xavier; Gehrels, Neil; Moseley, Harvey; Georgiev, Leonid; de Diego, José A.; Ramirez-Ruiz, Enrico

    2017-01-01

    We report on the first open-use based Atacama Large Millimeter/submm Array (ALMA) 345 GHz observation for the late afterglow phase of GRB 131030A. The ALMA observation constrained a deep limit at 17.1 d for the afterglow and host galaxy. We also identified a faint submillimeter source (ALMA J2300-0522) near the GRB 131030A position. The deep limit at 345 GHz and multifrequency observations obtained using Swift and RATIR yielded forward-shock modeling with a two-dimensional relativistic hydrodynamic jet simulation and described X-ray excess in the afterglow. The excess was inconsistent with the synchrotron self-inverse Compton radiation from the forward shock. The host galaxy of GRB 131030A and optical counterpart of ALMA J2300-0522 were also identified in the Subaru image. Based on the deep ALMA limit for the host galaxy, the 3σ upper limits of IR luminosity and the star formation rate (SFR) are estimated as LIR ALMA J2300-0522 may be one component of the GRB 131030A host galaxy, according to previous host galaxy cases.

  20. Constraining the orbits of young binary systems with ALMA

    Science.gov (United States)

    Nogueira, Natasha; Jensen, Eric L. N.; Akeson, Rachel L.

    2017-01-01

    Measuring the orbits of young binary systems can provide the stars' individual stellar masses as well as insight into the dynamical effects they should have on each others' protoplanetary disks. As a byproduct of our ALMA observations of disks in young binary systems, we are able to measure precise relative separations of binaries with separations of 0.22--0.35 arcsec (~ 30--50 AU at the distance of the Taurus star-forming region). Most of these systems were first resolved in the early 1990s, so our epoch 2015 observations add an additional point in the orbit that is 20--25 years after the discovery epoch. While this coverage does not yet yield a definitive orbit, the extended coverage allows improved constraints on the binary orbital parameters. We present updated orbital constraints on a number of young binary systems, including XZ Tau, GH Tau, GN Tau, IS Tau, V955 Tau, and JH 112.This work makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00150.S. and ADS/JAO.ALMA#2013.1.00105.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

  1. Alma-Ata: Rebirth and Revision 6 Interventions to address maternal, newborn, and child survival: what difference can integrated primary health care strategies make?

    Science.gov (United States)

    Bhutta, Zulfiqar A; Ali, Samana; Cousens, Simon; Ali, Talaha M; Haider, Batool Azra; Rizvi, Arjumand; Okong, Pius; Bhutta, Shereen Z; Black, Robert E

    2008-09-13

    Several recent reviews of maternal, newborn, and child health (MNCH) and mortality have emphasised that a large range of interventions are available with the potential to reduce deaths and disability. The emphasis within MNCH varies, with skilled care at facility levels recommended for saving maternal lives and scale-up of community and household care for improving newborn and child survival. Systematic review of new evidence on potentially useful interventions and delivery strategies identifies 37 key promotional, preventive, and treatment interventions and strategies for delivery in primary health care. Some are especially suitable for delivery through community support groups and health workers, whereas others can only be delivered by linking community-based strategies with functional first-level referral facilities. Case studies of MNCH indicators in Pakistan and Uganda show how primary health-care interventions can be used effectively. Inclusion of evidence-based interventions in MNCH programmes in primary health care at pragmatic coverage in these two countries could prevent 20-30% of all maternal deaths (up to 32% with capability for caesarean section at first-level facilities), 20-21% of newborn deaths, and 29-40% of all postneonatal deaths in children aged less than 5 years. Strengthening MNCH at the primary health-care level should be a priority for countries to reach their Millennium Development Goal targets for reducing maternal and child mortality.

  2. Lo que es la atención primaria de la salud: algunas consideraciones a casi treinta y cinco años de Alma-Ata

    Directory of Open Access Journals (Sweden)

    David A Tejada de Rivero

    Full Text Available La atención primaria de la salud fue concebida en la década de los 70 como una estrategia política para lograr la meta social de “Salud para todos”. Respondió a importantes cambios en los terrenos social, político y económico que ocurrieron a nivel global después la segunda guerra mundial, y que siguen ocurriendo hasta la actualidad. Por una desafortunada mala traducción del inglés al español y una errada interpretación de términos, la atención primaria de la salud ha sido malentendida por muchos como “atención en el nivel primario de salud” o como la “dotación de un paquete de prestaciones básicas pero insuficientes a los más pobres”, conceptos erróneos que mantienen las inaceptables inequidades sociales y de salud que hoy seguimos sufriendo. Este artículo explicita lo que es y lo que no es la atención primaria de la salud para abordar el tema desde su verdadero contexto, y hacia su verdadero norte.

  3. The International Lunar Decade Declaration

    Science.gov (United States)

    Beldavs, V.; Foing, B.; Bland, D.; Crisafulli, J.

    2015-10-01

    The International Lunar Decade Declaration was discussed at the conference held November 9-13, 2014 in Hawaii "The Next Giant Leap: Leveraging Lunar Assets for Sustainable Pathways to Space" - http://2014giantleap.aerospacehawaii.info/ and accepted by a core group that forms the International Lunar Decade Working Group (ILDWG) that is seeking to make the proposed global event and decade long process a reality. The Declaration will be updated from time to time by members of the ILDWreflecting new knowledge and fresh perspectives that bear on building a global consortium with a mission to progress from lunar exploration to the transformation of the Moon into a wealth gene rating platform for the expansion of humankind into the solar system. When key organizations have endorsed the idea and joined the effort the text of the Declaration will be considered final. An earlier International Lunar Decade proposal was issued at the 8th ICEUM Conference in 2006 in Beijing together with 13 specific initiatives for lunar exploration[1,2,3]. These initiatives have been largely implemented with coordination among the different space agencies involved provided by the International Lunar Exploration Working Group[2,3]. The Second International Lunar Decade from 2015 reflects current trends towards increasing involvement of commercial firms in space, particularly seeking opportunities beyond low Earth orbit. The central vision of the International Lunar Decade is to build the foundations for a sustainable space economy through international collaboration concurrently addressing Lunar exploration and building a shared knowledge base;Policy development that enables collabo rative research and development leading to lunar mining and industrial and commercial development;Infrastructure on the Moon and in cislunar space (communications, transport, energy systems, way-stations, other) that reduces costs, lowers risks and speeds up the time to profitable operations;Enabling technologies

  4. 40 CFR 52.122 - Negative declarations.

    Science.gov (United States)

    2010-07-01

    ... air pollution control districts submitted negative declarations for volatile organic compound source... Operations, Rubber Tire Manufacturing, Polymer Manufacturing, Industrial Wastewater, Ship Building and...

  5. The Global ALMA EPO programme: Communicating astronomy with the public at millimetre and submillimetre wavelengths

    Science.gov (United States)

    Adams, M.; Boffin, H. J.; Garnier, W.; Iono, D.

    2008-06-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) is a major 21st century international science research facility that will open new windows on celestial origins. ALMA construction is underway in the high-elevation Atacama Desert of northern Chile. Science operations will begin in 2010, and full science operations will start in 2013. The ALMA Education and Public Outreach (EPO) programme is a global collaboration that seeks to communicate the excitement and value of the ALMA mission, science, and technology to international audiences effectively. The ALMA EPO programme is the responsibility of the Joint ALMA Observatory (JAO), the National Radio Astronomy Observatory (NRAO), the European Organisation for Astronomical Research in the Southern Hemisphere (ESO), and the National Astronomical Observatory of Japan (NAOJ). This contribution provides an overview of the ALMA Project and the global ALMA EPO programme.

  6. The Dome Automations of ATA50 and MASS-DIMM Telescopes for DAG Project

    Science.gov (United States)

    Dogan, E.; Celik, H. I.; Ozbaldan, E. E.; Guney, Y.; Yesilyaprak, C.

    2016-12-01

    In the scope of Eastern Anatolia Observatory (DAG) Project, The DAG Technical Team has carried out various automation studies like dome, camera, atmospherical equipments, etc. The domes of ATA50 and MASS-DIMM Telescopes have almost similar opening systems. Both telescopes will run as robotic very soon; therefore it's mandatory and inevitable to make the automations of their domes. The automation studies as its electronics and software developed by DAG Technical Team are presented.

  7. ANALISIS PENERAPAN TAX PLANNING ATAS PAJAK PENGHASILAN BADAN PADA PT SEMEN TONASA PANGKEP

    OpenAIRE

    WIJAYA, AKBAR

    2014-01-01

    2014 ABSTRAK ANALISIS PENERAPAN TAX PLANNING ATAS PAJAK PENGHASILAN BADAN PADA PT SEMEN TONASA PANGKEP Implementation Analysis of Tax Planning on Board Incoming Tax of Semen Tonasa Ltd. Pangkep Akbar Wijaya Amiruddin Darmawati Penelitian ini bertujuan untuk mengetahui tax planning yang dilakukan oleh PT Semen Tonasa Pangkep, dan untuk menganalisis penerapan tax planning yang dilakukan oleh PT Semen Tonasa Pangkep dengan undang-undang perpajakan yang berlaku. Data...

  8. Kiat Menuju Keberhasilan Melakukan Restorasi dengan Menggunakan Pasak pada Gigi Anterior Rahang Atas

    Directory of Open Access Journals (Sweden)

    M. Yubhar

    2015-11-01

    Full Text Available Keberhasilan perawatan dengan mahkota pasak antara lain ditentukan oleh berbagai faktor. Kiat keberhasilan perawatan dengan mahkota pasa untuk gigi anterior atas perlu dipertimbangkan berbagai faktor seperti: pemilihan pasak dan preparasi yang disesuaikan dengan saluran akar, disamping mempertimbang ketebalan jaringan akar gigi; penggunaan Ferrule Design dalam melakukan preparasi atap akar serta penggunaan pasak berulir yang bersifat pasif, guna efisiensi perawatan dapat pula digunakan pasak siap pakai.

  9. Kiat Menuju Keberhasilan Melakukan Restorasi dengan Menggunakan Pasak pada Gigi Anterior Rahang Atas

    Directory of Open Access Journals (Sweden)

    M. Yubhar

    2015-11-01

    Full Text Available Keberhasilan perawatan denan mahkota pasak antara lain ditentukan oleh berbagai faktor. Kiat keberhasilan perawatan dengan mahkota pasak untuk gigi anterior atas perlu dipertimbangkan berbagai faktor seperti: pemilihan pasak dan preparasi yang disesuaikan denan saluran akar, disamping mempertimbang ketebalan jaringan akar gigi; penggunaan Ferrule Design dalam melakukan prepalarasi atap akar serta penggunaan pasak berulir yang bersifat pasif, guna efisiensi perawatan dapat pula digunakan pasak siap pakai.

  10. The transition from construction to operations on the ALMA control software

    Science.gov (United States)

    Marson, Ralph; Hiriart, Rafael

    2016-07-01

    The Atacama Large Millimeter/Submillimeter Array (ALMA) is a set of 66 millimeter wave antenna in the Andes in Northern Chile. All antennas are connected and operate as an interferometer making ALMA the most powerful millimeter telescope in the world. In 2013 ALMA formally marked the end of construction and the beginning of operations. This paper will focus on the impact, on the ALMA control software, of this transition from construction to operations.

  11. Carbonaceous particles in Muztagh Ata ice core, West Kunlun Mountains, China

    Institute of Scientific and Technical Information of China (English)

    LIU XianQin; XU BaiQing; YAO TanDong; WANG NingLian; WU GuangJian

    2008-01-01

    Carbonaceous particles concentrations of OC and EC are determined using a two-step gas chroma-tography system in Muztagh Ata ice core covering the time period of 1955-2000. Over the period rep-resented by the core, OC and EC concentrations appear to have changed significantly, varied in the range of 17.7-216.7 and 6.5-124.6, and averaged 61.8, 32.9 ng·g-1, respectively. The average concen-tration of EC in Muztagh Ata ice core is much lower than that in an Alpine ice core record (100-300 ng·g-1) during the same period, but it is a factor of 14 in Greenland ice core (2.3 ng.g-1), this may induce a strong impact on the snow albedo in the last 46 years in our study area. Observations indicate two periods with obviously high deposition concentrations (1955-1965 and 1974-1989) and two periods with low concentrations (1966-1973 and 1990-1995), as well as a recent increasing trend. By com-paring EC and SO42- concentration variations and deciphering OC/EC ratios recorded in the same ice core, we can judge roughly that the carbonaceous particles deposited in Muztagh Ata ice core were attributed to fossil fuel combustion sources.

  12. What determines the inhibition effectiveness of ATA, BTAH, and BTAOH corrosion inhibitors on copper?

    Science.gov (United States)

    Kokalj, Anton; Peljhan, Sebastijan; Finsgar, Matjaz; Milosev, Ingrid

    2010-11-24

    Three corrosion inhibitors for copper-3-amino-1,2,4-triazole (ATA), benzotriazole (BTAH), and 1-hydroxybenzotriazole (BTAOH)-were investigated by corrosion experiments and atomistic computer simulations. The trend of corrosion inhibition effectiveness of the three inhibitors on copper in near-neutral chloride solution is determined experimentally as BTAH ≳ ATA ≫ BTAOH. A careful analysis of the results of computer simulations based on density functional theory allowed to pinpoint the superior inhibiting action of BTAH and ATA as a result of their ability to form strong N-Cu chemical bonds in deprotonated form. While these bonds are not as strong as the Cl-Cu bonds, the presence of solvent favors the adsorption of inhibitor molecules onto the surface due to stronger solvation of the Cl(-) anions. Moreover, benzotriazole displays the largest affinity among the three inhibitors to form intermolecular aggregates, such as [BTA-Cu](n) polymeric complex. This is another factor contributing to the stability of the protective inhibitor film on the surface, thus making benzotriazole an outstanding corrosion inhibitor for copper. These findings cannot be anticipated on the basis of inhibitors' molecular electronic properties alone, thus emphasizing the importance of a rigorous modeling of the interactions between the components of the corrosion system in corrosion inhibition studies.

  13. Tindakan ‘Surgical Exposure’ pada Impaksi Gigi Insisif Satu Atas (Laporan Kasus

    Directory of Open Access Journals (Sweden)

    Sarworini B Budiardjo

    2015-11-01

    Full Text Available Gigi impaksi adalah gigi yang tertahan di dalam tulang rahang, secara klinis dapat dijumpai sebagai gigi yang lambat erupsi, gigi yang tertutup kembali oleh jaringan selama proses erupsi, atau proses erupsi yang berhenti. Penyebab terjadinya impaksi sebagai akibat gangguan patologik seperti ameloblastoma, ameloblastic fibrousodontoma, atau kista dentigerous dan gangguan non patologik berupa penebalan jaringan ikat akibat pencabutan gigi terlalu awal. Impaksi gigi insisif satu tetap atas sering dihubungkan dengan terjadinya odontoma, gigi supernumerary, pasien cleiocranial dysostosis, dan traumatic injuries. Perawatan gigi impaksi sesuai dengan penyebab; bila disebabkan faktor patologik, maka pengambilan seluruh gigi menjadi pilihan perawatan. Pada gigi impaksi akibat faktor non patologik, maka dilakukan tindakan bedah dengan tujuan membuka jalan erupsi (surgical exposure. Setelah surgical exposure dapat dilakukan pemasangan mahkota dari seluloid atau alumunium shell yang disemenkan pada mahkota gigi. Pada laporan kasus ini anak wanita usia 10 tahun dengan gigi insisif satu tetap atas kiri yang mengalami impaksi di bagian palatal dan untuk membantu erupsi dilakukan tindakan bedah disertai pemasangan mahkota seluloid. Tindakan tersebut dilakukan setelah mengalami kegagalan pada pembedahan pertama dengan terjadinya pertautan jaringan lunak, sehingga gigi tetap mengalami kesulitan erupsi. Hasil perawatan kedua menunjukkan keberhasilan, setelah 10 bulan perawatan gigi insisif satu tetap atas kiri erupsi lebih dari duapertiga mahkota.

  14. PENGEMBANGAN MODEL LATIHAN KARATE KIDS PADA ANAK USIA SEKOLAH DASAR KELAS ATAS

    Directory of Open Access Journals (Sweden)

    Widha Srianto

    2014-09-01

    Full Text Available Penelitian ini bertujuan untuk menghasilkan model latihan karate kids pada anak usia sekolah dasar (SD kelas atas (10-12 tahun. Penelitian pengembangan ini dilakukan dengan mengadaptasi langkah-langkah penelitian sebagai berikut: (1 pengumpulan informasi di lapangan, (2 melakukan analisis terhadap informasi yang telah dikumpulkan, (3 mengembangkan produk awal, (4 validasi ahli dan revisi, (5 uji coba lapangan skala kecil dan revisi,  (6 uji coba lapangan skala besar dan revisi, dan (7 pembuatan produk final. Uji coba skala kecil dilakukan di klub Forki Kota Yogyakarta berjumlah 7 anak. Uji coba skala besar di klub Inkanas DIY berjumlah 16 anak. Instrumen pengumpulan data yang digunakan yaitu: (1 pedoman wawancara, (2 skala nilai, (3 pedoman observasi model, (4 pedoman observasi keefektifan model, dan (5 kuesioner untuk siswa. Teknik analisis data yang dilakukan yaitu analisis deskriptif kuantitatif dan analisis deskriptif kualitatif. Hasil penelitian ini berupa model latihan karate kids pada anak usia SD kelas atas (10-12 tahun yaitu: (1 model latihan maegeri, (2 model latihan gyaku tsuki, (3 model latihan mawashigeri, dan (4 model latihan oi tsuki. Dari hasil analisis data penilaian para ahli materi dan kuesioner anak, dapat ditarik kesimpulan bahwa model latihan karate kids pada anak usia SD kelas atas (10-12 tahun ini dinilai baik dan efektif. Kata kunci: model latihan, karate kids

  15. 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.

  16. $\\eta$ 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...

  17. 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.

  18. 19 CFR 10.764 - Declaration.

    Science.gov (United States)

    2010-04-01

    ... English language. (d) Applicability of declaration. The declaration may be applicable to: (1) A single... ARTICLES CONDITIONALLY FREE, SUBJECT TO A REDUCED RATE, ETC. United States-Morocco Free Trade Agreement..., and a statement as to the origin and value of, any materials used in the article that are claimed...

  19. 19 CFR 10.804 - Declaration.

    Science.gov (United States)

    2010-04-01

    ... English language. (d) Applicability of declaration. The declaration may be applicable to: (1) A single... ARTICLES CONDITIONALLY FREE, SUBJECT TO A REDUCED RATE, ETC. United States-Bahrain Free Trade Agreement..., and a statement as to the origin and value of, any materials used in the article that are claimed...

  20. 77 FR 15179 - Disaster Declaration for Washington

    Science.gov (United States)

    2012-03-14

    ... Counties: Clallam, Grays Harbor, King, Klickitat, Lewis, Mason, Pierce, Skamania, Snohomish, Thurston... ADMINISTRATION [Disaster Declaration 13027 and 13028; Washington Disaster WA-00036] Disaster Declaration for Washington AGENCY: U.S. Small Business Administration. ] ACTION: Notice. SUMMARY: This is a Notice of...

  1. The Amstersam declaration on fungal nomenclature

    DEFF Research Database (Denmark)

    Hawksworth, David L.; Crous, Pedro W.; Redhead, Scott A.;

    2011-01-01

    to promote the implementation of the Declaration. In addition, but not forming part of the Declaration, are reports of discussions held during the symposium on the governance of the nomenclature of fungi, and the naming of fungi known only from an environmental nucleic acid sequence in particular. Possible...

  2. 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.

  3. A Deep ALMA Image of the Hubble Ultra Deep Field

    Science.gov (United States)

    Dunlop, J. S.

    2016-12-01

    Although primarily designed as a high-resolution imaging spectrometer at submillimetre/millimetre wavelengths, the Atacama Large Millimeter/submillimeter Array (ALMA) has a vital role to play in producing the key deep, unconfused, submillimetre/millimetre continuum surveys required to bridge the current gap in our understanding of visible and dust-obscured star formation in the young Universe. The first such survey has now been completed, comprising a mosaic of 45 ALMA pointings at a wavelength of 1.3 mm, covering the Hubble Ultra Deep Field (HUDF). This deep, homogeneous ALMA survey, combined with the wealth of existing data in the HUDF, has already provided new clarity on the nature of dusty star-forming galaxies, and the relative evolution of dust-obscured and unobscured star formation over cosmic time.

  4. HST, ALMA, and revealing the throes of planet formation

    Science.gov (United States)

    Boley, Aaron C.

    2017-01-01

    In this talk, I will highlight some of the synergy between HST and ALMA. In particular, I will focus on the impact of these observatories in shaping our understanding of debris systems and planet-forming discs. Both HST and ALMA can resolve gas and dust distributions at very high resolution, but they each, e.g., probe very different dust grain sizes and gas line transitions. The observatories can thus provide complementary views of the dynamics, composition, and morphologies of discs during planet building and its aftermath. As examples, I will discuss new ALMA results for HD141569 and Fomalhaut, as well as discuss work from other groups on systems such as Beta Pic.

  5. η Carinae Baby Homunculus uncovered by ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Abraham, Zulema; Beaklini, Pedro P. B. [Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, R. do Matão 1226, Cidade Universitária, CEP 05508-900 São Paulo, SP (Brazil); Falceta-Gonçalves, Diego, E-mail: zulema.abraham@iag.usp.br [Escola de Artes, Ciências e Humanidades, Universidade de São Paulo, R. Arlindo Bettio 1000, 03828-000 São Paulo, SP (Brazil)

    2014-08-20

    We report observations of η 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 H42α, He42α, H40α, He40α, H50β, H28α, He28α, H21α, and He21α were also detected, and their intensities reveal non-local thermodynamic equilibrium 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 η 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 high-temperature gas and requires a high-energy ionizing photon flux, which must be provided by the companion star. The mass-loss rate and wind velocity, necessary to explain the formation of the shell, are compatible with an luminous blue variable eruption. The position, velocity, and physical parameters of the shell coincide with those of the Weigelt blobs. The dynamics found for the expanding shell correspond to matter ejected by η Carinae in 1941 in an event similar to that which formed the Little Homunculus; for that reason, we called the new ejecta the 'Baby Homunculus'.

  6. Por mi alma subiré a Dios. El concepto de alma de san Agustín de Hipona

    OpenAIRE

    Saeteros Pérez, Tamara

    2013-01-01

    El presente artículo pretende recoger las claves fundamentales de la doctrina sobre el alma de san Agustín de Hipona. Magna natura et magna quaestio est (Hipona De; trad. 1968; 14; 4; 6); puesto que ocupará durante toda su vida el pensamiento y las obras del santo obispo. Buscar su propia alma; adentrarse en su santuario; descubrir la imagen de Dios en ella; su bondad; su grandeza; su vida para volverla luego a Dios; su origen y meta de todos sus esfuerzos. Tal es el itinerario que nos traza...

  7. The 2014 ALMA Long Baseline Campaign : An Overview

    NARCIS (Netherlands)

    ALMA Partnership, [Unknown; Fomalont, E. B.; 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.; Radiszcz, M.; Rodón, J. A.; Sawada, T.; Takahashi, S.; Tilanus, R. P. J.; van Kempen, T.; Vila Vilaro, B.; 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.; 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.; Diaz Trigo, M.; Fontani, F.; Franco-Hernandez, R.; Fuller, G.; Galvan Madrid, R.; Giannetti, A.; Ginsburg, A.; Graves, S. F.; Hatziminaoglou, E.; Hogerheijde, M.; Jachym, P.; Jimenez Serra, I.; Karlicky, M.; Klaasen, P.; Kraus, M.; Kunneriath, D.; Lagos, C.; Longmore, S.; Leurini, S.; Maercker, M.; Magnelli, B.; Marti Vidal, I.; 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.; Sanchez Monge, A.; 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., III; Brisbin, D. G.; Brunetti, N.; Carilli, C.; Crossley, J. H.; D’Addario, L.; Donovan Meyer, J. L.; 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.; Rao Venkata, U.; Rawlings, M. G.; Rosen, R.; Schnee, S. L.; Scott, K. S.; Sharp, N. K.; Sheth, K.; 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

  8. 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.

  9. 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...

  10. The Labour Market Effects of "Alma Mater": Evidence from Italy

    Science.gov (United States)

    Brunello, Giorgio; Cappellari, Lorenzo

    2008-01-01

    We use data from a nationally representative survey of Italian graduates to study whether "Alma Mater" matters for employment and earnings 3 years after graduation. We find that the attended college matters, and that there are important college-related differences, both among and within regions of the country. These differences, however,…

  11. 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…

  12. Modeling Protostar Envelopes and Disks Seen With ALMA

    Science.gov (United States)

    Terebey, Susan; Flores-Rivera, Lizxandra; Willacy, Karen

    2017-01-01

    Thermal continuum emission from protostars comes from both the envelope and circumstellar disk. The dust emits on a variety of spatial scales, ranging from sub-arcseconds for disks to roughly 10 arcseconds for envelopes for nearby protostars. We present models of what ALMA should detect that incorporate a self-consistent collapse solution, radiative transfer, and realistic dust properties.

  13. ALMA North American Integration Center Front-End Test System

    CERN Document Server

    Ediss, Geoffrey A; Crady, Kirk; Gaines, Erik; McLeod, Morgan; Morris, Greg; Williams, Rick; Perfetto, Antonio; Webber, John; 10.1007/s10762-010-9688-y

    2010-01-01

    The Atacama Large Millimeter/submillimeter (ALMA) Array Front End (FE) system is the first element in a complex chain of signal receiving, conversion, processing and recording. 70 Front Ends will be required for the project. The Front End is designed to receive signals in ten different frequency bands. In the initial phase of operations, the antennas will be fully equipped with six bands. These are Band 3 (84-116 GHz), Band 4 (125-163 GHz), Band 6 (211-275 GHz), Band 7 (275-373 GHz), Band 8 (385-500 GHz) and Band 9 (602-720 GHz). It is planned to equip the antennas with the missing bands at a later stage of ALMA operations, with a few Band 5 (163-211 GHz) and Band 10 (787-950 GHz) receivers in use before the end of the construction project. The ALMA Front End is far superior to any existing receiver systems; spin-offs of the ALMA prototypes are leading to improved sensitivities in existing millimeter and submillimeter observatories. The Front End units are comprised of numerous elements, produced at different...

  14. TINJAUAN ATAS DESAIN SAMPUL MUKA BUKU ANAK-ANAK REVOLUSI KARYA BUDIMAN SUDJATMIKO

    Directory of Open Access Journals (Sweden)

    Danu Widhyatmoko

    2014-10-01

    Full Text Available Desain sampul muka merupakan gambaran utuh dari karya publikasi, yang bukan saja berfungsi sebagai media promosi namun juga sebagai media identifikasi. Tulisan ini berisi tinjauan atas sampul muka buku Anak-anak Revolusi karya Budiman Sudjatmiko dengan menggunakan pendekatan desain komunikasi visual. Lalu juga akan dibahas pilihan pendekatan visual lain yang dapat diterapkan. Metode penelitian yang digunakan dalam penulisan ini adalah studi literatur yang dilanjutkan dengan analisa data reflektif. Hingga pada akhir tulisan bisa didapatkan gambaran yang lebih jelas terkait obyek yang ditinjau.(DW

  15. 19 CFR 10.704 - Declaration.

    Science.gov (United States)

    2010-04-01

    ... facts. (c) Language. The declaration must be completed in the English language. (d) Applicability of... ARTICLES CONDITIONALLY FREE, SUBJECT TO A REDUCED RATE, ETC. United States-Jordan Free Trade...

  16. Stress enhances reconsolidation of declarative memory

    OpenAIRE

    Bos, M; Schuijer, J; Lodestijn, F; Beckers, Tom; Kindt, M

    2014-01-01

    Retrieval of negative emotional memories is often accompanied by the experience of stress. Upon retrieval, a memory trace can temporarily return into a labile state, where it is vulnerable to change. An unresolved question is whether post-retrieval stress may affect the strength of declarative memory in humans by modulating the reconsolidation process. Here, we tested in two experiments whether post-reactivation stress may affect the strength of declarative memory in humans. In both experimen...

  17. 47 CFR 2.1072 - Limitation on Declaration of Conformity.

    Science.gov (United States)

    2010-10-01

    ... 47 Telecommunication 1 2010-10-01 2010-10-01 false Limitation on Declaration of Conformity. 2.1072... Conformity § 2.1072 Limitation on Declaration of Conformity. (a) The Declaration of Conformity signifies that...'s rules. (b) A Declaration of Conformity by the responsible party is effective until a...

  18. 47 CFR 68.320 - Supplier's Declaration of Conformity.

    Science.gov (United States)

    2010-10-01

    ... 47 Telecommunication 3 2010-10-01 2010-10-01 false Supplier's Declaration of Conformity. 68.320... Approval § 68.320 Supplier's Declaration of Conformity. (a) Supplier's Declaration of Conformity is a... Supplier's Declaration of Conformity attaches to all items subsequently marketed by the responsible...

  19. 37 CFR 1.69 - Foreign language oaths and declarations.

    Science.gov (United States)

    2010-07-01

    ... 37 Patents, Trademarks, and Copyrights 1 2010-07-01 2010-07-01 false Foreign language oaths and... Declaration § 1.69 Foreign language oaths and declarations. (a) Whenever an individual making an oath or declaration cannot understand English, the oath or declaration must be in a language that such individual...

  20. Funcionalidad de los cuadernos ATA dentro de las perspectivas del comercio exterior en Colombia

    Directory of Open Access Journals (Sweden)

    Ana Marí­a Heredia Rodríguez

    2017-02-01

    Full Text Available El objetivo de la investigación es elaborar un manual de implementación de cuadernos ATA (Admisión Temporal para las operaciones de comercio exterior en Colombia, como mecanismo dinamizador de los regí­menes suspensivos de importación y exportación. La metodologí­a llevada a cabo fue la revisión de la normatividad internacional y la normatividad interna en Colombia; posteriormente, la aplicación de encuestas para recolectar información de fuentes primarias, llevando así­ a realizar un análisis crí­tico del tema propuesto y concluyendo posteriormente que la normatividad aduanera en Colombia debe ser acorde a los convenios internacionales, y a su vez la perspectiva de competitividad en el entorno de la globalización no se puede limitar al desarrollo logí­stico e infraestructura vial, sino que requiere implementar en su totalidad el decreto 390 de 2016 (Estatuto Aduanero y generar estrategias de facilitación de las operaciones comerciales internacionales, como los cuadernos ATA.

  1. The 'affect tagging and consolidation' (ATaC) model of depression vulnerability.

    Science.gov (United States)

    Harrington, Marcus O; Pennington, Kyla; Durrant, Simon J

    2017-02-15

    Since the 1960's polysomnographic sleep research has demonstrated that depressive episodes are associated with REM sleep alterations. Some of these alterations, such as increased REM sleep density, have also been observed in first-degree relatives of patients and remitted patients, suggesting that they may be vulnerability markers of major depressive disorder (MDD), rather than mere epiphenomena of the disorder. Neuroimaging studies have revealed that depression is also associated with heightened amygdala reactivity to negative emotional stimuli, which may also be a vulnerability marker for MDD. Several models have been developed to explain the respective roles of REM sleep alterations and negatively-biased amygdala activity in the pathology of MDD, however the possible interaction between these two potential risk-factors remains uncharted. This paper reviews the roles of the amygdala and REM sleep in the encoding and consolidation of negative emotional memories, respectively. We present our 'affect tagging and consolidation' (ATaC) model, which argues that increased REM sleep density and negatively-biased amygdala activity are two separate, genetically influenced risk-factors for depression which interact to promote the development of negative memory bias - a well-known cognitive vulnerability marker for depression. Predictions of the ATaC model may motivate research aimed at improving our understanding of sleep dependent memory consolidation in depression aetiology.

  2. Pengaruh Pemberian Persepuluhan Atas Kerohanian Gereja Sidang Jemaat Allah Jemaat Victorius Worship Family Makassar

    Directory of Open Access Journals (Sweden)

    Christina Evi Paligi

    2010-04-01

    Full Text Available Yang menjadi pokok masalah dalam penulisan karya ilmiah ini adalah sejauh mana sikap jemaatdalam hal perpuluhan berpengaruh atas perkembangan rohani, dan sejauh mana sikap jemaat dalamperpuluhan berpengaruh atas perkembangan usaha. Tujuan penulisan ini ialah untuk mencari tahu faktorfaktorapa yang menyebabkan jemaat tidak setia dalam memberi persepuluhan kepada Tuhan, dan untukmencari tahu mengapa jemaat tidak memahami dengan benar tentang persepuluhan. Penelitian akanmengambil sample yang terdiri dari 50 anggota jemaat yang sudah berpenghasilan. Teknik pengumpulandata melalui angket dan teknik analisis data yaitu penggunaan analisis statistic dengan program SPSS 15.Adapu hasiul penelitian bahwa tingkat pendidikan jemaat GSJA Victorious Worship FamilyMakassar sangat berpengaruh terhadap perkembangan rohani jemaat, di mana apabila terjadi peningkatanpada tingkat pendidikan jemaat maka perkembangan rohaninya mengalami penurunan. Kedua, bahwatingkat pendidikan jemaat sangat berpengaruh terhadap keberhasilan usaha jemaat, di mana apabila terjadipeningkatan pada tingkat pendidikan jemaat maka keberhasilan usaha jemaat mengalami peningkatan.Ketiga, bahwa tingkat pendidikan jemaat sangat berpengaruh terhadap sikap memberi persepuluhan kepadaTuhan, di mana apabila terjadi peningkatan pada tingkat pendidikan maka tingkat sikap memberipersepuluhan kepada Tuhan mengalami perkembangan.

  3. The Evaluation of Ataşehir-İstanbul Mass Housing Development in the Context of Total Quality Management Approach

    Directory of Open Access Journals (Sweden)

    Nesrin Dengiz

    2003-05-01

    Full Text Available Today one of the most discussed issues about housing estates is ‘quality’. Here the ‘quality’ of a housing estate, Ataşehir is evaluated. According to the ideas brought by Total Quality Management today new approaches of ‘quality’ and ‘Total Quality’ emphasize the importance of the ‘user’, designer’ and ‘constructor’, which are the main tree groups of a quality production process. In this paper, we have tried to determine the level of “quality” of Ataşehir Housing Development.

  4. AtaA, a new member of the trimeric autotransporter adhesins from Acinetobacter sp. Tol 5 mediating high adhesiveness to various abiotic surfaces.

    Directory of Open Access Journals (Sweden)

    Masahito Ishikawa

    Full Text Available Acinetobacter sp. Tol 5 exhibits an autoagglutinating nature and noteworthy adhesiveness to various abiotic surfaces from hydrophobic plastics to hydrophilic glass and stainless steel. Although previous studies have suggested that bacterionanofibers on Tol 5 cells are involved in the adhesive phenotype of Tol 5, the fiber that directly mediates Tol 5 adhesion has remained unknown. Here, we present a new member of trimeric autotransporter adhesins designated AtaA, which we discovered by analyzing a less adhesive mutant of Tol 5, T1, obtained by transposon mutagenesis. AtaA forms thinner and shorter nanofibers than fimbriae on Tol 5 cells. We performed target disruption of ataA by allelic marker exchange, and the resulting ΔataA strain was complemented with ataA on the Escherichia coli-Acinetobacter shuttle vector, which was newly constructed. These results proved that AtaA is essential for Tol 5's autoagglutinating nature and high adhesiveness to surfaces of various materials. In addition, the adhesiveness to solid surfaces mediated by AtaA is notably higher than that mediated by YadA of Yersinia enterocolitica WA-314. Moreover, and importantly, these characteristics can be conferred to the non-adhesive, non-agglutinating bacterium Acinetobacter sp. ADP1 in trans by transformation with ataA, with expected applications to microbial immobilization.

  5. 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.

  6. 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.

  7. ALMA software releases versus quality management: and the winner is...

    Science.gov (United States)

    Allaert, Erik; Pasquato, Moreno; Soto, Rubén.

    2016-08-01

    After its inauguration and the formal completion of the construction phase, the software development effort at the Atacama Large Millimeter/submillimeter Array (ALMA) continues at roughly the same level as during construction - gradually adding capabilities as required by and offered to the scientific community. In the run-up to a new yearly Observing Cycle several software releases have to be prepared, incorporating this new functionality. However, the ALMA observatory is used on a daily basis to produce scientific data for the approved projects within the current Observing Cycle, and also by engineering teams to extend existing capabilities or to diagnose and fix problems - so the preparation of new software releases up to their deployment competes for resources with all other activities. Testing a new release and ensuring its quality is of course fundamental, but can on the other hand not monopolize the observatory's resources or jeopardize its commitments to the scientific community.

  8. 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

  9. Data products of the ALMA and NRAO archives

    Science.gov (United States)

    Lacy, Mark

    2016-07-01

    Radio astronomy archives present particular challenges due to the complexity of the data processing. New radio telescopes such as the Jansky-VLA and ALMA also have much larger data volumes than the previous generation of instruments, requiring large amounts of storage and processing. Here we describe the approach taken by NRAO towards making the data products of the VLA and ALMA available to our users. This includes traditional approaches of pipelining and imaging, and also on-demand server side processing, visualization and analysis. We discuss how the size of the image products is related to that of the visibility data, and how this places variable demands on the data flow from the telescope and its data center as configurations are changed throughout the year. Finally, we look ahead to the next generation of radio telescopes such as the SKA and ngVLA.

  10. A psicopatologia como uma experiência da alma

    Directory of Open Access Journals (Sweden)

    Anna Paula Zanoni

    2011-09-01

    Full Text Available Este trabalho teórico apresenta a visão do psicólogo arquetípico James Hillman sobre a psicopatologia. Ele defende que "patologizar" é um movimento da psique válido, necessário e autêntico, que permite um encontro com a alma e com os sentidos e que deve ser compreendido metaforicamente. Sua visão se contrapõe ao modelo médico e nominalista dominante, que tem uma visão literal da psicopatologia e que acaba por afastá-la dos sentidos, da alma e do próprio sujeito. A crítica maior de Hillman é sobre a relação literal da psicologia com as palavras e termos psicopatológicos.

  11. Comparison of Integer Programming (IP) Solvers for Automated Test Assembly (ATA). Research Report. ETS RR-15-05

    Science.gov (United States)

    Donoghue, John R.

    2015-01-01

    At the heart of van der Linden's approach to automated test assembly (ATA) is a linear programming/integer programming (LP/IP) problem. A variety of IP solvers are available, ranging in cost from free to hundreds of thousands of dollars. In this paper, I compare several approaches to solving the underlying IP problem. These approaches range from…

  12. 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...

  13. 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...

  14. 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...

  15. First ALMA Detection of a Galaxy Cluster Merger Shock

    Science.gov (United States)

    Basu, K.; Sommer, M.; Erler, J.; Eckert, D.; Vazza, F.; Magnelli, B.; Bertoldi, F.; Tozzi, P.

    2016-12-01

    We report on the first ALMA measurement of a galaxy cluster merger shock, observed at the location of a radio relic in the famous El Gordo galaxy cluster at redshift z 0.9. Located at about half the current age of the Universe, this is also the most distant example of a directly measured astrophysical shock. ALMA Band 3 was utilised to measure the Sunyaev-Zel'dovich (SZ) effect signature that confirms a small-scale change in pressure as expected from the passage of a shock in the intracluster medium. The results support a previous radio-based estimate of the shock Mach number and display similarities, and also some mild tensions, with the X-ray based results. Most importantly, these results show the potential of ALMA to detect galaxy cluster shocks, observations that will advance our knowledge of cluster formation, non-thermal particle acceleration and amplification of magnetic fields across the entire observable Universe where such relic shocks can be found.

  16. 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]).

  17. Experience with the operation of the European ALMA antennas

    Science.gov (United States)

    Stanghellini, Stefano; Laing, Robert; Rossi, Silvio; Wild, Wolfgang

    2016-07-01

    The 25 European antennas of ALMA were delivered by ESO to the ALMA project in Chile between April 2011 and September 2013. Their combined time of operation is already significant and allows us to draw conclusions regarding their ability to fulfil the original specification, in terms of both scientific performance and operational availability. In this paper, we will summarize the experience gained during the past five years of operation. We will characterize the performance of the antennas in routine operation and compare with the data obtained during acceptance testing. We will also describe the few technical issues experienced while operating at 5000m and the way in which these were treated during these first years of operation. We will evaluate the effective reliability obtained in service based on field data and draw some conclusions as to the way in which reliability and maintainability aspects were covered during the process which led to the final design of the antenna. We will discuss the smart use of software to handle redundancy in a flexible way and to exclude failed components without affecting overall antenna operability. The use of low-level diagnostics enabled by remote access allows us to shorten the trouble-shooting cycle and to optimise physical interventions on the antennas. Finally, the paper will cover Antenna maintenance manuals edited using an industrial interactive standard. It will be explained why this advanced and innovative concept has not achieved the success that was expected, and why the traditional form is preferred at the ALMA Observatory.

  18. Preliminary Results on Hydrological and Hydrochemical Features of Kartamak Glacier Area in Mt. Muztag Ata

    Institute of Scientific and Technical Information of China (English)

    ZHAO Huabiao; YAO Tandong; XU Baiqing

    2007-01-01

    The variations of the meltwater runoff draining from Kartamak Glacier in Mt. Muztag Ata in China were studied by using the measured hydrological data from 1 June to 25 August 2003. The meltwater runoff is mainly affected by ambient temperature and precipitation. Meltwater and precipitation samples were collected from 10 to 23 August 2003.Their pH, EC (electric conductivity) and the major ions (Na+, K+, Ca2+, Mg2+, Cl-, NO3-, SO42-) were determined. pH values showed a positive correlation with EC values for all samples. Meltwater samples were slightly alkaline. Sulfate and calcium were the dominant anion and cation in the measured ions, respectively. All the ion concentrations had inverse relationships with runoff or water level. In order to discuss the origins of dissolved chemical substances in the glacial meltwater, a principal component analysis was carried out. The results showed that water-rock interaction determined the ion components of the meltwater.

  19. PiHi Observations at the ATA, Conventional and Unconventional SETI

    Science.gov (United States)

    Harp, Gerald; Wilcox, B.; Arbunich, J.; Blair, S.; Backus, P. R.; Tarter, J. C.; Shostak, S.; Jordan, J.; Kilsdonk, T.; Ackermann, R. F.; Ross, J.; ATA Team

    2010-01-01

    Many radio SETI searches focus on the frequency range where the HI (1.42 GHz) and OH lines (1.6-1.7 GHz) lines are landmarks delineating the water hole This is only a small fraction of the terrestrial microwave window (TMW) from 1-10 GHz. This survey occurs near the center of the TMW at 4.462336275 GHz or π times the HI frequency. We call this the PiHI ("pie high") survey. The inspiration for PiHI observations comes from Carl Sagan in his book, Contact. This survey builds upon and extends a previous survey at PiHI (Blair, D. G. et al. (1992), MNRAS, 257, 105) with greater sensitivity, resolution, and coverage. We survey the nearest 94 main sequence stars in the HabCat catalog (Turnbull, M. C. and Tarter, J. C. (2003), ApJS, 145, 181) with spectral classes between F9 and G7 (max. radius 62 pc). The ATA's flexibility allows simultaneous measurements of targeted observations on stars (with beamformers) and 1° FOV "blind” observations of the areas around target stars (with imaging correlator). The targeted observations are carried out with a high resolution (0.7 Hz) spectrometer and integration times on the order of 200 s. The spectral imaging correlator measures a 50 x 50 grid of points with 3 kHz spectral resolution. This survey shows several signals of minor interest were discovered, though none of the signals reported are continuously "on,” which is an important characteristic for the positive identification of an ETI signal. The ATA has been funded through generous grants from the Paul G. Allen Family Foundation, the SETI Institute, UC Berkeley, the National Science Foundation (Grant No. 0540599), Sun Microsystems, Xilinx, Nathan Myhrvold, Greg Papadopoulos, and other corporations and individual donors.

  20. PEMODELAN PONDASI DANGKAL DENGAN MENGGUNAKAN TIGA LAPIS GEOTEKSTIL DI ATAS TANAH LIAT LUNAK

    Directory of Open Access Journals (Sweden)

    Subianto Tjandrawibawa

    2002-01-01

    Full Text Available It was common practice to apply a layer of ''sirtu'' (sandy gravel beneath the shallow foundations of buildings on soft subsoil. Though the bearing capacity is increased, it is usually limited to anticipate future consolidation settlements which might be detrimental. This could be overcome by reinforcing the ''sirtu'' layer with geotextiles. To study the effect of geotextile reinforcement, a laboratory foundation model was constructed on a soft soil deposit. The model measured 5x5x2cm³. The bearing capacity of this model was compared with the bearing capacity of the model on ''sirtu'' layer, and geotextile reinforced ''sirtu''. Geotextile reinforcement was laid in one, two and three layers. Based on the bearing capacity tests, it is concluded that with one geotextile layer the strength was increased 182,6% higher than soft soil, with two geotextile layers the strength increased 197,8% higher than soft soil and with three geotextile layer the strength increased 241,3% higher than soft soil. Abstract in Bahasa Indonesia : Bangunan di atas tanah yang lunak sering menggunakan lapisan sirtu di bawah pondasi dangkalnya. Cara ini dapat meningkatkan daya dukung pondasi namun daya dukung ini masih harus dibatasi untuk menghindari kemungkinan penurunan jangka panjang yang merugikan. Penurunan lapisan sirtu sendiri dapat ditanggulangi dengan memasang perkuatan berupa lapisanlapisan geotekstil di dalamnya. Sebuah model dibuat di laboratorium untuk mempelajari efektifitas lapisan-lapisan geotekstil ini terhadap peningkatan daya dukung. Model pondasi berukuran 5x5x2cm³. Daya dukung model ini, langsung di atas tanah lunak, dibandingkan dengan daya dukung model pondasi yang terletak pada lapisan sirtu dan lapisan sirtu yang diperkuat geotekstil. Lapisan sirtu diperkuat dengan satu, dua sampai tiga lapis geotekstil. Hasil percobaan menunjukkan dengan satu lapis geotekstil kekuatan meningkat sebesar 182,6% dibanding tanah lunak, dengan dua lapis geotekstil

  1. Reasoning about passive declarations in CHR

    DEFF Research Database (Denmark)

    Christiansen, Henning

    2005-01-01

    The programming language of Constraint Handling Rules (CHR) is gaining more and more popularity and this has motivated the development of new optimization techniques to be applied in implementations of CHR. As for other logic programming languages, a program written CHR can be understood declarat...... give different classifications of the effect of some passive declarations that do not affect the logical semantics. This may be used for reasoning about manual optimizations as well as proposals for automatic strategies to be applied by a compiler for adding passive declarations....

  2. Compiling ER Specifications into Declarative Programs

    CERN Document Server

    Braßel, Bernd; Muller, Marion

    2007-01-01

    This paper proposes an environment to support high-level database programming in a declarative programming language. In order to ensure safe database updates, all access and update operations related to the database are generated from high-level descriptions in the entity- relationship (ER) model. We propose a representation of ER diagrams in the declarative language Curry so that they can be constructed by various tools and then translated into this representation. Furthermore, we have implemented a compiler from this representation into a Curry program that provides access and update operations based on a high-level API for database programming.

  3. ALMA to Help Solving Acute Mountain Sickness Mystery

    Science.gov (United States)

    2007-04-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) astronomical project will not only enlarge our knowledge of the vast Universe beyond the imaginable. It will also help scientists learn more about the human body. Located 5000m above sea level, in the Chilean Atacama desert, ALMA is the highest site for ground-based astronomy. This property will be put to good use for academic institutions in Chile and in Europe in order to study the human response to extreme altitude conditions. During a ceremony held on 2 April in Antofagasta, the largest town close to ESO's Very Large Telescope, representatives from ALMA, ESO and the University of Antofagasta have officially launched a collaborative agreement that also involves the University of Chile and the University of Copenhagen (Denmark). The newly established cooperation aims at contributing to the promotion of teaching, scientific research, and the expansion of altitude physiology and medicine or other related areas considered appropriate. ESO PR Photo 20/07 ESO PR Photo 20/07 Working at 5000 metres "An increasing number of people are periodically exposed to brisk changes in altitude, and not only for astronomical research," said Jacques Lassalle, the ALMA Safety Manager. "Short stays at high altitude alternate with short stays at sea level but the corresponding shifts are very often established by agreement, and not based on scientific arguments. With this project, we aim at improving our knowledge and procedures in order to protect the long term health of the operators, engineers, and scientists as well as ALMA visitors of all ages and all physical conditions," he added. Around the world, a large number of people systematically commute between sea level and high altitude, for example when working in mountainous mines. This poses stringent conditions that may affect health, wellbeing and working performance. Some of the factors in question are the shift work regime, the perturbation of circadian rhythms, fatigue

  4. Application of the adhesive bacterionanofiber AtaA to a novel microbial immobilization method for the production of indigo as a model chemical.

    Science.gov (United States)

    Ishikawa, Masahito; Shigemori, Kazuki; Hori, Katsutoshi

    2014-01-01

    The toluene-degrading bacterium Acinetobacter sp. Tol 5 shows high adhesiveness mediated by the bacterionanofiber protein AtaA, which is a new member of the trimeric autotransporter adhesin (TAA) family. In contrast to other reported TAAs, AtaA mediates the adhesion of Tol 5 to various abiotic surfaces ranging from hydrophobic plastics to hydrophilic glass and stainless steel. The expression of ataA in industrially relevant bacteria improves their adhesiveness and enables immobilization directly onto support materials. This represents a new method that can be alternated with conventional immobilization via gel entrapment and chemical bonding. In this study, we demonstrate the feasibility of this immobilizing method by utilizing AtaA. As a model case for this method, the indigo producer Acinetobacter sp. ST-550 was transformed with ataA and immobilized on a polyurethane support. The immobilized ST-550 cells were transferred directly to a reaction solution containing indole as the substrate. The immobilized ST-550 cells showed a faster indigo production rate at high concentrations of indole compared with planktonic ST-550 not expressing the ataA gene, implying that immobilization enhanced the tolerance of ST-550 to the substrate indole. As a result, the immobilized ST-550 produced fivefold higher levels of indigo than planktonic ST-550. These results proved that AtaA is useful for bacterial immobilization.

  5. Sudan Genocide Declaration Stirs the World

    Science.gov (United States)

    Social Education, 2004

    2004-01-01

    One week after Secretary of State Colin Powell declared that the killings, rapes and other atrocities committed in Darfur amount to "genocide," in mid-September the United Nations' World Health Organization issued new figures saying 6,000 to 10,000 people are dying per month there in one of Africa's worst humanitarian crises. Powell had…

  6. Stress enhances reconsolidation of declarative memory

    NARCIS (Netherlands)

    Bos, M.G.N.; Schuijer, J.; Lodestijn, F.; Beckers, T.; Kindt, M.

    2014-01-01

    Retrieval of negative emotional memories is often accompanied by the experience of stress. Upon retrieval, a memory trace can temporarily return into a labile state, where it is vulnerable to change. An unresolved question is whether post-retrieval stress may affect the strength of declarative memor

  7. The Universal Declaration of Human Rights

    Science.gov (United States)

    Landorf, Hilary

    2012-01-01

    A study of human rights prepares students for their role as global citizens and their study of practices in the world's countries that relate to the rights of human beings. Today, when one talks of human rights it is usually with reference to the 1948 Universal Declaration of Human Rights (UDHR). It is the task of teachers to give students the…

  8. Declarative interpretations of session-based concurrency

    DEFF Research Database (Denmark)

    Cano, Mauricio; Rueda, Camilo; López-Acosta, Hugo-Andrés;

    2015-01-01

    Session-based concurrency is a type-based approach to the analysis of communication-intensive systems. Correct behavior in these systems may be specified in an operational or declarative style: the former defines how interactions are structured; the latter defines governing conditions. In this pa...

  9. 19 CFR 122.43 - General declaration.

    Science.gov (United States)

    2010-04-01

    ... 19 Customs Duties 1 2010-04-01 2010-04-01 false General declaration. 122.43 Section 122.43 Customs Duties U.S. CUSTOMS AND BORDER PROTECTION, DEPARTMENT OF HOMELAND SECURITY; DEPARTMENT OF THE TREASURY AIR COMMERCE REGULATIONS Aircraft Entry and Entry Documents; Electronic Manifest Requirements...

  10. Second World Materials Summit Suzhou Declaration

    Institute of Scientific and Technical Information of China (English)

    2009-01-01

    @@ Suzhou 2009 Declaration Clean energy and sustainability are global issues that require international collaboration.Materials play a critical role in addressing these challenges.The Second World Materials Summit in Suzhou provides an avenue to create international cooperation to address energy related materials solutions.Our priorities track the relevant sections of the Kyoto resolution.

  11. State of emergency declared for Gran Sasso

    CERN Multimedia

    2003-01-01

    "On June 27th the Council of Ministers has declared the state of socioeconomic and environmental emergency in the territory of L'Aquila and Teramo, the provinces involved in the safety of the Gran Sasso system. The measure includes the INFN Gran Sasso National Laboratories, the high-way tunnels, the environment in general and water in particular" (1 page).

  12. The Amsterdam Declaration on Fungal Nomenclature

    NARCIS (Netherlands)

    Hawksworth, D.L.; Crous, P.W.; Redhead, S.A.; Reynolds, D.R.; Samson, R.A.; Seifert, K.A.; Taylor, J.E.; Wingfield, M.J.; Abaci, Ö.; Aime, C.; Asan, A.; Bai, F.H.; de Beer, Z.W.; Begerow, D.; Berikten, D.; Boekhout, T.; Buchanan, P.K.; Burgess, T.I.; Buzina, W.; Cai, L.; Cannon, P.F.; Crane, J.L.; Damm, U.; Daniel, H.M.; van Diepeningen, A.D.; Druzhinina, I.; Dyer, P.S.; Eberhardt, U.; Fell, J.W.; Frisvad, J.C.; Geiser, D.M.; Geml, J.; Glienke, C.; Gräfenhan, T.; Groenewald, J.Z.; Groenewald, M.; de Gruyter, J.; Guého-Kellermann, E.; Guo, L-D.; Hibbett, D.S.; Hong, S.B.; de Hoog, G.S.; Houbraken, J.; Huhndorf, S.M.; Hyde, K.D.; Ismail, A.; Johnston, P.R.; Kadaifciler, D.G.; Kirk, P.M.; Kõljalg, U.; Kurtzman, C.P.; Lagneau, P-E.; Lévesque, C.A.; Liu, X.S.; Lombard, L.; Meyer, W.; Miller, A.N.; Minter, D.W.; Najafzadeh, M.J.; Norvell, L.L.; Ozerskaya, S.M.; Öziç, R.; Pennycook, S.R.; Peterson, S.W.; Pettersson, O.V.; Quaedvlieg, W.; Robert, V.; Ruibal, C.; Schnürer, J.; Schroers, H.J.; Shivas, R.G.; Slippers, B.; Spierenburg, H.; Takashima, M.; Taşkın, E.; Thines, M.; Thrane, U.; Uztan, A.H.; van Raak, M.; Varga, J.; Vasco, A.; Verkley, G.J.M.; Videira, S.I.R.; de Vries, R.P.; Weir, B.S.; Yilmaz, N.; Yurkov, A.; Zhang, N.

    2011-01-01

    The Amsterdam Declaration on Fungal Nomenclature was agreed at an international symposium convened in Amsterdam on 19-20 April 2011 under the auspices of the International Commission on the Taxonomy of Fungi (ICTF). The purpose of the symposium was to address the issue of whether or how the current

  13. 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

  14. "The Chennai declaration" - Indian doctors' fight against antimicrobial resistance

    NARCIS (Netherlands)

    Voss, A.; Ghafur, A.

    2013-01-01

    "The Chennai Declaration" is the result of the first ever joint meeting of medical societies in India addressing antibiotic resistance. The declaration is not a policy by itself, but a call for a national policy. The Declaration has looked into all major aspects of the problem of antimicrobial resis

  15. 37 CFR 1.68 - Declaration in lieu of oath.

    Science.gov (United States)

    2010-07-01

    ... 37 Patents, Trademarks, and Copyrights 1 2010-07-01 2010-07-01 false Declaration in lieu of oath. 1.68 Section 1.68 Patents, Trademarks, and Copyrights UNITED STATES PATENT AND TRADEMARK OFFICE... Declaration § 1.68 Declaration in lieu of oath. Any document to be filed in the Patent and Trademark...

  16. 47 CFR 68.324 - Supplier's Declaration of Conformity requirements.

    Science.gov (United States)

    2010-10-01

    ... 47 Telecommunication 3 2010-10-01 2010-10-01 false Supplier's Declaration of Conformity... Terminal Equipment Approval § 68.324 Supplier's Declaration of Conformity requirements. (a) Each responsible party shall include in the Supplier's Declaration of Conformity, the following information:...

  17. 24 CFR 41.3 - Assurance and declaration required.

    Science.gov (United States)

    2010-04-01

    ... require a declaration as to project drawings, specifications, and other construction documents. The... responsible official as designated by HUD, who has prepared such construction documents. The declaration shall affirm that the proposed project, to the best knowledge and belief of the declarer, conforms...

  18. 24 CFR 203.434 - Declaration of trust.

    Science.gov (United States)

    2010-04-01

    ... 24 Housing and Urban Development 2 2010-04-01 2010-04-01 false Declaration of trust. 203.434... Mortgage § 203.434 Declaration of trust. A sale of a beneficial interest in a group of insured mortgages... interest in a specific mortgage shall be made only pursuant to a declaration of trust, which has...

  19. 24 CFR 203.493 - Declaration of trust.

    Science.gov (United States)

    2010-04-01

    ... 24 Housing and Urban Development 2 2010-04-01 2010-04-01 false Declaration of trust. 203.493... Declaration of trust. A sale of a beneficial interest in a group of insured loans, where the interest to be... be made only pursuant to a declaration of trust, which has been approved by the Commissioner prior...

  20. MODEL PENGENALAN PERMAINAN DALAM PEMBELAJARAN LOMPAT JAUH PADA SISWA KELAS ATAS SEKOLAH DASAR

    Directory of Open Access Journals (Sweden)

    Kurnia Azis Setyawan

    2015-10-01

    Full Text Available Penelitian ini bertujuan untuk menghasilkan model pengenalan pembelajaran lompat jauh pada siswa sekolah dasar (SD kelas atas tahun pelajaran 2013/2014 di Kecamatan Srumbung, Kabupaten Magelang. Model pembelajaran yang dikembangkan diharapkan untuk digunakan guru SD sebagai salah satu bentuk pembelajaran lompat jauh yang baik dan efektif. Penelitian pengembangan ini dilakukan dengan mengadaptasi langkah-langkah penelitian pengembangan sebagai berikut: (1 pengumpulan informasi di lapangan, (2 melakukan analisis terhadap informasi yang telah dikumpul-kan, (3 mengembangkan produk awal (draf model, (4 validasi ahli dan revisi, (5 uji coba lapangan skala kecil dan revisi, (6 uji coba lapangan skala besar dan revisi, dan (7 pembuatan produk final. Uji coba skala kecil dilakukan terhadap siswa kelas 5 SD N Tegalrandu dan SD N Polengan, Kecamatan Srumbung yang berjumlah 31 siswa. Uji coba skala besar dilakukan terhadap siswa kelas 5 SD N Tegalrandu, SD N Polengan, SD N Pucanganom, SD N Pandanretno, SD N Soka 1 yang berjumlah 81 siswa. Instrumen pengumpulan data yang digunakan yaitu; (1 pedoman wawancara, (2 skala nilai, (3 pedoman observasi model pembelajaran, (4 pedoman observasi keefektifan model pembelajaran. Teknik analisis data yang dilakukan yaitu analisis deskriptif kuantitatif dan analisis deskriptif kualitatif. Hasil penelitian ini berupa buku dan video model pengenalan dalam pembelajaran lompat jauh pada SD kelas atas. Berdasarkan penilaian ahli materi cabang olahraga atletik dan guru penjasor-kes, produk model pengenalan dalam pembelajaran lompat jauh pada SD kelas atas, sudah sesuai dan layak untuk digunakan oleh guru penjasorkes dalam mengajarkan materi lompat jauh kepada siswanya dengan nilai rata-rata 98,1%. Kata kunci: pengembangan, permainan, model pengenalan pembelajaran lompat jauh   INTRODUCTION MODELS IN LEARNING GAMES OF LONG JUMP IN UPPER CLASS ELEMENTARY SCHOOL Abstract This study aims to produce introduction models of the

  1. 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.

  2. Pendidikan sebagai Perekrut dalam Komunitas Terbayang: Analisa Wacana dalam Film Denias Senandung di Atas Awan

    Directory of Open Access Journals (Sweden)

    Katarina Rima Melati

    2014-10-01

    Full Text Available Penelitian ini bertujuan untuk memahami wacana politik dan negara yang dibentukoleh sebuah film. Film Denias, Senandung Di Atas Awan (DSAW dipilih sebagaistudi kasus karena film ini pernah menjadi film terbaik Indonesia dan mewakiliIndonesia dalam seleksi piala Oscar 2008. Berdasarkan hasil penelitian dapatdipahami bahwa menjadi sebuah negara adalah membayangkan sebuah komunitasyang dibangun dengan unit politik yang sama dan melalui sentimen sebagai ‘sesamawarga negara’. Proses ini bukannya selalu berjalan mulus, malahan salah saturesikonya adalah tercabutnya nilai-nilai otentisitas kedaerahan yang telah mengakardalam sebuah komunitas untuk kemudian distandarisasi agar kokoh sebagaibangunan bernama negara. Imaginasi proyek negara ini diusung terus menerusmelalui wacana pembentukan nasionalisme kebangsaan salah satunya adalahmelalui sistem pendidikan yang dilembagakan dalam bentuk sekolah. Film DSAWmemberi gambaran bagaimana pendidikan terutama di lingkungan sekolah menjadiagenda politik dalam memasukkan ideologi kebangsaan termasuk dengan atributatributkenegaraan seperti militer melalui anggota Kopassus; budaya melalui bahasaIndonesia; pembentukan oposisi biner antara Jawa yang telah maju dibandingkandengan Papua yang tertinggal; termasuk Freeport sebagai representasi dari kapital.Film DSAW menjadi contoh bagi pembentukan bayangan komunitas sebagaikesatuan yang direkrut melalui ideologi-ideologi bahkan doktrin-doktrin yang adadalam sistem pendidikan.   The Education as a Means of Recruiting in the Imagined Community: TheDiscourse Analysis in Denias Movie, Senandung di Atas Awan. This study aimsto understand the political and state discourse formed by a movie. Denias movie ischosen as a case study because it has ever been the best Indonesian movie and representedIndonesia in the selection of 2008 Oscar Award. Based on the research result, it can beunderstood that being a nation is such a way of imagining a community built with asimilar

  3. The evolution of the simulation environment in the ALMA Observatory

    Science.gov (United States)

    Shen, Tzu-Chiang; Soto, Ruben; Saez, Norman; Velez, Gaston; Staig, Tomas; Sepulveda, Jorge; Saez, Alejandro; Ovando, Nicolas; Ibsen, Jorge

    2016-07-01

    The Atacama Large Millimeter /submillimeter Array (ALMA) has entered into operation phase since 2013. This transition changed the priorities within the observatory, in which, most of the available time will be dedicated to science observations at the expense of technical time. Therefore, it was planned to design and implement a new simulation environment, which must be comparable - or at least- be representative of the production environment. Concepts of model in the loop and hardware in the loop were explored. In this paper we review experiences gained and lessons learnt during the design and implementation of the new simulation environment.

  4. Model-based fault detection and diagnosis in ALMA subsystems

    Science.gov (United States)

    Ortiz, José; Carrasco, Rodrigo A.

    2016-07-01

    The Atacama Large Millimeter/submillimeter Array (ALMA) observatory, with its 66 individual telescopes and other central equipment, generates a massive set of monitoring data every day, collecting information on the performance of a variety of critical and complex electrical, electronic and mechanical components. This data is crucial for most troubleshooting efforts performed by engineering teams. More than 5 years of accumulated data and expertise allow for a more systematic approach to fault detection and diagnosis. This paper presents model-based fault detection and diagnosis techniques to support corrective and predictive maintenance in a 24/7 minimum-downtime observatory.

  5. Operational logs analysis at ALMA observatory based on ELK stack

    Science.gov (United States)

    Gil, Juan P.; Reveco, Johnny; Shen, Tzu-Chiang

    2016-07-01

    During operations, the ALMA observatory generates a huge amount of logs which contain not only valuable information related to specific failures but also for long term performance analysis. We implemented a big data solution based on Elasticsearch, Logstash and Kibana. They are configured as decoupled system which causes zero impact on the existent operations. It is able to keep more than six months of operation logs online. In this paper, we'll describe this infrastructure, applications built on top of it, and the problems that we faced during its implementation.

  6. Order within disorder: The atomic structure of ion-beam sputtered amorphous tantala (a-Ta2O5

    Directory of Open Access Journals (Sweden)

    Riccardo Bassiri

    2015-03-01

    Full Text Available Amorphous tantala (a-Ta2O5 is a technologically important material often used in high-performance coatings. Understanding this material at the atomic level provides a way to further improve performance. This work details extended X-ray absorption fine structure measurements of a-Ta2O5 coatings, where high-quality experimental data and theoretical fits have allowed a detailed interpretation of the nearest-neighbor distributions. It was found that the tantalum atom is surrounded by four shells of atoms in sequence; oxygen, tantalum, oxygen, and tantalum. A discussion is also included on how these models can be interpreted within the context of published crystalline Ta2O5 and other a-T2O5 studies.

  7. A Formal Model For Declarative Workflows

    DEFF Research Database (Denmark)

    Mukkamala, Raghava Rao

    it as a general formal model for specification and execution of declarative, event-based business processes, as a generalization of a concurrency model, the classic event structures. The model allows for an intuitive operational semantics and mapping of execution state by a notion of markings of the graphs and we...... the declarative nature of the projected graphs (which are also DCR graphs). We have also provided semantics for distributed executions based on synchronous communication among network of projected graphs and proved that global and distributed executions are equivalent. Further, to support modeling of processes......Current business process technology is pretty good in supporting well-structured business processes and aim at achieving a fixed goal by carrying out an exact set of operations. In contrast, those exact operations needed to fulfill a business pro- cess/workflow may not be always possible to foresee...

  8. Evaluation of Amigas Latinas Motivando el Alma (ALMA): a pilot promotora intervention focused on stress and coping among immigrant Latinas.

    Science.gov (United States)

    Tran, Anh N; Ornelas, India J; Perez, Georgina; Green, Melissa A; Lyn, Michelle; Corbie-Smith, Giselle

    2014-04-01

    Recent immigrant Latinas are at increased risk of poor mental health due to stressors associated with adapting to life in the United States. This study evaluated Amigas Latinas Motivando el Alma, a promotora intervention to reduce stress and promote health and coping among recent immigrant Latinas. Using a pre- and post-test design, we evaluated mental health outcomes, specifically, in promotoras. Promotoras' knowledge levels related to role of promotora and stress management increased, depressive symptoms and stress levels decreased, and coping responses and perceived social support increased as well. Results suggest that promotora programs may be an effective way to improve mental health in recent immigrant Latinas.

  9. The Petunia GRAS Transcription Factor ATA/RAM1 Regulates Symbiotic Gene Expression and Fungal Morphogenesis in Arbuscular Mycorrhiza.

    Science.gov (United States)

    Rich, Mélanie K; Schorderet, Martine; Bapaume, Laure; Falquet, Laurent; Morel, Patrice; Vandenbussche, Michiel; Reinhardt, Didier

    2015-07-01

    Arbuscular mycorrhiza (AM) is a mutual symbiosis that involves a complex symbiotic interface over which nutrients are exchanged between the plant host and the AM fungus. Dozens of genes in the host are required for the establishment and functioning of the interaction, among them nutrient transporters that mediate the uptake of mineral nutrients delivered by the fungal arbuscules. We have isolated in a genetic mutant screen a petunia (Petunia hybrida) Gibberellic Acid Insensitive, Repressor of Gibberellic Acid Insensitive, and Scarecrow (GRAS)-type transcription factor, Atypical Arbuscule (ATA), that acts as the central regulator of AM-related genes and is required for the morphogenesis of arbuscules. Forced mycorrhizal inoculations from neighboring wild-type plants revealed an additional role of ATA in restricting mycorrhizal colonization of the root meristem. The lack of ATA, which represents the ortholog of Required For Arbuscular Mycorrhiza1 in Medicago truncatula, renders the interaction completely ineffective, hence demonstrating the central role of AM-related genes for arbuscule development and function.

  10. The Petunia GRAS Transcription Factor ATA/RAM1 Regulates Symbiotic Gene Expression and Fungal Morphogenesis in Arbuscular Mycorrhiza1

    Science.gov (United States)

    Rich, Mélanie K.

    2015-01-01

    Arbuscular mycorrhiza (AM) is a mutual symbiosis that involves a complex symbiotic interface over which nutrients are exchanged between the plant host and the AM fungus. Dozens of genes in the host are required for the establishment and functioning of the interaction, among them nutrient transporters that mediate the uptake of mineral nutrients delivered by the fungal arbuscules. We have isolated in a genetic mutant screen a petunia (Petunia hybrida) GIBBERELLIC ACID INSENSITIVE, REPRESSOR of GIBBERELLIC ACID INSENSITIVE, and SCARECROW (GRAS)-type transcription factor, ATYPICAL ARBUSCULE (ATA), that acts as the central regulator of AM-related genes and is required for the morphogenesis of arbuscules. Forced mycorrhizal inoculations from neighboring wild-type plants revealed an additional role of ATA in restricting mycorrhizal colonization of the root meristem. The lack of ATA, which represents the ortholog of REQUIRED FOR ARBUSCULAR MYCORRHIZA1 in Medicago truncatula, renders the interaction completely ineffective, hence demonstrating the central role of AM-related genes for arbuscule development and function. PMID:25971550

  11. IMPORTANT -Declaration of income for 2001-

    CERN Multimedia

    Human Resources Division

    2002-01-01

    The local French tax authorities confirm that, in view of the particular procedure for income declaration for CERN members of the personnel, this year CERN income (as stated in the certificate of CERN remuneration provided by the Organization) may be exceptionally declared in either French Francs, or Euros (clearly specifying the currency selected). Practical information concerning the procedure for income declaration may be obtained at the following local information desks : Trésorerie de Gex: Tuesday 12 March 9 a.m. to 122 to 4 p.m. Trésoreriede Ferney: Monday 18 March 9 a.m. to 122 to 4 p.m. Trésoreriede Divonne: Thursday 21 March 9 a.m. to 122 to 4 p.m. French tax authorities have also organised the following information services:Web site Minitel: 3615 IR Service Vocal Server: 08 36 67 10 10 Telephone information: 08 20 32 42 52 Human Resources Division Tel. 72838

  12. Confidential Declaration of Family Situation (CDFS)

    CERN Multimedia

    Human Resources Department

    2005-01-01

    The Confidential Declaration of Family Situation (CDFS) becomes a new computerized EDH form from October 2005 In accordance with Article R IV 1.17 of the Staff Regulations, Staff Members and Fellows, married or separated, must notify any changes in their spouse's income or health insurance cover in writing to CERN, within 30 calendar days of the change. This is necessary for the Organization to determine if a supplementary contribution is payable to the CERN Health Insurance Scheme (CHIS) for the spouse's coverage and, if so, the amount. Until now a paper form called « Confidential Declaration of Family Situation » (CDFS) was used for that purpose.  From early October 2005 the CDFS will be computerized for the whole Organization. Henceforth, any changes in a spouse's income or health insurance cover must be notified using EDH (Electronic Document Handling). Additionally, annual updates of the declaration will be required and will be requested by automatic e-mail. Early October an email will be sent to...

  13. Confidential Declaration of Family Situation (CDFS)

    CERN Multimedia

    Human Resources Department

    2005-01-01

    The Confidential Declaration of Family Situation (CDFS) becomes a new computerized EDH form from October 2005 In accordance with Article R IV 1.17 of the Staff Regulations, Staff Members and Fellows, married or separated, must notify any changes in their spouse's income or health insurance cover in writing to CERN, within 30 calendar days of the change. This is necessary for the Organization to determine if a supplementary contribution is payable to the CERN Health Insurance Scheme (CHIS) for the spouse's coverage and, if so, the amount. Until now a paper form called « Confidential Declaration of Family Situation » (CDFS) was used for that purpose.  From early October 2005 the CDFS will be computerized for the whole Organization. Henceforth, any changes in a spouse's income or health insurance cover must be notified using EDH (Electronic Document Handling). Additionally, annual updates of the declaration will be required and will be requested by automatic e-mail. Early October an email will be...

  14. UNVEILING THE DUST NUCLEATION ZONE OF IRC+10216 WITH ALMA

    Energy Technology Data Exchange (ETDEWEB)

    Cernicharo, J.; Daniel, F.; Goicoechea, J. R. [Departamento de Astrofísica, Centro de Astrobiología, CSIC-INTA, Ctra. de Torrejón a Ajalvir km 4, E-28850 Madrid (Spain); Castro-Carrizo, A.; Guélin, M. [Institut de Radioastronomie Millimétrique, 300 rue de la Piscine, F-38406, Saint Martin dHères (France); Agundez, M. [Univ. Bordeaux, LAB, UMR 5804, F-33270, Floirac (France); Marcelino, N. [NRAO, 520 Edgemont Road, Charlottesville, VA 22902 (United States); Joblin, C. [Université de Toulouse, UPS-OMP, IRAP, Toulouse (France)

    2013-12-01

    We report the detection in IRC+10216 of lines of HNC J = 3 – 2 pertaining to nine excited vibrational states with energies up to ∼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 current early ALMA data, the radius inferred for the emitting region is ∼0.''06 (i.e., ≅ 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{sub 2} is 10{sup –8} < χ(HNC) <10{sup –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 present throughout the inner envelope, such as vibrationally excited HCN, SiS, CS, or SiO, should allow us to characterize the physical and chemical conditions in the dust formation zone.

  15. 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...

  16. ALMA Band 8 Continuum Emission from Orion Source I

    Science.gov (United States)

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

    2016-12-01

    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 × 20 au, is consistent with those reported previously at other millimeter/submillimeter wavelengths. The flux density can be well fitted to the optically thick blackbody spectral energy distribution, 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, in which the continuum emission was proposed to arise from the edge-on circumstellar disk via thermal dust emission, unless the continuum source consists of an unresolved structure with a smaller beam filling factor.

  17. 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 ($&...

  18. La ciencia del alma en IBN Bayya (Avempace

    Directory of Open Access Journals (Sweden)

    Lomba, Joaquín

    2007-01-01

    Full Text Available 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

  19. 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.

  20. 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.

  1. 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.

  2. 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.

  3. 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...

  4. 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.

  5. 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 ...

  6. 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...

  7. 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...

  8. 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

  9. Catherine Pozzi y Marcelle Sauvageot: escribir la soledad del alma en un cuerpo de escritura

    OpenAIRE

    Peral-Crespo, Amelia

    2012-01-01

    La escritura de Catherine Pozzi y Marcelle Sauvageot está íntimamente ligada a la soledad que ha determinado sus vidas. La relación existente entre la soledad y la escritura como refugio del ser y a su vez como impulso escritural no se puede separar de los conceptos de alma y cuerpo presentes sobre todo en la obra de Catherine Pozzi. ¿Cómo separar el alma del cuerpo, y el cuerpo del alma? se preguntaba Pozzi en Peau d’Âme. ¿No sería acaso como separar la escritura de la soledad que la aliment...

  10. 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.

  11. 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.

  12. 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

  13. Declarative business process modelling: principles and modelling languages

    Science.gov (United States)

    Goedertier, Stijn; Vanthienen, Jan; Caron, Filip

    2015-02-01

    The business process literature has proposed a multitude of business process modelling approaches or paradigms, each in response to a different business process type with a unique set of requirements. Two polar paradigms, i.e. the imperative and the declarative paradigm, appear to define the extreme positions on the paradigm spectrum. While imperative approaches focus on explicitly defining how an organisational goal should be reached, the declarative approaches focus on the directives, policies and regulations restricting the potential ways to achieve the organisational goal. In between, a variety of hybrid-paradigms can be distinguished, e.g. the advanced and adaptive case management. This article focuses on the less-exposed declarative approach on process modelling. An outline of the declarative process modelling and the modelling approaches is presented, followed by an overview of the observed declarative process modelling principles and an evaluation of the declarative process modelling approaches.

  14. Stress enhances reconsolidation of declarative memory.

    Science.gov (United States)

    Bos, Marieke G N; Schuijer, Jantien; Lodestijn, Fleur; Beckers, Tom; Kindt, Merel

    2014-08-01

    Retrieval of negative emotional memories is often accompanied by the experience of stress. Upon retrieval, a memory trace can temporarily return into a labile state, where it is vulnerable to change. An unresolved question is whether post-retrieval stress may affect the strength of declarative memory in humans by modulating the reconsolidation process. Here, we tested in two experiments whether post-reactivation stress may affect the strength of declarative memory in humans. In both experiments, participants were instructed to learn neutral, positive and negative words. Approximately 24h later, participants received a reminder of the word list followed by exposure to the social evaluative cold pressor task (reactivation/stress group, nexp1=20; nexp2=18) or control task (reactivation/no-stress group, nexp1=23; nexp2=18). An additional control group was solely exposed to the stress task, without memory reactivation (no-reactivation/stress group, nexp1=23; nexp2=21). The next day, memory performance was tested using a free recall and a recognition task. In the first experiment we showed that participants in the reactivation/stress group recalled more words than participants in the reactivation/no-stress and no-reactivation/stress group, irrespective of valence of the word stimuli. Furthermore, participants in the reactivation/stress group made more false recognition errors. In the second experiment we replicated our observations on the free recall task for a new set of word stimuli, but we did not find any differences in false recognition. The current findings indicate that post-reactivation stress can improve declarative memory performance by modulating the process of reconsolidation. This finding contributes to our understanding why some memories are more persistent than others.

  15. Oskar Kokoschka and Alma Mahler: art as diary and as therapy.

    Science.gov (United States)

    Blum, Harold P

    2011-01-01

    The Austrian artist, Oskar Kokoschka, had an affair with Alma Mahler, widow of the composer Gustav Mahler, 1912-1914. This affair profoundly influenced his life and art. His palette at first brightened, with thick brush strokes and flashes of light and dark, indicating his psychological and emotional lability. Painting what he did not or could not express in words, his art of this period can be understood as an intimate visual diary of the vicissitudes of his relationship with Alma Mahler. For Kokoschka his work became a form of art therapy, following the crushing loss of Alma Mahler and near fatal physical injuries sustained in World War I. His gradual recovery was associated with his extraordinary attachment to and destruction of a lifelike effigy of Alma Mahler, thereby working through childhood trauma.

  16. 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.

  17. Guangzhou Customs Guide to "Local Declaration & Port Clearance"

    Institute of Scientific and Technical Information of China (English)

    2009-01-01

    @@ Ⅰ.Characteristic of the supervision mode of "Local Declaration & Port Clearance" This new mode means that the consignor,consignee or agent (hereafter referred to as "declarant") could choose any competent customs under the jurisdiction of Guangzhou Customs to make declaration and go through the formalities of document-checking and duty-paying,and then finish the cargo-examination and cargo-release at the customs office of entry or exit.

  18. Declarative vs. Procedural Memory: Roles in Second Language Acquisition

    Directory of Open Access Journals (Sweden)

    Laleh Fakhraee Faruji

    2012-04-01

    Full Text Available Memory is not a single faculty but is a combination of multiple distinct abilities (Schacter, 1987. The declarative-procedural distinction is used both with regard to knowledge and memory that stores this knowledge. Ellis (2008 used the terms explicit/implicit, and declarative/procedural interchangeably. In this article the researcher aims at identifying the different aspects of declarative/procedural memory, interaction between these two types of memory, and the role they may play in second language acquisition.

  19. 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.

  20. ALMA Reveals the Molecular Medium Fueling the Nearest Nuclear Starburst

    Science.gov (United States)

    Leroy, Adam K.; Bolatto, Alberto D.; Ostriker, Eve C.; Rosolowsky, Erik; Walter, Fabian; Warren, Steven R.; Donovan Meyer, Jennifer; Hodge, Jacqueline; Meier, David S.; Ott, Jürgen; Sandstrom, Karin; Schruba, Andreas; Veilleux, Sylvain; Zwaan, Martin

    2015-03-01

    We use ALMA observations to derive mass, length, and time scales associated with NGC 253's nuclear starburst. This region forms ~2 M ⊙ yr-1 of stars and resembles other starbursts in ratios of gas, dense gas, and star formation tracers, with star formation consuming the gas reservoir at a normalized rate 10 times higher than in normal galaxy disks. We present new ~35 pc resolution observations of bulk gas tracers (CO), high critical density transitions (HCN, HCO+, and CS), and their isotopologues. The starburst is fueled by a highly inclined distribution of dense gas with vertical extent factor implied by our cloud calculations is approximately Galactic, contrasting with results showing a low value for the whole starburst region. The contrast provides resolved support for the idea of mixed molecular ISM phases in starburst galaxies.

  1. ALMA Explores How Supermassive Black Holes Talk to Their Galaxies

    Science.gov (United States)

    Kohler, Susanna

    2017-03-01

    We believe that supermassive black holes evolve in tandem with their host galaxies but how do the two communicate? Observations from the Atacama Large Millimeter/submillimeter Array (ALMA) have revealed new clues about how a monster black hole talks to its galaxy.A Hubble image of the central galaxy in the Phoenix cluster. [Adapted from Russell et al. 2017]Observing FeedbackActive galactic nuclei (AGN), the highly luminous centers of some galaxies, are thought to radiate due to active accretion onto the supermassive black hole at their center.Its long been suspected that the radiation and outflowing material which often takes the form of enormous bipolar radio jets emitted into the surroundings influence the AGNs host galaxy, affecting star formation rates and the evolution of the galaxy. This AGN feedback has been alternately suggested to trigger star formation, quench it, and truncate the growth of massive galaxies.The details of this feedback process, however, have yet to be thoroughly understood in part because its difficult to obtain detailed observations of how AGN outflows interact with the galactic gas surrounding them. Now, a team of scientists led by Helen Russell (Institute of Astronomy in Cambridge, UK) has published the results of a new, high-resolution look at the gas in a massive galaxy in the center of the Phoenix cluster.Many Uses for FuelThe Phoenix cluster, a nearby (z = 0.596) group of star-forming galaxies, is the most luminous X-ray cluster known. The central galaxy in the cluster is especially active: it hosts a starburst of 500800 solar masses per year, the largest starburst found in any galaxy below a redshift of z= 1.The star formation in this galaxy is sustained by an enormous reservoir of cold molecular gas roughly 20 billion solar masses worth. This reservoir also powers the galaxys central black hole, fueling powerful radio jets that extend into the hot atmosphere of the galaxy and blow a giant bubble into the hot gas at each pole.ALMA

  2. 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.

  3. 67-116 GHz optics development for ALMA band 2-3 receivers

    Science.gov (United States)

    Yagoubov, Pavel; Gonzalez, A.; Tapia, V.; Reyes, N.; Mena, F. P.; Nesti, R.; Cuttaia, F.; Ricciardi, S.; Villa, F.

    2016-12-01

    In this paper we report the first results of the optical components development and the overall optical design for a wideband receiver to simultaneously cover ALMA bands 2 and 3. Two types of feed horns and OMTs have been designed to couple to the ALMA telescope beam using a modified Fresnel lens. Both types of hardware have been manufactured and tested in a near field beam scanner. The measured beam patterns and optical efficiencies are in good agreement with simulations.

  4. ALMA / porten til det kolde, støvede og fjerne univers

    DEFF Research Database (Denmark)

    Linden-Vørnle, Michael

    2012-01-01

    I det nordlige Chile er det enorme ALMA-teleskop ved at tage form, men allerede nu giver det enestående astronomiske øje os et helt nyt syn på universet.......I det nordlige Chile er det enorme ALMA-teleskop ved at tage form, men allerede nu giver det enestående astronomiske øje os et helt nyt syn på universet....

  5. 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 $\

  6. 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.

  7. 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.

  8. 33 CFR 127.317 - Declaration of inspection.

    Science.gov (United States)

    2010-07-01

    ... (CONTINUED) WATERFRONT FACILITIES WATERFRONT FACILITIES HANDLING LIQUEFIED NATURAL GAS AND LIQUEFIED HAZARDOUS GAS Waterfront Facilities Handling Liquefied Natural Gas Operations § 127.317 Declaration...

  9. ALMA Deep Field in SSA22: Source Catalog and Number Counts

    CERN Document Server

    Umehata, Hideki; Kohno, Kotaro; Ivison, R J; Smail, Ian; Hatsukade, Bunyo; Nakanishi, Kouichiro; Kato, Yuta; Ikarashi, Soh; Matsuda, Yuichi; Fujimoto, Seiji; Iono, Daisuke; Lee, Minju; Steidel, Charles C; Saito, Tomoki; Alexander, D M; Yun, Min S; Kubo, Mariko

    2016-01-01

    We present results from a deep 2'x3' (comoving scale of 3.7 Mpc x 5.5 Mpc at z=3) survey at 1.1 mm taken with the Atacama Large Millimeter/submillimeter Array (ALMA) in the SSA22 field. We observe the core region of a z = 3.09 protocluster, achieving a typical rms sensitivity of 60 micro-Jy/beam at a spatial resolution of 0".7. We detect 18 robust ALMA sources at a signal-to-noise ratio (SNR) > 5. Comparison between the ALMA map and a 1.1 mm map taken with the AzTEC camera on the Atacama Submillimeter Telescope Experiment (ASTE) indicates that three submillimeter sources discovered by the AzTEC/ASTE survey are resolved into eight individual submillimeter galaxies (SMGs) by ALMA. At least ten of our 18 ALMA SMGs have spectroscopic redshifts of z = 3.09, placing them in the protocluster. This shows that a number of dusty starburst galaxies are forming simultaneously in the core of the protocluster. The nine brightest ALMA SMGs with SNR > 10 have a median intrinsic angular size of 0".32+0".13-0".06 (2.4+1.0-0.4 ...

  10. 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.

  11. Declarative flow control for distributed instrumentation

    Energy Technology Data Exchange (ETDEWEB)

    Parvin, Bahram; Taylor, John; Fontenay, Gerald; Callahan, Daniel

    2001-06-01

    We have developed a 'microscopy channel' to advertise a unique set of on-line scientific instruments and to let users join a particular session, perform an experiment, collaborate with other users, and collect data for further analysis. The channel is a collaborative problem solving environment (CPSE) that allows for both synchronous and asynchronous collaboration, as well as flow control for enhanced scalability. The flow control is a declarative feature that enhances software functionality at the experimental scale. Our testbed includes several unique electron and optical microscopes with applications ranging from material science to cell biology. We have built a system that leverages current commercial CORBA services, Web Servers, and flow control specifications to meet diverse requirements for microscopy and experimental protocols. In this context, we have defined and enhanced Instrument Services (IS), Exchange Services (ES), Computational Services (CS), and Declarative Services (DS) that sit on top of CORBA and its enabling services (naming, trading, security, and notification) IS provides a layer of abstraction for controlling any type of microscope. ES provides a common set of utilities for information management and transaction. CS provides the analytical capabilities needed for online microscopy. DS provides mechanisms for flow control for improving the dynamic behavior of the system.

  12. APLIKASI SISTEM INFORMASI PERTANAHAN BERDASARKAN JENIS-JENIS HAK ATAS TANAH DI KANTOR PERTANAHAN KOTA SURABAYA II (STUDI KASUS KELURAHAN GENTENG, KECAMATAN GENTENG, SURABAYA

    Directory of Open Access Journals (Sweden)

    Ery Abdul Baary

    2015-02-01

    Full Text Available Di Kantor Pertanahan Kota Surabaya II, sistem informasi pertanahan belum diterapkan, jadi untuk melaksanakan tugasnya hanya menggunakan sebatas peta digital, maka dari itu perlu adanya sistem informasi pertanahan yang terpadu dan mutakhir untuk mendukung dan mengoptimalkan pengelolaan sistem informasi pertanahan di Kota Surabaya II.Pada penelitian ini akan dilakukan pembuatan sistem informasi pertanahan berdasarkan jenis hak atas tanah dengan menggunakan peta digital Kelurahan Genteng, Kecamatan Genteng, Surabaya skala 1:1000, citra Quickbird 2010, database mengenai bidang tanah dan data hasil survey. Pengolahan data menggunakan software utama Autodesk Land Dekstop 2009, ArcGIS 9.3. Pembuatan program aplikasi menggunakan software Visual Basic 6.0 yang dilengkapi dengan software tambahan MapObject 2.2.Dari hasil pembuatan Sistem informasi pertanahan di Kelurahan Genteng, Program ini mampu mengidentifikasi informasi bidang tanah mengenai jenis hak atas tanah yang meliputi 224 bidang tanah yang terdiri dari 132 bidang tanah atas hak guna bangunan, 89 bidang tanah atas hak milik, dan 3 bidang tanah atas hak pakai, serta dilengkapi dengan buku panduan sehingga dapat digunakan untuk membantu dalam pengambilan kebijakan dalam rencana pelaksanaan program inventarisasi penguasaan, pemilikan, penggunaan, dan pemanfaatan tanah.

  13. Demonstrating A New Census of INfrared Galaxies with ALMA (DANCING-ALMA). I. FIR Size and Luminosity Relation at z = 0-6

    OpenAIRE

    Fujimoto, Seiji; Ouchi, Masami; Shibuya, Takatoshi; Nagai, Hiroshi

    2017-01-01

    We present the large statistics of the galaxy effective radius in the rest-frame far-infrared (FIR) wavelength Re(FIR) obtained from 1258 deep Atacama Large Millimeter/submillimeter Array (ALMA) 1-mm band maps that are open for public by 2016 December. Our ALMA sample consists of 736 sources at z=0-6 that typically have the star-formation rate of ~50-1000 M$_{\\odot}$/yr and the stellar mass of ~10$^{10}$-10$^{11.5}$ M$_{\\odot}$. We homogeneously derive Re(FIR) and FIR luminosity L_FIR of our ...

  14. POLA PEMBERIAN KORTIKOSTEROID PADA PASIEN ISPA BAGIAN ATAS DI PUSKESMAS SUKASADA II PADA BULAN MEI – JUNI 2014

    Directory of Open Access Journals (Sweden)

    Adi Yulianto

    2015-06-01

    Full Text Available ISPA merupakan penyakit yang umum dan global di masyarakat. Pada pusat layanan primer seperti di Puskesmas Sukasada II, angka kunjungan pasien ISPA tercatat sebanyak 3,091 pasien pada tahun 2013 dan tercatat sebanyak 1,452 pasien di periode Januari - Juni 2014. Penelitian ini bertujuan untuk mengetahui pola pemberian kortikosteroid pada pasien ISPA bagian atas dan indikasi pemberiannya. Kriteria pasien dalam penelitian adalah pasien rawat jalan yang terdiagnosis ISPA bagian atas yang tercatat di Puskesmas Sukasada II pada Mei – Juni 2014. Penelitian menggunakan metode studi deskriprif cross-sectional menggunakan pengumpulan data sekunder yang berasal dari register dan rekam medis pasien ISPA bagian atas yang berobat di Puskesmas Sukasada II. Karakteristik berdasarkan umur pasien ISPA di Puskesmas Sukasada II adalah balita (46,5%. Berdasarkan jenis kelamin, prevalensi tertinggi terdapat pada jenis kelamin laki-laki (52,8% dan berdasarkan letak desa, tertinggi di Desa Pancasari (54,2%. Berdasarkan tanda dan gejala keluhan demam (21,4%, batuk (20,4%, pilek (14,8%, bersin (14,8%, sekret hidung (14,8%, sakit tenggorok (7,1%, dan sakit kepala (6,7%. Diagnosis ISPA bagian atas dibagi menjadi sinusitis (8,3%, common cold (11,1%, rinitis (13,9%, tonsilitis (25,0%, dan faringitis (41,7%. Pemberian kortikosteroid pada pasien ISPA mencapai 27,1% dengan kortikosteroid yang digunakan adalah prednison (15,3% dan deksametason (11,8%. Pemberian kortikosteroid berdasarkan gejala dan tanda klinis pada pasien ISPA sudah sesuai berdasarkan penelitian yang telah dilakukan akan tetapi belum ada pedoman indikasi pemberian kortikosteroid yang pasti pada pasien ISPA. Pemberian kortikosteroid pada pasien ISPA berdasarkan diagnosis meliputi, tonsillitis (41,6%, faringitis (26,7%, rinitis (25%, common cold (18,9%, dan sinusitis (0%. Pemberian kortikosteroid pada pasien infeksi, termasuk ISPA adalah kontraindikasi kecuali pada pasien sepsis bakteri gram negatif dan

  15. 50 CFR 14.63 - Export declaration requirements.

    Science.gov (United States)

    2010-10-01

    ... PLANTS IMPORTATION, EXPORTATION, AND TRANSPORTATION OF WILDLIFE Wildlife Declarations § 14.63 Export... Declaration for Importation or Exportation of Fish or Wildlife (Form 3-177) signed by the exporter, or the exporter's agent, shall be filed with the Service prior to the export of any wildlife at the port...

  16. 47 CFR 2.906 - Declaration of Conformity.

    Science.gov (United States)

    2010-10-01

    ... 47 Telecommunication 1 2010-10-01 2010-10-01 false Declaration of Conformity. 2.906 Section 2.906... Conformity. (a) A Declaration of Conformity is a procedure where the responsible party, as defined in § 2.909... of Conformity attaches to all items subsequently marketed by the responsible party which...

  17. 76 FR 9231 - New Customs Declarations Label Requirements

    Science.gov (United States)

    2011-02-17

    ... 111 New Customs Declarations Label Requirements AGENCY: Postal Service\\TM\\. ACTION: Final rule..., Domestic Mail Manual (DMM ) 608.2.4 to require all mailpieces containing goods that enter the Customs Territory of the United States (CTUS), from outside the CTUS, to bear a customs declaration...

  18. 13 CFR 123.3 - How are disaster declarations made?

    Science.gov (United States)

    2010-01-01

    ... Overview § 123.3 How are disaster declarations made? (a) There are five ways in which disaster declarations... lower, and, as a direct result of such physical damage, 25 percent or more of the work force in their... that at least five small business concerns in a disaster area have suffered substantial economic...

  19. 28 CFR 8.8 - Advertisement and declaration of forfeiture.

    Science.gov (United States)

    2010-07-01

    ... 28 Judicial Administration 1 2010-07-01 2010-07-01 false Advertisement and declaration of forfeiture. 8.8 Section 8.8 Judicial Administration DEPARTMENT OF JUSTICE FBI FORFEITURE AUTHORITY FOR CERTAIN STATUTES § 8.8 Advertisement and declaration of forfeiture. (a) The notice required by...

  20. From Paper Based Clinical Practice Guidelines to Declarative Workflow Management

    DEFF Research Database (Denmark)

    Lyng, Karen Marie; Hildebrandt, Thomas; Mukkamala, Raghava Rao

    2009-01-01

    a sub workflow can be described in a declarative workflow management system: the Resultmaker Online Consultant (ROC). The example demonstrates that declarative primitives allow to naturally extend the paper based flowchart to an executable model without introducing a complex cyclic control flow graph....

  1. 9 CFR 93.322 - Declaration for horses.

    Science.gov (United States)

    2010-01-01

    ... 9 Animals and Animal Products 1 2010-01-01 2010-01-01 false Declaration for horses. 93.322 Section... FOR MEANS OF CONVEYANCE AND SHIPPING CONTAINERS Horses Mexico 18 § 93.322 Declaration for horses. For all horses offered for importation from Mexico, the importer or his or her agent shall present...

  2. 19 CFR 148.111 - Written declaration for unaccompanied articles.

    Science.gov (United States)

    2010-04-01

    ... 19 Customs Duties 2 2010-04-01 2010-04-01 false Written declaration for unaccompanied articles... of the United States § 148.111 Written declaration for unaccompanied articles. The baggage... covers articles which do not accompany him and: (a) The articles are entitled to free entry under the...

  3. Language Support for Declarative Future Commitments

    CERN Document Server

    Harrison, William

    2011-01-01

    Sequential programming and work-flow programming are two useful, but radically different, ways of describing computational processing. Of the two, it is sequential programming that we teach all programmers and support by programming languages, whether in procedural, objectoriented, or functional paradigms. We teach workflow as a secondary style of problem decomposition for use in special situations, like distributed or networked processing. Both styles offer complementary advantages, but the fact that they employ radically different models for ownership of continuations interferes with our ability to integrate them in a way that allows them to be taught and used in a single programming language. This paper describes a programming language construct, declarative future commitments, that permit better integration of the two.

  4. POLA PEMBERIAN ANTIBIOTIK PADA PASIEN ISPA BAGIAN ATAS DI PUSKESMAS SUKASADA II PADA BULAN MEI – JUNI 2014

    Directory of Open Access Journals (Sweden)

    Hermawan Hermawan

    2015-01-01

    Full Text Available ISPA merupakan masalah global kesehatan masyarakat dengan prevalensi dan beban biaya kesehatan yang tinggi. Di Puskesmas Sukasada II, ISPA merupakan penyakit terbanyak yang datang ke puskesmas Sukasada II sebesar 3,091 pasien pada tahun 2013 dan 1,452 pasien dari bulan Januari - Juni 2014. Tujuan penelitian ini adalah untuk mengetahui pola pemberian antibiotik pada pasien ISPA bagian atas rawat jalan di wilayah kerja Puskesmas Sukasada II pada bulan Mei – Juni 2014. Metode penelitian yang digunakan adalah studi deskriprif cross-sectional dengan cara pengumpulan data sekunder register dan rekam medis pasien ISPA yang berkunjung di Puskesmas Sukasada II. Karakteristik sebaran kategori umur penderita ISPA di wilayah kerja Puskesmas Sukasada II sebagian besar merupakan balita (46,5% dengan prevalensi tertinggi pada jenis kelamin laki-laki (52,8% dan tertinggi di Desa Pancasari (54,2%. Diagnosis ISPA diklasifikasikan dengan sebaran  faringitis (41,7%, tonsilitis (25,0% , rinitis (13,9% , common cold ( 11,1% dan sinusitis (8,3%. Pemberian antibiotik pada pasien ISPA mencapai 93,8% dengan antibiotik terbanyak yang digunakan adalah kotrimoksasol, penoksimetil penisilin, amoksisilin dan siprofloksasin. Pemberian antibiotik berdasarkan diagnosis pasien ISPA bagian atas masih ada yang belum sesuai dengan pedoman pengobatan yang ditetapkan.  

  5. PERSEPSI GURU DAN SISWA TERHADAP PENGGUNAAN BAHASA INGGRIS DI KELAS BILINGUAL DI SEKOLAH MENENGAH ATAS BERSTATUS RSBI DI BALI

    Directory of Open Access Journals (Sweden)

    Luh Putu Artini

    2011-11-01

    Full Text Available Abstract: Perception of the teachers and Students Towards the Use of English in Bilingual Senior High School Classes This study aimed at analyzing teachers and students' perceptions towards the use of English in the teaching and learning process in bilingual classes in piloted international standard senior high schools in Bali. The number of subject was 100, comprising 4 school principals, 16 teachers and 80 students; utilizing questionnaires, observation and interview. The data which were analyzed descriptively revealed that there was a consistency between teachers and students' perceptions about the advantage and effectiveness of the use of English as a media of instruction in the classroom. Abstrak: Persepsi Guru dan Siswa terhadap Penggunaan Bahasa Inggris di Kelas Bilingual di Seko­lah Menengah Atas Berstatus RSBI di Bali. Penelitian ini bertujuan untuk menganalisis persepsi guru dan siswa terhadap penggunaan bahasa Inggris dalam proses belajar mengajar di kelas bilingual di SMA RSBI di Bali. Subjek penelitian adalah 100 orang yang terdiri atas 4 orang kepala sekolah, 16 orang guru, dan 80 orang siswa dengan menggunakan kuesioner, observasi, dan wawancara. Data yang dianalisis se­cara deskriptif kualitatif menunjukkan adanya konsistensi persepsi guru dan siswa tentang manfaat dan efektifitas penggunaan bahasa Inggris sebagai bahasa pengantar di kelas.

  6. ARTIKULASI POLITIK PEREMPUAN MADURA (Studi atas Hambatan Kultural dan Tafsir Agama pada Partisipasi Politik Perempuan di Sumenep

    Directory of Open Access Journals (Sweden)

    Abd. Warits

    2012-02-01

    Full Text Available Abstrak:Dalam sejarah manusia, perempuan sering mendapatkan tempat kedudukan di bawah laki-laki. Dalam pandangan berbagai agama, perempuan mendapatkan diskriminasi, menganalisasi yang dibentuk oleh ketidakadilan struktural sebagai akibat dari pandang bias gender di masyarakat. Dalam komunikasi mungkin sering ditunjukkan adanya ketidakadilan di atas, akibat penfsiran yang bias gender yang dilakukan atas sebagian tokoh agama. Akibatnya perempuan tidak dapat mengaktualisasikan sejarah dan perannya di ranah publik termasuk di dalamnya di wilayah politik praktis.  Untuk Masyarakat Sumenep yang relegius, di mana fatwâ agama (fatwâ kiai menjadi referensi dan pijakan utama setiap kali menyelesaikan persoalan sosial kemasyarakatan, maka akan sangat tepat bila pembebasan perempuan dari diskriminasi dimulai dengan membangun tafsîr yang ramah perempuanKata kunci:Perempuan, Madura, dan politikAbstract:In the history of mankind, woman is always placed under man. Even form the view of any religions, woman is descriminated and marginalized as a result of structural unjustice and gender bias. The unfair treatment has been justified from the gender bias interpretation commited by certain religious scholars. Thus, women are able to actualize their history and roles in public domain including practical practice domain. In Sumenep context, constructing a kind interpretation on woman role must be a brilliant choice since Sumenep people are religious and they hold on the religion fatwa (a binding ruling tightly.Key words:Perempuan, Madura, dan politic

  7. 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.

  8. 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

  9. PENDUGAAN CADANGAN KARBON ATAS PERMUKAAN TANAH PADA TIPE PENGGUNAAN LAHAN DUSUNG DI PULAU AMBON

    Directory of Open Access Journals (Sweden)

    Aryanto Boreel

    2016-11-01

    Full Text Available Tujuan penelitian ini untuk mengestimasi jumlah kandungan karbon (carbon stock dan jumlah serapan karbon pada tipe penggunaan lahan dusung di Pulau Ambon. Penelitian dilakukan dalam bulan April – November 2015, dan difokuskan untuk mendapatkan data dan informasi jumlah kandungan dan serapan karbon pada tipe penggunaan lahan dusung di pulau Ambon dengan lokasi pengambilan data ditentukan secara purposive sampling berdasarkan peta tutupan lahan (land cover pulau ambon dan nilai spektral (NDVI citra landsat 8. Pembuatan dem plot untuk pengukuran teresterial dilakukan pada desa Hative Besar dan Desa Soya dengan mempertimbangakan kondisi fisik wilayah dan keberadaan aktivitas masyarakat yang memiliki dusung. Pengukuran dan pendugaan cadangan karbon dalam penelitian ini mengacu pada Standar Nasional Indonesia nomor 7724 tahun 2011. Hasil analisis secara spasial berdasarkan nilai indeks vegetasi (NDVI di lokasi penelitian diperoleh 3 (tiga kelas kerapatan vegetasi, yakni kerapatan jarang (-1£NDVI<0,32, kerapatan sedang (0,32 < NDVI < 0,42 dan kerapatan tinggi/lebat (0,42atas permukaan tanah pada tipe pengunaan lahan dusung di Desa Hative Besar adalah 43,9989 ton/ha dengan rata-rata serapan CO2 sebesar 161,4760 ton/ha, sedangkan di Desa Soya rata-rata potensi karbon tersimpan adalah 40,6447 ton/ha dengan rata-rata serapan CO2 sebesar 149,1659 ton/ha The aim of the research is to estimate the amount of carbon (carbon stock and total carbon uptake on land use types Dusung on the island of Ambon. The study was conducted in the months of April to November 2015, and focused on obtaining data and information on the amount of content and carbon uptake on land use types Dusung on the island of Ambon with the location of the data determined by purposive sampling based land cover maps (land cover island of Ambon and spectral value (NDVI Landsat imagery 8. Making dem plot for

  10. Faktor-faktor yang Memengaruhi Insiden Miopia Pada Siswa Sekolah Menengah Atas di Kota Padang

    Directory of Open Access Journals (Sweden)

    Martga Bella Rahimi

    2015-09-01

    Full Text Available Abstrak Miopia merupakan kelainan refraktif yang paling banyak ditemukan di dunia. Hampir 90% miopia terjadi di negara berkembang. Berbagai faktor diduga berhubungan dengan insiden miopia seperti jenis kelamin, indeks masa tubuh (IMT, aktivitas dekat (dengan atau tanpa layar, aktivitas jauh (dengan atau tanpa layar, sosioekonomi, orangtua menderita miopia, serta riwayat kelahiran prematur atau berat badan lahir rendah (BBLR. Tujuan penelitian ini adalah menentukan hubungan antara faktor-faktor tersebut dan insiden miopia pada siswa Sekolah Menengah Atas(SMA di Kota Padang. Penelitian dilakukan pada siswa SMA di Kota Padang yang berusia 15-17 tahun, dengan desain case-control study, population based dengan jumlah sampel 140 orang, yang terdiri dari 70 orang untuk kelompok kontrol dan 70 orang untuk kelompok kasus. Dikelompokkan setelah menguji ketajaman visus. Kemudian dilanjutkan dengan pengukuran tinggi badan, berat badan, serta pengisian kuesioner. Selanjutnya, data diolah dengan uji statistik chi-square. Aktivitas dekat dengan layar, IMT dan aktivitas jauh dengan layar merupakan faktor dominan yang memengaruhi insiden miopia pada siswa SMA di Kota Padang. Dibuktikan juga bahwa jenis kelamin, sosioekonomi, orangtua menderita miopia, riwayat lahir prematur ataupun BBLR tidak  memengaruhi insiden miopia. Kesimpulan penelitian ini adalah ada hubungan positif antara faktor risiko dengan insiden miopia.Kata kunci: miopia, faktor risiko, pelajar SMAAbstract Myopia is the most common refractive error in the world. Almost 90% of myopia patients are found in the developing countries. There are several factors suspected to be related to the incidence of myopia, such as gender, body mass index, close-range activities (with or without screen, distance activities (with or without screen, socioeconomic state, history of myopia in parents, and history of prematurity or low birth weight. The objective of this study was to determine the relation of those

  11. AGREGAÇÃO DE VALOR A FRUTOS DE ATA ATRAVÉS DO DESENVOLVIMENTO DE NÉCTAR MISTO DE MARACUJÁ (PASSIFLORA EDULIS SIMS E ATA (ANNONA SQUAMOSA L.

    Directory of Open Access Journals (Sweden)

    MARESSA CALDEIRA MORZELLE

    2010-03-01

    Full Text Available

    Atualmente, observa-se uma nova tendência no consumo alimentar, com uma demanda cada vez maior por alimentos com elevadas propriedades nutricionais e funcionais. Pelo crescente interesse em produtos saudáveis, houve uma expansão na agroindústria de frutas, principalmente aquelas com características sensoriais exóticas. Sendo assim, o presente trabalho teve como objetivo geral desenvolver um néctar misto, à base dos frutos de ata e maracujá, que atendesse ao requerimento de aceitação pelo público; considerando assim essa mistura de frutas uma saída para um melhor aproveitamento tecnológico dessas matérias-primas com agregação de valor. Avaliou-se as características sensoriais, microbiológicas e físico-químicas: pH, acidez total titulável e sólidos solúveis. Foram estudadas duas formulações de néctar variando o teor de polpa (50% polpa de ata e 50% polpa de maracujá e 30% polpa de maracujá com 70% polpa de ata de cada fruta, as quais foram avaliadas por 100 consumidores utilizando a escala hedônica estruturada de nove pontos para a aceitabilidade e escala estruturada de cinco pontos de intenção de compra. Os resultados de aceitação global não diferiram signifi cativamente (p< 0,05, sendo que as duas formulações foram bem aceitas com média de aceitação 8, equivalente ao termo “gostei muito”, o que sugere alto potencial para mercado.

  12. Dinamika Islam Politik Pasca Orde baru: Kajian Psikoanalisi Lacanian atas Hubungan KAMMI dan PKS

    Directory of Open Access Journals (Sweden)

    Ahmad Rizky Mardhatillah Umar

    2014-07-01

    Full Text Available This article aims at analyzing the relations between student movement andpolitical party in post-reform era of Indonesia. KAMMI, a prominent Islamiststudent movement in Indonesia, often associated with PKS (Prosperous JusticeParty in terms of identity and political practices. It has created ‘independencedilemma’ for KAMMI because since its first Congress in 1998, this studentorganization has declared ‘independent from all political forces’. This article,using Lacanian psychoanalytical tradition, exposes the forms of KAMMI’ssubjectivity and PKS interpellation that enable this political party to dominateKAMMI’s articulatory practices. The interpellation process is supported withthe projection of fantacy, emotion, and mirror in the development of KAMMIsince 1998 until present. It leads to PKS creating the KAMMI identity andthus made KAMMI’s articulatory practices identical with this party. However,there were several attempts to dislocate the hegemony through several internalreform movements. These attempts, although made contribution to internaldynamics within KAMMI, were unable to create alternative discourse dueto several limits of those movements. The case of KAMMI can be a model toexplain how other student movements develop and relate to political parties inIndonesian post-reform.

  13. 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.

  14. ALMA observations of the kinematics and chemistry of disc formation

    CERN Document Server

    Lindberg, Johan E; Brinch, Christian; Haugbølle, Troels; Bergin, Edwin A; Harsono, Daniel; Persson, Magnus V; Visser, Ruud; Yamamoto, Satoshi

    2014-01-01

    Context: The R CrA cloud hosts a handful of Class 0/I low-mass young stellar objects. The chemistry and physics at scales $>500$ AU in this cloud are dominated by the irradiation from the nearby Herbig Be star R CrA. The luminous large-scale emission makes it necessary to use high-resolution spectral imaging to study the chemistry and dynamics of the inner envelopes and discs of the protostars. Aims: We aim to better understand the structure of the inner regions of these protostars and in particular the interplay between the chemistry and the presence of discs. Methods: Using Atacama Large Millimeter/submillimeter Array (ALMA) high-resolution spectral imaging interferometry observations, we study the molecular line and dust continuum emission at submillimetre wavelengths. Results: We detect dust continuum emission from four circumstellar discs around Class 0/I objects within the R CrA cloud. Towards IRS7B we detect C$^{17}$O emission showing a rotation curve consistent with a Keplerian disc with a well-define...

  15. 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...

  16. Overall performance of the ALMA antenna during solar observation

    Science.gov (United States)

    Busatta, A.; Brunelli, A.; Rampini, F.; Marchiori, G.

    2012-09-01

    The Atacama Large Millimeter Array (ALMA) consists of a large number of 12m diameter antennas that will operate up to 950GHz. The antenna must meet all primary operational performances also during solar observation. When the antenna is pointing directly the sun or when the sun is close to the boresight axis, the solar power concentrated by the mirrors cannot damage any part of the antenna. When the antenna is pointing toward the sun, the power absorbed by a black body positioned in the secondary focal area shall not exceed 0.3 W/cm2. To achieve these requirements, the primary surface of the antenna has a suitable surface scattering treatment. The same thing was done for the surface of the subreflector. Specific tests were performed on the panels surface and secondary mirror during the prototype and production phase in order to optimize the best behaviour. A particular care must be applied in the control of the secondary area, where the entire solar power spectrum, from the UV to the infrared, reflected by the primary mirror, can contribute to overheat reflecting areas support structures. In this report we provide a series of analysis and results obtained during the solar observation.

  17. 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.

  18. 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.

  19. 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...

  20. Exploring No-SQL alternatives for ALMA monitoring system

    Science.gov (United States)

    Shen, Tzu-Chiang; Soto, Ruben; Merino, Patricio; Peña, Leonel; Bartsch, Marcelo; Aguirre, Alvaro; Ibsen, Jorge

    2014-07-01

    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. This paper describes the experience gained after several years working with the monitoring system, which has a strong requirement of collecting and storing up to 150K variables with a highest sampling rate of 20.8 kHz. The original design was built on top of a cluster of relational database server and network attached storage with fiber channel interface. As the number of monitoring points increases with the number of antennas included in the array, the current monitoring system demonstrated to be able to handle the increased data rate in the collection and storage area (only one month of data), but the data query interface showed serious performance degradation. A solution based on no-SQL platform was explored as an alternative to the current long-term storage system. Among several alternatives, mongoDB has been selected. In the data flow, intermediate cache servers based on Redis were introduced to allow faster streaming of the most recently acquired data to web based charts and applications for online data analysis.

  1. 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...

  2. Detection of Infall in the Protostar B335 with ALMA

    CERN Document Server

    Evans, Neal J; Lee, Jeong-Eun; Jørgensen, Jes K; Choi, Minho; Myers, Philip C; Mardones, Diego

    2015-01-01

    Observations of the isolated globule B335 with ALMA have yielded absorption features against the continuum that are redshifted from the systemic velocity in both HCN and HCO$^+$ lines. These features provide unambiguous evidence for infall toward a central luminosity source. Previously developed models of inside-out collapse can match the observed line profiles of HCN and HCO$^+$ averaged over the central 50 AU. At the new distance of 100 pc, the inferred infall radius is 0.012 pc, the mass infall rate is $3 \\times 10^{-6}$ solar masses per year, the age is 50,000 years, and the accumulated mass in the central zone is 0.15 solar masses, most of which must be in the star or in parts of a disk that are opaque at 0.8 mm. The continuum detection indicates an optically thin mass (gas and dust) of only $7.5\\times 10^{-4}$ solar masses in the central region, consistent with only a very small disk mass.

  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. 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...

  5. 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...

  6. 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...

  7. ALMA and VLA Observations of Proplyd Candidates near Sgr A*

    Science.gov (United States)

    Yusef-Zadeh, Farhad; Cotton, William D.; Royster, Marc; Kunneriath, Devaky; Wardle, M.; Roberts, D. A.; Wootten, Al; Schoedel, R.

    2017-01-01

    Using the VLA, we recently detected a large number of protoplanetary disk (proplyd) candidates lying within a couple of light years of the massive black hole Sgr A*. The bow-shock appearance of proplyd candidates point toward the young massive stars located near Sgr A*. Similar to Orion proplyds, the strong UV radiation from the cluster of massive stars at the Galactic center is expected to photoevaporate and photoionize the circumstellar disks around young, low mass stars, thus allowing detection of the ionized outflows. To confirm this interpretation, ALMA observations detect millimeter emission at 226 GHz from five proplyd candidates that had been detected at 44 and 34 GHz with the VLA. We determine the mass of protoplanetary disks from cool dust emission. These measurements show the presence of on-going star formation with the implication that gas clouds can survive near Sgr A* and the relative importance of high vs low-mass star formation in the strong tidal and radiation fields of the Galactic center.

  8. ALMA Reveals the Molecular Medium Fueling the Nearest Nuclear Starburst

    CERN Document Server

    Leroy, Adam K; Ostriker, Eve C; Rosolowsky, Erik; Walter, Fabian; Warren, Steven R; Meyer, Jennifer Donovan; Hodge, Jacqueline; Meier, David S; Ott, Jürgen; Sandstrom, Karin; Schruba, Andreas; Veilleux, Sylvain; Zwaan, Martin

    2014-01-01

    We use ALMA to derive the mass, length, and time scales associated with the nuclear starburst in NGC 253. This region forms ~2 M_sun/yr of stars and resembles other starbursts in scaling relations, with star formation consuming the gas reservoir 10 times faster than in galaxy disks. We present observations of CO, the high effective density transitions HCN(1-0), HCO+(1-0), CS(2-1), and their isotopologues. We identify ten clouds that appear as peaks in line emission and enhancements in the HCN-to-CO ratio. These clouds are massive (~10^7 M_sun) structures with sizes (~30 pc) similar to GMCs in other systems. Compared to disk galaxy GMCs, they show high line widths (~20-40 km/s) given their size, with implied Mach numbers ~90. The clouds also show high surface (~6,000 M_sun/pc^2) and volume densities (n_H2~2,000 cm^-3). Given these, self-gravity can explain the line widths. This short free fall time (~0.7 Myr) helps explain the more efficient star formation in NGC 253. We also consider the starburst region as a...

  9. 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...

  10. 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...

  11. ALMA Measurements of Circumstellar Material in the GQ Lup System

    CERN Document Server

    MacGregor, Meredith A; Czekala, Ian; Andrews, Sean M; Dai, Y Sophia; Herczeg, Gregory J; Kratter, Kaitlin M; Kraus, Adam L; Ricci, Luca; Testi, Leonardo

    2016-01-01

    We present ALMA observations of the GQ Lup system, a young Sun-like star with a substellar mass companion in a wide-separation orbit. These observations of 870 $\\mu$m continuum and CO J=3-2 line emission with beam size $\\sim0.3''$ ($\\sim45$ AU) resolve the disk of dust and gas surrounding the primary star, GQ Lup A, and provide deep limits on any circumplanetary disk surrounding the companion, GQ Lup b. The circumprimary dust disk is compact with a FWHM of $59\\pm12$ AU, while the gas has a larger extent with a characteristic radius of $46.5\\pm1.8$ AU. By forward-modeling the velocity field of the circumprimary disk based on the CO emission, we constrain the mass of GQ Lup A to be $M_* = (1.03\\pm0.05)*(d/156\\text{ pc})$ $M_\\odot$, where $d$ is a known distance, and determine that we view the disk at an inclination angle of $60.5^\\circ\\pm0.5^\\circ$ and a position angle of $346^\\circ \\pm1^\\circ$. The $3\\sigma$ upper limit on the 870 $\\mu$m flux density of any circumplanetary disk associated with GQ Lup b of $<...

  12. Signs of Early-Stage Disk Growth Revealed with ALMA

    CERN Document Server

    Yen, Hsi-Wei; Takakuwa, Shigehisa; Krasnopolsky, Ruben; Ohashi, Nagayoshi; Aso, Yusuke

    2016-01-01

    We present ALMA 1.3 mm continuum, 12CO, C18O, and SO data for the Class 0 protostars, Lupus 3 MMS, IRAS 15398-3559, and IRAS 16253-2429 at resolutions of ~100 AU. By measuring a rotational profile in C18O, a 100 AU Keplerian disk around a 0.3 Msun protostar is observed in Lupus 3 MMS. No 100 AU Keplerian disks are observed in IRAS 15398-3559 and IRAS 16253-2429. Nevertheless, embedded compact (<30 AU) continuum components are detected. The C18O emission in IRAS 15398-3559 shows signatures of infall with a constant angular momentum. IRAS 16253-2429 exhibits signatures of infall and rotation, but its rotational profile is unresolved. By fitting the C18O data with our kinematic models, the protostellar masses and the disk radii are inferred to be 0.01 Msun and 20 AU in IRAS 15398-3559, and 0.03 Msun and 6 AU in IRAS 16253-2429. By comparing the specific angular momentum profiles from 10,000 to 100 AU in 8 Class 0 and I protostars, we find that the evolution of envelope rotation can be described with conventio...

  13. 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 ...

  14. An ALMA Survey of Planet Forming Disks in Rho Ophiuchus

    Science.gov (United States)

    Guilfoil Cox, Erin; Looney, Leslie; Harris, Robert J.; Dong, Jiayin; Segura-Cox, Dominique; Tobin, John J.; Sadavoy, Sarah; Li, Zhi-Yun; Dunham, Michael; Perez, Laura M.; Chandler, Claire J.; Kratter, Kaitlin M.; Melis, Carl; Chiang, Hsin-Fang

    2017-01-01

    Relatively evolved (~ 1 Myr old) protostars with little residual natal envelope, but massive disks, are commonly assumed to be the sites of ongoing planet formation. Critical to our study of these objects is information about the available mass reservior and dust structure, as they directly tie in to how much mass is available for planets as well as the modes of planet formation that occur (i.e., core-accretion vs. gravitational instability). Millimeter-wave observations provide this critical information as continuum emission is relatively optically thin, allowing for mass estimates, and the availability of high-resolution interferometry, allowing structure constraints. We present high-resolution observations of the population of Class II protostars in the Rho-Ophiuchus cloud (d ~ 130 pc). Our survey observed ~50 of these older protostars at 870µm, using the Atacama Large Millimeter/submillimeter Array (ALMA). Out of these sources, there are ~10 transition disks, where we see a ring of dust emission surrounding the central protostar -- indicative of ongoing planet formation -- as well as many binary systems. Both of these stages have implications for star and planet formation. We present results from both 1-D and 2-D disk modeling, where we try to understand disk substructure that might indicate on-going planet formation, in particular, transition disk cavities, disk gaps, and asymmetries in the dust emission.

  15. The ALMA View of Dense Molecular Gas in 30 Doradus

    Science.gov (United States)

    Bittle, Lauren E.; Indebetouw, Remy; Brogan, Crystal L.; Hunter, Todd R.; Leroy, Adam

    2017-01-01

    At a distance of 50 kpc, the 30 Doradus region within the Large Magellanic Cloud (LMC) hosts several sites of star formation including R136, a starburst region home to dozens of evolved O stars. The intense radiation from R136 creates an extreme environment for nearby star formation in such a low-metallicity, low mass galaxy. We have targeted a star-forming region ~15 pc away from R136 within 30 Doradus using the Atacama Large Millimeter/submillimeter Array (ALMA) to map the molecular gas to study the sites of star formation. We are conducting a clump-by-clump analysis of the intensities and line ratios of dense gas (HCO+, HCN, CS, H13CO+, H13CN) and diffuse gas (CO, 13CO, C18O) tracers at sub-parsec resolution. We identify and characterize ~100 molecular clumps within the region. With the observed molecular species, we aim to determine the physical conditions of each clump (e.g. size, internal turbulence, molecular abundance). We compare the intensities and line ratios to non-LTE Radex model grids of the excitation temperature, molecular column density, and volume density of the H2 collider to determine the physical excitation conditions within the clumps. We compare these properties of each clump to both associated and embedded star formation properties to quantify the relative importance of internal feedback from the star formation itself versus external feedback processes from R136 and determine which process dominates in this region.

  16. 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.

  17. ALMA Observations of the HH 46/47 Molecular Outflow

    CERN Document Server

    Arce, Hector G; Corder, Stuartt; Garay, Guido; Noriega-Crespo, Alberto; Raga, Alejandro C; Cabrit, Sylvie

    2013-01-01

    The morphology, kinematics and entrainment mechanism of the HH 46/47 molecular outflow were studied using new ALMA Cycle 0 observations. Results show that the blue and red lobes are strikingly different. We argue that these differences are partly due to contrasting ambient densities that result in different wind components having a distinct effect on the entrained gas in each lobe. A 29-point mosaic, covering the two lobes at an angular resolution of about 3", detected outflow emission at much higher velocities than previous observations, resulting in significantly higher estimates of the outflow momentum and kinetic energy than previous studies of this source, using the CO(1-0) line. The morphology and the kinematics of the gas in the blue lobe are consistent with models of outflow entrainment by a wide-angle wind, and a simple model may describe the observed structures in the position-velocity diagram and the integrated intensity map. The red lobe exhibits a more complex structure, and there is evidence tha...

  18. ALMA reveals VYCMa's sub-mm maser and dust distribution

    CERN Document Server

    Richards, A M S; Humphreys, E M; Vlahakis, C; Vlemmings, W; Baudry, A; De Beck, E; Decin, L; Etoka, S; Gray, M D; Harper, G M; Hunter, T R; Kervella, P; Kerschbaum, F; McDonald, I; Melnick, G; Muller, S; Neufeld, D; O'Gorman, E; Parfenov, S Yu; Peck, A B; Shinnaga, H; Sobolev, A M; Testi, L; Uscanga, L; Wootten, A; Yates, J A; Zijlstra, A

    2014-01-01

    Cool, evolved stars have copious, enriched winds. The structure of these winds and the way they are accelerated is not well known. We need to improve our understanding by studying the dynamics from the pulsating stellar surface to about 10 stellar radii, where radiation pressure on dust is fully effective. Some red supergiants have highly asymmetric nebulae, implicating additional forces. We retrieved ALMA Science Verification data providing images of sub-mm line and continuum emission from VY CMa. This enables us to locate water masers with milli-arcsec precision and resolve the dusty continuum. The 658-, 321- and 325-GHz masers lie in irregular, thick shells at increasing distances from the centre of expansion. For the first time this is confirmed as the stellar position, coinciding with a compact peak offset to the NW of the brightest continuum emission. The maser shells (and dust formation zone) overlap but avoid each other on tens-au scales. Their distribution is broadly consistent with excitation models...

  19. 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.

  20. 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.

  1. 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...

  2. No cortés la soga que me ata a tu alma. L’inquiétante étrangeté de « Tetro »

    Directory of Open Access Journals (Sweden)

    Carmen Bernand

    2010-01-01

    Full Text Available Je ne suis qu’une simple spectatrice, attirée dans la salle parisienne qui passait « Tetro », par une critique sévère parue dans un hebdomadaire français que j’affectionne. En lisant ce que le journaliste reprochait au cinéaste, je compris qu’il ne s’agissait pas d’une œuvre convenue, voire commerciale, et je me décidai à voir le film de toute urgence. J’en fus bouleversée du début à la fin et, ne voulant pas quitter cet univers coppolien trop vite, je livre ici quelques commentaires inspiré...

  3. From Declarative to Imperative UML/OCL Operation Specifications

    Science.gov (United States)

    Cabot, Jordi

    An information system maintains a representation of the state of the domain in its Information Base (IB). The state of the IB changes due to the execution of the operations defined in the behavioral schema. There are two different approaches for specifying the effect of an operation: the imperative and the declarative approaches. In conceptual modeling, the declarative approach is preferable since it allows a more abstract and concise definition of the operation effect and conceals all implementation issues. Nevertheless, in order to execute the conceptual schema, declarative specifications must be transformed into equivalent imperative ones.

  4. Monitoring harm reduction in European prisons via the Dublin Declaration.

    Science.gov (United States)

    Lines, Rick; Stöver, Heino; Donochoe, Martin C; Lazarus, Jeffrey V

    2009-01-01

    The Dublin Declaration on Partnership to fight HIV/AIDS in Europe and Central Asia is the key policy document on HIV/AIDS in the European Region as a whole Among the Declaration's 33 actions for governments are many that apply to prison populations. Based upon an analysis of these commitments, and a review of the current status of states in meeting those targets, it is clear that the scale-up of HIV/AIDS prevention and treatment programmes and services in prisons lags far behind what is needed, what is available outside of prisons, and what is mandated within the Declaration itself.

  5. Reflexiones sobre problemas de biología reproductiva del mango Ataúlfo en el Soconusco, Chiapas

    Directory of Open Access Journals (Sweden)

    Malc R. Gehrke Vélez

    2013-05-01

    Full Text Available El Soconusco, en el Estado mexicano de Chiapas, es una región de gran potencial agroproductivo. Sin embargo, desde los años 50 del siglo pasado, sus ecosistemas han sido constantemente devastados por tecnologías inapropiadas de producción agropecuaria, lo cual ha afectado negativamente su productividad y muchos de los cultivos que parecían promisorios han quedado descartados por incosteabilidad. Hoy surge una nueva posibilidad de desarrollo sostenible con la plantación de mango “Ataúlfo”, una variedad de origen local que ha sido desarrollada hasta llegar a ser uno de los cultivos más importantes de la región desde el punto de vista de productividad y rentabilidad. El fruto de esta variedad presenta características morfológicas y organolépticas muy deseables y, a escala mundial, se está posicionando como una fruta de alta calidad y deseabilidad en el mercado. Sin embargo, después de más de cuarenta años de desarrollo, los huertos de Ataúlfo están siendo afectados por problemas de biología reproductiva que están causando falta de prendimiento y aborto de flores y frutas. En huertos donde se llegaron a producir más de 15 toneladas de fruta por hectárea, ahora se cosechan menos de cuatro. Se hizo una revisión exhaustiva de trabajos de investigación en diversas partes del mundo lo cual genera una hipótesis sobre las posibles causas del fenómeno del “mango niño” y del mango “partenocárpico”, así como de la caída prematura de flores y frutos. Se discute también la posibilidad de una incompatibilidad alo- y endogámica de la variedad Ataúlfo. Todos estos fenómenos parecen estar relacionados con cambios en la temperatura y precipitación en el área, causados por prácticas inapropiadas de cultivo en épocas anteriores y por fenómenos globales, como la incidencia de huracanes y el calentamiento global.  Finalmente, se hacen recomendaciones para desarrollar líneas de investigación que resuelvan estos

  6. Penatalaksanaan impaksi caninus permanen rahang atas dengan surgical exposure (The management of impacted permanent canine with surgical exposure

    Directory of Open Access Journals (Sweden)

    Syeh Brata Wijaya

    2014-09-01

    Full Text Available Background: Impacted tooth is often unidentified because there is no symptom. It is found when patient is examined by dentist. The maxillary canine should be retained for strength masticatory function, esthetics and child development. Purpose: The article was aimed to report treatment options of impacted canine in the 13 years old child. Case: Thirteen years-old girl came to the Universitas Gadjah Mada Dental Hospital with complaints of the upper right permanent canine had not erupted, with no history of pain. Periapical radiograph showed the impacted position of tooth #13 mesioangular. The shift sketch technique radiograph showed the impacted canine located at the palatal site. Case management: surgical exposure the upper right maxillary canine was done, followed by orthodontic treatment to direct tooth position into occlusal line. Fixed orthodontic appliance used was Roth bracket with straight wire technique. After surgery and orthodontic treatment, #13 was in normal occlusion. Conclusion: The surgical exposure followed by orthodontic treatment could be done successfully with special consideration to the patient’s age, the dental space, location of dental crowns, dental inclination, the apical root form of impacted tooth and patient cooperation.Latar belakang: Terjadinya gigi impaksi biasanya diketahui setelah melakukan pemeriksaan ke dokter gigi karena jarang menimbulkan keluhan. Gigi caninus rahang atas sebaiknya dipertahankan untuk kekuatan fungsi pengunyahan, estetik dan tumbuh kembang anak. Tujuan: Artikel ini bertujuan untuk melaporkan perawatan impaksi gigi kaninus atas pada anak 13 tahun. Kasus: Anak perempuan usia 13 tahun datang ke Rumah sakit Gigi dan Mulut Fakultas Kedokteran Gigi Universitas Gadjah Mada dengan keluhan gigi kaninus permanen kanan atas yang belum erupsi, tanpa ada riwayat sakit di area tersebut. Hasil radiografi periapikal menunjukkan posisi gigi #13 impaksi mesioangular. Hasil radiografi dengan teknik shift

  7. 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...

  8. 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.

  9. 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.

  10. 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.

  11. Magnetic fields in protoplanetary discs: from MHD simulations to ALMA observations

    Science.gov (United States)

    Bertrang, G. H.-M.; Flock, M.; Wolf, S.

    2017-01-01

    Magnetic fields significantly influence the evolution of protoplanetary discs 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 discs, 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 Atacama Large Millimeter/submillimeter Array (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 disc regions.

  12. Observing Turbulent Fragmentation In Simulations: Through the Looking Glass of CARMA and ALMA

    Science.gov (United States)

    Offner, Stella; Capodilupo, J.; Schnee, S.; Goodman, A.

    2012-01-01

    We use the CASA software package to synthetically observe binaries forming as a result of turbulent fragmentation in a radiation-hydrodynamic simulation of a collapsing molecular cloud. By following the evolution of such pairs beginning in the prestellar core stage, we are able to make predictions about the feasibility of observing such fragmentation using the Combined Array for Research in Millimeter-wave Astronomy (CARMA) and the Atacama Large Millimeter/submillimeter Array (ALMA). We find that while intermediate ALMA configurations may potentially resolve structure with one fourth the integration time of CARMA, both instruments only marginally resolve sub-structure within 25 kyr of the onset of gravitational collapse. In addition, interferometric spatial filtering significantly reduces traces of filamentary gas morphology on < 0.1 pc scales. Thus, even with the improved sub-arcsecond resolution of ALMA, constraining stellar multiplicity at the earliest stages of star formation will be challenging.

  13. Declarative Terrain Modeling for Military Training Games

    Directory of Open Access Journals (Sweden)

    Ruben M. Smelik

    2010-01-01

    Full Text Available Military training instructors increasingly often employ computer games to train soldiers in all sorts of skills and tactics. One of the difficulties instructors face when using games as a training tool is the creation of suitable content, including scenarios, entities, and corresponding terrain models. Terrain plays a key role in many military training games, as for example, in our case game Tactical Air Defense. However, current manual terrain editors are both too complex and too time-consuming to be useful for instructors; automatic terrain generation methods show a lot of potential, but still lack user control and intuitive editing capabilities. We present a novel way for instructors to model terrain for their training games: instead of constructing a terrain model using complex modeling tools, instructors can declare the required properties of their terrain using an advanced sketching interface. Our framework integrates terrain generation methods and manages dependencies between terrain features in order to automatically create a complete 3D terrain model that matches the sketch. With our framework, instructors can easily design a large variety of terrain models that meet their training requirements.

  14. Streamlining environmental product declarations: a stage model

    Science.gov (United States)

    Lefebvre, Elisabeth; Lefebvre, Louis A.; Talbot, Stephane; Le Hen, Gael

    2001-02-01

    General public environmental awareness and education is increasing, therefore stimulating the demand for reliable, objective and comparable information about products' environmental performances. The recently published standard series ISO 14040 and ISO 14025 are normalizing the preparation of Environmental Product Declarations (EPDs) containing comprehensive information relevant to a product's environmental impact during its life cycle. So far, only a few environmentally leading manufacturing organizations have experimented the preparation of EPDs (mostly from Europe), demonstrating its great potential as a marketing weapon. However the preparation of EPDs is a complex process, requiring collection and analysis of massive amounts of information coming from disparate sources (suppliers, sub-contractors, etc.). In a foreseeable future, the streamlining of the EPD preparation process will require product manufacturers to adapt their information systems (ERP, MES, SCADA) in order to make them capable of gathering, and transmitting the appropriate environmental information. It also requires strong functional integration all along the product supply chain in order to ensure that all the information is made available in a standardized and timely manner. The goal of the present paper is two fold: first to propose a transitional model towards green supply chain management and EPD preparation; second to identify key technologies and methodologies allowing to streamline the EPD process and subsequently the transition toward sustainable product development

  15. Protoplanetary disks in Taurus: Probing the role of multiplicity with ALMA observations

    Science.gov (United States)

    Laos, Stefan; Akeson, Rachel L.; Jensen, Eric L. N.

    2017-01-01

    We present results from an ALMA survey of single and multiple young systems in Taurus designed to probe how protoplanetary disk mass depends on both stellar mass and multiplicity. In observations taken in Cycles 0 and 2, we detect over 25 new disks. These detections include disks around stars in both single and multiple systems and are predominantly around lower mass stars with spectral types from M0 to M6. Combined with previous detections, these observations reveal a wide range of disk mass around both primary and companion stars, and allow us to test if the relation previously seen between disk and stellar mass continues at lower stellar masses. We find that within multiple systems the ratio of primary to secondary stellar mass is not correlated with the ratio of primary to secondary disk mass. In some cases, the secondary star hosts the more massive disk, contrary to theoretical predictions. We will discuss the implications of these results for the process of planet formation in multiple systems.This work makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00150.S. and ADS/JAO.ALMA#2013.1.00105.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

  16. ALMA Deep Field in SSA22: Source Catalog and Number Counts

    Science.gov (United States)

    Umehata, Hideki; Tamura, Yoichi; Kohno, Kotaro; Ivison, R. J.; Smail, Ian; Hatsukade, Bunyo; Nakanishi, Kouichiro; Kato, Yuta; Ikarashi, Soh; Matsuda, Yuichi; Fujimoto, Seiji; Iono, Daisuke; Lee, Minju; Steidel, Charles C.; Saito, Tomoki; Alexander, D. M.; Yun, Min S.; Kubo, Mariko

    2017-01-01

    We present results from a deep 2‧ × 3‧ (comoving scale of 3.7 Mpc × 5.5 Mpc at z = 3) survey at 1.1 mm, taken with the Atacama Large Millimeter/submillimeter Array (ALMA) in the SSA22 field. We observe the core region of a z = 3.09 protocluster, achieving a typical rms sensitivity of 60 μJy beam‑1 at a spatial resolution of 0.″7. We detect 18 robust ALMA sources at a signal-to-noise ratio (S/N) > 5. Comparison between the ALMA map and a 1.1 mm map, taken with the AzTEC camera on the Atacama Submillimeter Telescope Experiment (ASTE), indicates that three submillimeter sources discovered by the AzTEC/ASTE survey are resolved into eight individual submillimeter galaxies (SMGs) by ALMA. At least 10 of our 18 ALMA SMGs have spectroscopic redshifts of z ≃ 3.09, placing them in the protocluster. This shows that a number of dusty starburst galaxies are forming simultaneously in the core of the protocluster. The nine brightest ALMA SMGs with S/N > 10 have a median intrinsic angular size of 0\\buildrel{\\prime\\prime}\\over{.} {32}-0.06+0.13 ({2.4}-0.4+1.0 physical kpc at z = 3.09), which is consistent with previous size measurements of SMGs in other fields. As expected, the source counts show a possible excess compared to the counts in the general fields at S1.1mm ≥ 1.0 mJy, due to the protocluster. Our contiguous mm mapping highlights the importance of large-scale structures on the formation of dusty starburst galaxies.

  17. Density functional theory study of ATA, BTAH, and BTAOH as copper corrosion inhibitors: adsorption onto Cu(111) from gas phase.

    Science.gov (United States)

    Kokalj, Anton; Peljhan, Sebastijan

    2010-09-21

    A low-coverage gas-phase adsorption of three corrosion inhibitors-3-amino-1,2,4-triazole (ATA), benzotriazole (BTAH), and 1-hydroxybenzotriazole (BTAOH)-on perfect Cu(111) surface has been studied and characterized using density functional theory calculations. We find that the molecules in neutral form chemisorb weakly to the perfect surface in an upright geometry. The strength of the chemisorption increases in the order BTAH BTA· with the adsorption energies of -1.65, -2.22, and -2.78 eV, respectively. This order is compatible with the trend of experimentally observed corrosion inhibition effectiveness on copper in near-neutral chloride solutions. Although the calculations are performed at the metal/vacuum interface, they provide enough insight to rationalize why in some experiments the BTAH was observed to be adsorbed with an upright geometry and in the others with parallel geometry.

  18. The Brussels Declaration: the need for change in asthma management

    DEFF Research Database (Denmark)

    Holgate, S.; Bisgaard, H.; Bjermer, L.

    2008-01-01

    Asthma is a highly prevalent condition across Europe and numerous guidelines have been developed to optimise management. However, asthma can be neither cured nor prevented, treatment choices are limited and many patients have poorly controlled or uncontrolled asthma. The Brussels Declaration on A...... reviews the evidence supporting the need for change in asthma management and summarises the ten key points contained in the Brussels Declaration Udgivelsesdato: 2008/12......Asthma is a highly prevalent condition across Europe and numerous guidelines have been developed to optimise management. However, asthma can be neither cured nor prevented, treatment choices are limited and many patients have poorly controlled or uncontrolled asthma. The Brussels Declaration...... on Asthma, sponsored by The Asthma, Allergy and Inflammation Research Charity, was developed to call attention to the shortfalls in asthma management and to urge European policy makers to recognise that asthma is a public health problem that should be a political priority. The Declaration urges recognition...

  19. 16 CFR 456.4 - Declaration of Commission Intent.

    Science.gov (United States)

    2010-01-01

    ... 16 Commercial Practices 1 2010-01-01 2010-01-01 false Declaration of Commission Intent. 456.4 Section 456.4 Commercial Practices FEDERAL TRADE COMMISSION TRADE REGULATION RULES OPHTHALMIC PRACTICE... ophthalmologist's or optometrist's prescription....

  20. 50 CFR 14.62 - Exceptions to import declaration requirements.

    Science.gov (United States)

    2010-10-01

    ... reasonably practicable using the best available taxonomic information, and must declare the country of origin... the household effects of persons moving their residence to the United States, except that an...

  1. Thematic development of declarations on Sustainability in Higher Education

    DEFF Research Database (Denmark)

    Grindsted, Thomas Skou; Holm, Tove

    2012-01-01

    of the international SHE literature reveals no study that deals specifically with the interaction between declarations developed by the university sector and declarations developed by governmental and intergovernmental institutions. An analysis of this type can give us important insights in what themes these parties...... think should be given top priority in order to develop a sustainable society. Hence, the article addresses the following issues: (1) a thematic analysis of the relation between declarations developed by the university sector and those developed by governmental and intergovernmental institutions; (2......) an analysis of themes the two types of declarations might have in common; and if so (3) an analysis of how they have developed during the past decade. The article finds four new themes that previous research has not identified, and shows how the valuation of nature is under reconfiguration in higher education...

  2. New procedure for declaring accidents resulting in bodily injuries

    CERN Multimedia

    2014-01-01

    The HR Department would like to remind members of personnel that, according to Administrative Circular No. 14 (Rev. 3), entitled “Protection of members of the personnel against the financial consequences of illness, accident and incapacity for work”, accidents resulting in bodily injuries and presumed to be of an occupational nature should, under normal circumstances, be declared within 10 working days of the accident having occurred, accompanied by a medical certificate. In an effort to streamline procedures, occupational accident declarations should be made via EDH using the “declaration of occupational accident” electronic form. For the declaration of non-occupational accidents resulting in bodily injuries of members of the CERN Health Insurance Scheme (CHIS), a new paper form has been elaborated that can be downloaded from the CHIS website and is also available from the UNIQA Helpdesk in the Main Building. If you encounter technical difficulties with these new ...

  3. Working, declarative and procedural memory in specific language impairment

    DEFF Research Database (Denmark)

    Lum, J. A. G.; Conti-Ramsden, G.; Page, D.

    2012-01-01

    in turn explain the grammar problems in the disorder. The abnormalities are also likely to lead to problems with other, non-procedural functions, such as working memory, that rely at least partly on the affected brain structures. In contrast, declarative memory is expected to remain largely intact...... at declarative memory for visual information, and at declarative memory in the verbal domain after controlling for working memory and language. Visuo-spatial short-term memory was intact, whereas verbal working memory was impaired, even when language deficits were held constant. Correlation analyses showed...... neither visuo-spatial nor verbal working memory was associated with either lexical or grammatical abilities in either the SLI or TD children. Declarative memory correlated with lexical abilities in both groups of children. Finally, grammatical abilities were associated with procedural memory in the TD...

  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. O impossível regime das paixões da alma

    Directory of Open Access Journals (Sweden)

    Paulo José Carvalho da Silva

    2008-03-01

    Full Text Available Este artigo pretende analisar o lugar das paixões da alma no ideal de saúde conforme a obra Âncora medicinal para conservar a vida em saúde (1721 do português Francisco da Fonseca Henriques, médico do rei D. João V. As paixões da alma eram consideradas um dos aspectos determinantes do regime de saúde. Elas eram relacionadas ao excesso, aos limites extremos do corpo e à morte.

  6. ALMA Resolves the Nuclear Disks of Arp 220

    Science.gov (United States)

    Scoville, Nick; Murchikova, Lena; Walter, Fabian; Vlahakis, Catherine; Koda, Jin; Vanden Bout, Paul; 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

    2017-02-01

    We present 90 mas (37 pc) resolution ALMA imaging of Arp 220 in the CO (1-0) line and continuum at λ =2.6 {mm}. The internal gas distribution and kinematics of both galactic nuclei are well resolved for the first time. In the west nucleus, the major gas and dust emission extends out to 0.″2 radius (74 pc); the central resolution element shows a strong peak in the dust emission but a factor of 3 dip in the CO line emission. In this nucleus, the dust is apparently optically thick ({τ }2.6{mm}∼ 1) at λ =2.6 {mm} with a dust brightness temperature of ∼147 K. The column of interstellar matter at this nucleus is {N}{{H}2}≥slant 2× {10}26 cm‑2, corresponding to ∼900 gr cm‑2. The east nucleus is more elongated with radial extent 0.″3 or ∼111 pc. The derived kinematics of the nuclear disks provide a good fit to the line profiles, yielding the emissivity distributions, the rotation curves, and velocity dispersions. In the west nucleus, there is evidence of a central Keplerian component requiring a central mass of 8 × 108 {M}ȯ . The intrinsic widths of the emission lines are {{Δ }}v({FWHM})=250 (west) and 120 (east) km s‑1. Given the very short dissipation timescales for turbulence (≲105 years), we suggest that the line widths may be due to semicoherent motions within the nuclear disks. The symmetry of the nuclear disk structures is impressive, implying the merger timescale is significantly longer than the rotation period of the disks.

  7. Signs of Early-stage Disk Growth Revealed with ALMA

    Science.gov (United States)

    Yen, Hsi-Wei; Koch, Patrick M.; Takakuwa, Shigehisa; Krasnopolsky, Ruben; Ohashi, Nagayoshi; Aso, Yusuke

    2017-01-01

    We present ALMA 1.3 mm continuum, 12CO, C18O, and SO data for the Class 0 protostars Lupus 3 MMS, IRAS 15398‑3559, and IRAS 16253‑2429 at resolutions of ∼100 au. By measuring a rotational profile in C18O, a 100 au Keplerian disk around a 0.3 M⊙ protostar is observed in Lupus 3 MMS. No 100 au Keplerian disks are observed in IRAS 15398‑3559 and IRAS 16253‑2429. Nevertheless, embedded compact (<30 au) continuum components are detected. The C18O emission in IRAS 15398‑3559 shows signatures of infall with a constant angular momentum. IRAS 16253‑2429 exhibits signatures of infall and rotation, but its rotational profile is unresolved. By fitting the C18O data with our kinematic models, the protostellar masses and the disk radii are inferred to be 0.01 M⊙ and 20 au in IRAS 15398‑3559, and 0.03 M⊙ and 6 au in IRAS 16253‑2429. By comparing the specific angular momentum profiles from 10,000 au to 100 au in eight Class 0 and I protostars, we find that the evolution of envelope rotation can be described with conventional inside-out collapse models. In comparison with a sample of 18 protostars with known disk radii, our results reveal signs of disk growth, with the disk radius increasing as {{M}* }0.8+/- 0.14 or {t}1.09+/- 0.37 in the Class 0 stage, where M* is the protostellar mass and t is the age. The disk growth rate slows down in the Class I stage. In addition, we find a hint that the mass accretion rate declines as {t}-0.26+/- 0.04 from the Class 0 to the Class I stages.

  8. ALMA OBSERVATIONS OF THE HH 46/47 MOLECULAR OUTFLOW

    Energy Technology Data Exchange (ETDEWEB)

    Arce, Hector G. [Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101 (United States); Mardones, Diego; Garay, Guido [Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago (Chile); Corder, Stuartt A. [Joint ALMA Observatory, Av. Alonso de Cordova 3107, Vitacura, Santiago (Chile); Noriega-Crespo, Alberto [Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125 (United States); Raga, Alejandro C. [Instituto de Ciencias Nucleares, UNAM, Ap. 70-543, 04510 D.F. (Mexico)

    2013-09-01

    The morphology, kinematics, and entrainment mechanism of the HH 46/47 molecular outflow were studied using new ALMA Cycle 0 observations. Results show that the blue and red lobes are strikingly different. We argue that these differences are partly due to contrasting ambient densities that result in different wind components having a distinct effect on the entrained gas in each lobe. A 29 point mosaic, covering the two lobes at an angular resolution of about 3'', detected outflow emission at much higher velocities than previous observations, resulting in significantly higher estimates of the outflow momentum and kinetic energy than previous studies of this source, using the CO(1-0) line. The morphology and the kinematics of the gas in the blue lobe are consistent with models of outflow entrainment by a wide-angle wind, and a simple model describes the observed structures in the position-velocity diagram and the velocity-integrated intensity maps. The red lobe exhibits a more complex structure, and there is evidence that this lobe is entrained by a wide-angle wind and a collimated episodic wind. Three major clumps along the outflow axis show velocity distribution consistent with prompt entrainment by different bow shocks formed by periodic mass ejection episodes which take place every few hundred years. Position-velocity cuts perpendicular to the outflow cavity show gradients where the velocity increases toward the outflow axis, inconsistent with outflow rotation. Additionally, we find evidence for the existence of a small outflow driven by a binary companion.

  9. The ALMA View of the OMC1 Explosion in Orion

    Science.gov (United States)

    Bally, John; Ginsburg, Adam; Arce, Hector; Eisner, Josh; Youngblood, Allison; Zapata, Luis; Zinnecker, Hans

    2017-03-01

    Most massive stars form in dense clusters where gravitational interactions with other stars may be common. The two nearest forming massive stars, the BN object and Source I, located behind the Orion Nebula, were ejected with velocities of ∼29 and ∼13 km s‑1 about 500 years ago by such interactions. This event generated an explosion in the gas. New ALMA observations show in unprecedented detail, a roughly spherically symmetric distribution of over a hundred 12CO J = 2‑1 streamers with velocities extending from V LSR = ‑150 to +145 km s‑1. The streamer radial velocities increase (or decrease) linearly with projected distance from the explosion center, forming a “Hubble Flow” confined to within 50″ of the explosion center. They point toward the high proper-motion, shock-excited H2 and [Fe ii] “fingertips” and lower-velocity CO in the H2 wakes comprising Orion's “fingers.” In some directions, the H2 “fingers” extend more than a factor of two farther from the ejection center than the CO streamers. Such deviations from spherical symmetry may be caused by ejecta running into dense gas or the dynamics of the N-body interaction that ejected the stars and produced the explosion. This ∼1048 erg event may have been powered by the release of gravitational potential energy associated with the formation of a compact binary or a protostellar merger. Orion may be the prototype for a new class of stellar explosiozn responsible for luminous infrared transients in nearby galaxies.

  10. "The Chennai declaration" - Indian doctors' fight against antimicrobial resistance

    OpenAIRE

    2013-01-01

    “The Chennai Declaration” is the result of the first ever joint meeting of medical societies in India addressing antibiotic resistance. The declaration is not a policy by itself, but a call for a national policy. The Declaration has looked into all major aspects of the problem of antimicrobial resistance, has suggested practical solutions, explained in detail the responsibility of each and every stakeholder.

  11. The world alliance against antibiotic resistance: consensus for a declaration.

    Science.gov (United States)

    Carlet, Jean

    2015-06-15

    Antibiotic resistance is increasing worldwide and has become a very important threat to public health. The overconsumption of antibiotics is the most important cause of this problem. We created a World Alliance Against Antibiotic Resistance (WAAAR), which now includes 720 people from 55 different countries and is supported by 145 medical societies or various groups. In June 2014, WAAAR launched a declaration against antibiotic resistance. This article describes the process and the content of this declaration.

  12. Analysis of declarations in distance based road toll schemes

    OpenAIRE

    Menzel, Gerhard

    2010-01-01

    The main focus of the master thesis lies on developing a methodology to analyse the accuracy of toll declarations within a satellite based toll system. This methodology employs two different approaches to determine reasons why Toll Service Providers (TSP) deliver toll declarations that show charge inaccuracies. Both approaches are carried out to analyse the results of the ARENA project’s field test which was held in April 2010 to test On Board Unit (OBU) solutions for toll collection. In part...

  13. Making it Politic(al: closing the Gap in a Generation: Health Equity Through Action on the Social Determinants of Health

    Directory of Open Access Journals (Sweden)

    Anne-Emanuelle Birn

    2009-09-01

    Full Text Available The anniversary of the publication of Closing the Gap in a Generation (CGG offers a moment to reflect on the report’s contributions and shortcomings, as well as to consider the political waters ahead. The issuance of CGG was not the first time the World Health Organization (WHO raised the problem of global inequalities in health. Numerous analysts and advocates have compared CGG to the 1978 Declaration of Alma-Ata. Some see CGG as a continuation of Alma-Ata; others malign it for paying insufficient attention to the principles, background documents, and lines of action proposed in the Alma-Ata declaration. We might understand the two reports as bookends to 30 years of brutal global capitalism, punctuated by the “lost decade” of the 1980s, the end of the Cold War, and, more recently, the implosion of global finance. This period saw the publication of two seminal neoliberal health manifestos –the World Bank’s 1993 World Development Report and the WHO’s 2002 Commission on Macroeconomics and Health report. Both feature the term “investing in health” in their title, conveying “a double meaning—investing [through “cost-effective,” narrow, technical interventions] to improve health, economic productivity, and poverty; and investing capital, especially private capital, as a route to private profit in the health sector.”

  14. Gender-Related Systematics in the NRAO and ALMA Proposal Review Processes

    CERN Document Server

    Lonsdale, Carol J; Hunt, Gareth

    2016-01-01

    A study has been made of the evidence for gender-related systematics in the proposal review processes for the four facilities operated by NRAO: the Jansky Very Large Array (JVLA; hereafter VLA), the Very Long Baseline Array (VLBA), the Green Bank Telescope (GBT) and the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile which is operated by NRAO/AUI in partnership with the European Southern Observatory (ESO) and the National Astronomical Observatories of Japan (NAOJ), in cooperation with the Republic of Chile. A significant gender-related effect is found in the proposal rankings in favor of men over women in the ALMA Proposal Review Processes (PRP) for ALMA Cycles 2-4, with reliability of 99.998% that the underlying rank distributions for male and female PIs are not the same. The effect is largest and most significant for ALMA Cycle 3. A similar overall result is found for the other three NRAO telescopes over proposal Semesters 2012A-2017A, but with lower reliability level overall (98.3%), and with ...

  15. 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.

  16. 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.

  17. 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

  18. Constraint on dust evolution processes in normal galaxies at $z>6$ detected by ALMA

    CERN Document Server

    Wang, W -C; Hou, K -C

    2016-01-01

    Recent ALMA observations of high-redshift normal galaxies have been providing a great opportunity to clarify the general origin of dust in the Universe, not biased to very bright special objects even at $z>6$. To clarify what constraint we can get for the dust enrichment in normal galaxies detected by ALMA, we use a theoretical model that includes major processes driving dust evolution in a galaxy; that is, dust condensation in stellar ejecta, dust growth by the accretion of gas-phase metals, and supernova destruction. Using the dust emission fluxes detected in two normal galaxies at $z>6$ by ALMA as a constraint, we can get the range of the time-scales (or efficiencies) of the above mentioned processes. We find that if we assume extremely high condensation efficiency in stellar ejecta ($f_{\\mathrm{in}} \\ga 0.5$), rapid dust enrichment by stellar sources in the early phase may be enough to explain the observed ALMA flux, unless dust destruction by supernovae in those galaxies is stronger than that in nearby g...

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

    Science.gov (United States)

    2005-12-01

    ESO, the European Organisation for Astronomical Research in the Southern Hemisphere, announced today that it has signed a contract with the consortium led by Alcatel Alenia Space and composed also of European Industrial Engineering (Italy) and MT Aerospace (Germany), to supply 25 antennas for the Atacama Large Millimeter Array (ALMA) project, along with an option for another seven antennas. The contract, worth 147 million euros, covers the design, manufacture, transport and on-site integration of the antennas. It is the largest contract ever signed in ground-based astronomy in Europe. The ALMA antennas present difficult technical challenges, since the antenna surface accuracy must be within 25 microns, the pointing accuracy within 0.6 arc seconds, and the antennas must be able to be moved between various stations on the ALMA site. This is especially remarkable since the antennas will be located outdoor in all weather conditions, without any protection. Moreover, the ALMA antennas can be pointed directly at the Sun. ALMA will have a collecting area of more than 5,600 square meters, allowing for unprecedented measurements of extremely faint objects. The signing ceremony took place on December 6, 2005 at ESO Headquarters in Garching, Germany. "This contract represents a major milestone. It allows us to move forward, together with our American and Japanese colleagues, in this very ambitious and unique project," said ESO's Director General, Dr. Catherine Cesarsky. "By building ALMA, we are giving European astronomers access to the world's leading submillimetre facility at the beginning of the next decade, thereby fulfilling Europe's desire to play a major role in this field of fundamental research." Pascale Sourisse, Chairman and CEO of Alcatel Alenia Space, said: "We would like to thank ESO for trusting us to take on this new challenge. We are bringing to the table not only our recognized expertise in antenna development, but also our long-standing experience in

  20. 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...

  1. 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.

  2. VizieR Online Data Catalog: ALMA Frontier Fields Survey. I. (Gonzalez-Lopez+, 2017)

    Science.gov (United States)

    Gonzalez-Lopez, J.; Bauer, F. E.; Romero-Canizales, C.; Kneissl, R.; Villard, E.; Carvajal, R.; Kim, S.; Laporte, N.; Anguita, T.; Aravena, M.; Bouwens, R. J.; Bradley, L.; Carrasco, M.; Demarco, R.; Ford, H.; Ibar, E.; Infante, L.; Messias, H.; Munoz Arancibia, A. M.; Nagar, N.; Padilla, N.; Treister, E.; Troncoso, P.; Zitrin, A.

    2016-10-01

    Tables presenting detection properties of mm sources behind the 3 Frontier Fields Abell 2744, MACSJ0416.1-2403 and MACSJ1149.5+2223. We present the properties of the detected sources in the ALMA observations. We also present the intrinsic properties of the sources in the image plane as well as the separations to the optical counterpart. (6 data files).

  3. 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

  4. Planet gaps in the dust layer of 3D protoplanetary disks. II. Observability with ALMA

    CERN Document Server

    Gonzalez, J -F; Maddison, S T; Ménard, F; Fouchet, L

    2012-01-01

    [Abridged] Aims: We provide predictions for ALMA observations of planet gaps that account for the specific spatial distribution of dust that results from consistent gas+dust dynamics. Methods: In a previous work, we ran full 3D, two-fluid Smoothed Particle Hydrodynamics (SPH) simulations of a planet embedded in a gas+dust T Tauri disk for different planet masses and grain sizes. In this work, the resulting dust distributions are passed to the Monte Carlo radiative transfer code MCFOST to construct synthetic images in the ALMA wavebands. We then use the ALMA simulator to produce images that include thermal and phase noise for a range of angular resolutions, wavelengths, and integration times, as well as for different inclinations, declinations and distances. We also produce images which assume that gas and dust are well mixed with a gas-to-dust ratio of 100 to compare with previous ALMA predictions, all made under this hypothesis. Results: Our findings clearly demonstrate the importance of correctly incorporat...

  5. What's New in CASA: 'tclean' and the Cycle 4 ALMA Pipeline

    Science.gov (United States)

    Donovan Meyer, Jennifer; CASA Development Team; ALMA Pipeline Working Group; NAASC Software Support Team

    2017-01-01

    CASA, the Common Astronomy Software Applications package, undergoes continuous development to support calibration and imaging of astronomical data at radio wavelengths for both single dish and interferometric telescopes. It is largely focused on supporting the post-processing needs of the next generation of radio telescopes such as ALMA and the JVLA. The most recent release of CASA, version 4.7, includes major upgrades in its imaging capabilities via the implementation of a task called 'tclean', which will eventually replace the current imaging task 'clean'. It has a new, more straightforward interface, allows more combinations of imaging algorithms, has a more flexible outlier approach, and includes algorithms for autoboxing. Further, the new 'tclean' task has been implemented in the Cycle 4 ALMA Interferometric Pipeline with great success; this pipeline software can be obtained bundled with CASA 4.7 at https://casa.nrao.edu/. A major goal of the ALMA project [and the National Radio Astronomical Observatory (NRAO)] is to provide Science-Ready Data Products to our user community, and the ALMA Cycle 4 Pipeline is a major step forward in that direction.

  6. 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

  7. 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

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

    Science.gov (United States)

    Bujarrabal, V.; Castro-Carrizo, A.; Alcolea, J.; Santander-García, M.; Van Winckel, H.; Sánchez Contreras, C.

    2016-01-01

    Aims We aim to study the rotating and expanding gas in the Red Rectangle, which is a well known object that recently left the asymptotic giant branch (AGB) phase. We analyze the properties of both components and the relation between them. Rotating disks have been very elusive in post-AGB nebulae, in which gas is almost always found to be in expansion. Methods We present new high-quality ALMA observations of 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 observations of lines of CO, CII, and CI, was performed using a sophisticated code that includes an accurate nonlocal treatment of radiative transfer in 2D. These observations (of low- and high-opacity lines requiring various degrees of excitation) and the corresponding modeling allowed us to deepen the analysis of the nebular properties. We also stress the uncertainties, particularly in the determination of the boundaries of the CO-rich gas and some properties of the outflow. Results 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 M⊙, and that of the CO-rich outflow is around ten 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 of disks around post-AGB stars typically range between 5000 and more than 20000 yr. The angular momentum of the disk is found to be high, ~ 9 M⊙ AU km s−1, which is comparable to that of the stellar system at present. Our observations of H13CN show a particularly wide velocity dispersion and indicate that this molecule is only abundant in the inner Keplerian disk, at

  9. 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

  10. 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

  11. 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

  12. 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.

  13. 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.

  14. 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.

  15. Dust evolution processes in normal galaxies at z > 6 detected by ALMA

    Science.gov (United States)

    Wang, Wei-Chen; Hirashita, Hiroyuki; Hou, Kuan-Chou

    2017-03-01

    Recent Atacama Large Millimetre/submillimetre Array (ALMA) observations of high-redshift normal galaxies have been providing a great opportunity to clarify the general origin of dust in the Universe, not biased to very bright special objects even at z > 6. To clarify what constraint we can get for the dust enrichment in normal galaxies detected by ALMA, we use a theoretical model that includes major processes driving dust evolution in a galaxy; that is, dust condensation in stellar ejecta, dust growth by the accretion of gas-phase metals and supernova destruction. Using the dust emission fluxes detected in two normal galaxies at z > 6 by ALMA as a constraint, we can get the range of the time-scales (or efficiencies) of the above mentioned processes. We find that if we assume extremely high-condensation efficiency in stellar ejecta (fin ≳ 0.5), rapid dust enrichment by stellar sources in the early phase may be enough to explain the observed ALMA flux, unless dust destruction by supernovae in those galaxies is stronger than that in nearby galaxies. If we assume a condensation efficiency expected from theoretical calculations (fin ≲ 0.1), strong dust growth (even stronger than assumed for nearby galaxies if they are metal-poor galaxies) is required. These results indicate that the normal galaxies detected by ALMA at z > 6 are biased to objects (i) with high dust condensation efficiency in stellar ejecta, (ii) with strong dust growth in very dense molecular clouds or (iii) with efficient dust growth because of fast metal enrichment up to solar metallicity. A measurement of metallicity is crucial to distinguish among these possibilities.

  16. 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.

  17. Gambaran Klinis dan Endoskopi Saluran Cerna Bagian Atas Pasien Dispepsia di Bagian RSUP Dr. M. Djamil Padang

    Directory of Open Access Journals (Sweden)

    Citra Yuriana Putri

    2016-08-01

    Full Text Available AbstrakDispepsia ialah suatu sindrom yang terdiri dari nyeri atau rasa tidak nyaman di ulu hati, kembung, mual, muntah, sendawa, rasa cepat kenyang, perut rasa penuh/begah. Salah satu alat diagnostik untuk dispepsia adalah endoskopi. Alat ini dapat menentukan jenis lesi dan lokasi lesi pada saluran cerna atas pasien dispepsia. Tujuan penelitian ini adalah mementukan frekuensi keluhan, derajat keluhan, insiden pasien dispepsia yang mengalami tanda bahaya berdasarkan jenis kelamin, faktor risiko dispepsia, diagnosis endoskopi  dan lokasi lesi saluran cerna atas pasien dispepsia. Desain penelitian ini adalah deskriptif observasional. Subjek penelitian  terdiri dari 54 orang pasien dispepsia yang dilakukan pemeriksaan esofagogastroduodenoskopi (EGD di RSUP Dr. M. Djamil dari Mei hingga Juni 2014. Data dikumpulkan dengan cara pengisian kuisioner melalui wawancara, pencatatan hasil pemeriksaan endoskopi. Hasil penelitian didapatkan bahwa keluhan terbanyak dari pasien dispepsia adalah nyeri ulu hati (98,15%, derajat keluhan terbanyak adalah derajat sedang (38,89%, insiden tanda bahaya lebih banyak pada pria, faktor risiko terbanyak adalah konsumsi makanan berlemak (92,59%, diagnosis endoskopi dispepsia terbanyak adalah gastritis (61,11%, lokasi lesi saluran cerna atas terbanyak adalah gaster (85,19%. Kata kunci: dispepsia, gambaran klinis, endoskopi AbstractDyspepsia is a syndrome that consist of pain or discomfort in upper abdominal, bloating, nausea, vomiting, bletching, early satiation  and post-prandial fullness. One of the diagnostic tool for dyspepsia was endoscopy. It can be determined the type and the location of upper gastrointestinal’s lesions in patient with dyspepsia. The objective of this study was to determined the frequency of dyspepsia’s complaints, the degree of dyspepsia’s complaints, the incident of alarm sign based on gender, the frequency of  risk factors of dyspepsia, endoscopic diagnosis and the location of upper

  18. Perawatan Satu\tKunjungan\tpada\tPremolar Pertama Atas Menggunakan Protaper Rotary dan Restorasi Resin Komposit

    Directory of Open Access Journals (Sweden)

    Sherli Diana

    2013-06-01

    Full Text Available Preparasi kemomekanik pada saluran akar meliputi instrumentasi mekanis dan irigasi antibakteri yang secara prinsip dapat langsung mengeliminasi mikroorganisme pada sistem saluran akar. sejak diperkenalkan pada tahun 1988, instrumen rotary nikel-titanium (niti telah digunakan secara umum dalam perawatan endodontik karena kemampuannya membentuk saluran akar dengan prosedur komplikasi yang minimal. Tujuan dari laporan kasus ini adalah untuk memaparkan perawatan saluran akar satu kunjungan menggunakan protaper rotary dan restorasi resin komposit gigi premolar. Penderita pria 21 tahun datang ke RSGM Prof. Soedomo UGM Yogyakarta mengeluhkan gigi belakang atas kiri yang berlubang tapi tidak sakit dan pasien ingin  dirawat.Gigi  Premolar satu atas  kiri terdapat kavitas disto oklusal dengan pulpa terbuka. Pemeriksan objektif pada gigi 24 sondasi, perkusi, palpasi, dan tes termal menunjukkan hasil negatif.Pemeriksaan radiografis tidak terdapat lesi, lamina dura tidak terputus dan saluran akar jelas dan lurus. Pada kasus ini dilakukan perawatan saluran akar dengan menggunakan ProTaper rotary ( X-Smart, Dentsply. Pasca perawatan saluran akar, gigi premolar satu atas kiri dilakukan tumpatan resin komposit kelas II.Hasil evaluasi klinik saat kontrol tidak ada keluhan rasa sakit, pemeriksaan objektif juga tidak ada rasa sakit, warna gigi serasi dengan warna gigi tetangga.prognosis pada kasus ini baik dan tidak ada keluhan. Kesimpulan paska perawatan saluran akar satu kunjungan dengan instrumenrotary, tidak terdapat keluhan.Penggunaan Instrumen rotary Nikel-Titanium (NiTi sangat flexible dengan prosedur komplikasi yang minimal, dan hemat waktu. One Visit Treatment of Upper Premolar Tooth Using Rotary Protaper and Composite Resin Restoration. Chemomechanical preparation for root canal including mechanic instrumentation and anti-bacterial irrigation principally could eliminate microorganisms in root canal system. Many instruments and techniques have been

  19. REMINDER : Changes in family situation are to be declared promptly

    CERN Multimedia

    HR Department

    2012-01-01

    All changes in the family situation of members of the personnel (employed or associated) have to be declared without delay and in writing to the Organization.   Among the changes that shall be notified within 30 calendar days of their occurrence, the most frequent ones are: • marriage; • divorce; • entering into a partnership officially registered in a Member State; • dissolution of such a partnership; • death of the spouse or partner; and • birth or death of a child. For more information, in particular on how to declare any of the above changes, please see the CERN Admin e-guide. In addition, any change to the health insurance situation, the income or retirement pension of the spouse or partner of any staff member or fellow also has to be declared to the Organization in writing within 30 calendar days of its occurrence. Such changes shall be declared using the EDH “CHIS Declaration of health insurance situation spouse/partner&...

  20. "Tres ataúdes blancos" de Antonio Ungar: juegos de falsedad y discursos de poder en la América Latina contemporánea

    Directory of Open Access Journals (Sweden)

    Felipe Cammaert

    2012-10-01

    Full Text Available Tres Ataúdes Blancos, novela del escritor colombiano Antonio Ungar, propone una lecturanovedosa de la realidad latinoamericana adoptando la forma de una sátira política. Esta novela escenificalos juegos de poder en Miranda, país imaginario que es una suma de los abusos del ejercicio político en elcontinente a lo largo de su historia. Para ello, elabora una profunda reflexión en torno a la falsedad y laalteridad. Tres ataúdes blancos plantea una relectura del canon latinoamericano donde la representación dela realidad política ocupa un lugar preponderante en el universo ficcional.

  1. New procedure for declaring changes in family and personal situation

    CERN Multimedia

    2014-01-01

    On taking up their appointment, Members of the Personnel (employed and associated) are required to provide official documents as evidence of their family situation. Any subsequent change in their personal situation, or that of their family members, must be declared in writing to the Organization within 30 calendar days.   As part of their efforts to simplify procedures, the Administrative Processes Section (DG-RPC-PA) and the HR and GS Departments have produced a new EDH form entitled “Change of family and personal situation", which must be used to declare the following changes: birth or adoption of a child; marriage; divorce; entry into a civil partnership officially registered in a Member State; dissolution of such a partnership; change of name; change of nationality or new nationality.   Members of the Personnel must create the form themselves and provide the information required for the type of declaration concerned, indicating, if applicable, any benefit...

  2. Not to declare dead someone still alive: Case reports

    Directory of Open Access Journals (Sweden)

    Anđelić Slađana

    2015-01-01

    Full Text Available Introduction. Diagnosing death represents an activity that carries a great deal of public responsibility for medical professionals and is continually exposed to the control of citizens and media. Although this is a taboo subject in medical circles, unfortunately in medical practice there are situations when the physician issues a death diagnosis form without even examining the person or for an already buried person. Such physician’s action is impermissible and it leads to the possibility of professional and criminal law punishment. Case Outline. By giving examples from practice, we wish to point out the need for exceptional caution when confirming and diagnosing death in order to diagnose the true, i.e. rule out apparent death and consequently avoid the mistake of declaring dead someone still alive. Conclusion. When confirming and declaring death, exceptional caution of the physician is necessary so as not to declare dead someone still alive!

  3. Hierarchical control of procedural and declarative category-learning systems.

    Science.gov (United States)

    Turner, Benjamin O; Crossley, Matthew J; Ashby, F Gregory

    2017-02-16

    Substantial evidence suggests that human category learning is governed by the interaction of multiple qualitatively distinct neural systems. In this view, procedural memory is used to learn stimulus-response associations, and declarative memory is used to apply explicit rules and test hypotheses about category membership. However, much less is known about the interaction between these systems: how is control passed between systems as they interact to influence motor resources? Here, we used fMRI to elucidate the neural correlates of switching between procedural and declarative categorization systems. We identified a key region of the cerebellum (left Crus I) whose activity was bidirectionally modulated depending on switch direction. We also identified regions of the default mode network (DMN) that were selectively connected to left Crus I during switching. We propose that the cerebellum-in coordination with the DMN-serves a critical role in passing control between procedural and declarative memory systems.

  4. Women and the Environment: Declaration Encourages Active Participation

    Institute of Scientific and Technical Information of China (English)

    JANE SHAW

    1994-01-01

    JUNE 5, 1994 has been mandated World Environment Day. On this day the first meeting on Women and the Environment in China was held in Beijing and the Declaration of Chinese Women on Environment was established. According to the declaration, environmental pollution and the destruction of the ecology have posed a serious threat to the survival of the human race. It has become a great issue of common concern. The functions of women in procreation and social development are directly affected by the deterioration of the environment. It is the common interest of the populations of the world to protect the environment. The declaration notes that Chinese women are greatly concerned about the environmental conditions of their

  5. A compensatory role for declarative memory in neurodevelopmental disorders

    Science.gov (United States)

    Ullman, Michael T.; Pullman, Mariel Y.

    2015-01-01

    Most research on neurodevelopmental disorders has focused on their abnormalities. However, what remains intact may also be important. Increasing evidence suggests that declarative memory, a critical learning and memory system in the brain, remains largely functional in a number of neurodevelopmental disorders. Because declarative memory remains functional, and because this system can learn and retain numerous types of information, functions, and tasks, it should be able to play compensatory roles for multiple types of impairments across the disorders. Here, we examine this hypothesis for specific language impairment, dyslexia, autism spectrum disorder, Tourette syndrome, and obsessive-compulsive disorder. We lay out specific predictions for the hypothesis and review existing behavioral, electrophysiological, and neuroimaging evidence. Overall, the evidence suggests that declarative memory indeed plays compensatory roles for a range of impairments across all five disorders. Finally, we discuss diagnostic, therapeutic and other implications. PMID:25597655

  6. Summary of ATA Interface Technology and Its Application in Ruggedized Product Design%ATA接口技术及在加固产品设计中的应用

    Institute of Scientific and Technical Information of China (English)

    陈威

    2013-01-01

    On the basis of introducing the development and specifications of the ATA Interface standards, this paper discusses the development trends of ATA Interface. During Power-on Self-TEST of BIOS, disk code information error will occur in ATA hard disk, resulting in entering system failed. The paper deeply analyzes this problem and gives out some solutions. In addition, because of the limitation of speed, parallel ATA interface can not satisfy user's demand during application. In view of the disadvantage of parallel ATA and the advantages and potential capability of serial ATA, the industry commonly considers serial ATA as the next generation interface of hard disk. At last, the serial ATA interface is introduced.%文章在介绍了ATA接口标准的发展由来和各个时期的技术指标的基础上,对ATA接口的发展趋势进行了探讨。BIOS自检时,ATA硬盘在实际应用中会出现硬盘标识信息错误,导致不能进入系统。文章深入分析了这种故障现象,并给出了相应的解决办法。另外,由于受到速度等方面的限制,并行ATA接口已经不能满足用户在使用过程中的要求。鉴于并行ATA接口的不足及串行ATA的优势及其潜在的技术发展能力,业内普遍认为Serial ATA将会取代并行ATA接口类型成为将来硬盘的主流接口类型。最后,本文对SATA接口进行了介绍。

  7. Diversity of flavin-binding monooxygenase genes (almA) in marine bacteria capable of degradation long-chain alkanes.

    Science.gov (United States)

    Wang, Wanpeng; Shao, Zongze

    2012-06-01

    Many bacteria have been reported as degraders of long-chain (LC) n-alkanes, but the mechanism is poorly understood. Flavin-binding monooxygenase (AlmA) was recently found to be involved in LC-alkane degradation in bacteria of the Acinetobacter and Alcanivorax genera. However, the diversity of this gene and the role it plays in other bacteria remains unclear. In this study, we surveyed the diversity of almA in marine bacteria and in bacteria found in oil-enrichment communities. To identify the presence of this gene, a pair of degenerate PCR primers were was designed based on conserved motifs of the almA gene sequences in public databases. Using this approach, we identified diverse almA genes in the hydrocarbon-degrading bacteria and in bacterial communities from the surface seawater of the Xiamen coastal area, the South China Sea, the Indian Ocean, and the Atlantic Ocean. As a result, almA was positively detected in 35 isolates belonging to four genera, and a total of 39 different almA sequences were obtained. Five isolates were confirmed to harbor two to three almA genes. From the Xiamen coastal area and the Atlantic Ocean oil-enrichment communities, a total of 60 different almA sequences were obtained. These sequences mainly formed two clusters in the phylogenetic tree, named Class I and Class II, and these shared 45-56% identity at the amino acid level. Class I contained 11 sequences from bacteria represented by the Salinisphaera and Parvibaculum genera. Class II was larger and more diverse, and it was composed of 88 sequences from Proteobacteria, Gram-negative bacteria, and the enriched bacterial communities. These communities were represented by the Alcanivorax and Marinobacter genera, which are the two most popular genera hosting the almA gene. AlmA was also detected across a wide geographical range, as determined by the origin of the bacterial host. Our results demonstrate the diversity of almA and confirm its high rate of occurrence in hydrocarbon

  8. Conflict-of-interest, copyright and other declarations.

    Science.gov (United States)

    Peh, W C; Ng, K H

    2010-11-01

    Declarations of exclusive publication, author contribution, conflict-of-interest and copyright transfer are important formalities required by most biomedical journals. Conflict-of-interest may be personal, commercial, political, academic or financial. It is particularly important for authors to provide a full and complete disclosure of any financial relationship with a commercial organisation that may have an interest in the contents of the submitted manuscript. Editors, editorial board members and reviewers should also declare any possible conflicts-of-interest. The handling of conflict-of-interest during manuscript preparation, peer review and editorial decision making impacts the credibility of published articles and scientific research in general.

  9. An Analysis of Individualism in the Declaration of Independence

    Institute of Scientific and Technical Information of China (English)

    钱微

    2007-01-01

    The awareness of individualism can be traced back to the period of American Revolution when the Declaration of Independence was produced.It expressed basic beliefs concerning freedom,equality,democracy,privacy and the relationship between people and government,which were exactly what the philosophy of individualism mostly dealt with at that time.This paper is to exploit the essence of individualism by analyzing the Declaration .The analysis enables us to reconsider its significance to the issue of America human rights and foreign policies.

  10. Sobre a origem das preposições ibero-românicas hasta, ata e até

    Directory of Open Access Journals (Sweden)

    Mário Eduardo Viaro

    2013-01-01

    Full Text Available Considerable controversy surrounds Ibero-Romance prepositions expressing the end-point of a movement. Each of the solutions proposed focuses on an etymon that explains the state of affairs in one language while failing to explain that in another. It is widely accepted that there is an Arabic element involved besides the Romance component. On account of the polymorphism of early ata, it is also common for partial solutions to leave unexplained a large number of variants. In an attempt to find an explanation which integrates this range of prepositions into the common Romance element, the present article delves into rival forms expressing the limitative notion in the prepositions of other languages and dialects of the Iberian Peninsula, as well as formal similarities between the dialects and languages throughout the Romance linguistic territory, since prepositions generally display conservatism in their form, while borrowing is rare among the languages of the world​. Crossovers between the classes of preposition, place adverb and temporal conjunction will be explored, looking for conservative structures that at first glance would not appear in a traditional etymological analysis, given idiosyncratic preference for some forms. Adopting an inductive perspective, this research points to an unusual transformation of Latin intra as the most likely etymon of the prepositions in question.

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

    Science.gov (United States)

    Baryshev, A. M.; Hesper, R.; 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.; van den Bemt, M.; Koops, A.; Keizer, K.; Pieters, C.; Koops van het Jagt, J.; 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.

    2015-05-01

    Aims: We describe the design, construction, and characterization of the Band 9 heterodyne receivers (600-720 GHz) for the Atacama Large Millimeter/submillimeter Array (ALMA). First-light Band 9 data, obtained during ALMA commissioning and science verification phases, are presented as well. Methods: The ALMA Band 9 receiver units (so-called "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 superconductor-insulator-superconductor (SIS) junction that performs the heterodyne down-conversion. Finally, the generated intermediate frequency (IF) signals are amplified by cryogenic and room-temperature HEMT amplifiers and exported to the telescope's IF back end for further processing and, finally, correlation. Results: The receivers have been constructed and tested in the laboratory and they show an excellent performance, complying with ALMA requirements. Performance statistics on all 73 Band 9 receivers are reported. Importantly, two different tunnel-barrier technologies (necessitating different tuning circuits) for the SIS junctions have been used, namely conventional AlOx barriers and the more recent high-current-density AlN barriers. On-sky characterization and tests of the performance of the Band 9 cartridges are presented using commissioning data. Continuum and line images of the low-mass protobinary IRAS 16293-2422 are presented which were obtained as part

  12. 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...

  13. MOCQL: A Declarative Language for Ad-Hoc Model Querying

    DEFF Research Database (Denmark)

    Störrle, Harald

    2013-01-01

    Language (MOCQL), an experimental declarative textual language to express queries (and constraints) on models. We introduce MOCQL by examples and its grammar, evaluate its usability by means of controlled experiments, and find that modelers perform better and experience less cognitive load when working...

  14. Sustainability Accounting Courses, Talloires Declaration and Academic Research

    Science.gov (United States)

    Khan, Tehmina

    2013-01-01

    Purpose: The purpose of this article is to identify the offering and nature (scope) of sustainability accounting courses at universities that have signed the Talloires Declaration and also at universities with prominent sustainability accounting researchers' affiliations. For this purpose a university web sites content analysis for sustainability…

  15. 78 FR 70065 - Agency Information Collection Activities: Customs Declaration

    Science.gov (United States)

    2013-11-22

    ... SECURITY U.S. Customs and Border Protection Agency Information Collection Activities: Customs Declaration AGENCY: U.S. Customs and Border Protection (CBP), Department of Homeland Security ACTION: 60-Day notice... and other Federal agencies to comment on an information collection requirement concerning the...

  16. The Analysis of a Real Life Declarative Process

    DEFF Research Database (Denmark)

    Debois, Søren; Slaats, Tijs

    2015-01-01

    This paper reports on a qualitative study of the use of declarative process notations used in a commercial setting. Specifically, we investigate the actual use of a system implemented in terms of DCR graphs for the Danish "Dreyer Foundation" by our industry partner Exformatics A/S. The study is p...

  17. 33 CFR 156.150 - Declaration of inspection.

    Science.gov (United States)

    2010-07-01

    ... (CONTINUED) POLLUTION OIL AND HAZARDOUS MATERIAL TRANSFER OPERATIONS Oil and Hazardous Material Transfer Operations § 156.150 Declaration of inspection. (a) No person may transfer oil or hazardous material to or... facility and the receiving vessel or facility; (2) The address of the facility or location of the...

  18. Declarative Parallel Programming in Spreadsheet End-User Development

    DEFF Research Database (Denmark)

    Biermann, Florian

    2016-01-01

    . In this literature study, we provide an overview of the publications on spreadsheet end-user programming and declarative array programming to inform further research on parallel programming in spreadsheets. Our results show that there is a clear overlap between spreadsheet programming and array programming and we...

  19. Adding state to declarative languages to enable web applications

    NARCIS (Netherlands)

    Jansen, A.J.

    2009-01-01

    On the web, media tend to be encoded in declarative formats, which facilitate accessibility, reuse, and transformation. Web applications, on the other hand, are created with more procedural technology and do not enjoy these benefits. In this thesis we examine how this can be fixed. We examine a smal

  20. Transcranial direct current stimulation during sleep improves declarative memory.

    Science.gov (United States)

    Marshall, Lisa; Mölle, Matthias; Hallschmid, Manfred; Born, Jan

    2004-11-03

    In humans, weak transcranial direct current stimulation (tDCS) modulates excitability in the motor, visual, and prefrontal cortex. Periods rich in slow-wave sleep (SWS) not only facilitate the consolidation of declarative memories, but in humans, SWS is also accompanied by a pronounced endogenous transcortical DC potential shift of negative polarity over frontocortical areas. To experimentally induce widespread extracellular negative DC potentials, we applied anodal tDCS (0.26 mA) [correction] repeatedly (over 30 min) bilaterally at frontocortical electrode sites during a retention period rich in SWS. Retention of declarative memories (word pairs) and also nondeclarative memories (mirror tracing skills) learned previously was tested after this period and compared with retention performance after placebo stimulation as well as after retention intervals of wakefulness. Compared with placebo stimulation, anodal tDCS during SWS-rich sleep distinctly increased the retention of word pairs (p affect declarative memory. Procedural memory was also not affected by tDCS. Mood was improved both after tDCS during sleep and during wake intervals. tDCS increased sleep depth toward the end of the stimulation period, whereas the average power in the faster frequency bands (,alpha, and beta) was reduced. Acutely, anodal tDCS increased slow oscillatory activity sleep-dependent consolidation of declarative memories.

  1. Declarative Joint Attention as a Foundation of Theory of Mind

    Science.gov (United States)

    Sodian, Beate; Kristen-Antonow, Susanne

    2015-01-01

    Theories of social-cognitive development have attributed a foundational role to declarative joint attention. The present longitudinal study of 83 children, who were assessed on a battery of social-cognitive tasks at multiple measurement points from the age of 12 to 50 months, tested a predictive model of theory of mind (false-belief…

  2. Methylphenidate significantly improves declarative memory functioning of adults with ADHD.

    NARCIS (Netherlands)

    Verster, J.C.; Bekker, E.M.; Kooij, J.J.; Buitelaar, J.K.; Verbaten, M.N.; Volkerts, E.R.; Olivier, B.

    2010-01-01

    BACKGROUND: Declarative memory deficits are common in untreated adults with attention-deficit hyperactivity disorder (ADHD), but limited evidence exists to support improvement after treatment with methylphenidate. The objective of this study was to examine the effects of methylphenidate on memory fu

  3. Exformatics Declarative Case Management Workflows as DCR Graphs

    DEFF Research Database (Denmark)

    Slaats, Tijs; Mukkamala, Raghava Rao; Hildebrandt, Thomas

    2013-01-01

    with researchers at IT University of Copenhagen (ITU) to create tools for the declarative workflow language Dynamic Condition Response Graphs (DCR Graphs) and incorporate them into their products and in teaching at ITU. In this paper we give a status report over the work. We start with an informal introduction...

  4. A Declaration on Learning--A Commentary Discourse

    Science.gov (United States)

    Walton, John S.

    2005-01-01

    This paper subjects "A Declaration on Learning" published in the UK in 2000 to a critical review. A brief synopsis of the text is followed by a commentary discourse drawing upon critical discourse analysis (Fairclough 2001) and incorporating meta content analysis, rhetorical analysis and genre analysis. Conclusions are drawn related to the…

  5. A Better Life for Future Generations: Amsterdam Declaration, November 1989.

    Science.gov (United States)

    1989-01-01

    This document contains the text of the Amsterdam Declaration "A Better Life for Future Generations," which was issued on November 9, 1989, by the International Forum on Population in the Twenty-First Century. The Declaration opens with a preamble which emphasizes our responsibilities towards future generations; acknowledges the interdependent nature of population size, resources, and development; expresses concern about rapid growth; recognizes the central position occupied by women in development and population growth; and recognizes that the goal of development is to improve quality of life. The Declaration continues by presenting current population figures and their implications. Other topics considered include population and sustainable development; population goals, objectives, and program priorities; and resource requirements. The Declaration issued a call to action asking all governments, intergovernmental agencies, nongovernmental organizations, and the private sector to increase their financial commitments to fulfill ongoing and emerging population needs. Specific requests were then directed to all countries; all developing countries; all donors; parliamentarians and community leaders; the press and media; the UN and its specialized agencies; the World Bank and regional development banks; the UN Population Fund and its governing bodies; nongovernmental, professional, and other voluntary organizations; and women's organizations.

  6. Declarative Business Process Modelling and the Generation of ERP Systems

    DEFF Research Database (Denmark)

    Schultz-Møller, Nicholas Poul; Hølmer, Christian; Hansen, Michael Reichhardt

    2009-01-01

    We present an approach to the construction of Enterprise Resource Planning (ERP) Systems, which is based on the Resources, Events and Agents (REA) ontology. This framework deals with processes involving exchange and flow of resources in a declarative, graphically-based manner describing what the ...

  7. 9 CFR 93.219 - Declaration for poultry.

    Science.gov (United States)

    2010-01-01

    ... 9 Animals and Animal Products 1 2010-01-01 2010-01-01 false Declaration for poultry. 93.219... AGRICULTURE EXPORTATION AND IMPORTATION OF ANIMALS (INCLUDING POULTRY) AND ANIMAL PRODUCTS IMPORTATION OF CERTAIN ANIMALS, BIRDS, FISH, AND POULTRY, AND CERTAIN ANIMAL, BIRD, AND POULTRY PRODUCTS;...

  8. Declaration of Basic Principles for the Treatment of Prisoners.

    Science.gov (United States)

    Cosman, J. W.

    1989-01-01

    Education does not flourish in prisons because of prevailing notions about the punitive and retributive purposes of prisons. The United Nations is considering a Declaration of Basic Principles for the Treatment of Prisoners that is intended to bring education to the forefront of criminal justice policy. (SK)

  9. 19 CFR 122.44 - Crew baggage declaration.

    Science.gov (United States)

    2010-04-01

    ... 19 Customs Duties 1 2010-04-01 2010-04-01 false Crew baggage declaration. 122.44 Section 122.44 Customs Duties U.S. CUSTOMS AND BORDER PROTECTION, DEPARTMENT OF HOMELAND SECURITY; DEPARTMENT OF THE TREASURY AIR COMMERCE REGULATIONS Aircraft Entry and Entry Documents; Electronic Manifest Requirements...

  10. 37 CFR 1.63 - Oath or declaration.

    Science.gov (United States)

    2010-07-01

    ... Section 1.63 Patents, Trademarks, and Copyrights UNITED STATES PATENT AND TRADEMARK OFFICE, DEPARTMENT OF... or declaration acknowledges the duty to disclose to the Office all information known to the person to..., or 365(c); and (ii) If one or more inventor(s) or legal representative(s) who refused to join in...

  11. How Effective Is Example Generation for Learning Declarative Concepts?

    Science.gov (United States)

    Rawson, Katherine A.; Dunlosky, John

    2016-01-01

    Declarative concepts (i.e., key terms and corresponding definitions for abstract concepts) represent foundational knowledge that students learn in many content domains. Thus, investigating techniques to enhance concept learning is of critical importance. Various theoretical accounts support the expectation that example generation will serve this…

  12. 18 CFR 367.2380 - Account 238, Dividends declared.

    Science.gov (United States)

    2010-04-01

    ... ACT Balance Sheet Chart of Accounts Current and Accrued Liabilities § 367.2380 Account 238, Dividends... declared. 367.2380 Section 367.2380 Conservation of Power and Water Resources FEDERAL ENERGY REGULATORY COMMISSION, DEPARTMENT OF ENERGY REGULATIONS UNDER THE PUBLIC UTILITY HOLDING COMPANY ACT OF 2005,...

  13. 75 FR 30417 - Tennessee; Amendment No. 7 to Notice of a Major Disaster Declaration

    Science.gov (United States)

    2010-06-01

    ... adversely affected by the event declared a major disaster by the President in his declaration of May 4, 2010..., Lauderdale, Lewis, Madison, McNairy, Montgomery, Obion, Smith, Stewart, Tipton, Wayne, and Wilson...

  14. 75 FR 65502 - Minnesota; Amendment No. 2 to Notice of a Major Disaster Declaration

    Science.gov (United States)

    2010-10-25

    ... notice of a major disaster declaration for the State of Minnesota (FEMA-1941-DR), dated October 13, 2010... determined to have been adversely affected by the event declared a major disaster by the President in...

  15. 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.

  16. Debris Disks in Nearby Young Moving Groups in the ALMA Era

    CERN Document Server

    Kóspál, Á

    2015-01-01

    Many members of nearby young moving groups exhibit infrared excess attributed to circumstellar debris dust, formed via erosion of planetesimals. With their proximity and well-dated ages, these groups are excellent laboratories for studying the early evolution of debris dust and of planetesimal belts. ALMA can spatially resolve the disk emission, revealing the location and extent of these belts, putting constraints on planetesimal evolution models, and allowing us to study planet-disk interactions. While the main trends of dust evolution in debris disks are well-known, there is almost no information on the evolution of gas. During the transition from protoplanetary to debris state, even the origin of gas is dubious. Here we review the exciting new results ALMA provided by observing young debris disks, and discuss possible future research directions.

  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. 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.

  19. Development of the ALMA-North America Sideband-Separating SIS Mixers

    CERN Document Server

    Kerr, Anthony R; Claude, Stéphane M X; Dindo, Philip; Lichtenberger, Arthur W; Lauria, Eugene F

    2013-01-01

    As the Atacama Large Millimeter/submillimeter Array (ALMA) nears completion, 73 dual-polarization receivers have been delivered for each of Bands 3 (84-116 GHz) and 6 (211-275 GHz). The receivers use sideband-separating superconducting Nb/Al-AlOx/Nb tunnel-junction (SIS) mixers, developed for ALMA to suppress atmospheric noise in the image band. The mixers were designed taking into account dynamic range, input return loss, and signal-to-image conversion (which can be significant in SIS mixers). Typical SSB receiver noise temperatures in Bands 3 and 6 are 30 K and 60 K, resp., and the image rejection is typically 15 dB.

  20. The Impacts of ALMA Primary Variables on Profitability An Empirical Study of Indonesian Banking

    Directory of Open Access Journals (Sweden)

    Sapto Jumono

    2015-04-01

    Full Text Available This study aims to determine the impact of liquidity on BEP and ROE in Indonesian banking industry. The supporting theory in this study is ALMA theory. Based on annual data for the period 2001-2014 and following purposive sampling technique, the acquired amount of sample study is 97 banks. The data is analyzed using panel data regression of GMM Arrelano Bond, as a novelty in data processing, therefore the speed of adjustment can be known. The ALMA variables such as LAR, capital, leverage, operating expenses, interest income, and CAR sensitivity have a significant effect on BEP and ROE. Meanwhile LDR, NPL, the FBI have no impact on profitability. The implication of this study is the fact that banking performance in Indonesia can be leveled up through the reduction in mortgage interest rates and increment of credit volume and FBI.

  1. 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).

  2. 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.

  3. 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.

  4. 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.

  5. 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.

  6. Effect of two prednisone exposures on mood and declarative memory.

    Science.gov (United States)

    Brown, E Sherwood; Beard, Laura; Frol, Alan B; Rush, A John

    2006-07-01

    Corticosteroids are essential for life and an integral part of the stress response. However, in excess, corticosteroids can be associated with a variety of effects on the brain including hippocampal atrophy and even neuronal death, mood changes, and declarative memory impairment. The magnitude of mood change in patients receiving prednisone is reportedly associated with previous lifetime corticosteroid exposure, consistent with a sensitization or kindling process whereby greater effects are observed with repeated exposure. To our knowledge, the effect of multiple corticosteroid exposures on mood and memory has not been previously examined prospectively in animals or humans. In this study, 30 human volunteers, with no history of systemic prescription corticosteroid therapy, were given (in random order using a crossover design) two 3-day exposures of prednisone (60 mg/day) and one of identical placebo, with 11-day washouts between each medication exposure. Before and after each 3-day prednisone/placebo exposure, declarative memory was assessed using different versions of the Rey Auditory Verbal Learning Test (RAVLT) to minimize practice or learning effects, while mood was assessed with the 21-item Hamilton Rating Scale for Depression, Young Mania Rating Scale and Internal State Scale. No significant mood changes were found. However, a significant decrease in aspects of RAVLT performance was observed after the first prednisone exposure consistent with a decline in declarative memory performance. The decline in RAVLT performance was significantly smaller after the second prednisone exposure as compared to the initial prednisone exposure. Thus, a second prednisone exposure was associated with an attenuated prednisone-effect on declarative memory. These data suggest tolerance or habituation, rather than sensitization, to prednisone effects on declarative memory during a second exposure. Implications and possible explanations for the findings are discussed.

  7. 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...

  8. ALMA resolves the torus of NGC 1068: continuum and molecular line emission

    CERN Document Server

    Garcia-Burillo, S; Almeida, C Ramos; Usero, A; Krips, M; Alonso-Herrero, A; Aalto, S; Casasola, V; Hunt, L K; Martin, S; Viti, S; Colina, L; Costagliola, F; Eckart, A; Fuente, A; Henkel, C; Marquez, I; Neri, R; Schinnerer, E; Tacconi, L J; van der Werf, P P

    2016-01-01

    We have used the Atacama Large Millimeter Array (ALMA) to map the emission of the CO(6-5) molecular line and the 432 {\\mu}m continuum emission from the 300 pc-sized circumnuclear disk (CND) of the nearby Seyfert 2 galaxy NGC 1068 with a spatial resolution of ~4 pc. These observations spatially resolve the CND and image, for the first time, the dust emission and the molecular gas distribution and kinematics from a 7-10 pc-diameter disk that represents the submillimeter counterpart of the putative torus of NGC 1068. We fitted the nuclear spectral energy distribution of the torus using ALMA and near and mid-infrared (NIR/MIR) data with CLUMPY models. The mass and radius of the best-fit solution for the torus are both consistent with the values derived from the ALMA data alone: Mgas_torus=(1+-0.3)x10^5 Msun and Rtorus=3.5+-0.5 pc. The dynamics of the molecular gas in the torus show non-circular motions and enhanced turbulence superposed on the rotating pattern of the disk. The kinematic major axis of the CO torus...

  9. 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...

  10. 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...

  11. 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...

  12. 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...

  13. 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...

  14. 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...

  15. 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...

  16. 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.

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

    CERN Document Server

    Eguchi, Satoshi; 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 to reduce network traffic: we prepare, in advance, "compressed" FITS files of 2x2x1 (horizontal, vertical, and spectral directions, respectively) binning, 2x2x2 binning, 4x4x2 binning data, and so on. These files are hidden from users, and Web QL automatically choose proper one by 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, I in...

  18. 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.

  19. 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...

  20. Centralized operations and maintenance planning at the Atacama Large Millimeter/submillimeter Array (ALMA)

    Science.gov (United States)

    Lopez, Bernhard; Whyborn, Nicholas D.; Guniat, Serge; Hernandez, Octavio; Gairing, Stefan

    2016-07-01

    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 consists of 54 twelve-meter antennas and 12 seven-meter antennas operating as an aperture synthesis array in the (sub)millimeter wavelength range. Since the inauguration of the observatory back in March 2013 there has been a continuous effort to establish solid operations processes for effective and efficient management of technical and administrative tasks on site. Here a key aspect had been the centralized maintenance and operations planning: input is collected from science stakeholders, the computerized maintenance management system (CMMS) and from the technical teams spread around the world, then this information is analyzed and consolidated based on the established maintenance strategy, the observatory long-term plan and the short-term priorities definitions. This paper presents the high-level process that has been developed for the planning and scheduling of planned- and unplanned maintenance tasks, and for site operations like the telescope array reconfiguration campaigns. We focus on the centralized planning approach by presenting its genesis, its current implementation for the observatory operations including related planning products, and we explore the necessary next steps in order to fully achieve a comprehensive centralized planning approach for ALMA in steady-state operations.

  1. 75 FR 79035 - Nationally Recognized Testing Laboratories; Supplier's Declaration of Conformity

    Science.gov (United States)

    2010-12-17

    ... Declaration of Conformity AGENCY: Occupational Safety and Health Administration, Labor. ACTION: Notice... use of a Supplier's Declaration of Conformity as a means of ensuring the safety of products currently... received to permit use of a Supplier's Declaration of Conformity (SDoC) as an alternative to OSHA's...

  2. 76 FR 27738 - Connecticut Disaster #CT-00021 Declaration of Economic Injury

    Science.gov (United States)

    2011-05-12

    ... ADMINISTRATION Disaster Declaration 12547 Connecticut Disaster CT-00021 Declaration of Economic Injury AGENCY: U... Disaster Loan (EIDL) declaration for the State of Connecticut, dated 05/04/2011. Incident: Southbury Main Street Fire. Incident Period: 02/18/2011. Effective Date: 05/04/2011. EIDL Loan Application Deadline...

  3. 27 CFR 46.253 - Destruction of articles by a Presidentially-declared major disaster.

    Science.gov (United States)

    2010-04-01

    ... a Presidentially-declared major disaster. 46.253 Section 46.253 Alcohol, Tobacco Products and....253 Destruction of articles by a Presidentially-declared major disaster. After the dealer has paid the..., or condemned because of a Presidentially-declared major disaster. Subpart C of this part...

  4. A World Worth Living in ICAE 8th World Assembly Declaration (June 2011)

    Science.gov (United States)

    Adult Learning, 2012

    2012-01-01

    This article presents the International Council of Adult Education (ICAE) 8th World Assembly Declaration (June 2011). This declaration focuses on adult educators' conviction in the possibility of a "world worth living in," and their declaration of their collective determination to work towards making it a reality all around the planet.

  5. 77 FR 6135 - Agency Information Collection Activities: Cargo Manifest/Declaration, Stow Plan, Container Status...

    Science.gov (United States)

    2012-02-07

    .../ Declaration, Stow Plan, Container Status Messages and Importer Security Filing AGENCY: U.S. Customs and Border... Manifest/Declaration, Stow Plan, Container Status Messages and Importer Security Filing. This is a proposed... forms of information. Title: Cargo Manifest/Declaration, Stow Plan, Container Status Messages...

  6. Snow accumulation variability at altitude of 7010 m a.s.l. in Muztag Ata Mountain in Pamir Plateau during 1958-2002

    Science.gov (United States)

    Duan, Keqin; Xu, Baiqin; Wu, Guanjian

    2015-12-01

    Precipitation over high mountain is significant for glacier development and river runoff in arid Tarim Basin in the northwest China. However, a coherent perspective of precipitation variability at high-altitude in Tarim Basin has not been presented until now. Here, a 41-m ice core at altitude of 7010 m a.s.l. was drilled and gotten to determine annual snow accumulation rates at Muztag Ata Mountain in the headwater of Tarim River in Pamir Plateau during summer 2003. Using strong seasonally variation of oxygen isotope and β-radioactivity reference layers, the core was dated reliably back to 1958 and resulted in a 45-year record between 1958 and 2002. The mean annual snow accumulation was about 605 mm water equivalent, which is almost 10 times than precipitation in piedmont with elevation below 3000 m a.s.l. The snow accumulation is characterized by high values in 1960s and early 1970s, followed by a drop in the middle 1970s and a recent decreasing trend. Further analysis suggests the upstream zonal flow variation as the major mechanism linking the regional snow accumulation fluctuation to macroscale circulation conditions. During the high snow accumulation years, the westerly winds between 30 and 50°N from the Mediterranean Sea to Pamir Plateau are weakened. The decreased upstream westerly winds generate anomalous cyclonic flows in the Pamir Plateau, which results in an enhanced advection of moisture from the tropics to the vicinity of Muztag Ata Mountain and is thus consistent with enhanced snow accumulation at the core site. During the low snow accumulation years, the above processes are reversed. On the basis of this high-altitude snow accumulation and temperature, a linear regression model is established to simulate annual mass balance in Muztag Ata region. Results reveal that snow accumulation conditions largely determine the annual mass-balance, which has stronger impaction on Tarim River runoff.

  7. ATA homozigosity in the IL-10 gene promoter is a risk factor for schizophrenia in Spanish females: a case control study

    Directory of Open Access Journals (Sweden)

    Fernandez-Piqueras Jose

    2011-06-01

    Full Text Available Abstract Background Three IL-10 gene promoter single nucleotide polymorphisms -1082G > A, -819C > T and -592C > A and the haplotypes they define in Caucasians, GCC, ACC, ATA, associated with different IL-10 production rates, have been linked to schizophrenia in some populations with conflicting results. On the basis of the evidence of the sex-dependent effect of certain genes in many complex diseases, we conducted a sex-stratified case-control association study to verify the linkage of the IL-10 gene promoter SNPs and haplotypes with schizophrenia and the possible sex-specific genetic effect in a Spanish schizophrenic population. Methods 241 DSM-IV diagnosed Spanish schizophrenic patients and 435 ethnically matched controls were genotyped for -1082G > A and -592C > A SNPs. Chi squared tests were performed to assess for genetic association of alleles, genotypes and haplotypes with the disease. Results The -1082A allele (p = 0.027, A/A (p = 0.008 and ATA/ATA (p = 0.003 genotypes were significantly associated with schizophrenia in females while neither allelic nor genotypic frequencies reached statistical significance in the male population. Conclusions Our results highlight the hypothesis of an imbalance towards an inflammatory syndrome as the immune abnormality of schizophrenia. Anyway, a better understanding of the involvement of the immune system would imply the search of immune abnormalities in endophenotypes in whose sex and ethnicity might be differential factors. It also reinforces the need of performing complex gene studies based on multiple cytokine SNPs, including anti and pro-inflammatory, to clarify the immune system abnormalities direction in the etiology of schizophrenia.

  8. Web-Based Modelling and Collaborative Simulation of Declarative Processes

    DEFF Research Database (Denmark)

    Slaats, Tijs; Marquard, Morten; Shahzad, Muhammad

    2015-01-01

    As a provider of Electronic Case Management solutions to knowledge-intensive businesses and organizations, the Danish company Exformatics has in recent years identified a need for flexible process support in the tools that we provide to our customers. We have addressed this need by adapting DCR......-user discussions on how knowledge workers really work, by enabling collaborative simulation of processes. In earlier work we reported on the integration of DCR Graphs as a workflow execution formalism in the existing Exformatics ECM products. In this paper we report on the advances we have made over the last two...... years, we describe the new declarative process modelling portal, discuss its features, describe the process of its development, report on the findings of an initial evaluation of the usability of the tool, resulting from a tutorial on declarative modelling with DCR Graphs that we organized at last years...

  9. 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 ...

  10. Quiescent Prominences in the Era of ALMA: Simulated Observations Using the 3D Whole-prominence Fine Structure Model

    Science.gov (United States)

    Gunár, Stanislav; Heinzel, Petr; Mackay, Duncan H.; Anzer, Ulrich

    2016-12-01

    We use the detailed 3D whole-prominence fine structure model to produce the first simulated high-resolution ALMA observations of a modeled quiescent solar prominence. The maps of synthetic brightness temperature and optical thickness shown in the present paper are produced using a visualization method for synthesis of the submillimeter/millimeter radio continua. We have obtained the simulated observations of both the prominence at the limb and the filament on the disk at wavelengths covering a broad range that encompasses the full potential of ALMA. We demonstrate here extent to which the small-scale and large-scale prominence and filament structures will be visible in the ALMA observations spanning both the optically thin and thick regimes. We analyze the relationship between the brightness and kinetic temperature of the prominence plasma. We also illustrate the opportunities ALMA will provide for studying the thermal structure of the prominence plasma from the cores of the cool prominence fine structure to the prominence-corona transition region. In addition, we show that detailed 3D modeling of entire prominences with their numerous fine structures will be important for the correct interpretation of future ALMA observations of prominences.

  11. Marginal capacity: the dilemmas faced in assessment and declaration.

    OpenAIRE

    Ho, V.

    1995-01-01

    Ontario is adopting informed-consent legislation that reflects increasing emphasis on patient autonomy and self-determination. Capacity assessment and declaration by physicians and other health care professionals are pivotal under the new legislation. While grossly capable or incapable patients provide few management difficulties, marginally capable patients provide a challenge for physicians who must assess capacity, and decisions concerning them emphasize the ethical dilemma involved in any...

  12. IMPORTANT — Declaration of income for 2001 —

    CERN Multimedia

    Human Resources Division

    2002-01-01

    The local French tax authorities confirm that, in view of the particular procedure for income declaration for CERN members of the personnel, this year CERN income (as stated in the certificate of CERN remuneration provided by the Organization) may be exceptionally declared in either French Francs, or Euros (clearly specifying the currency selected). Practical information concerning the procedure for income declaration may be obtained at the following local information desks : Trésorerie deGex: Tuesday12 March 9 a.m. to 122 to 4 p.m. Trésorerie deFerney: Monday18 March 9 a.m. to 122 to 4 p.m. Trésorerie deDivonne: Thursday21 March 9 a.m. to 122 to 4 p.m. French tax authorities have also organised the following information services: Web site: http://www.impots.gouv.fr/ Minitel: 3615 IR Service Vocal Server: 08 36 67 10 10 Telephone information: 08 20 32 42 52 Human Resources Division Tel. 72838

  13. The Alma-Bacon County Story: A Model for Rural America. Committee Print, 92nd Congress, 2nd Session, July 24, 1972.

    Science.gov (United States)

    Nipp, Robert E.

    Designed to illustrate the revitalization process of a small rural community via use of the Model Cities Program, this case study of Alma-Bacon County, Georgia traces Alma-Bacon's: (1) historical background; (2) community development beginnings; (3) political development; (4) outstanding problems; and (5) development plans and accomplishments…

  14. Terorisme atas Nama Agama

    Directory of Open Access Journals (Sweden)

    Abdul Muis Naharong

    2013-10-01

    Full Text Available In the wake of 9/11 the role of religion in promoting acts of violence considered as terrorism has been widely discussed by scholars, journalists, and policy makers. Several scholars, however, claim that religion does not have anything to do with terrorism. In their views religion is innocent and victim of unscrupulous political activists. Several others do believe that religion has to do with terrorism because religion has the power to motivate people to do good as well bad things. This article aims to elaborate religious or sacred terrorism or ‘new terrorism’ according to some scholars. The first part of this article tries to elaborate the meanings of ‘terrorism’ and ‘religion’, and to explain its root and trigger causes. The second part tries to discuss the opinions of scholars who claim that religious terrorism is real and not as a mere mask of other worldly interests, to elaborate the characteristics of religious terrorism, and to explain why religious terrorism is mostly associated with Islam.DOI: 10.15408/ref.v13i5.915

  15. 甲码(Alma)全力抢滩中国造船市场%Alma full ahead in the China Shipbuilding market

    Institute of Scientific and Technical Information of China (English)

    2008-01-01

    二十五年来,以生产切割、套料、排序软件著称的甲码(Alma)始终活跃于国际造船市场。早在八十年代初期,“海洋君主号”远洋客轮就已开始使用上述软件。多年的发展,甲码(Alma)迅速成为业内知名企业,并在造船和近海作业平台等领域屡有斩获,从而一举奠定了欧洲市场的领先地位。甲码中国(AlmaChina)作为Alma于2007年在中国上海设立的子公司,

  16. The Impacts of ALMA Primary Variables on Profitability An Empirical Study of Indonesian Banking (13-32

    Directory of Open Access Journals (Sweden)

    Sapto Jumono

    2016-06-01

    Full Text Available This study aims to determine the impact of liquidity on BEP and ROE in Indonesian banking industry. The supporting theory in this study is ALMA theory. Based on annual data for the period 2001-2014 and following purposive sampling technique, the acquired amount of sample study is 97 banks. The data is analyzed using panel data regression of GMM Arrelano Bond, as a novelty in data processing, therefore the speed of adjustment can be known. The ALMA variables such as LAR, capital, leverage, operating expenses, interest income, and CAR sensitivity have a significant effect on BEP and ROE. Meanwhile LDR, NPL, the FBI have no impact on profitability. The implication of this study is the fact that banking performance in Indonesia can be leveled up through the reduction in mortgage interest rates and increment of credit volume and FBI. Keywords: Bank,ALMA,BEP,ROE,LAR,LDR,NPL,Capital

  17. Probing turbulent, magnetized star formation with ALMA observations and next-generation AREPO simulations

    Science.gov (United States)

    Hull, Charles L. H.; Mocz, Philip; Burkhart, Blakesley K.; Miquel Girart, Josep; Goodman, Alyssa A.; Cortes, Paulo; Li, Zhi-Yun; Lai, Shih-Ping; Hernquist, Lars; Springel, Volker

    2017-01-01

    The first polarization data from ALMA have been delivered, and are both expanding and confounding our understanding of the role of magnetic fields in low-mass star formation. Here I will show the highest resolution and highest sensitivity polarization images ever made of a Class 0 protostellar source. These new ALMA observations of the source, known as Ser-emb 8, achieve 140 AU resolution, allowing us to probe polarization -- and thus magnetic field orientation -- in the innermost regions surrounding the protostar. The collapse of strongly magnetized dense gas is predicted to pinch the magnetic field into an hourglass shape that persists down to scales <100 AU. However, in contrast with more than 50 years of theory, the ALMA data definitively rule out an hourglass morphology and instead reveal a chaotic magnetic field that has not been inherited from the field in the interstellar medium surrounding the source. We have simulated the star formation process with cutting-edge, moving-mesh AREPO simulations on scales from a million AU (5 pc) down to 60 AU. We find that only in the case of a very strong magnetic field (~100 microgauss on 5 pc scales) is the field direction preserved from cloud to disk scales. When the field is weak, turbulence in the interstellar gas shapes the field on large scales, and the forming star system re-shapes the field again on small scales, divorcing the field from its history on larger scales. We conclude that this is what has happened in Ser-emb 8. The main distinction from the strong-field star formation model is that in the weak-field case it is turbulence -- not the magnetic field -- that shapes the material that forms the protostar.

  18. ALMA Resolves the Torus of NGC 1068: Continuum and Molecular Line Emission

    Science.gov (United States)

    García-Burillo, S.; Combes, F.; Ramos Almeida, C.; Usero, A.; Krips, M.; Alonso-Herrero, A.; Aalto, S.; Casasola, V.; Hunt, L. K.; Martín, S.; Viti, S.; Colina, L.; Costagliola, F.; Eckart, A.; Fuente, A.; Henkel, C.; Márquez, I.; Neri, R.; Schinnerer, E.; Tacconi, L. J.; van der Werf, P. P.

    2016-05-01

    We used the Atacama Large Millimeter Array (ALMA) to map the emission of the CO(6-5) molecular line and the 432 μm continuum emission from the 300 pc sized circumnuclear disk (CND) of the nearby Seyfert 2 galaxy NGC 1068 with a spatial resolution of ˜4 pc. These observations spatially resolve the CND and, for the first time, image the dust emission, the molecular gas distribution, and the kinematics from a 7-10 pc diameter disk that represents the submillimeter counterpart of the putative torus of NGC 1068. We fitted the nuclear spectral energy distribution of the torus using ALMA and near- and mid-infrared (NIR/MIR) data with CLUMPY torus models. The mass and radius of the best-fit solution for the torus are both consistent with the values derived from the ALMA data alone: {M}{{gas}}{{torus}}=(1+/- 0.3)× {10}5 {M}⊙ and R torus = 3.5 ± 0.5 pc. The dynamics of the molecular gas in the torus show strong non-circular motions and enhanced turbulence superposed on a surprisingly slow rotation pattern of the disk. By contrast with the nearly edge-on orientation of the H2O megamaser disk, we found evidence suggesting that the molecular torus is less inclined (i = 34°-66°) at larger radii. The lopsided morphology and complex kinematics of the torus could be the signature of the Papaloizou-Pringle instability, long predicted to likely drive the dynamical evolution of active galactic nuclei tori.

  19. ALMA OBSERVATIONS OF SPT-DISCOVERED, STRONGLY LENSED, DUSTY, STAR-FORMING GALAXIES

    Energy Technology Data Exchange (ETDEWEB)

    Hezaveh, Y. D. [Department of Physics, McGill University, 3600 Rue University, Montreal, Quebec H3A 2T8 (Canada); Marrone, D. P.; Spilker, J. S.; Bothwell, M. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Fassnacht, C. D. [Department of Physics, University of California, One Shields Avenue, Davis, CA 95616 (United States); Vieira, J. D. [California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Aguirre, J. E. [University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Aird, K. A. [University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Aravena, M.; De Breuck, C. [European Southern Observatory, Karl-Schwarzschild Strasse, D-85748 Garching bei Muenchen (Germany); Ashby, M. L. N.; Bayliss, M. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Benson, B. A.; Bleem, L. E.; Carlstrom, J. E.; Chang, C. L.; Crawford, T. M.; Crites, A. T. [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Brodwin, M. [Department of Physics and Astronomy, University of Missouri, 5110 Rockhill Road, Kansas City, MO 64110 (United States); Chapman, S. C. [Department of Physics and Atmospheric Science, Dalhousie University, Halifax, NS B3H 3J5 (Canada); and others

    2013-04-20

    We present Atacama Large Millimeter/submillimeter Array (ALMA) 860 {mu}m imaging of four high-redshift (z = 2.8-5.7) dusty sources that were detected using the South Pole Telescope (SPT) at 1.4 mm and are not seen in existing radio to far-infrared catalogs. At 1.''5 resolution, the ALMA data reveal multiple images of each submillimeter source, separated by 1''-3'', consistent with strong lensing by intervening galaxies visible in near-IR imaging of these sources. We describe a gravitational lens modeling procedure that operates on the measured visibilities and incorporates self-calibration-like antenna phase corrections as part of the model optimization, which we use to interpret the source structure. Lens models indicate that SPT0346-52, located at z = 5.7, is one of the most luminous and intensely star-forming sources in the universe with a lensing corrected FIR luminosity of 3.7 Multiplication-Sign 10{sup 13} L{sub Sun} and star formation surface density of 4200 M{sub Sun} yr{sup -1} kpc{sup -2}. We find magnification factors of 5 to 22, with lens Einstein radii of 1.''1-2.''0 and Einstein enclosed masses of 1.6-7.2 Multiplication-Sign 10{sup 11} M{sub Sun }. These observations confirm the lensing origin of these objects, allow us to measure their intrinsic sizes and luminosities, and demonstrate the important role that ALMA will play in the interpretation of lensed submillimeter sources.

  20. ALMA IMAGING OF MILLIMETER/SUBMILLIMETER CONTINUUM EMISSION IN ORION KL

    Energy Technology Data Exchange (ETDEWEB)

    Hirota, Tomoya; Honma, Mareki [National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo 181–8588 (Japan); Kim, Mi Kyoung [Korea Astronomy and Space Science Institute, Hwaam-dong 61-1, Yuseong-gu, Daejeon, 305-348 (Korea, Republic of); Kurono, Yasutaka, E-mail: tomoya.hirota@nao.ac.jp [Chile Observatory, National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo 181-8588 (Japan)

    2015-03-10

    We have carried out high-resolution observations with the Atacama Large Millimeter/Submillimeter Array (ALMA) of continuum emission from the Orion Kleinmann–Low (KL) region. We identify 11 compact sources at ALMA band 6 (245 GHz) and band 7 (339 GHz), including the Hot Core, Compact Ridge, SMA1, IRc4, IRc7, and a radio source I (Source I). A 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{sup −} free–free emission as an opacity source of this optically thick emission. The temperature, density, and mass of the circumstellar disk associated with Source I are constrained by the SED of H{sup −} free–free emission. Still, the fitting result shows a significant deviation from the observed flux densities. Combined with the thermal dust graybody SED to explain excess emission at higher frequency, a smaller power-law index of 1.60 for the H{sup −} free–free emission is obtained in the SED fitting. The power-law index smaller than two would suggest a compact source size or a clumpy structure unresolved with the present study. Future higher resolution observations with ALMA are essential to reveal more detailed spatial structure and physical properties of Source I.

  1. Alma Soprano半导体冰点激光脱毛的临床观察

    Institute of Scientific and Technical Information of China (English)

    黄欣; 傅丽清; 樊秋晓; 曾莲蓉; 麦慧

    2012-01-01

    目的 观察Alma Soprano半导体冰点激光脱毛的临床效果.方法 对157例患者采用Alma Soprano半导体冰点激光脱毛仪进行脱毛治疗,波长810 nm,脉冲宽度400 ms,光斑大小10 mm×12 mm,能量密度10 J/cm2(冰点模式),频率10 Hz,统计不同部位的累计能量、治疗间隔、治疗次数,观察治疗中患者的疼痛感、不良反应、再生毛发的情况,治疗终结半年后观察最终效果.结果 157例患者经过4~10次的治疗,治愈151例,显效6例.每次治疗后再生的毛发均变细、变稀疏、颜色变浅.治疗操作的时间短,治疗中患者的疼痛感不明显,未观察到明显并发症.结论 Alma Soprano半导体冰点激光脱毛安全、有效,操作时间短,患者疼痛感轻,无明显并发症.

  2. Bartolomé Cairasco de Figueroa y el auto sacramental: La Comedia del Alma

    Directory of Open Access Journals (Sweden)

    Gutiérrez, José Ismael

    2004-06-01

    Full Text Available In spite of its title, Comedia del Alma, by Bartolomé Cairasco de Figueroa, is an allegorical religious play. This literary work not only is an inusual testimony of this gender in Canarian Islands; it's also one of the best allegorical religious plays of the Spanish Renaissance. Comedia del Alma alternates between humor and seriousness, abstract ideas and humanization, learned and popular style, verse and prose. However, its principal characteristic concerns the allusions which the characters make to the reality close to the audience and the fierce attack launder on the Canarian society.La Comedia del Alma, de Bartolomé Cairasco de Figueroa, pese a su título, pertenece al género dramático conocido como «auto sacramental». No sólo es uno de los escasos autos sacramentales escritos en las Islas Canarias, sino que además es uno de los mejores del siglo XVI español. La pieza teatral se ajusta en muchos aspectos a las características del género: mezcla lo serio y lo cómico, lo abstracto y la humanización, lo culto y lo popular, la prosa y el verso... Pero quizás la mayor particularidad de la obra sean las referencias a la realidad inmediata de los espectadores que aparecen en ella y las críticas que algunos personajes alegóricos hacen de las costumbres de la sociedad canaria de la época.

  3. Revealing H2D+ depletion and compact structure in starless and protostellar cores with ALMA

    DEFF Research Database (Denmark)

    Friesen, R. K.; Di Francesco, J.; Bourke, T. L.;

    2014-01-01

    We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the submillimeter dust continuum and H2D+ 110-111 emission toward two evolved, potentially protostellar cores within the Ophiuchus molecular cloud, Oph A SM1 and SM1N. The data reveal small-scale condensations within...... hydrostatic core, or HD (and consequently H2D+) depletion in the cold center of the condensation. We propose that SM1 is protostellar and that the condensation detected by ALMA is a warm (T ~ 30-50 K) accretion disk. The less concentrated emission of the SM1N condensation suggests that it is still starless...

  4. 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

  5. AlmaViva Teatro: clásicos desde el compromiso

    OpenAIRE

    Olivas Fuentes, Marta

    2014-01-01

    Este artículo aborda la trayectoria de la compañía AlmaViva Teatro y su trabajo con la puesta en escena del teatro aurisecular. Estos montajes están basados no solo en la reivindicación de la actualidad del propio texto o el mensaje de compromiso social que pueda transmitir al espectador del siglo xxi con respecto a su propio contexto, sino también en la apuesta por espacios escénicos no convencionales que resignifican el texto y lo conectan aún más con la concepción colectiva del Teatro. Pal...

  6. 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 (codex, can

  7. 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

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

    Science.gov (United States)

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

    2017-01-01

    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.

  9. 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.

  10. 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.

  11. 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 $\

  12. 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.

  13. Europe, Japan and North America Prepare for Joint Construction of the Giant Radio Telescope "ALMA" in Chile

    Science.gov (United States)

    2001-04-01

    Caption : PR Photo 14/01 shows how the ALMA facility may look like when it is ready at Chajnantor. Courtesy NAOJ . Representatives from Europe, Japan, and North America met in Tokyo today and signed a Resolution affirming their mutual intent to construct and operate a giant radio telescope in co-operation with the Republic of Chile, where the telescope will be located. The Atacama Large Millimeter/Submillimeter Array (ALMA) is conceived as a radio telescope comprised of sixty-four transportable 12-meter diameter antennas distributed over an area 14 km in extent. Japanese participation will allow enhanced imaging and spectroscopy, especially at submillimeter wavelengths. By pointing all the antennas in unison toward a single astronomical object, and combining the signals detected by all the antennas with a super-fast digital signal processor, this gigantic radio telescope achieves an imaging detail 10 times better than that of the Hubble Space Telescope. The combined area of all 64 antennas used to collect signals from celestial objects is more than 40 times larger than that available to astronomers using existing submillimeter telescopes. ALMA will be built on the Andean plateau at 5,000 meters altitude near the Atacama Desert of northern Chile. This site provides the exceptionally dry atmospheric conditions necessary for astronomical observations at millimeter and submillimeter wavelengths (wavelengths between the radio and far-infrared spectral regions). Observations with this telescope will have a profound impact on virtually all fields of astrophysical research. The most important targets include the most distant (i.e., the youngest) galaxies as they emerged in the early Universe. These are expected to have become rapidly enshrouded in the dust produced by the first stars; the dust absorbs much of the starlight making the galaxies difficult to see in the optical wavebands, but these same galaxies shine brightly at millimeter and submillimeter wavelengths. In

  14. Optimized Parallel Execution of Declarative Programs on Distributed Memory Multiprocessors

    Institute of Scientific and Technical Information of China (English)

    沈美明; 田新民; 等

    1993-01-01

    In this paper,we focus on the compiling implementation of parlalel logic language PARLOG and functional language ML on distributed memory multiprocessors.Under the graph rewriting framework, a Heterogeneous Parallel Graph Rewriting Execution Model(HPGREM)is presented firstly.Then based on HPGREM,a parallel abstact machine PAM/TGR is described.Furthermore,several optimizing compilation schemes for executing declarative programs on transputer array are proposed.The performance statistics on transputer array demonstrate the effectiveness of our model,parallel abstract machine,optimizing compilation strategies and compiler.

  15. Declarative Business Process Modelling and the Generation of ERP Systems

    Science.gov (United States)

    Schultz-Møller, Nicholas Poul; Hølmer, Christian; Hansen, Michael R.

    We present an approach to the construction of Enterprise Resource Planning (ERP) Systems, which is based on the Resources, Events and Agents (REA) ontology. This framework deals with processes involving exchange and flow of resources in a declarative, graphically-based manner describing what the major entities are rather than how they engage in computations. We show how to develop a domain-specific language on the basis of REA, and a tool which automatically can generate running web-applications. A main contribution is a proof-of-concept showing that business-domain experts can generate their own applications without worrying about implementation details.

  16. Declarative Modelling and Safe Distribution of Healthcare Workflows

    DEFF Research Database (Denmark)

    Hildebrandt, Thomas; Mukkamala, Raghava Rao; Slaats, Tijs

    2012-01-01

    a set of local process graphs communicating by shared events, such that the distributed execution of the local processes is equivalent to executing the original process. The technique is based on our recent similar work on safe distribution of Dynamic Condition Response (DCR) Graphs applied to cross......We present a formal technique for safe distribution of workflow processes described declaratively as Nested Condition Response (NCR) Graphs and apply the technique to a distributed healthcare workflow. Concretely, we provide a method to synthesize from a NCR Graph and any distribution of its events...

  17. Solidarity and the Universal Declaration on Bioethics and Human Rights.

    Science.gov (United States)

    Gunson, Darryl

    2009-06-01

    Recent work has stressed the importance of the concept of solidarity to bioethics and social philosophy generally. But can and should it feature in documents such as the Universal Declaration on Bioethics and Human Rights as anything more than a vague notion with multiple possible interpretations? Although noting the tension between universality and particularity that such documents have to deal with, and also noting that solidarity has a political content, the paper explores the suggestion that solidarity should feature more centrally in international regulations. The paper concludes with the view that when solidarity is seen aright, the UDBHR is an implicitly solidaristic document.

  18. The Universal Declaration of Human Rights and Armed Conflicts

    OpenAIRE

    Aurey, Xavier

    2009-01-01

    International audience; Born out of the horror of war, the Universal Declaration of Human Rights seems to leave outside any traces of its bellicose ancestry. As a figure of the intimate relationship between the State and its citizens, Human Rights Law reports to the sole domestic sphere of States. Between a Law of War as the perfect expression of States’ sovereignty and an international community still in its infancy, the UDHR seemed to be able to “guide” men and nations only in those periods...

  19. 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...

  20. ALMA reveals the feeding of the Seyfert 1 nucleus in NGC 1566

    CERN Document Server

    Combes, F; Casasola, V; Hunt, L; Krips, M; Baker, A J; Boone, F; Eckart, A; Marquez, I; Neri, R; Schinnerer, E; Tacconi, L J

    2014-01-01

    We report ALMA observations of CO(3-2) emission in the Seyfert 1 galaxy NGC 1566, at a spatial resolution of 25 pc. Our aim is to investigate the morphology and dynamics of the gas inside the central kpc, and to probe nuclear fueling and feedback phenomena. NGC 1566 has a nuclear bar of 1.7 kpc radius and a conspicuous grand design spiral starting from this radius. The ALMA field of view, of diameter 0.9 kpc, lies well inside the nuclear bar and reveals a molecular trailing spiral structure of \\sim 100 pc in size, which is possibly fueling the nucleus. The spiral starts with a large pitch angle from the center and then winds up in a pseudo-ring at the inner Lindblad resonance (ILR) of the nuclear bar. This is the first time that a trailing spiral structure is clearly seen driving the gas inwards inside the ILR ring of the nuclear bar. This phenomenon shows that the massive central black hole has a significant dynamical influence on the gas, triggering its fueling. The gaseous spiral is well correlated with th...

  1. 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...

  2. Molecular Gas in the X-ray Bright Group NGC 5044 as Revealed by ALMA

    CERN Document Server

    David, Laurence P; Forman, William; Vrtilek, Jan; Combes, Francoise; Salome, Philippe; Edge, Alastair; Jones, Christine; Sun, Ming; O'Sullivan, Ewan; Gastaldello, Fabio; Temi, Pasquale; Schmitt, Henrique; Ohyama, Youichi; Hamer, Stephen; Mathews, William; Brighenti, Fabrizio; Giacintucci, Simona; Bardelli, Sandro; Trung, Dinh-V

    2014-01-01

    A short 30 minute ALMA observation of the early-type galaxy NGC 5044, which resides at the center of an X-ray bright group with a moderate cooling flow, has detected 24 molecular structures within the central 2.5 kpc. The masses of the molecular structures vary from 3e5 to 1e7 Mo3 and the CO(2-1) linewidths vary from 15 to 65 km/s. Given the large CO(2-1) linewidths, the observed structures are likely giant molecular associations (GMAs) and not individual molecular clouds (GMCs). Only a few of the GMAs are spatially resolved with the cycle 0 ALMA beam and the average density of these GMAs yields a GMC volume filling factor of about 15%. The observed masses of the resolved GMAs are insufficient for them to be gravitationally bound, however, the most massive GMA does contain a less massive component with a linewidth of 5.5 km/s (typical of an individual virialized GMC). We also show that the GMAs cannot be pressure confined by the hot gas. Given the observed CO(2-1) linewidths of the GMAs (i.e., the velocity di...

  3. Resolving the stellar activity of the Mira AB binary with ALMA

    CERN Document Server

    Vlemmings, W H T; O'Gorman, E; Humphreys, E M L; Wittkowski, M; Baudry, A; Karovska, M

    2015-01-01

    We present the size, shape and flux densities at millimeter continuum wavelengths, based on ALMA science verification observations in Band 3 (~94.6 GHz) and Band 6 (~228.7 GHz), from the binary Mira A (o Ceti) and Mira B. The Mira AB system has been observed with ALMA at a spatial resolution of down to ~25 mas. The extended atmosphere of Mira A and the wind around Mira B sources are resolved and we derive the size of Mira A and of the ionized region around Mira B. The spectral indices within Band 3 (between 89-100 GHz) and between Band 3 and Band 6 are also derived. The spectral index of Mira A is found to change from 1.71+-0.05 within Band 3 to 1.54+-0.04 between Band 3 and 6. The spectral index of Mira B is 1.3+-0.2 in Band 3, in good agreement with measurements at longer wavelengths. However it rises to 1.72+-0.11 between the bands. For the first time the extended atmosphere of a star is resolved at these frequencies and for Mira A the diameter is ~3.7x2.9 AU in Band 3 (with brightness temperature Tb~6000 ...

  4. ALMA and Herschel Observations of the Prototype Dusty and Polluted White Dwarf G29-38

    CERN Document Server

    Farihi, J; Greaves, J S; Bonsor, A; Sibthorpe, B; Panić, O

    2014-01-01

    ALMA Cycle 0 and Herschel PACS observations are reported for the prototype, nearest, and brightest example of a dusty and polluted white dwarf, G29-38. These long wavelength programs attempted to detect an outlying, parent population of bodies at 1-100 AU, from which originates the disrupted planetesimal debris that is observed within 0.01 AU and which exhibits L_IR/L = 0.039. No associated emission sources were detected in any of the data down to L_IR/L ~ 1e-4, generally ruling out cold dust masses greater than 1e24 - 1e25 g for reasonable grain sizes and properties in orbital regions corresponding to evolved versions of both asteroid and Kuiper belt analogs. Overall, these null detections are consistent with models of long-term collisional evolution in planetesimal disks, and the source regions for the disrupted parent bodies at stars like G29-38 may only be salient in exceptional circumstances, such as a recent instability. A larger sample of polluted white dwarfs, targeted with the full ALMA array, has th...

  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. ALMA Observations of SPT-Discovered, Strongly Lensed, Dusty, Star-Forming Galaxies

    CERN Document Server

    Hezaveh, Y D; Fassnacht, C D; Spilker, J S; Vieira, J D; Aguirre, J E; Aird, K A; Aravena, M; Ashby, M L N; Bayliss, M; Benson, B A; Bleem, L E; Bothwell, M; Brodwin, M; Carlstrom, J E; Chang, C L; Chapman, S C; Crawford, T M; Crites, A T; De Breuck, C; de Haan, T; Dobbs, M A; Fomalont, E B; George, E M; Gladders, M D; Gonzalez, A H; Greve, T R; Halverson, N W; High, F W; Holder, G P; Holzapfel, W L; Hoover, S; Hrubes, J D; Husband, K; Hunter, T R; Keisler, R; Lee, A T; Leitch, E M; Lueker, M; Luong-Van, D; Malkan, M; McIntyre, V; McMahon, J J; Mehl, J; Menten, K M; Meyer, S S; Mocanu, L M; Murphy, E J; Natoli, T; Padin, S; Plagge, T; Reichardt, C L; Rest, A; Ruel, J; Ruhl, J E; Sharon, K; Schaffer, K K; Shaw, L; Shirokoff, E; Stalder, B; Staniszewski, Z; Stark, A A; Story, K; Vanderlinde, K; Weiß, A; Welikala, N; Williamson, R

    2013-01-01

    We present Atacama Large Millimeter/submillimeter Array (ALMA) 860 micrometer imaging of four high-redshift (z=2.8-5.7) dusty sources that were detected using the South Pole Telescope (SPT) at 1.4 mm and are not seen in existing radio to far-infrared catalogs. At 1.5 arcsec resolution, the ALMA data reveal multiple images of each submillimeter source, separated by 1-3 arcsec, consistent with strong lensing by intervening galaxies visible in near-IR imaging of these sources. We describe a gravitational lens modeling procedure that operates on the measured visibilities and incorporates self-calibration-like antenna phase corrections as part of the model optimization, which we use to interpret the source structure. Lens models indicate that SPT0346-52, located at z=5.7, is one of the most luminous and intensely star-forming sources in the universe with a lensing corrected FIR luminosity of 3.7 X 10^13 L_sun and star formation surface density of 4200 M_sun yr^-1 kpc^-2. We find magnification factors of 5 to 22, w...

  7. ALMA OBSERVATIONS OF THE OUTFLOW FROM SOURCE I IN THE ORION-KL REGION

    Energy Technology Data Exchange (ETDEWEB)

    Zapata, Luis A.; Rodriguez, Luis F.; Loinard, Laurent [Centro de Radioastronomia y Astrofisica, UNAM, Apdo. Postal 3-72 (Xangari), 58089 Morelia, Michoacan (Mexico); Schmid-Burgk, Johannes; Menten, Karl M. [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, 53121 Bonn (Germany); Curiel, Salvador [Instituto de Astronomia, Universidad Nacional Autonoma de Mexico, Ap. 70-264, 04510 DF (Mexico)

    2012-07-20

    In this Letter, we present sensitive millimeter SiO (J = 5-4; {nu} = 0) line observations of the outflow arising from the enigmatic object Orion Source I made with the Atacama Large Millimeter/Submillimeter Array (ALMA). The observations reveal that at scales of a few thousand AU, the outflow has a marked 'butterfly' morphology along a northeast-southwest axis. However, contrary to what is found in the SiO and H{sub 2}O maser observations at scales of tens of AU, the blueshifted radial velocities of the moving gas are found to the northwest, while the redshifted velocities are in the southeast. The ALMA observations are complemented with SiO (J = 8-7; {nu} = 0) maps (with a similar spatial resolution) obtained with the Submillimeter Array. These observations also show a similar morphology and velocity structure in this outflow. We discuss some possibilities to explain these differences at small and large scales across the flow.

  8. 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...

  9. 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...

  10. 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

  11. Interaction design challenges and solutions for ALMA operations monitoring and control

    Science.gov (United States)

    Pietriga, Emmanuel; Cubaud, Pierre; Schwarz, Joseph; Primet, Romain; Schilling, Marcus; Barkats, Denis; Barrios, Emilio; Vila Vilaro, Baltasar

    2012-09-01

    The ALMA radio-telescope, currently under construction in northern Chile, is a very advanced instrument that presents numerous challenges. From a software perspective, one critical issue is the design of graphical user interfaces for operations monitoring and control that scale to the complexity of the system and to the massive amounts of data users are faced with. Early experience operating the telescope with only a few antennas has shown that conventional user interface technologies are not adequate in this context. They consume too much screen real-estate, require many unnecessary interactions to access relevant information, and fail to provide operators and astronomers with a clear mental map of the instrument. They increase extraneous cognitive load, impeding tasks that call for quick diagnosis and action. To address this challenge, the ALMA software division adopted a user-centered design approach. For the last two years, astronomers, operators, software engineers and human-computer interaction researchers have been involved in participatory design workshops, with the aim of designing better user interfaces based on state-of-the-art visualization techniques. This paper describes the process that led to the development of those interface components and to a proposal for the science and operations console setup: brainstorming sessions, rapid prototyping, joint implementation work involving software engineers and human-computer interaction researchers, feedback collection from a broader range of users, further iterations and testing.

  12. 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)...

  13. 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 ...

  14. 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...

  15. The Inner Mass Distribution of the Gravitational Lens SDP.81 from ALMA Observations

    CERN Document Server

    Wong, Kenneth C; Matsushita, Satoki

    2015-01-01

    The central image of a strongly lensed background source places constraints on the foreground lens galaxy's inner mass profile slope, core radius and mass of its nuclear supermassive black hole. Using high-resolution long-baseline Atacama Large Millimeter/submillimeter Array (ALMA) observations and archival $Hubble~Space~Telescope$ ($HST$) imaging, we model the gravitational lens H-ATLAS J090311.6+003906 (also known as SDP.81) and search for the demagnified central image. There is central continuum emission from the lens galaxy's active galactic nucleus (AGN) but no evidence of the central lensed image in any molecular line. We use the CO $J$=5-4 map to determine the flux limit of the central image excluding the AGN continuum. We predict the flux density of the central image and use the limits from the ALMA data to constrain the inner mass distribution of the lens. For the core radius of $0.15"$ measured from $HST$ photometry of the lens galaxy assuming that the central flux is completely attributed to the AG...

  16. 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...

  17. 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.

  18. ALMA Observations of the Coldest Place in the Universe: The Boomerang Nebula

    CERN Document Server

    Sahai, R; Huggins, P J; Nyman, L-A; Gonidakis, I

    2013-01-01

    The Boomerang Nebula is the coldest known object in the Universe, and an extreme member of the class of Pre-Planetary Nebulae, objects which represent a short-lived transitional phase between the AGB and Planetary Nebula evolutionary stages. Previous single-dish CO (J=1-0) observations (with a 45 arcsec beam) showed that the high-speed outflow in this object has cooled to a temperature significantly below the temperature of the cosmic background radiation. Here we report the first observations of the Boomerang with ALMA in the CO J=2-1 and J=1-0 lines to resolve the structure of this ultra-cold nebula. We find a central hourglass-shaped nebula surrounded by a patchy, but roughly round, cold high-velocity outflow. We compare the ALMA data with visible-light images obtained with HST and confirm that the limb-brightened bipolar lobes seen in these data represent hollow cavities with dense walls of molecular gas and dust producing both the molecular-emission-line and scattered-light structures seen at millimeter ...

  19. 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.

  20. Millimeter Emission Structure in the first ALMA Image of the AU Mic Debris Disk

    CERN Document Server

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

    2012-01-01

    We present 1.3 millimeter ALMA Cycle 0 observations of the edge-on debris disk around the nearby, ~10 Myr-old, M-type star AU Mic. These observations obtain 0.6 arcsec (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 about 1 lunar mass 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 ~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 chara...

  1. The Space Infrared Interferometric Telescope (SPIRIT) and its Complementarity to ALMA

    Science.gov (United States)

    Leisawitz, Dave

    2007-01-01

    We report results of a pre-Formulation Phase study of SPIRIT, a candidate NASA Origins Probe mission. SPIRIT is a spatial and spectral interferometer with an operating wavelength range 25 - 400 microns. SPIRIT will provide sub-arcsecond resolution images and spectra with resolution R = 3000 in a 1 arcmin field of view to accomplish three primary scientific objectives: (1) Learn how planetary systems form from protostellar disks, and how they acquire their chemical organization; (2) Characterize the family of extrasolar planetary systems by imaging the structure in debris disks to understand how and where planets of different types form; and (3) Learn how high-redshift galaxies formed and merged to form the present-day population of galaxies. In each of these science domains, SPIRIT will yield information complementary to that obtainable with the James Webb Space Telescope (JWST)and the Atacama Large Millimeter Array (ALMA), and all three observatories could operate contemporaneously. Here we shall emphasize the SPIRIT science goals (1) and (2) and the mission's complementarity with ALMA.

  2. 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

    2016-06-01

    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 (12)CO(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.

  3. ON THE NATURE OF THE TERTIARY COMPANION TO FW TAU: ALMA CO OBSERVATIONS AND SED MODELING

    Energy Technology Data Exchange (ETDEWEB)

    Caceres, Claudio; Hardy, Adam; Schreiber, Matthias R.; Cánovas, Héctor [Instituto de Física y Astronomía, Universidad de Valparaíso, Av. Gran Bretaña 1111, 2360102 Valparaíso (Chile); Cieza, Lucas A. [Núcleo de Astronomía, Universidad Diego Portales, Av. Ejército 441, Santiago (Chile); Williams, Jonathan P. [Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822 (United States); Hales, Antonio [Atacama Large Millimeter/Submillimeter Array, Joint ALMA Observatory, Alonso de Córdova 3107, Vitacura, 763-0355 Santiago (Chile); Pinte, Christophe [Univ. Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble (France); Ménard, Francois [UMI-FCA, CNRS/INSU, UMI 3386 (France); Wahhaj, Zahed [European Southern Observatory, Av. Alonso de Córdova 3107, Vitacura, 19001 Santiago (Chile)

    2015-06-20

    It is thought that planetary mass companions may form through gravitational disk instabilities or core accretion. Identifying such objects in the process of formation would provide the most direct test for the competing formation theories. One of the most promising candidates for a planetary mass object still in formation is the third object in the FW Tau system. We present here ALMA cycle 1 observations confirming the recently published 1.3 mm detection of a dust disk around this third object and present for the first time a clear detection of a single peak {sup 12}CO (2–1) line, providing direct evidence for the simultaneous existence of a gas disk. We perform radiative transfer modeling of the third object in FW Tau and find that current observations are consistent with either a brown dwarf embedded in an edge-on disk or a planet embedded in a low inclination disk, which is externally irradiated by the binary companion. Further observations with ALMA, aiming for high SNR detections of non-contaminated gas lines, are required to conclusively unveil the nature of the third object in FW Tau.

  4. The End of Protoplanetary Disk Evolution: An ALMA Survey of Upper Scorpius

    Science.gov (United States)

    Barenfeld, Scott A.; Carpenter, John M.; Sargent, Anneila I.; Ricci, Luca; Isella, Andrea

    2017-01-01

    The evolution of the mass of solids in circumstellar disks is a key factor in determining how planets form. Infrared observations have established that the dust in primordial disks vanishes around the majority of stars by an age of 5-10 Myr. However, how this disappearance proceeds is poorly constrained. Only with longer wavelength observations, where the dust emission is optically thin, is it possible to measure disk dust mass and how it varies as a function of age. To this end, we have obtained ALMA 0.88 mm observations of over 100 sources with suspected circumstellar disks in the Upper Scorpius OB Association (Upper Sco). The 5-11 Myr age of Upper Sco suggests that any such disks will be quite evolved, making this association an ideal target to compare to systems of younger disks in order to study evolution. With ALMA, we achieve an order of magnitude improvement in sensitivity over previous (sub)millimeter surveys of Upper Sco and detect 58 disks in the continuum. We calculate the total dust masses of these disks and compare their masses to those of younger disks in Taurus, Lupus, and Chamaeleon. We find strong evidence for a decline in disk dust mass between these 1-3 Myr old systems and the 5-11 Myr old Upper Sco. Our results represent the first definitive measurement of a decline in disk dust mass with age.

  5. 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.

  6. 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...

  7. 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...

  8. 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...

  9. 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 ...

  10. Scientific and technological Challenges in the development of astronomical instrumentation: E-ELT & ALMA

    Science.gov (United States)

    Barrado, David; Gallego, Jesús

    2009-12-01

    The answers to the present astrophysical questions require the development of highly sophisticated instrumentation, which needs long-term scheduling and large assets of human and material resources, managed by consortia of several institutions. Spain has carried in the last years serious efforts in this direction (GTC, ESO, ESA), but there is still a notable offset between astronomical research at the theoretical and observational levels and the development of instrumentation. Now, the incorporation of new countries to ESO (in particular Spain) to ESO and several future big projects (ALMA, E-ELT, Cosmic Vision), raise the level of exigency. The goal of this workshop is to gather the scientific teams and the industries of the sector to expose their needs and projects, and share experiences. The workshop is aimed as well at serving as an echo to convince financing agencies and the astronomical community in general of the need to promote with decision the development of astrophysical instrumentation and the tools for the analysis of related data. The formation and acknowledgement of instrumentation astronomers will be a key factor for Spain to meet the requirements of its position in Astronomy in the next decades. Here, we present the contributions most closely related to the development of E-ELT, ALMA and ESA missions.

  11. Alma Observations of Massive Molecular Gas Filaments Encasing Radio Bubbles in the Phoenix Cluster

    Science.gov (United States)

    Russell, H. R.; McDonald, M.; 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.

    2017-02-01

    We report new ALMA observations of the CO(3-2) line emission from the 2.1+/- 0.3× {10}10 {M}ȯ molecular gas reservoir in the central galaxy of the Phoenix cluster. The cold molecular gas is fueling a vigorous starburst at a rate of 500{--}800 {M}ȯ {{yr}}-1 and powerful black hole activity in the forms 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 {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 induced in low-entropy gas lifted in the updraft of the bubbles. These new data provide compelling evidence for close coupling between the radio bubbles and the cold gas, which is essential to explain the self-regulation of feedback. The very feedback mechanism that heats hot atmospheres and suppresses star formation may also paradoxically stimulate production of the cold gas required to sustain feedback in massive galaxies.

  12. 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...

  13. Declarative Modeling–An Academic Dream or the Future for BPM?

    DEFF Research Database (Denmark)

    Reijers, Hajo; Slaats, Tijs; Stahl, Christian

    2014-01-01

    Declarative modeling has attracted much attention over the last years, resulting in the development of several academic declarative modeling techniques and tools. The absence of empirical evaluations on their use and usefulness, however, raises the question whether practitioners are attracted...... to using those techniques. In this paper, we present a study on what practitioners think of declarative modeling. We show that the practitioners we involved in this study are receptive to the idea of a hybrid approach combining imperative and declarative techniques, rather than making a full shift from...

  14. 76 FR 32370 - Tennessee; Amendment No. 2 to Notice of a Major Disaster Declaration

    Science.gov (United States)

    2011-06-06

    ... declaration of May 1, 2011. Carroll, Crockett, Hardin, Henry, and Madison Counties for Individual Assistance. Benton, Carroll, Chester, Crockett, Fayette, Gibson, Hardeman, Hardin, Henderson, Henry, Lake,...

  15. 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

    Science.gov (United States)

    Jørgensen, J. K.; van der Wiel, M. H. D.; 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.

    2016-11-01

    Context. The inner regions of the envelopes surrounding young protostars are characterized by a complex chemistry, with prebiotic molecules present on the scales where protoplanetary disks eventually may form. The Atacama Large Millimeter/submillimeter Array (ALMA) provides an unprecedented view of these regions zooming in on solar system scales of nearby protostars and mapping the emission from rare species. Aims: The goal is to introduce a systematic survey, the Protostellar Interferometric Line Survey (PILS), of the chemical complexity of one of the nearby astrochemical templates, the Class 0 protostellar binary IRAS 16293-2422, using ALMA in order to understand the origin of the complex molecules formed in its vicinity. In addition to presenting the overall survey, the analysis in this paper focuses on new results for the prebiotic molecule glycolaldehyde, its isomers, and rarer isotopologues and other related molecules. Methods: An unbiased spectral survey of IRAS 16293-2422 covering the full frequency range from 329 to 363 GHz (0.8 mm) has been obtained with ALMA, in addition to a few targeted observations at 3.0 and 1.3 mm. The data consist of full maps of the protostellar binary system with an angular resolution of 0.5'' (60 AU diameter), a spectral resolution of 0.2 km s-1, and a sensitivity of 4-5 mJy beam-1 km s-1, which is approximately two orders of magnitude better than any previous studies. Results: More than 10 000 features are detected toward one component in the protostellar binary, corresponding to an average line density of approximately one line per 3 km s-1. Glycolaldehyde; its isomers, methyl formate and acetic acid; and its reduced alcohol, ethylene glycol, are clearly detected and their emission well-modeled with an excitation temperature of 300 K. For ethylene glycol both lowest state conformers, aGg' and gGg', are detected, the latter for the first time in the interstellar medium (ISM). The abundance of glycolaldehyde is comparable to or

  16. ALMA observations of anisotropic dust mass loss in the inner circumstellar environment of the red supergiant VY Canis Majoris

    NARCIS (Netherlands)

    O'Gorman, E.; Vlemmings, W.; Richards, A.M.S.; Baudry, A.; De Beck, E.; Decin, L.; Harper, G.M.; Humphreys, E.M.; Kervella, P.; Khouri, T.; Muller, S.

    2015-01-01

    The processes leading to dust formation and the subsequent role it plays in driving mass loss in cool evolved stars is an area of intense study. Here we present high resolution ALMA Science Verification data of the continuum emission around the highly evolved oxygen-rich red supergiant VY CMa. These

  17. Molecular line emission in NGC 1068 imaged with ALMA. II. The chemistry of the dense molecular gas

    NARCIS (Netherlands)

    Viti, S.; García-Burillo, S.; Fuente, A.; Hunt, L. K.; Usero, A.; Henkel, C.; Eckart, A.; Martin, S.; Spaans, M.; Muller, S.; Combes, F.; Krips, M.; Schinnerer, E.; Casasola, V.; Costagliola, F.; Marquez, I.; Planesas, P.; van der Werf, P. P.; Aalto, S.; Baker, A. J.; Boone, F.; Tacconi, L. J.

    2014-01-01

    Aims: We present a detailed analysis of Atacama Large Millimeter/submillimeter Array (ALMA) Bands 7 and 9 data of CO, HCO+, HCN, and CS, augmented with Plateau de Bure Interferometer (PdBI) data of the ~200 pc circumnuclear disc (CND) and the ~1.3 kpc starburst ring (SB ring) of NGC 1068, a nearby (

  18. An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: High resolution 870um source counts

    CERN Document Server

    Karim, Alexander; Hodge, Jackie; Smail, Ian; Walter, Fabian; Biggs, Andy; Simpson, James; Danielson, Alice; Alexander, David; Bertoldi, Frank; Chapman, Scott; Coppin, Kristen; Dannerbauer, Helmut; Edge, Alastair; Greve, Thomas; Ivison, Rob; Knudsen, Kirsten; Menten, Karl; Schinnerer, Eva; Wardlow, Julie; Weiß, Axel; van der Werf, Paul

    2012-01-01

    We report the first counts of faint submillimetre galaxies (SMG) in the 870-um band derived from arcsecond resolution observations with the Atacama Large Millimeter Array (ALMA). We have used ALMA to map a sample of 122 870-um-selected submillimetre sources drawn from the (0.5x0.5)deg^2 LABOCA Extended Chandra Deep Field South Submillimetre Survey (LESS). These ALMA maps have an average depth of sigma(870um)~0.4mJy, some ~3x deeper than the original LABOCA survey and critically the angular resolution is more than an order of magnitude higher, FWHM of ~1.5" compared to ~19" for the LABOCA discovery map. This combination of sensitivity and resolution allows us to precisely pin-point the SMGs contributing to the submillimetre sources from the LABOCA map, free from the effects of confusion. We show that our ALMA-derived SMG counts broadly agree with the submillimetre source counts from previous, lower-resolution single-dish surveys, demonstrating that the bulk of the submillimetre sources are not caused by blendi...

  19. Revolutionary thoughts on taxonomy: declarations of independence and interdependence

    Directory of Open Access Journals (Sweden)

    Quentin D. Wheeler

    2009-03-01

    Full Text Available Credible biological research depends on accurate species identifications, reliable scientific names, and an evolutionary context provided by a phylogeny or phylogenetic classification. The emphasis on such taxonomic services has detracted from the fundamental taxonomic research necessary to create and sustain such knowledge systems. A taxonomic declaration of independence is presented, emphasizing the unique mission, goals, and needs of taxonomists and taxonomic (collection-based institutions and the non-experimental yet scientifically rigorous epistemology of taxonomy. At the same time taxonomic interdependence is declared. Questions pursued by taxonomists are planetary in scale and can only be answered given international collaboration and coordination in the growth and development of natural history collections and taxonomic hypotheses. Reciprocity of open access is urged between all nations and the taxonomic community creating information. Countries home to species diversity should allow access to taxon experts so that the world's species are discovered and described. In exchange all specimens collected should be in publicly accessible museums and all resultant taxonomic data, information, and knowledge should be openly available to all who can use them.

  20. Product declaration for small refrigerators; Produktdeklaration fuer Kleinkuehlschraenke. Ausschreibungsformular - Schlussbericht

    Energy Technology Data Exchange (ETDEWEB)

    Burri, A.

    2008-07-01

    This final report for the Swiss Federal Office of Energy (SFOE) reports on a project that looked at the optimisation of cooling technology used in small refrigerators. This optimisation alone is considered as being not sufficient to increase the market perspectives for efficient refrigeration units. In contrast to household units, no energy declaration standards exist for the type of mini-bar used in hotel rooms. An 'Energy Declaration - Small Refrigerator' form created as a part of this project is discussed which makes it easier to compare the energy costs of various units. The form is based on uniform criteria, and increases the market perspectives for the most efficient units, even if they are somewhat more expensive. The Swiss Federal Office of Energy is now supplying this form (in German, French and Italian) to all manufacturers and vendors of small refrigerators. The vendor can fill out this form and include it in his offer. Likewise, the customer can request the form from the vendor. In this form the total energy costs for ten years of operation are added to the purchase price, so that the customer can obtain a clear indication of total life cycle costs.