WorldWideScience

Sample records for hubble witnesses fireworks

  1. Fireworks Information Center

    Science.gov (United States)

    ... or a garden hose handy in case of fire or other mishap. Light fireworks one at a time, then move back quickly. Never carry fireworks in a pocket or shoot them off in metal or glass containers. After fireworks complete ... it to prevent a trash fire. Make sure fireworks are legal in your area ...

  2. Should Fireworks Be Banned?

    Institute of Scientific and Technical Information of China (English)

    2011-01-01

    During the Spring Festival,which fell on February 3 this year,a large number of fires and injuries to people were triggered by fireworks. A new round of debate over whether to again put firework bans in place

  3. Come to the fireworks...

    CERN Multimedia

    2004-01-01

    Don't miss the Geneva Festival's (Fêtes de Genève) curtain-raising firework display, where CERN is the guest of honour. Inspired by the creation of the Universe, the big bang starts tonight (Friday 30 July) at 10.15 p.m. by the Lake.http://www.cern.ch/cern50/

  4. Edwin Hubble

    Institute of Scientific and Technical Information of China (English)

    泓傑

    2006-01-01

    Edwin Powell Hubble(1889—1953)was an American astronomer, renowned for his discovery of galaxies beyond the Milky Way and the cosmological Redshift. Hubble was a tall,elegant,athletic man who at age 30 had an

  5. PERSPECTIVE: Fireworks and radioactivity

    Science.gov (United States)

    Breitenecker, Katharina

    2009-09-01

    Katharina Breitenecker Fireworks, the one and only amongst all other pyrotechnic applications, have pleased the hearts and minds of billions of people all over the world for almost 1000 years. Even though pyrotechnics were originally developed in order to fulfil the needs of military purposes, fireworks began to form a unique part of the cultural heritage of many countries, presumably starting in ancient China during the Song Dynasty (960-1280 AD). Festivities like New Year's Eve, national holidays or activities like music festivals and parish fairs are crowned by a firework display. Fireworks have traditionally been associated with Independence Day celebrations, like 4 July in the United States, Guy Fawkes' Night (5 November) in Britain, or Bastille Day (14 July) in France. Much of Chinese culture is associated with the use of firecrackers to celebrate the New Year and other important occasions. The fascination of fireworks and firecrackers is due to the brilliant colours and booming noises, which have a universal appeal to our basic senses [1]. The basic components of any traditional civil firework is black powder, a mixture of about 75% potassium nitrate, 15% charcoal, and about 10% sulfur [2]. Without the addition of a colouring agent, the fuel would provide an almost white light. Therefore, several metal salts can be added to cause colourful luminescence upon combustion. In general barium is used to obtain a green coloured flame, strontium for red, copper for blue and sodium for yellow [2, 3]. The use of pyrotechnics has raised issues pertaining to health concerns. The health aspects are not only restricted to injuries by accidental ignition of certain devices. Moreover, several recent works identified fireworks and pyrotechnics as causing environmental pollution, which might result in a potential hazard concerning health aspects. The fundamental problem in this respect is that all chemicals used are dispersed in the environment by combustion. This includes

  6. Foundation Fireworks CS4

    CERN Document Server

    Smith, N; Heerema, Matt; Mallott, Chuch; King, R; Erskine, Craig

    2009-01-01

    Are you a web designer who is looking for a new and quicker way to prototype and create for the web? Perhaps you are a programmer who finds most design tools to be overkill for what you need to get done. Or, maybe you're an old Fireworks pro, who wants to keep up to date on the latest changes in Creative Suite 4. Either way, this book has something for you. * Coverage of all that's new and powerful for the Web designer and developer in Fireworks CS4* Targets developers who want design tools that don't get in their way and designers who want development tools that don't constrain their creativi

  7. Hubble Diagram

    Science.gov (United States)

    Djorgovski, S.; Murdin, P.

    2000-11-01

    Initially introduced as a way to demonstrate the expansion of the universe, and subsequently to determine the expansion rate (the HUBBLE CONSTANT H0), the Hubble diagram is one of the classical cosmological tests. It is a plot of apparent fluxes (usually expressed as magnitudes) of some types of objects at cosmological distances, against their REDSHIFTS. It is used as a tool to measure the glob...

  8. Facial Firework Injury: A Case Series

    Directory of Open Access Journals (Sweden)

    Kashyap Tadisina

    2014-07-01

    Full Text Available Fireworks are used to celebrate a variety of religious, patriotic, and cultural holidays and events around the world. Fireworks are common in the United States, with the most popular holiday for their use being national Independence Day, also known as July Fourth. The use of fireworks within the context of celebrations and holidays presents the ideal environment for accidents that lead to severe and dangerous injuries. Injuries to the face from explosions present a challenging problem in terms of restoring ideal ocular, oral, and facial function. Despite the well documented prevalence of firework use and injury, there is a relatively large deficit in the literature in terms of firework injury that involves the face. We present a unique case series that includes 4 adult male patients all with severe firework injuries to the face that presented at an urban level 1 trauma center. These four patients had an average age of 26.7 years old and presented within 5 hours of each other starting on July Fourth. Two patients died from their injuries and two patients underwent reconstructive surgical management, one of which had two follow up surgeries. We explore in detail their presentation, management, and subsequent outcomes as an attempt to add to the very limited data in the field of facial firework blast injury. In addition, the coincidence of their presentation within the same 5 hours brings into question the availability of the fireworks involved, and the possibility of similar injuries related to this type of firework in the future.

  9. COLORFUL FIREWORKS FINALE CAPS A STAR'S LIFE

    Science.gov (United States)

    2002-01-01

    Glowing gaseous streamers of red, white, and blue -- as well as green and pink -- illuminate the heavens like Fourth of July fireworks. The colorful streamers that float across the sky in this photo taken by NASA's Hubble Space Telescope were created by one of the biggest firecrackers seen to go off in our galaxy in recorded history, the titanic supernova explosion of a massive star. The light from the exploding star reached Earth 320 years ago, nearly a century before our United States celebrated its birth with a bang. The dead star's shredded remains are called Cassiopeia A, or 'Cas A' for short. Cas A is the youngest known supernova remnant in our Milky Way Galaxy and resides 10,000 light-years away in the constellation Cassiopeia, so the star actually blew up 10,000 years before the light reached Earth in the late 1600s. This stunning Hubble image of Cas A is allowing astronomers to study the supernova's remains with great clarity, showing for the first time that the debris is arranged into thousands of small, cooling knots of gas. This material eventually will be recycled into building new generations of stars and planets. Our own Sun and planets are constructed from the debris of supernovae that exploded billions of years ago. This photo shows the upper rim of the supernova remnant's expanding shell. Near the top of the image are dozens of tiny clumps of matter. Each small clump, originally just a small fragment of the star, is tens of times larger than the diameter of our solar system. The colors highlight parts of the debris where chemical elements are glowing. The dark blue fragments, for example, are richest in oxygen; the red material is rich in sulfur. The star that created this colorful show was a big one, about 15 to 25 times more massive than our Sun. Massive stars like the one that created Cas A have short lives. They use up their supply of nuclear fuel in tens of millions of years, 1,000 times faster than our Sun. With their fuel exhausted, heavy

  10. Equilibrium calculations of firework mixtures

    Energy Technology Data Exchange (ETDEWEB)

    Hobbs, M.L. [Sandia National Labs., Albuquerque, NM (United States); Tanaka, Katsumi; Iida, Mitsuaki; Matsunaga, Takehiro [National Inst. of Materials and Chemical Research, Tsukuba, Ibaraki (Japan)

    1994-12-31

    Thermochemical equilibrium calculations have been used to calculate detonation conditions for typical firework components including three report charges, two display charges, and black powder which is used as a fuse or launch charge. Calculations were performed with a modified version of the TIGER code which allows calculations with 900 gaseous and 600 condensed product species at high pressure. The detonation calculations presented in this paper are thought to be the first report on the theoretical study of firework detonation. Measured velocities for two report charges are available and compare favorably to predicted detonation velocities. However, the measured velocities may not be true detonation velocities. Fast deflagration rather than an ideal detonation occurs when reactants contain significant amounts of slow reacting constituents such as aluminum or titanium. Despite such uncertainties in reacting pyrotechnics, the detonation calculations do show the complex nature of condensed phase formation at elevated pressures and give an upper bound for measured velocities.

  11. Hubble, Hubble's law and the expanding universe

    OpenAIRE

    Bagla, J. S.

    2009-01-01

    Hubble's name is associated closely with the idea of an expanding universe as he discovered the relation between the recession velocity and distances of galaxies. Hubble also did a lot of pioneering work on the distribution of galaxies in the universe. In this article we take a look at Hubble's law and discuss how it relates with models of the universe. We also give a historical perspective of the discoveries that led to the Hubble's law.

  12. Hubble, Hubble's law and the expanding universe

    OpenAIRE

    Bagla, J. S.

    2009-01-01

    Hubble's name is associated closely with the idea of an expanding universe as he discovered the relation between the recession velocity and distances of galaxies. Hubble also did a lot of pioneering work on the distribution of galaxies in the universe. In this article we take a look at Hubble's law and discuss how it relates with models of the universe. We also give a historical perspective of the discoveries that led to the Hubble's law.

  13. Cosmic Collisions The Hubble Atlas of Merging Galaxies

    CERN Document Server

    Christensen, Lars Lindberg; Martin, Davide

    2009-01-01

    Lars Lindberg Christensen, Raquel Yumi Shida & Davide De Martin Cosmic Collisions: The Hubble Atlas of Merging Galaxies Like majestic ships in the grandest night, galaxies can slip ever closer until their mutual gravitational interaction begins to mold them into intricate figures that are finally, and irreversibly, woven together. It is an immense cosmic dance, choreographed by gravity. Cosmic Collisions contains a hundred new, many thus far unpublished, images of colliding galaxies from the NASA/ESA Hubble Space Telescope. It is believed that many present-day galaxies, including the Milky Way, were assembled from such a coalescence of smaller galaxies, occurring over billions of years. Triggered by the colossal and violent interaction between the galaxies, stars form from large clouds of gas in firework bursts, creating brilliant blue star clusters. The importance of these cosmic encounters reaches far beyond the stunning Hubble images. They may, in fact, be among the most important processes that shape ...

  14. Delivering Hubble Discoveries to the Classroom

    Science.gov (United States)

    Eisenhamer, B.; Villard, R.; Weaver, D.; Cordes, K.; Knisely, L.

    2013-04-01

    Today's classrooms are significantly influenced by current news events, delivered instantly into the classroom via the Internet. Educators are challenged daily to transform these events into student learning opportunities. In the case of space science, current news events may be the only chance for educators and students to explore the marvels of the Universe. Inspired by these circumstances, the education and news teams developed the Star Witness News science content reading series. These online news stories (also available in downloadable PDF format) mirror the content of Hubble press releases and are designed for upper elementary and middle school level readers to enjoy. Educators can use Star Witness News stories to reinforce students' reading skills while exposing students to the latest Hubble discoveries.

  15. Process simulation using WITNESS

    CERN Document Server

    Al-Aomar, Raid; Ulgen, Onur M

    2015-01-01

    Teaches basic and advanced modeling and simulation techniques to both undergraduate and postgraduate students and serves as a practical guide and manual for professionals learning how to build simulation models using WITNESS, a free-standing software package. This book discusses the theory behind simulation and demonstrates how to build simulation models with WITNESS. The book begins with an explanation of the concepts of simulation modeling and a "guided tour" of the WITNESS modeling environment. Next, the authors cover the basics of building simulation models using WITNESS and mode

  16. Consumers fireworks - Differences between European members states

    Energy Technology Data Exchange (ETDEWEB)

    Astondoa, I. [Pirotecnia Astondoa, S. A. (Spain); Rodriguez-Brunchu, G. [A..F. A. P. E. Pirotecnia S. A. (Spain)

    2000-04-01

    The availability of fireworks to consumers varies between European countries in terms of policies and legislation that control their sale, the types of fireworks legally available, the quantities and times of the year when fireworks can be purchased and used. The authors of this paper attempt to provide an assessment of the situation in seven member countries of the European Community, namely, the United Kingdom, Belgium, Denmark, France, Germany, the Netherlands and Spain. The quality and quantity of data available varies from country to country, however, the objectives of providing an up-to-date picture of the legislation, policies, classification, frequency of sale, age restrictions on purchase, and special prohibitions applicable to fireworks in each of the countries, is achieved. 1 ref., tabs.

  17. Can fireworks-related injuries to children during festivities be ...

    African Journals Online (AJOL)

    Most of the fireworks accidents occurred in or around the patients' homes. There were more fireworks-related injuries around Guy Fawkes Day (85%) than New Year's ... Current legislation should be more strictly enforced, especially the sale to ...

  18. The use of chemicals for fireworks

    Energy Technology Data Exchange (ETDEWEB)

    Lancaster, R. [Kimbolton Fireworks Limited (United Kingdom)

    2000-04-01

    The history of chemicals that over time have become the fundamental building blocks of pyrotechnic compositions, and newer materials that are part of many of today's fireworks formulations, are discussed. The relationship between fireworks and the discovery of gunpowder is revisited as an important event in the origin of fireworks. While charcoal and potassium chlorate are the principal ingredients, salts of antimony, arsenic mercury, mica, borax, some lead compounds and zinc filings, along with powdered glass and porcelain, also have been tried at various times and with varying degrees of success. Nitrates of strontium, barium and sodium have been used since the earliest times in the history of fireworks to produce colors, but potassium chlorate, mixed with sulphur and sugar provided the lifting powder that made possible the production of stars, although it also produced some very bad explosions throughout history. In more recent times, chlorinated compounds, magnesium and especially aluminum, have added considerable brilliance to fireworks. The problem of corrosion, hence limited shelf-life, however, continues to be a challenge. Reference is also made to the increasing volume of regulation in Western Europe that is pushing European fireworks manufacturers to extinction. 5 refs.

  19. Hubble's diagram and cosmic expansion

    OpenAIRE

    Kirshner, Robert P.

    2003-01-01

    Edwin Hubble's classic article on the expanding universe appeared in PNAS in 1929 [Hubble, E. P. (1929) Proc. Natl. Acad. Sci. USA 15, 168–173]. The chief result, that a galaxy's distance is proportional to its redshift, is so well known and so deeply embedded into the language of astronomy through the Hubble diagram, the Hubble constant, Hubble's Law, and the Hubble time, that the article itself is rarely referenced. Even though Hubble's distances have a large systematic error, Hubble's velo...

  20. Hubble's diagram and cosmic expansion

    OpenAIRE

    Kirshner, Robert P.

    2003-01-01

    Edwin Hubble's classic article on the expanding universe appeared in PNAS in 1929 [Hubble, E. P. (1929) Proc. Natl. Acad. Sci. USA 15, 168–173]. The chief result, that a galaxy's distance is proportional to its redshift, is so well known and so deeply embedded into the language of astronomy through the Hubble diagram, the Hubble constant, Hubble's Law, and the Hubble time, that the article itself is rarely referenced. Even though Hubble's distances have a large systematic error, Hubble's velo...

  1. Fireworks 小技巧

    Institute of Scientific and Technical Information of China (English)

    2002-01-01

    @@ 几个特殊的图像导出功能 一、"File/Export Special/Export as Files…" 这个功能一次性将各个图像元素导出为各自不同的文件,您可以在导出设置中修改"Files From"选项,使Fireworks2自动将层(layer)、静态图象部件(slic objects)或帧(frames)导出为独立的文件.我认为这个功能在您需要将一个有许多帧的gif动画一帧帧地导出为图片时能够为您省去许多麻烦.

  2. Constructing optimal entanglement witnesses

    Science.gov (United States)

    Chruściński, Dariusz; Pytel, Justyna; Sarbicki, Gniewomir

    2009-12-01

    We provide a class of indecomposable entanglement witnesses. In 4×4 case, it reproduces the well-known Breuer-Hall witness. We prove that these witnesses are optimal and atomic, i.e., they are able to detect the “weakest” quantum entanglement encoded into states with positive partial transposition. Equivalently, we provide a construction of indecomposable atomic maps in the algebra of 2k×2k complex matrices. It is shown that their structural physical approximations give rise to entanglement breaking channels. This result supports recent conjecture by Korbicz [Phys. Rev. A 78, 062105 (2008)].

  3. Witnessing the Future

    DEFF Research Database (Denmark)

    Elgaard Jensen, Torben

    2007-01-01

    the journalists into witnesses. It compares the manager's strategy to other cases of effective witnessing in courtrooms and in science. It concludes that the manager's persuasiveness is derived from his ability to articulate a series of pointed contrasts between the attractive working life within the firm......Abstract: The paper explores the phenomenon of witnessing the future through a case study of how a Scandinavian new economy firm managed to persuade a number of business journalists that it was "the future". It describes the procedures and rhetorical strategies that the manager deployed to turn...... and the problematic work life elsewhere. Finally, it notes that the manager's strategy enacts a timeworld characterised by dramatic epochal changes, which is radically different from the more stable and knowable time-world that is enacted in ordinary scientific discourses. Key words: actor-network theory, witnessing...

  4. Potential impact of fireworks on respiratory health

    Directory of Open Access Journals (Sweden)

    Caroline Gouder

    2014-01-01

    Full Text Available The world-wide use of fireworks with their consequent detrimental effect on the air quality is widely recognized with elevated ambient air levels of particulate matter and its several metallic components and gases identified in several studies carried out during such events. Exposed individuals may be at risk following inhalation of such produced pollutants. This review focuses on the impact of fireworks on air quality and the potential effect of fireworks on the respiratory system of healthy individuals as well as those suffering from underlying respiratory diseases, particularly asthma and chronic obstructive pulmonary disease (COPD. This applies not only to spectators including children but also to pyrotechnicians themselves. An extensive Medline search revealed that a strong evidence of the impact of fireworks on respiratory health is lacking in susceptible as well as healthy individuals with no formal studies on COPD or asthma, other than a few case reports in the latter. The implementation of global strategies to control the use of fireworks and hence improve air quality could possibly reduce their likely detrimental effect on human respiratory health in exposed individuals, but clearly a more targeted research is needed.

  5. Witnessing the Future

    Directory of Open Access Journals (Sweden)

    Torben Elgaard Jensen

    2007-01-01

    Full Text Available The paper explores the phenomenon of witnessing the future through a case study of how a Scandinavian new economy firm managed to persuade a number of business journalists that it was "the future". It describes the procedures and rhetorical strategies that the manager deployed to turn the journalists into witnesses. It compares the manager's strategy to other cases of effective witnessing in courtrooms and in science. It concludes that the manager's persuasiveness is derived from his ability to articulate a series of pointed contrasts between the attractive working life within the firm and the problematic work life elsewhere. Finally, it notes that the manager's strategy enacts a time-world characterised by dramatic epochal changes, which is radically different from the more stable and knowable time-world that is enacted in ordinary scientific discourses. URN: urn:nbn:de:0114-fqs070119

  6. Waste inspection tomography (WIT)

    Energy Technology Data Exchange (ETDEWEB)

    Bernardi, R.T. [Bio-Imaging Research, Inc., Lincolnshire, IL (United States)

    1995-10-01

    Waste Inspection Tomography (WIT) provides mobile semi-trailer mounted nondestructive examination (NDE) and assay (NDA) for nuclear waste drum characterization. WIT uses various computed tomography (CT) methods for both NDE and NDA of nuclear waste drums. Low level waste (LLW), transuranic (TRU), and mixed radioactive waste can be inspected and characterized without opening the drums. With externally transmitted x-ray NDE techniques, WIT has the ability to identify high density waste materials like heavy metals, define drum contents in two- and three-dimensional space, quantify free liquid volumes through density and x-ray attenuation coefficient discrimination, and measure drum wall thickness. With waste emitting gamma-ray NDA techniques, WIT can locate gamma emitting radioactive sources in two- and three-dimensional space, identify gamma emitting, isotopic species, identify the external activity levels of emitting gamma-ray sources, correct for waste matrix attenuation, provide internal activity approximations, and provide the data needed for waste classification as LLW or TRU.

  7. Seeing, Witnessing, Contributing

    DEFF Research Database (Denmark)

    Peters, Chris; Allan, Stuart

    on findings from a qualitative study of a demographic cohort often described as ‘millennial’ users (people born between 1980 and 1999) to consider: 1) respondents’ views regarding the prospective role of them bearing witness and what it entails; 2) suspected motivations of those engaging in this type...

  8. Victim/Witness Assistance.

    Science.gov (United States)

    Rosenblum, Robert H.; Blew, Carol Holliday

    This monograph highlights the elements of four victim-assistance programs which demonstrate the range of services currently being offered. It provides a preliminary look at the impact of such programs and points out where more information is needed. Major topics include victim and witness services and monitoring thereof. The two goals of…

  9. Hubble Deep Fields

    Science.gov (United States)

    Ferguson, H.; Murdin, P.

    2000-11-01

    The Hubble Deep Fields are two small areas of the sky that were carefully selected for deep observations by the HUBBLE SPACE TELESCOPE (HST). They represent the deepest optical observations to date and reveal galaxies as faint as V=30, 4 billion times fainter than can be seen with the unaided eye....

  10. The Management of Horses during Fireworks in New Zealand

    Directory of Open Access Journals (Sweden)

    Gabriella Gronqvist

    2016-03-01

    Full Text Available Within popular press there has been much coverage of the negative effects associated with firework and horses. The effect of fireworks has been documented in companion animals, yet no studies have investigated the negative effects, or otherwise, of fireworks on horses. This study aims to document horse responses and current management strategies to fireworks via an online survey. Of the total number of horses, 39% (1987/4765 were rated as “anxious”, 40% (1816/4765 “very anxious” and only 21% (965/4765 rated as “not anxious” around fireworks. Running (82%, 912/1107 was the most common behaviour reported, with no difference between property type (p > 0.05 or location (p > 0.05. Possibly as a consequence of the high frequency of running, 35% (384/1107 of respondents reported having horses break through fences in response to fireworks and a quarter (26%, 289/1099 reported that their horse(s had received injuries associated with fireworks. The most common management strategy was moving their horse(s to a paddock away from the fireworks (77% and to stable/yard them (55%. However, approximately 30% reported these management strategies to be ineffective. Of the survey participants, 90% (996/1104 were against the sale of fireworks for private use.

  11. ETHIOPIAN WITNESS PROTECTION SYSTEM: COMPARATIVE ...

    African Journals Online (AJOL)

    ANALYSIS WITH UNHCHR AND GOOD PRACTICES OF. WITNESS ... Oromia Justice Sector Professionals Training and Legal Research Institute; he can be reached at ... affect its implementation by comparing it with good practices of witness .... witness protection were a matter for individual police forces and approaches.

  12. Dismantling Hubble's Legacy?

    Science.gov (United States)

    Way, Michael J.

    2014-01-01

    Edwin Hubble is famous for a number of discoveries that are well known to amateur and professional astronomers, students and even the general public. The origins of three of the most well-known discoveries are examined: The distances to nearby spiral nebulae, the classification of extragalactic-nebulae and the Hubble constant. In the case of the first two a great deal of supporting evidence was already in place, but little credit was given. The Hubble Constant had already been estimated in 1927 by Georges Lemaitre with roughly the same value that Hubble obtained in 1929 using redshifts provided mostly by Vesto M. Slipher. These earlier estimates were not adopted or were forgotten by the astronomical community for complex scientific, sociological and psychological reasons.

  13. The Hubble effective potential

    Energy Technology Data Exchange (ETDEWEB)

    Janssen, T.M.; Miao, S.P.; Prokopec, T. [Institute for Theoretical Physics and Spinoza Institute, Utrecht University, Leuvenlaan 4, Postbus 80.195, 3508 TD Utrecht (Netherlands); Woodard, R.P., E-mail: T.M.Janssen@uu.nl, E-mail: S.Miao@uu.nl, E-mail: T.Prokopec@uu.nl, E-mail: woodard@phys.ufl.edu [Department of Physics, University of Florida, Gainesville, FL 32611 (United States)

    2009-05-15

    We generalize the effective potential to scalar field configurations which are proportional to the Hubble parameter of a homogeneous and isotropic background geometry. This may be useful in situations for which curvature effects are significant. We evaluate the one loop contribution to the Hubble Effective Potential for a massless scalar with arbitrary conformal and quartic couplings, on a background for which the deceleration parameter is constant. Among other things, we find that inflationary particle production leads to symmetry restoration at late times.

  14. 76 FR 38053 - Clarification of the Fireworks Approvals Policy

    Science.gov (United States)

    2011-06-29

    .... Background The pyrotechnic industry is a global logistics supply chain comprised of mostly foreign fireworks.... All participants throughout the supply chain will be held accountable for their regulatory... document. One commenter requests PHMSA consider waste management of used or defective fireworks...

  15. 78 FR 74048 - Eleventh Coast Guard District Annual Fireworks Events

    Science.gov (United States)

    2013-12-10

    ... following events. The first proposed safety zone is for the ``Colorado Belle & Edgewater Hotel/Casino... Hotel/Casino New Years Eve Fireworks'' event occurring on the lower Colorado River at Laughlin, NV. The... Laughlin Tourism Committee. Event Description Fireworks Display. Two events over the 4th of July...

  16. 36 CFR 331.5 - Explosives and fireworks.

    Science.gov (United States)

    2010-07-01

    ... 36 Parks, Forests, and Public Property 3 2010-07-01 2010-07-01 false Explosives and fireworks. 331... CONSERVATION AREA, KENTUCKY AND INDIANA § 331.5 Explosives and fireworks. Unless otherwise authorized in... or use of explosives is prohibited. ...

  17. Perioperative Jehovah's Witnesses: a review.

    Science.gov (United States)

    Lawson, T; Ralph, C

    2015-11-01

    There are many patient groups who may refuse blood products; the most well known amongst them is the Jehovah's Witness faith. Treatment of anaemia and bleeding in such patients presents a challenge to medical, anaesthetic, and surgical teams. This review examines the perioperative issues and management of Jehovah's Witnesses. The history and beliefs of Jehovah's Witnesses are outlined together with their impact on ethics and the law, and different management options throughout the perioperative period are discussed.

  18. Hubble's Nobel Prize

    CERN Document Server

    Soares, D S L

    2001-01-01

    Astronomy is not in the list of natural sciences aimed at by the Nobel awards. In spite of that, there were, throughout the 1930s until the early 1950s, effective moves by important scientists to distinguish Hubble with the Prize. A short report on these attempts is made as well as speculation on what would be the citation for the prize in view of the broad range of Hubble's scientific achievements. Within this context, the opportunity is also taken for publicizing the Crafoord Prize which does consider astronomy.

  19. Did Edwin Hubble plagiarize?

    CERN Document Server

    Shaviv, Giora

    2011-01-01

    Recently Block published an astro-ph [arXiv:1106.3928 (2011)] insinuating that Hubble censored a prior publication of his famous and seminal discovery of the expansion of the universe. This issue was investigated by us in detail as part of the book: The Quest for Chemical Element Genesis and What the Chemical Elements Tell about the Universe (Accepted for publication, Springer Pub. Heidelberg, 2011.) Since the book is due in few months, we extract here the relevant parts. Our summary: We exonerate Hubble from the charge that he censored or ignored or plagiarized Lemaitre's earlier theoretical discovery.

  20. Public fireworks displays -- legislation, regulation, and policies, -- Europe and America

    Energy Technology Data Exchange (ETDEWEB)

    Astondoa, I. [Pirotecnia Astondoa, S. A. (Spain); Rodriguez-Brunchu, G. [A..F. A. P. E. Pirotecnia S. A. (Spain)

    2000-04-01

    A brief description of the legislation regulating public fireworks displays in Denmark, France, Spain and the United States is provided. While the quality and completeness of the information varies from country to country, the paper manages to provide a reasonably accurate assessment of the current state of affairs in each of the target countries with respect to requirements for fireworks and equipment, operator qualifications, audience separation distances, and operator liability regarding damages or personal injuries or accidents arising from a fireworks display event. 3 refs., tabs.

  1. Hubble 15 years of discovery

    CERN Document Server

    Lindberg Christensen, Lars; Kornmesser, M

    2006-01-01

    Hubble: 15 Years of Discovery was a key element of the European Space Agency's 15th anniversary celebration activities for the 1990 launch of the NASA/ESA Hubble Space Telescope. As an observatory in space, Hubble is one of the most successful scientific projects of all time, both in terms of scientific output and its immediate public appeal.

  2. The Big Bang: Facial Trauma Caused by Recreational Fireworks.

    Science.gov (United States)

    Molendijk, Josher; Vervloet, Bob; Wolvius, Eppo B; Koudstaal, Maarten J

    2016-06-01

    In the Netherlands, it is a tradition of setting off fireworks to celebrate the turn of the year. In our medical facility, each year patients with severe skeletal maxillofacial trauma inflicted by recreational fireworks are encountered. We present two cases of patients with severe blast injury to the face, caused by direct impact of rockets, and thereby try to contribute to the limited literature on facial blast injuries, their treatment, and clinical outcome. These patients require multidisciplinary treatment, involving multiple reconstructive surgeries, and the overall recovery process is long. The severity of these traumas raises questions about the firework traditions and legislations not only in the Netherlands but also worldwide. Therefore, the authors support restrictive laws on personal use of fireworks in the Netherlands.

  3. Constructing new optimal entanglement witnesses

    CERN Document Server

    Chruscinski, Dariusz; Sarbicki, Gniewomir

    2009-01-01

    We provide a new class of indecomposable entanglement witnesses. In 4 x 4 case it reproduces the well know Breuer-Hall witness. We prove that these new witnesses are optimal and atomic, i.e. they are able to detect the "weakest" quantum entanglement encoded into states with positive partial transposition (PPT). Equivalently, we provide a new construction of indecomposable atomic maps in the algebra of 2k x 2k complex matrices. It is shown that their structural physical approximations give rise to entanglement breaking channels. This result supports recent conjecture by Korbicz et. al.

  4. The Hubble Exoplanet Classroom

    Science.gov (United States)

    Stevens, Laura; Carson, J.; Ruwadi, D.; Low, K.; Jordan, S.; Schneider, G.

    2013-01-01

    We present a status report on the Hubble Exoplanet Classroom, an interactive website designed to engage 8-12th grade students in physical science concepts using the exciting field of exoplanet studies. Addressing national teaching standards, the webpage allows educators to enhance their physical science, physics, and astronomy curriculum with student-driven lessons. The webpage records students' performance on lessons and quizzes and compiles the results, which can be accessed by the instructor using a secure website.

  5. Dismantling Hubble's Legacy?

    CERN Document Server

    Way, Michael J

    2013-01-01

    Edwin Hubble is famous for a number of discoveries that are well known to amateur and professional astronomers, students and the general public. The origins of these discoveries are examined and it is demonstrated that, in each case, a great deal of supporting evidence was already in place. In some cases the discoveries had either already been made, or competing versions were not adopted for complex scientific and sociological reasons.

  6. Dismantling Hubble's Legacy?

    Science.gov (United States)

    Way, Michael Joseph

    2013-01-01

    Edwin Hubble is famous for a number of discoveries that are well known to amateur and professional astronomers, students and the general public. The origins of these discoveries are examined and it is demonstrated that, in each case, a great deal of supporting evidence was already in place. In some cases the discoveries had either already been made, or competing versions were not adopted for complex scientific and sociological reasons.

  7. The Hubble Constant.

    Science.gov (United States)

    Jackson, Neal

    2015-01-01

    I review the current state of determinations of the Hubble constant, which gives the length scale of the Universe by relating the expansion velocity of objects to their distance. There are two broad categories of measurements. The first uses individual astrophysical objects which have some property that allows their intrinsic luminosity or size to be determined, or allows the determination of their distance by geometric means. The second category comprises the use of all-sky cosmic microwave background, or correlations between large samples of galaxies, to determine information about the geometry of the Universe and hence the Hubble constant, typically in a combination with other cosmological parameters. Many, but not all, object-based measurements give H0 values of around 72-74 km s(-1) Mpc(-1), with typical errors of 2-3 km s(-1) Mpc(-1). This is in mild discrepancy with CMB-based measurements, in particular those from the Planck satellite, which give values of 67-68 km s(-1) Mpc(-1) and typical errors of 1-2 km s(-1) Mpc(-1). The size of the remaining systematics indicate that accuracy rather than precision is the remaining problem in a good determination of the Hubble constant. Whether a discrepancy exists, and whether new physics is needed to resolve it, depends on details of the systematics of the object-based methods, and also on the assumptions about other cosmological parameters and which datasets are combined in the case of the all-sky methods.

  8. Cardiopulmonary bypass in Jehovah's Witnesses

    African Journals Online (AJOL)

    Jehovah's Witnesses do not accept heterologous blood transfusion for religious ... cuit allowed successful open-heart surgery using cardiop- ulmonary bypass. .... 2 after isovolaemic hacmodilution and was between 5.8g% (Hct. 17.4%) and ...

  9. Influences of fireworks on chemical characteristics of atmospheric fine and coarse particles during Taiwan's Lantern Festival

    Science.gov (United States)

    Tsai, Hsieh-Hung; Chien, Li-Hsing; Yuan, Chung-Shin; Lin, Yuan-Chung; Jen, Yi-Hsiu; Ie, Iau-Ren

    2012-12-01

    In recent years, the celebration activities of various folk-custom festivals have been getting more and more attention from the citizens in Taiwan. Festivities throughout the whole island are traditionally accompanied by loud and brightly colored firework displays. Among these activities, the firework displays during Taiwan's Lantern Festival in Kaohsiung harbor is one of the largest festivals in Taiwan each year. Therefore, it is of importance to investigate the influence of fireworks displays on the ambient air quality during the Taiwan's Lantern Festival. Field measurements of atmospheric particulate matter (PM) were conducted on February 9th-11th, 2009 during Taiwan's Lantern Festival in Kaohsiung City. Moreover, three kinds of fireworks powders obtained from the same manufacturing factory producing Kaohsiung Lantern Festival fireworks were burned in a self-designed combustion chamber to determine the physicochemical properties of the fireworks' particles and to establish the source profile of firework burning. Several metallic elements of PM during the firework display periods were notably higher than those during the non-firework periods. The concentrations of Mg, K, Pb, and Sr in PM2.5 during the firework periods were 10 times higher than those during the non-firework periods. Additionally, the Cl-/Na+ ratio was approximately 3 during the firework display periods as Cl- came from the chlorine content of the firework powder. Moreover, the OC/EC ratio increased up to 2.8. Results obtained from PCA and CMB receptor modeling showed that major sources of atmospheric particles during the firework display periods in Kaohsiung harbor were fireworks, vehicular exhausts, soil dusts and marine sprays. Particularly, on February 10th, the firework displays contributed approximately 25.2% and 16.6% of PM10 at two downwind sampling sites, respectively.

  10. 78 FR 45061 - Safety Zone; Sister Bay Marina Fest Fireworks and Ski Show, Sister Bay, WI

    Science.gov (United States)

    2013-07-26

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Sister Bay Marina Fest Fireworks and Ski... intended to restrict vessels from a portion of Sister Bay due to a fireworks display and ski show. This... with the fireworks display and ski show in Sister Bay on August 31, 2013. DATES: This rule is...

  11. 77 FR 29251 - Safety Zone; Carnival Fireworks Display, Nantasket Beach, Hull, MA

    Science.gov (United States)

    2012-05-17

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Carnival Fireworks Display, Nantasket Beach... vicinity of Hull, MA for a Carnival fireworks display. This temporary safety zone is necessary to protect... Youth Football is sponsoring a Carnival fireworks display on the waters off of Nantasket Beach in the...

  12. 33 CFR 165.1191 - Safety zones: Northern California annual fireworks events.

    Science.gov (United States)

    2010-07-01

    ... Sausalito. Event Description Fireworks Display. Date July 4th. Location 1,000 feet off-shore from Sausalito... Sponsor North Tahoe Fire Protection District. Event Description Fireworks Display. Date July 4th. Location... radius of the launch platform. July 4th Fireworks Display Sponsor North Tahoe Fire Protection...

  13. 77 FR 57494 - Safety Zone; Fleet Week Fireworks, San Francisco Bay, San Francisco, CA

    Science.gov (United States)

    2012-09-18

    ... SECURITY Coast Guard 33 CFR Part 165 Safety Zone; Fleet Week Fireworks, San Francisco Bay, San Francisco... will enforce the safety zone for the Fleet Week Fireworks in the Captain of the Port, San Francisco...'' W (NAD83) for the Fleet Week Fireworks in 33 CFR 165.1191, Table 1, item number 25. This safety...

  14. 77 FR 40511 - Safety Zone; GR Symphony Fireworks Display, Kalamazoo Lake, Saugatuck, MI

    Science.gov (United States)

    2012-07-10

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; GR Symphony Fireworks Display, Kalamazoo... restrict vessels from a portion of Kalamazoo Lake during the GR Symphony Fireworks display. This temporary... the safety of spectators and vessels during the GR Symphony Fireworks. This zone will be effective...

  15. 77 FR 39406 - Safety Zone; Tom Graves Memorial Fireworks, Port Bay, Wolcott, NY

    Science.gov (United States)

    2012-07-03

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Tom Graves Memorial Fireworks, Port Bay... from a portion of Port Bay during the Tom Graves Memorial Fireworks display. This temporary safety zone... vessels during the Tom Graves Memorial Fireworks. This zone will be effective and enforced from 9:30 p.m...

  16. 76 FR 30584 - Safety Zones; Eleventh Coast Guard District Annual Fireworks Events

    Science.gov (United States)

    2011-05-26

    ... National Technology Transfer and Advancement Act (NTTAA) (15 U.S.C. 272 note) directs agencies to use... fireworks display. 28. San Francisco New Years Eve Fireworks Display Sponsor City of San Francisco. Event Description Fireworks Display. Date New Years Eve, December 31st. Location 1,000 feet off Pier 2,...

  17. 76 FR 7131 - Safety Zones; Eleventh Coast Guard District Annual Fireworks Events

    Science.gov (United States)

    2011-02-09

    ... National Technology Transfer and Advancement Act (NTTAA) (15 U.S.C. 272 note) directs agencies to use... fireworks display. 28. San Francisco New Years Eve Fireworks Display Sponsor City of San Francisco. Event Description Fireworks Display. Date New Years Eve, December 31st. Location 1,000 feet off Pier 2,...

  18. 76 FR 50669 - Safety Zones; Eleventh Coast Guard District Annual Fireworks Events

    Science.gov (United States)

    2011-08-16

    ... under Executive Order 13211. Technical Standards The National Technology Transfer and Advancement Act... fireworks display. 28. San Francisco New Years Eve Fireworks Display Sponsor City of San Francisco. Event Description Fireworks Display. Date New Years Eve, December 31st. Location 1,000 feet off Pier 2,...

  19. Southern Fireworks above ESO Telescopes

    Science.gov (United States)

    1999-05-01

    are brief flashes of high-energy radiation. Satellites in orbit around the Earth and spacecraft in interplanetary orbits have detected several thousand such events since they were first discovered in the late 1960s. Earlier investigations established that they were so evenly distributed in the sky that they must be very distant (and hence very powerful) outbursts of some kind. Only in 1997 it became possible to observe the fading "afterglow" of one of these explosions in visible light, thanks to accurate positions available from the BeppoSAX satellite. Soon thereafter, another optical afterglow was detected; it was located in a faint galaxy whose distance could be measured. In 1998, a gamma-ray burst was detected in a galaxy over 8,300 million light-years away. Even the most exotic ideas proposed for these explosions, e.g. supergiant stars collapsing to black holes, black holes merging with neutron stars or other black holes, and other weird and wonderful notions have trouble accounting for explosions with the power of 10,000 million million suns. [2] The various reports issued by astronomers working on this and other gamma-ray burst events are available as GCN Circulars on the GRB Coordinates Network web-noteboard. [3] See also the Press Release, issued by SAAO on this occasion. [4] In astronomy, the redshift (z) denotes the fraction by which the lines in the spectrum of an object are shifted towards longer wavelengths. The observed redshift of a distant galaxy or intergalactic cloud gives a direct estimate of the universal expansion (i.e. the "recession velocity"). The detailed relation between redshift and distance depends on such quantities as the Hubble Constant, the average density of the universe, and the 'cosmological' Constant. For a standard cosmological model, redshift z = 1.6 corresponds to a distance of about 7,000 million light-years. [5] Assuming a Hubble Constant H 0 = 70 km/s/Mpc, mean density Omega 0 = 0.3 and a Cosmological Constant Lambda = 0. How

  20. The Hubble Constant

    Directory of Open Access Journals (Sweden)

    Neal Jackson

    2015-09-01

    Full Text Available I review the current state of determinations of the Hubble constant, which gives the length scale of the Universe by relating the expansion velocity of objects to their distance. There are two broad categories of measurements. The first uses individual astrophysical objects which have some property that allows their intrinsic luminosity or size to be determined, or allows the determination of their distance by geometric means. The second category comprises the use of all-sky cosmic microwave background, or correlations between large samples of galaxies, to determine information about the geometry of the Universe and hence the Hubble constant, typically in a combination with other cosmological parameters. Many, but not all, object-based measurements give H_0 values of around 72–74 km s^–1 Mpc^–1, with typical errors of 2–3 km s^–1 Mpc^–1. This is in mild discrepancy with CMB-based measurements, in particular those from the Planck satellite, which give values of 67–68 km s^–1 Mpc^–1 and typical errors of 1–2 km s^–1 Mpc^–1. The size of the remaining systematics indicate that accuracy rather than precision is the remaining problem in a good determination of the Hubble constant. Whether a discrepancy exists, and whether new physics is needed to resolve it, depends on details of the systematics of the object-based methods, and also on the assumptions about other cosmological parameters and which datasets are combined in the case of the all-sky methods.

  1. The Carnegie Hubble Program

    Science.gov (United States)

    Freedman, Wendy L.; Madore, Barry F.; Scowcroft, Vicky; Mnso, Andy; Persson, S. E.; Rigby, Jane; Sturch, Laura; Stetson, Peter

    2011-01-01

    We present an overview of and preliminary results from an ongoing comprehensive program that has a goal of determining the Hubble constant to a systematic accuracy of 2%. As part of this program, we are currently obtaining 3.6 micron data using the Infrared Array Camera (IRAC) on Spitzer, and the program is designed to include JWST in the future. We demonstrate that the mid-infrared period-luminosity relation for Cepheids at 3.6 microns is the most accurate means of measuring Cepheid distances to date. At 3.6 microns, it is possible to minimize the known remaining systematic uncertainties in the Cepheid extragalactic distance scale. We discuss the advantages of 3.6 micron observations in minimizing systematic effects in the Cepheid calibration of the Hubble constant including the absolute zero point, extinction corrections, and the effects of metallicity on the colors and magnitudes of Cepheids. We are undertaking three independent tests of the sensitivity of the mid-IR Cepheid Leavitt Law to metallicity, which when combined will allow a robust constraint on the effect. Finally, we are providing a new mid-IR Tully-Fisher relation for spiral galaxies.

  2. Hubble Space Telescope satellite

    Science.gov (United States)

    Mitchell, R. E.

    1985-01-01

    The Hubble Space Telescope, named for the American astronomer Edwin Powell Hubble, will be the largest and most powerful astronomical instrument ever orbited. Placed above the obscuring effects of the earth's atmosphere in a 600-km orbit, this remotely-controlled, free-flying satellite observatory will expand the terrestrial-equivalent resolution of the universe by a factor of seven, or a volumetric factor of 350. This telescope has a 2.4-m primary mirror and can accommodate five scientific instruments (cameras, spectrographs and photometers). The optics are suitable for a spectral range from 1100 angstrom to 1 mm wavelength. With a projected service life of fifteen years, the spacecraft can be serviced on-orbit for replacement of degraded systems, to insert advanced scientific instruments, and to reboost the telescope from decayed altitudes. The anticipated image quality will be a result of extremely precise lambda/20 optics, stringent cleanliness, and very stable pointing: jitter will be held to less than 0.01 arcsecond for indefinite observation periods, consistent with instrument apertures as small as 0.1 arcsecond.

  3. The Carnegie Hubble Program

    CERN Document Server

    Freedman, Wendy L; Scowcroft, Vicky; Monson, Andy; Persson, S E; Seibert, Mark; Rigby, Jane; Sturch, Laura; Stetson, Peter

    2011-01-01

    We present an overview of and preliminary results from an ongoing comprehensive program that has a goal of determining the Hubble constant to a systematic accuracy of 2%. As part of this program, we are currently obtaining 3.6 micron data using the Infrared Array Camera (IRAC) on Spitzer, and the program is designed to include JWST in the future. We demonstrate that the mid-infrared period-luminosity relation for Cepheids at 3.6 microns is the most accurate means of measuring Cepheid distances to date. At 3.6 microns, it is possible to minimize the known remaining systematic uncertainties in the Cepheid extragalactic distance scale. We discuss the advantages of 3.6 micron observations in minimizing systematic effects in the Cepheid calibration of the Hubble constant including the absolute zero point, extinction corrections, and the effects of metallicity on the colors and magnitudes of Cepheids. We are undertaking three independent tests of the sensitivity of the mid-IR Cepheid Leavitt Law to metallicity, whi...

  4. Expert witness and Jungian archetypes.

    Science.gov (United States)

    Lallave, Juan Antonio; Gutheil, Thomas Gordon

    2012-01-01

    Jung's theories of archetype, shadow, and the personal and collective unconscious provide a postmodern framework in which to consider the role of the expert witness in judicial proceedings. Archetypal themes, motifs, and influences help to illuminate the shadow of the judicial system and projections and behaviors among the cast of the court in pursuing justice. This article speaks to archetypal influences and dialectical tensions encountered by the expert witness in this judicial drama. The archetype of Justice is born from the human need for order and relational fairness in a world of chaos. The persona of justice is the promise of truth in the drama. The shadow of justice is untruth, the need to win by any means. The dynamics of the trickster archetype serve and promote injustice. These influences are examined by means of a case example. This approach will deepen understanding of court proceedings and the role of the expert witness in the heroic quest for justice.

  5. Environmental impacts of perchlorate with special reference to fireworks--a review.

    Science.gov (United States)

    Sijimol, M R; Mohan, Mahesh

    2014-11-01

    Perchlorate is an inorganic anion that is used in solid rocket propellants, fireworks, munitions, signal flares, etc. The use of fireworks is identified as one of the main contributors in the increasing environmental perchlorate contamination. Although fireworks are displayed for entertainment, its environmental costs are dire. Perchlorates are also emerging as potent thyroid disruptors, and they have an impact on the ecology too. Many studies have shown that perchlorate contaminates the groundwater and the surface water, especially in the vicinity of fireworks manufacturing sites and fireworks display sites. The health and ecological impacts of perchlorate released in fireworks are yet to be fully assessed. This paper reviews fireworks as a source of perchlorate contamination and its expected adverse impacts.

  6. Cosmology: From Hubble to HST

    Energy Technology Data Exchange (ETDEWEB)

    Turner, Michael S.

    1997-03-01

    The Hubble constant sets the size and age of the Universe, and, together with independent determinations of the age, provides a consistency check of the standard cosmology. The Hubble constant also provides an important test of our most attractive paradigm for extending the standard cosmology, inflation and cold dark matter.

  7. Fireworks algorithm for mean-VaR/CVaR models

    Science.gov (United States)

    Zhang, Tingting; Liu, Zhifeng

    2017-10-01

    Intelligent algorithms have been widely applied to portfolio optimization problems. In this paper, we introduce a novel intelligent algorithm, named fireworks algorithm, to solve the mean-VaR/CVaR model for the first time. The results show that, compared with the classical genetic algorithm, fireworks algorithm not only improves the optimization accuracy and the optimization speed, but also makes the optimal solution more stable. We repeat our experiments at different confidence levels and different degrees of risk aversion, and the results are robust. It suggests that fireworks algorithm has more advantages than genetic algorithm in solving the portfolio optimization problem, and it is feasible and promising to apply it into this field.

  8. The Hubble Constant

    Directory of Open Access Journals (Sweden)

    Jackson Neal

    2007-09-01

    Full Text Available I review the current state of determinations of the Hubble constant, which gives the length scale of the Universe by relating the expansion velocity of objects to their distance. In the last 20 years, much progress has been made and estimates now range between 60 and 75 km s^-1 Mpc^-1, with most now between 70 and 75 km s^-1 Mpc^-1, a huge improvement over the factor-of-2 uncertainty which used to prevail. Further improvements which gave a generally agreed margin of error of a few percent rather than the current 10% would be vital input to much other interesting cosmology. There are several programmes which are likely to lead us to this point in the next 10 years.

  9. Constructing optimal entanglement witnesses. II

    CERN Document Server

    Chruscinski, Dariusz

    2010-01-01

    We provide a class of optimal nondecomposable entanglement witnesses for 4N x 4N composite quantum systems or, equivalently, a new construction of nondecomposable positive maps in the algebra of 4N x 4N complex matrices. This construction provides natural generalization of the Robertson map. It is shown that their structural physical approximations give rise to entanglement breaking channels.

  10. Expanding space, quasars and St. Augustine's fireworks

    CERN Document Server

    Chashchina, O I

    2014-01-01

    An attempt is made to explain time non-dilation allegedly observed in quasar light curves. The explanation is based on the assumption that quasar black holes are, in some sense, foreign for our Friedmann-Robertson-Walker universe and do not participate in the Hubble flow. Although at first sight such a weird explanation requires unreasonably fine-tuned Big Bang initial conditions, we find a natural justification for it using the Milne cosmological model as an inspiration.

  11. Expanding Space, Quasars and St. Augustine's Fireworks

    Science.gov (United States)

    Chashchina, Olga; Silagadze, Zurab

    2015-10-01

    An attempt is made to explain time non-dilation allegedly observed in quasar light curves. The explanation is based on the assumption that quasar black holes are, in some sense, foreign for our Friedmann-Robertson-Walker universe and do not participate in the Hubble flow. Although at first sight such a weird explanation requires unreasonably fine-tuned Big Bang initial conditions, we find a natural justification for it using the Milne cosmological model as an inspiration.

  12. HUBBLE VISION: A Planetarium Show About Hubble Space Telescope

    Science.gov (United States)

    Petersen, Carolyn Collins

    1995-05-01

    In 1991, a planetarium show called "Hubble: Report From Orbit" outlining the current achievements of the Hubble Space Telescope was produced by the independent planetarium production company Loch Ness Productions, for distribution to facilities around the world. The program was subsequently converted to video. In 1994, that program was updated and re-produced under the name "Hubble Vision" and offered to the planetarium community. It is periodically updated and remains a sought-after and valuable resource within the community. This paper describes the production of the program, and the role of the astronomical community in the show's production (and subsequent updates). The paper is accompanied by a video presentation of Hubble Vision.

  13. Entanglement witnessing in superconducting beamsplitters

    Science.gov (United States)

    Soller, H.; Hofstetter, L.; Reeb, D.

    2013-06-01

    We analyse a large class of superconducting beamsplitters for which the Bell parameter (CHSH violation) is a simple function of the spin detector efficiency. For these superconducting beamsplitters all necessary information to compute the Bell parameter can be obtained in Y-junction setups for the beamsplitter. Using the Bell parameter as an entanglement witness, we propose an experiment which allows to verify the presence of entanglement in Cooper pair splitters.

  14. A characterization of optimal entanglement witnesses

    CERN Document Server

    Qi, Xiaofei

    2011-01-01

    In this paper, we present a characterization of optimal entanglement witnesses in terms of positive maps and then provide a general method of checking optimality of entanglement witnesses. Applying it, we obtain new indecomposable optimal witnesses which have no spanning property. These also provide new examples which support a recent conjecture saying that the so-called structural physical approximations to optimal positive maps (optimal entanglement witnesses) give entanglement breaking maps (separable states).

  15. Fireworks induced particle pollution: A spatio-temporal analysis

    Science.gov (United States)

    Kumar, M.; Singh, R. K.; Murari, V.; Singh, A. K.; Singh, R. S.; Banerjee, T.

    2016-11-01

    Diwali-specific firework induced particle pollution was measured in terms of aerosol mass loading, type, optical properties and vertical distribution. Entire nation exhibited an increase in particulate concentrations specifically in Indo-Gangetic Plain (IGP). Aerosol surface mass loading at middle IGP revealed an increase of 56-121% during festival days in comparison to their background concentrations. Space-borne measurements (Aqua and Terra-MODIS) typically identified IGP with moderate to high AOD (0.3-0.8) during pre-festive days which transmutes to very high AOD (0.4-1.8) during Diwali-day with accumulation of aerosol fine mode fractions (0.3-1.0). Most of the aerosol surface monitoring stations exhibited increase in PM2.5 especially on Diwali-day while PM10 exhibited increase on subsequent days. Elemental compositions strongly support K, Ba, Sr, Cd, S and P to be considered as firework tracers. The upper and middle IGP revealed dominance of absorbing aerosols (OMI-AI: 0.80-1.40) while CALIPSO altitude-orbit-cross-section profiles established the presence of polluted dust which eventually modified with association of smoke and polluted continental during extreme fireworks. Diwali-specific these observations have implications on associating fireworks induced particle pollution and human health while inclusion of these observations should improve regional air quality model.

  16. 43 CFR 423.30 - Weapons, firearms, explosives, and fireworks.

    Science.gov (United States)

    2010-10-01

    ... 43 Public Lands: Interior 1 2010-10-01 2010-10-01 false Weapons, firearms, explosives, and... WATERBODIES Rules of Conduct § 423.30 Weapons, firearms, explosives, and fireworks. (a) You may possess... exceptions: (1) You must not have a weapon in your possession when at or in a Reclamation facility. (2) You...

  17. `EXPLONET`- an Internet-based module for family fireworks safety

    Energy Technology Data Exchange (ETDEWEB)

    Corbett, G. [Natural Resources Canada, Explosives Regulatory Division, Ottawa, ON (Canada); Brown, J. [Health Canada, Laboratory Center for Disease Control, Ottawa, ON (Canada)

    1998-12-01

    In an effort to reduce preventable injuries resulting from family fireworks displays, the Explosives Regulatory Division of Natural Resources Canada is developing a client service regulatory package - EXPLONET - which will be made available on the Internet. EXPLONET includes several components which address industry and public concerns. The initial component described here is the family educational safety module, designed to deal with the safe use of family fireworks. The objective is to reduce injuries to elementary school-age children through the delivery of an Internet-based lesson plan. The lesson plan is expected to be implemented on a pilot program basis to reach the target audience during the 1998 Halloween season when the use of fireworks is high. The lesson plan consists of four units and will be delivered over a period of four weeks prior to Hallo wen. Students will be active participants in the web-based sessions. The sessions will cover off-aspects of mathematics, history and science clustered around the central theme of fireworks safety, presented in a way to keep the children interested. The lesson will also include follow-up queries after Hallo wen, providing the children (and teachers) the opportunity to comment on what they have learned, and to identify product or safety improvements. Provision is also made for parent involvement. The module will be implemented on a pilot project basis in two schools, one in Nova Scotia and one in British Columbia. 6 refs., 1 tab., 10 figs.

  18. 76 FR 28312 - Safety Zones; Fireworks Display Kanawha River, WV

    Science.gov (United States)

    2011-05-17

    ... Federal Register (73 FR 3316). Public Meeting We do not now plan to hold a public meeting. But you may... West Virginia Special Olympics Fireworks Display, is located between mile 57.9 and 58.9 in Charleston... of Energy Effects under Executive Order 13211. Technical Standards The National Technology...

  19. 75 FR 35968 - Safety Zone; Fireworks Display in Stevenson, WA

    Science.gov (United States)

    2010-06-24

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Fireworks Display in Stevenson, WA AGENCY... temporary safety zone covering the waters of the Columbia River in the vicinity of Stevenson, Washington... Columbia River in the vicinity of Stevenson, Washington. Specifically, the safety zone would include...

  20. HUBBLE CAPTURES DYNAMICS OF CRAB NEBULA (color)

    Science.gov (United States)

    2002-01-01

    A new sequence of Hubble Space Telescope images of the remnant of a tremendous stellar explosion is giving astronomers a remarkable look at the dynamic relationship between the tiny Crab Pulsar and the vast nebula that it powers. This colorful photo shows a ground-based image of the entire Crab Nebula, the remnant of a supernova explosion witnessed over 900 years ago. The nebula, which is 10 light-years across, is located 7,000 light-years away in the constellation Taurus. The green, yellow and red filaments concentrated toward the edges of the nebula are remnants of the star that were ejected into space by the explosion. At the center of the Crab Nebula lies the Crab Pulsar -- the collapsed core of the exploded star. The Crab Pulsar is a rapidly rotating neutron star -- an object only about six miles across, but containing more mass than our Sun. As it rotates at a rate of 30 times per second the Crab Pulsar's powerful magnetic field sweeps around, accelerating particles, and whipping them out into the nebula at speeds close to that of light. The blue glow in the inner part of the nebula -- light emitted by energetic electrons as they spiral through the Crab's magnetic field -- is powered by the Crab Pulsar. Credit: Jeff Hester and Paul Scowen (Arizona State University), and NASA

  1. [Evaluation of Wits appraisal with superimposition method].

    Science.gov (United States)

    Xu, T; Ahn, J; Baumrind, S

    1999-07-01

    To compare the conventional Wits appraisal with superimposed Wits appraisal in evaluation of sagittal jaw relationship change between pre and post orthodontic treatment. The sample consists of 48-case pre and post treatment lateral head films. Computerized digitizing is used to get the cephalometric landmarks and measure conventional Wits value, superimposed Wits value and ANB angle. The correlation analysis among these three measures was done by SAS statistical package. The change of ANB angle has higher correlation with the change of superimposed Wits than that of the conventional Wits. The r-value is as high as 0.849 (P < 0.001). The superimposed Wits appraisal reflects the change of sagittal jaw relationship more objectively than the conventional one.

  2. Planck Scale to Hubble Scale

    CERN Document Server

    Sidharth, B G

    1998-01-01

    Within the context of the usual semi classical investigation of Planck scale Schwarzchild Black Holes, as in Quantum Gravity, and later attempts at a full Quantum Mechanical description in terms of a Kerr-Newman metric including the spinorial behaviour, we attempt to present a formulation that extends from the Planck scale to the Hubble scale. In the process the so called large number coincidences as also the hitherto inexplicable relations between the pion mass and the Hubble Constant, pointed out by Weinberg, turn out to be natural consequences in a consistent description.

  3. How to construct indecomposable entanglement witnesses

    Energy Technology Data Exchange (ETDEWEB)

    Chruscinski, Dariusz; Kossakowski, Andrzej [Institute of Physics, Nicolaus Copernicus University, Grudziadzka 5/7, 87-100 Torun (Poland)

    2008-04-11

    We present a very simple method for constructing indecomposable entanglement witnesses out of a given pair-an entanglement witness W and the corresponding state detected by W. This method may be used to produce new classes of atomic witnesses which are able to detect the 'weakest' quantum entanglement. Actually, it works perfectly in the multipartite case, too. Moreover, this method provides a powerful tool for constructing new examples of bound entangled states.

  4. How to construct indecomposable entanglement witnesses

    Science.gov (United States)

    Chruściński, Dariusz; Kossakowski, Andrzej

    2008-04-01

    We present a very simple method for constructing indecomposable entanglement witnesses out of a given pair—an entanglement witness W and the corresponding state detected by W. This method may be used to produce new classes of atomic witnesses which are able to detect the 'weakest' quantum entanglement. Actually, it works perfectly in the multipartite case, too. Moreover, this method provides a powerful tool for constructing new examples of bound entangled states.

  5. Effect of fireworks on ambient air quality in Malta

    Science.gov (United States)

    Camilleri, Renato; Vella, Alfred J.

    2010-11-01

    Religious festivals ( festas) in the densely populated Maltese archipelago (Central Mediterranean) are ubiquitous during summer when 86 of them are celebrated between June and October, each involving the burning of fireworks both in ground and aerial displays over a period of 3 days or longer per festival. We assessed the effect of fireworks on the air quality by comparing PM 10 and its content of Al, Ba, Cu, Sr and Sb which materials are used in pyrotechnic compositions. PM 10 was collected mainly from two sites, one in Malta (an urban background site) and the other in Gozo (a rural site) during July-August 2005 when 59 feasts were celebrated and September-October 2005 when only 11 feasts occurred. For both Malta and Gozo, PM 10 and metal concentration levels measured as weekly means were significantly higher during July-August compared to September-October and there exist strong correlations between PM 10 and total metal content. Additionally, for Malta dust, Al, Ba, Cu and Sr correlated strongly with each other and also with total concentration of all five metals. The same parameters measured in April 2006 in Malta were at levels similar to those found in the previous October. Ba and Sb in dust from the urban background site in Malta during July-August were at comparable or higher concentration than recently reported values in PM 10 from a heavily-trafficked London road and this suggests that these metals are locally not dominated by sources from roadside materials such as break liner wear but more likely by particulate waste from fireworks. Our findings point to the fact that festa firework displays contribute significantly and for a prolonged period every year to airborne dust in Malta where PM 10 is an intractable air quality concern. The presence in this dust of elevated levels of Ba and especially Sb, a possible carcinogen, is of concern to health.

  6. 76 FR 33639 - Safety Zone; New York Water Taxi 10th Anniversary Fireworks

    Science.gov (United States)

    2011-06-09

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; New York Water Taxi 10th Anniversary... to celebrate the 10th Anniversary of New York Water Taxi. The fireworks will commence at 9 p.m. on... Water Taxi 10th Anniversary Fireworks, Upper New York Bay, Red Hook, NY. (a) Location. The following...

  7. 78 FR 39601 - Safety Zone, Sugar House Casino Fireworks Display, Delaware River; Philadelphia, PA

    Science.gov (United States)

    2013-07-02

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone, Sugar House Casino Fireworks Display... out zone that covers part of the Delaware River. Sugar House Casino has contracted with Pyrotecnico... Sugar House Casino Fireworks Display will pose significant risks to the public. The purpose of the...

  8. 77 FR 37326 - Safety Zone; Grand Hotel 125th Anniversary Fireworks Celebration, Mackinaw Island, MI

    Science.gov (United States)

    2012-06-21

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Grand Hotel 125th Anniversary Fireworks... launched from a point on Lake Huron to commemorate the Grand Hotel's 125th anniversary. The Captain of the Port, Sector Sault Sainte Marie, has determined that the Grand Hotel Celebration Fireworks Display...

  9. 76 FR 77175 - New York Fun Factory Fireworks Display, Western Long Island Sound; Mamaroneck, NY

    Science.gov (United States)

    2011-12-12

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 New York Fun Factory Fireworks Display, Western Long... Island Sound in the vicinity of Mamaroneck, NY in support of the New York Fun Factory Fireworks display... Guard to define regulatory safety zones. On May 10, 2012 New York Fun Factory Events is sponsoring...

  10. 77 FR 35619 - Safety Zone; Old Fashion 4th July Fireworks, Presque Isle Bay, Erie, PA

    Science.gov (United States)

    2012-06-14

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Old Fashion 4th July Fireworks, Presque... vessels from a portion of Presque Isle Bay during the Old Fashion 4th July Fireworks display. This... temporary safety zone is necessary to ensure the safety of spectators and vessels during the Old Fashion 4th...

  11. 33 CFR 100.114 - Fireworks displays within the First Coast Guard District.

    Science.gov (United States)

    2010-07-01

    ... 4th Name: Stewart′s 4th of July Fireworks Display.Sponsor: W.P. Stewart. Time: 9 p.m. to 9:30 p.m... (NAD 1983). Connecticut: 7.33 July 4th Name: Old Lyme Fireworks.Sponsor: Mr. James R. Rice. Time: 8...

  12. 78 FR 74009 - Safety Zone; Nike Fireworks, Upper New York Bay, Ellis Island, NY

    Science.gov (United States)

    2013-12-10

    ... From the Federal Register Online via the Government Publishing Office DEPARTMENT OF HOMELAND SECURITY Coast Guard 33 CFR Part 165 Safety Zone; Nike Fireworks, Upper New York Bay, Ellis Island, NY..., 2011 (76 FR 69614). ] Table 1 1. Nike Fireworks Ellis Launch site: A barge located Island Safety...

  13. 36 CFR 327.13 - Explosives, firearms, other weapons and fireworks.

    Science.gov (United States)

    2010-07-01

    ... weapons and fireworks. 327.13 Section 327.13 Parks, Forests, and Public Property CORPS OF ENGINEERS... ADMINISTERED BY THE CHIEF OF ENGINEERS § 327.13 Explosives, firearms, other weapons and fireworks. (a) The... other weapons is prohibited unless: (1) In the possession of a Federal, state or local law enforcement...

  14. 76 FR 37650 - Safety Zone; 4th of July Festival Berkeley Marina Fireworks Display Berkeley, CA

    Science.gov (United States)

    2011-06-28

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; 4th of July Festival Berkeley Marina... Berkeley Pier, Berkeley, CA in support of the 4th of July Festival Berkeley Marina Fireworks Display... used in the fireworks display. Background and Purpose The City of Berkeley Marina will sponsor the 4th...

  15. 78 FR 39599 - Safety Zone; Independence Day Fireworks, Kings Beach, CA

    Science.gov (United States)

    2013-07-02

    ... SECURITY Coast Guard 33 CFR Part 165 Safety Zone; Independence Day Fireworks, Kings Beach, CA AGENCY: Coast... safety zone for the Independence Day Fireworks, Kings Beach, CA in the Captain of the Port, San Francisco... Marina to the launch site off of Kings Beach, CA in approximate position 39 13'55'' N, 120 01'42'' W...

  16. 77 FR 38005 - Safety Zone; Independence Day Fireworks, Kings Beach, CA

    Science.gov (United States)

    2012-06-26

    ... SECURITY Coast Guard 33 CFR Part 165 Safety Zone; Independence Day Fireworks, Kings Beach, CA AGENCY: Coast... safety zone for the Kings Beach Independence Day Fireworks display from 7 a.m. until 10 p.m. on July 3... from Tahoe Keys Marina to the launch site off of Kings Beach, CA at position 39 13'55'' N, 120...

  17. 75 FR 34367 - Safety Zone; Shore Thing & Independence Day Fireworks, Chesapeake Bay, Norfolk, VA

    Science.gov (United States)

    2010-06-17

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Shore Thing & Independence Day Fireworks... is establishing a temporary safety zone on the Chesapeake Bay in the vicinity of Ocean View Beach Park, Norfolk, VA in support of the Shore Thing & Independence Day Fireworks event. This action...

  18. 75 FR 26155 - Safety Zone; Shore Thing & Independence Day Fireworks, Chesapeake Bay, Norfolk, VA

    Science.gov (United States)

    2010-05-11

    ... View Beach Park, Norfolk, VA in support of the Shore Thing & Independence Day Fireworks event. This... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Shore Thing & Independence Day Fireworks... Federal Register (73 FR 3316). Public Meeting We do not now plan to hold a public meeting. But you...

  19. 76 FR 38300 - Safety Zone; Shore Thing and Independence Day Fireworks, Chesapeake Bay, Norfolk, VA

    Science.gov (United States)

    2011-06-30

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Shore Thing and Independence Day Fireworks... is establishing a temporary safety zone on the Chesapeake Bay in the vicinity of Ocean View Beach Park, Norfolk, VA in support of the Shore Thing and Independence Day Fireworks event. This action...

  20. Ocular firework trauma : a systematic review on incidence, severity, outcome and prevention

    NARCIS (Netherlands)

    Wisse, R. P. L.; Bijlsma, W. R.; Stilma, J. S.

    2010-01-01

    Aim To provide a systematic review on ocular firework trauma with emphasis on incidence and patient demographics, the extent of ocular trauma and visual function loss, and firework regulation effects on injury rates. Methods A literature search was performed using predetermined inclusion and exclusi

  1. 75 FR 19882 - Safety Zone; Benchmark Destination Corporate Party, Fireworks Display, San Francisco, CA

    Science.gov (United States)

    2010-04-16

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Benchmark Destination Corporate Party... support of the Benchmark Destination Corporate Party Fireworks Display. This safety zone is being... City of San Francisco will sponsor the Benchmark Destinations Corporate Party Fireworks Display on...

  2. 75 FR 18056 - Safety Zone; Fireworks Display, Patuxent River, Solomons Island Harbor, MD

    Science.gov (United States)

    2010-04-09

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Fireworks Display, Patuxent River, Solomons... establishing a temporary safety zone upon specified waters of Solomons Island Harbor, a tributary of the... fireworks display launched from discharge barge located in Solomons Island, Calvert County, Maryland. This...

  3. 78 FR 42016 - Safety Zone; Discovery World Fireworks, Milwaukee Harbor, Milwaukee, WI

    Science.gov (United States)

    2013-07-15

    ... docket, go to http://www.regulations.gov , type the docket number in the ``SEARCH'' box and click... arc of a circle with a 300-foot radius from the fireworks launch site located in approximate position... Discovery World Marina, within the arc of a circle with a 300-foot radius from the fireworks launch...

  4. 78 FR 29022 - Safety Zone; Fourth of July Fireworks, Berkeley Marina, Berkeley, CA

    Science.gov (United States)

    2013-05-17

    ... SECURITY Coast Guard 33 CFR Part 165 Safety Zone; Fourth of July Fireworks, Berkeley Marina, Berkeley, CA... enforce the safety zone for the Berkeley Marina Fourth of July Fireworks display in the Captain of the... Berkeley Pier in approximate position 37 51'40'' N, 122 19'19'' W (NAD 83) from 9:30 p.m. until 10:15...

  5. 78 FR 39992 - Safety Zone; Feast of Lanterns Fireworks Display, Pacific Grove, CA

    Science.gov (United States)

    2013-07-03

    ...) 366-9826. SUPPLEMENTARY INFORMATION: Table of Acronyms DHS Department of Homeland Security FR Federal... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Feast of Lanterns Fireworks Display... in support of The Feast of Lanterns Fireworks Event on July 27, 2013. This safety zone is...

  6. 76 FR 24843 - Safety Zone; Rudey/Braga Wedding Fireworks Display, Cos Cob Harbor, Greenwich, CT

    Science.gov (United States)

    2011-05-03

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Rudey/Braga Wedding Fireworks Display, Cos...: The Coast Guard proposes to establish a temporary safety zone around a fireworks display in Cos Cob... private estate in Cos Cob Harbor. This rule proposes to create a 600 foot safety zone on the...

  7. 77 FR 64411 - Safety Zone; Cooper T. Smith Fireworks Event; Mobile River; Mobile, AL

    Science.gov (United States)

    2012-10-22

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Cooper T. Smith Fireworks Event; Mobile... establishing a temporary safety zone for a portion of the Mobile River, Mobile, AL in the vicinity of Cooper... during the Cooper T. Smith Fireworks Event. Entry into, transiting or anchoring in this zone...

  8. 77 FR 51912 - Safety Zone; Tom Lyons Productions Fireworks, Long Island Sound, Sands Point, NY

    Science.gov (United States)

    2012-08-28

    ... From the Federal Register Online via the Government Publishing Office DEPARTMENT OF HOMELAND SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Tom Lyons Productions Fireworks, Long.... 165.T01-0618 to read as follows: Sec. 165.T01-0618 Safety Zone; Tom Lyons Productions Fireworks, Long...

  9. 76 FR 45693 - Safety Zone; San Diego POPS Fireworks, San Diego, CA

    Science.gov (United States)

    2011-08-01

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; San Diego POPS Fireworks, San Diego, CA... temporary safety zone on the navigable waters of San Diego Bay in support of the San Diego POPS Fireworks... Diego, CA; telephone (619) 278- 7262, e-mail Shane.E.Jakcson@uscg.mil . If you have questions on viewing...

  10. 78 FR 32121 - When Pigs Fly Fireworks Display; San Diego, CA

    Science.gov (United States)

    2013-05-29

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 When Pigs Fly Fireworks Display; San Diego, CA AGENCY... on the navigable waters of the San Diego Bay in support of the When Pigs Fly Fireworks Display on... Management, U.S. Coast Guard Sector San Diego, Coast Guard; telephone 619-278-7656, email...

  11. 75 FR 38412 - Safety Zone; San Diego POPS Fireworks, San Diego, CA

    Science.gov (United States)

    2010-07-02

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; San Diego POPS Fireworks, San Diego, CA... zone on the ] navigable waters of San Diego Bay in support of the San Diego POPS Fireworks. This safety.... Coast Guard Sector San Diego, CA; telephone 619-278- 7262, e-mail Shane.E.Jackson@uscg.mil . If you have...

  12. 77 FR 30451 - Safety Zone; Olcott Fireworks, Lake Ontario, Olcott, NY

    Science.gov (United States)

    2012-05-23

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Olcott Fireworks, Lake Ontario, Olcott, NY... establish a temporary safety zone on Lake Ontario, Olcott, NY. This proposed rule is intended to restrict vessels from a portion of Lake Ontario during the Olcott fireworks display. The safety zone established...

  13. 77 FR 38492 - Safety Zone; Olcott Fireworks, Lake Ontario, Olcott, NY

    Science.gov (United States)

    2012-06-28

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Olcott Fireworks, Lake Ontario, Olcott, NY... temporary safety zone on Lake Ontario, Olcott, New York. This safety zone is intended to restrict vessels from a portion of Lake Ontario during the Olcott fireworks on July 3, 2012. The safety zone...

  14. The age of the universe, the Hubble constant, the accelerated expansion and the Hubble effect

    OpenAIRE

    Soares,Domingos

    2009-01-01

    The idea of an accelerating universe comes almost simultaneously with the determination of Hubble's constant by one of the Hubble Space Telescope Key Projects. The age of the universe dilemma is probably the link between these two issues. In an appendix, I claim that "Hubble's law" might yet to be investigated for its ultimate cause, and suggest the "Hubble effect" as the searched candidate.

  15. The age of the universe, the Hubble constant, the accelerated expansion and the Hubble effect

    OpenAIRE

    Soares, Domingos

    2009-01-01

    The idea of an accelerating universe comes almost simultaneously with the determination of Hubble's constant by one of the Hubble Space Telescope Key Projects. The age of the universe dilemma is probably the link between these two issues. In an appendix, I claim that "Hubble's law" might yet to be investigated for its ultimate cause, and suggest the "Hubble effect" as the searched candidate.

  16. The 1% concordance Hubble constant

    Energy Technology Data Exchange (ETDEWEB)

    Bennett, C. L.; Larson, D.; Weiland, J. L. [Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States); Hinshaw, G., E-mail: cbennett@jhu.edu [Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1 (Canada)

    2014-10-20

    The determination of the Hubble constant has been a central goal in observational astrophysics for nearly a hundred years. Extraordinary progress has occurred in recent years on two fronts: the cosmic distance ladder measurements at low redshift and cosmic microwave background (CMB) measurements at high redshift. The CMB is used to predict the current expansion rate through a best-fit cosmological model. Complementary progress has been made with baryon acoustic oscillation (BAO) measurements at relatively low redshifts. While BAO data do not independently determine a Hubble constant, they are important for constraints on possible solutions and checks on cosmic consistency. A precise determination of the Hubble constant is of great value, but it is more important to compare the high and low redshift measurements to test our cosmological model. Significant tension would suggest either uncertainties not accounted for in the experimental estimates or the discovery of new physics beyond the standard model of cosmology. In this paper we examine in detail the tension between the CMB, BAO, and cosmic distance ladder data sets. We find that these measurements are consistent within reasonable statistical expectations and we combine them to determine a best-fit Hubble constant of 69.6 ± 0.7 km s{sup –1} Mpc{sup –1}. This value is based upon WMAP9+SPT+ACT+6dFGS+BOSS/DR11+H {sub 0}/Riess; we explore alternate data combinations in the text. The combined data constrain the Hubble constant to 1%, with no compelling evidence for new physics.

  17. Evolving and Combining Facial Composites: Between-Witness and Within-Witness Morphs Compared

    Science.gov (United States)

    Valentine, Tim; Davis, Josh P.; Thorner, Kate; Solomon, Chris; Gibson, Stuart

    2010-01-01

    Student participant-witnesses produced 4 composites of unfamiliar faces with a system that uses a genetic algorithm to evolve appearance of artificial faces. Morphs of 4 composites produced by different witnesses (between-witness morphs) were judged better likenesses (Experiment 1) and were more frequently named (Experiment 2) by participants who…

  18. Witnessing non-Markovianity of quantum evolution

    Science.gov (United States)

    Chruściński, Dariusz; Kossakowski, Andrzej

    2014-01-01

    We provide further characterization of non-Markovian quantum dynamics based on the concept of divisible dynamical maps. In analogy to entanglement witness we propose a non-Markovianity witness and introduce the corresponding measure of non-Markovianity. We also provide characterization of non-Markovianity in terms of Wigner-Yanase-Dyson skew information.

  19. Bay Area Students Help Victims and Witnesses.

    Science.gov (United States)

    Mandel, Dave

    1978-01-01

    Aid to Victims and Witnesses (AVW), sponsored by the San Mateo (California) Probation Department and staffed almost entirely by citizen and student volunteers, offers immediate financial and emotional aid to victims of violent crime after police call AVW's hot line. AVW also helps witnesses to crime in court appearances. (MF)

  20. Victim/Witness Assistance: A Selected Bibliography.

    Science.gov (United States)

    Cain, Anthony A., Comp.; Kravitz, Marjorie, Comp.

    This annotated bibliography highlights the literature available on two important aspects of assistance to victims and witnesses of crime. The first section, victim and witness services, covers the need, function and implementation of services to assist victims, elements of effective programs and evaluation of specific programs. The second section,…

  1. 42 CFR 3.538 - Witnesses.

    Science.gov (United States)

    2010-10-01

    ... HEALTH SERVICE, DEPARTMENT OF HEALTH AND HUMAN SERVICES GENERAL PROVISIONS PATIENT SAFETY ORGANIZATIONS AND PATIENT SAFETY WORK PRODUCT Enforcement Program § 3.538 Witnesses. (a) Except as provided in... consumption of time; and (3) Protect witnesses from harassment or undue embarrassment. (d) The ALJ must permit...

  2. 12 CFR 308.532 - Witnesses.

    Science.gov (United States)

    2010-01-01

    ... 12 Banks and Banking 4 2010-01-01 2010-01-01 false Witnesses. 308.532 Section 308.532 Banks and Banking FEDERAL DEPOSIT INSURANCE CORPORATION PROCEDURE AND RULES OF PRACTICE RULES OF PRACTICE AND PROCEDURE Program Fraud Civil Remedies and Procedures § 308.532 Witnesses. (a) Except as provided in...

  3. 12 CFR 308.524 - Witness fees.

    Science.gov (United States)

    2010-01-01

    ... 12 Banks and Banking 4 2010-01-01 2010-01-01 false Witness fees. 308.524 Section 308.524 Banks and Banking FEDERAL DEPOSIT INSURANCE CORPORATION PROCEDURE AND RULES OF PRACTICE RULES OF PRACTICE AND PROCEDURE Program Fraud Civil Remedies and Procedures § 308.524 Witness fees. The party requesting a...

  4. Hubble Law: Measure and Interpretation

    Science.gov (United States)

    Paturel, Georges; Teerikorpi, Pekka; Baryshev, Yurij

    2017-09-01

    We have had the chance to live through a fascinating revolution in measuring the fundamental empirical cosmological Hubble law. The key progress is analysed: (1) improvement of observational means (ground-based radio and optical observations, space missions); (2) understanding of the biases that affect both distant and local determinations of the Hubble constant; (3) new theoretical and observational results. These circumstances encourage us to take a critical look at some facts and ideas related to the cosmological red-shift. This is important because we are probably on the eve of a new understanding of our Universe, heralded by the need to interpret some cosmological key observations in terms of unknown processes and substances.

  5. Hubble multi-scalar inflation

    CERN Document Server

    Abedi, Habib

    2016-01-01

    Multiple field models of inflation exhibit new features than single field models. In this work, we study the hierarchy of parameters based on Hubble expansion rate in curved field space and derive the system of flow equations that describe their evolution. Then we focus on obtaining derivatives of number of $e$-folds with respect to scalar fields during inflation and at hypersurface of the end of inflation.

  6. The Hubble Catalog of Variables

    Science.gov (United States)

    Sokolovsky, K.; Bonanos, A.; Gavras, P.; Yang, M.; Hatzidimitriou, D.; Moretti, M. I.; Karampelas, A.; Bellas-Velidis, I.; Spetsieri, Z.; Pouliasis, E.; Georgantopoulos, I.; Charmandaris, V.; Tsinganos, K.; Laskaris, N.; Kakaletris, G.; Nota, A.; Lennon, D.; Arviset, C.; Whitmore, B.; Budavari, T.; Downes, R.; Lubow, S.; Rest, A.; Strolger, L.; White, R.

    2017-09-01

    We aim to construct an exceptionally deep (V ≲ 27) catalog of variable objects in selected Galactic and extragalactic fields visited multiple times by the Hubble Space Telescope (HST). While HST observations of some of these fields were searched for specific types of variables before (most notably, the extragalactic Cepheids), we attempt a systematic study of the population of variable objects of all types at the magnitude range not easily accessible with ground-based telescopes. The variability timescales that can be probed range from hours to years depending on how often a particular field has been visited. For source extraction and cross-matching of sources between visits we rely on the Hubble Source Catalog which includes 107 objects detected with WFPC2, ACS, and WFC3 HST instruments. The lightcurves extracted from the HSC are corrected for systematic effects by applying local zero-point corrections and are screened for bad measurements. For each lightcurve we compute variability indices sensitive to a broad range of variability types. The indices characterize the overall lightcurve scatter and smoothness. Candidate variables are selected as having variability index values significantly higher than expected for objects of similar brightness in the given set of observations. The Hubble Catalog of Variables will be released in 2018.

  7. The Hubble Catalog of Variables

    Directory of Open Access Journals (Sweden)

    Sokolovsky K.

    2017-01-01

    Full Text Available We aim to construct an exceptionally deep (V ≲ 27 catalog of variable objects in selected Galactic and extragalactic fields visited multiple times by the Hubble Space Telescope (HST. While HST observations of some of these fields were searched for specific types of variables before (most notably, the extragalactic Cepheids, we attempt a systematic study of the population of variable objects of all types at the magnitude range not easily accessible with ground-based telescopes. The variability timescales that can be probed range from hours to years depending on how often a particular field has been visited. For source extraction and cross-matching of sources between visits we rely on the Hubble Source Catalog which includes 107 objects detected with WFPC2, ACS, and WFC3 HST instruments. The lightcurves extracted from the HSC are corrected for systematic effects by applying local zero-point corrections and are screened for bad measurements. For each lightcurve we compute variability indices sensitive to a broad range of variability types. The indices characterize the overall lightcurve scatter and smoothness. Candidate variables are selected as having variability index values significantly higher than expected for objects of similar brightness in the given set of observations. The Hubble Catalog of Variables will be released in 2018.

  8. The Hubble-Depth Survey

    Directory of Open Access Journals (Sweden)

    Changbom Park

    2007-01-01

    Full Text Available Mediante una simulaci n de N cuerpos de un modelo ACDM hemos desarrollado una b squeda de galaxias ficticias hasta la profundidad del Hubble. Para encontrar las galaxias en la distribuci on de part culas, identificamos los halos estables y autoligados mediante un m todo de b squeda de halos en el espacio real y en el cono de luz. Suponemos que cada halo contiene solamente una galaxia con un brillo monot nicamente proporcional a la masa del halo, para as ajustar la funci n de masa con la funci n de luminosidad gal actica obtenida en el Sloan Digital Sky Survey (SDSS. Despu s de aplicar la correcciones K, y de evoluci n a las luminosidades observadas de las galaxias ficticias, hicimos estudios del corrimiento al rojo bajo varias restricciones observacionales. En particular, proponemos un nuevo estudio de corrimientos al rojo, llamado el Hubble Depth Survey, el cual est limitado hasta la magnitud r = 22 y alcanza la distancia de Hubble dH = 3000 h -1 Mpe

  9. Witnessing Continuous Variable Entanglement with Discrete Measurements

    CERN Document Server

    Schneeloch, James; Howland, Gregory A; Broadbent, Curtis J; Howell, John C

    2012-01-01

    In this Letter, we derive an entropic Einstein-Podolsky-Rosen (EPR) steering inequality for continuous variable (CV) systems using only experimentally measured discrete probability distributions and details of the measurement apparatus. We use this inequality to witness entanglement between the positions and momenta of photon pairs generated in spontaneous parametric downconversion (SPDC). We examine the asymmetry between parties in this inequality, and show that this asymmetry can be used to reduce the technical requirements of experimental setups intended to witness entanglement. Furthermore, we develop a more stringent steering inequality that is symmetric between parties, and use it to witness symmetric EPR steering.

  10. Experimentally witnessing the quantumness of correlations

    CERN Document Server

    Auccaise, R; Celeri, L C; Soares-Pinto, D O; deAzevedo, E R; Bonagamba, T J; Sarthour, R S; Oliveira, I S; Serra, R M

    2011-01-01

    The quantification of quantum correlations (other than entanglement) usually entails laboured numerical optimization procedures demanding quantum state tomographic methods. Thus it is interesting to have a laboratory friendly witness for the nature of correlations. In this article we report a direct experimental implementation of such a witness in a room temperature system by using a nuclear magnetic resonance setup. In our experiment the nature of correlations is revealed by performing only few local magnetization measurements. We also compare the witness results with those for the quantum discord and we obtained a fairly good agreement.

  11. Fireworks-related injury surveillance in the Philippines: trends in 2010–2014

    Directory of Open Access Journals (Sweden)

    John Bobbie Roca

    2015-11-01

    Full Text Available Analysis of the annual fireworks-related injury surveillance data collected by the Philippines Department of Health (DOH in 2010–2014 was conducted to describe the profile of such injuries in the Philippines. Surveillance data were collected from DOH’s Online National Electronic Injury Surveillance System and analysed. A case was defined as any person who had sustained injury from fireworks in any form within the 16-day surveillance period (21 December to 5 January and had presented to any of the 50 sentinel hospitals. Of the 4649 cases, there were 4706 fireworks-related injuries involving 5076 anatomic sites in 2010–2014. A significant decrease of cases in 2014 was observed when compared with the previous study years (P = 0.02. The number of cases peaked at public holidays. Males (80% were more commonly injured, and children aged 5 to 14 years were primarily affected (47%. Ignition of illegal fireworks accounted for half (50% of the injuries; most injuries (68% occurred in street settings. The majority of injuries (57% were sustained by fireworks igniters. The most common anatomic injury sites were hands (44%, legs (21% and eyes (14%. Illegal fireworks were related to 100% (4/4 of the deaths and 49% (105/214 of the cases who needed amputations. Fireworks-related injuries declined significantly in 2014. Public awareness campaigns may have contributed to reducing the injury occurrences. As illegal fireworks accounted for all deaths and more than half of the amputations, law enforcement should be directed toward preventing importing, distributing and using illegal fireworks.

  12. Mobility Tolerant Firework Routing for Improving Reachability in MANETs

    Directory of Open Access Journals (Sweden)

    Gen Motoyoshi

    2014-03-01

    Full Text Available In this paper, we investigate our mobility-assisted and adaptive broadcast routing mechanism, called Mobility Tolerant Firework Routing (MTFR, which utilizes the concept of potentials for routing and improves node reachability, especially in situations with high mobility, by including a broadcast mechanism. We perform detailed evaluations by simulations in a mobile environment and demonstrate the advantages of MTFR over conventional potential-based routing. In particular, we show that MTFR produces better reachability in many aspects at the expense of a small additional transmission delay and intermediate traffic overhead, making MTFR a promising routing protocol and feasible for future mobile Internet infrastructures.

  13. Toxicology of explosives and fireworks in small animals.

    Science.gov (United States)

    Gahagan, Patti; Wismer, Tina

    2012-03-01

    Intoxication with explosives or fireworks in dogs or cats is not common, but serious toxicosis can result from exposure to different types of explosives depending on the chemical class of explosive involved. This article will discuss the different types of materials/chemicals, clinical signs of toxicosis, and their treatment. Despite the complexities of explosives and plethora of different devices currently in use worldwide, the toxic potential is more easily explained by looking at the relatively short list of chemical classes used to produce these materials. This article combines structurally similar explosives into different groups and focuses on the toxicity of the most commonly available explosives.

  14. Experimental implementation of a NMR entanglement witness

    CERN Document Server

    Filgueiras, J G; Auccaise, R E; Vianna, R O; Sarthour, R S; Oliveira, I S

    2012-01-01

    Entanglement witnesses (EW) allow the detection of entanglement in a quantum system, from the measurement of some few observables. They do not require the complete determination of the quantum state, which is regarded as a main advantage. On this paper it is experimentally analyzed an entanglement witness recently proposed in the context of Nuclear Magnetic Resonance (NMR) experiments to test it in some Bell-diagonal states. We also propose some optimal entanglement witness for Bell-diagonal states. The efficiency of the two types of EW's are compared to a measure of entanglement with tomographic cost, the generalized robustness of entanglement. It is used a GRAPE algorithm to produce an entangled state which is out of the detection region of the EW for Bell-diagonal states. Upon relaxation, the results show that there is a region in which both EW fails, whereas the generalized robustness still shows entanglement, but with the entanglement witness proposed here with a better performance.

  15. 29 CFR 1603.212 - Witness fees.

    Science.gov (United States)

    2010-07-01

    ... STATE AND LOCAL GOVERNMENT EMPLOYEE COMPLAINTS OF EMPLOYMENT DISCRIMINATION UNDER SECTION 304 OF THE... served, or, if the witness appears voluntarily, at the time of appearance. A federal agency...

  16. 49 CFR 511.44 - Expert witnesses.

    Science.gov (United States)

    2010-10-01

    ...) Definition. An expert witness is one who, by reason of education, training, experience, or profession, has... the methodology underlying any analysis, and a full disclosure of the basis of any opinion. The...

  17. The Griffiths Question Map: A Forensic Tool For Expert Witnesses' Assessments of Witnesses and Victims' Statements.

    Science.gov (United States)

    Dodier, Olivier; Denault, Vincent

    2017-02-27

    Expert witnesses are sometimes asked to assess the reliability of young witnesses and victims' statements because of their high susceptibility to memory biases. This technical note aims to highlight the relevance of the Griffiths Question Map (GQM) as a professional forensic tool to improve expert witnesses' assessments of young witnesses and victims' testimonies. To do so, this innovative question type assessment grid was used to proceed to an in-depth analysis of the interview of an alleged 13-year-old victim of a sexual assault and two rapes. Overall, the GQM stressed how the interview was mainly conducted in an inappropriate manner. The results are examined with regard to scientific knowledge on young witnesses and victims' memory. Finally, it is argued that expert witnesses in inquisitorial systems might use the GQM while encountering difficulties to fulfill the legal standards for expert evidence in adversarial systems because of the lack of studies regarding its reliability. © 2017 American Academy of Forensic Sciences.

  18. Hubble Systems Optimize Hospital Schedules

    Science.gov (United States)

    2009-01-01

    Don Rosenthal, a former Ames Research Center computer scientist who helped design the Hubble Space Telescope's scheduling software, co-founded Allocade Inc. of Menlo Park, California, in 2004. Allocade's OnCue software helps hospitals reclaim unused capacity and optimize constantly changing schedules for imaging procedures. After starting to use the software, one medical center soon reported noticeable improvements in efficiency, including a 12 percent increase in procedure volume, 35 percent reduction in staff overtime, and significant reductions in backlog and technician phone time. Allocade now offers versions for outpatient and inpatient magnetic resonance imaging (MRI), ultrasound, interventional radiology, nuclear medicine, Positron Emission Tomography (PET), radiography, radiography-fluoroscopy, and mammography.

  19. Friedmann equation and Hubble condition

    CERN Document Server

    Baumgaertel, Hellmut

    2014-01-01

    The note presents results on the solutions of the Friedmann equation, which satisfy the Hubble condition, where the radiation term is taken into account. For these solutions the equation $\\sigma=\\sigma_{cr}$, where $\\sigma$ is the radiation invariant of the Friedmann equation and $\\sigma_{cr}$ the "critical radiation parameter", introduced in [5], is an analytic relation between the matter density and the radiation density at the present time and the cosmological constant which can be represented by two function branches, expressing the cosmological constant as unique functions of the matter and radiation density. These functions are the "frontier lines" between regions of constant type.

  20. Modified Hubble law, the time-varying Hubble parameter and the problem of dark energy

    OpenAIRE

    Liu, Jian-Miin

    2005-01-01

    In the framework of the solvable model of cosmology constructed in the Earth-related coordinate system, we derive the modified Hubble law. This law carries the slowly time-varying Hubble parameter. The modified Hubble law eliminates the need for dark energy.

  1. Modified Hubble law, the time-varying Hubble parameter and the problem of dark energy

    OpenAIRE

    Liu, Jian-Miin

    2005-01-01

    In the framework of the solvable model of cosmology constructed in the Earth-related coordinate system, we derive the modified Hubble law. This law carries the slowly time-varying Hubble parameter. The modified Hubble law eliminates the need for dark energy.

  2. 75 FR 38716 - Safety Zone; Vietnam Veterans of America Fireworks Display, Brookings, OR

    Science.gov (United States)

    2010-07-06

    ...-9319, e-mail D13-SG-SecPortlandWWM@uscg.mil . If you have questions on viewing the docket, call Renee V... America are holding a fireworks display near Brookings, Oregon on July 4, 2010. Due to the...

  3. Anions in pre- and post-blast consumer fireworks by capillary electrophoresis.

    Science.gov (United States)

    Martín-Alberca, Carlos; de la Ossa, Ma Ángeles Fernández; Sáiz, Jorge; Ferrando, José Luis; García-Ruiz, Carmen

    2014-11-01

    Consumer fireworks are a heterogeneous group of pyrotechnic items widely used by citizens around the world. There are a wide number of forensic cases related to consumer fireworks that require knowing their chemical composition and variety of designs to conduct accurate and comprehensive analyses. In this research paper, a selection of six consumer firework types (firecracker, rocket, pyrotechnic fountain, pyrotechnic battery, sparkler, and smoke bomb) is physically described and their anionic compositions are determined. Preblast (fuses and charges) samples and postblast residues of the different consumer fireworks were analyzed by CE in order to determine their anionic composition. Different types of chemical compositions in fuses and pyrotechnic charges were determined, although they were not related to any type of item. Additionally, several discrepancies were found between the analytical results and the declared item compositions. Regarding postblast residues, a huge variety of anions were identified and attributed to some unconsumed starting materials and different chemical reactions occurring during combustion.

  4. 75 FR 19304 - Safety Zones; Annual Fireworks Events in the Captain of the Port Detroit Zone

    Science.gov (United States)

    2010-04-14

    ... hold one at a time and place announced by a later notice in the Federal Register. Background and... determined annually. (54) Bay City Fireworks Festival, Bay City, MI: (i) Location: All waters of the Saginaw...

  5. 33 CFR 165.151 - Safety Zones; Long Island Sound annual fireworks displays.

    Science.gov (United States)

    2010-07-01

    ... Festival Fireworks Safety Zone. All waters of New Haven Harbor on Long Island Sound within a 1200-foot... thick on a white background. (c) Enforcement period. Specific zones in this section will be enforced...

  6. Determine disturbance impacts of fireworks at the Coquille Point seabird colony complex near Bandon, Oregon

    Data.gov (United States)

    US Fish and Wildlife Service, Department of the Interior — The USFWS conducted a monitoring study at Pirate Cove Rock during 2011 to determine if the Independence Day fireworks display had any adverse effects on seabirds,...

  7. 77 FR 42179 - Safety Zone; Fireworks Display, Potomac River, Charles County, Newburg, MD

    Science.gov (United States)

    2012-07-18

    ... Rule Digital Lightning, of Kensington, Maryland, will conduct a fireworks display launched from a barge located on the Potomac River, adjacent to Gilligan's Pier Restaurant, at Newburg in Charles...

  8. 77 FR 35857 - Safety Zone, Fireworks Display, Lake Superior; Duluth, MN

    Science.gov (United States)

    2012-06-15

    ... fireworks display will occur in the vicinity of Duluth Harbor in Duluth, MN. Based on accidents that have... Ombudsman and the Regional Small Business Regulatory Fairness Boards. The Ombudsman evaluates these actions...

  9. 75 FR 38714 - Safety Zone; Macy's Fourth of July Fireworks Display, Hudson River, New York, NY

    Science.gov (United States)

    2010-07-06

    ... fireworks display. Based on accidents that have occurred in other Captain of the Port zones, and the... the Regional Small Business Regulatory Fairness Boards. The Ombudsman evaluates these actions annually...

  10. Estimation of direct and indirect impacts of fireworks on the physicochemical characteristics of atmospheric fine and coarse particles

    Science.gov (United States)

    Tian, Y.-Z.; Wang, J.; Peng, X.; Shi, G.-L.; Feng, Y.-C.

    2014-05-01

    To quantify total, direct and indirect impacts of fireworks individually, size-resolved PM samples were collected before, during, and after a Chinese folk-custom festival (Chinese New Year) in a megacity in China. Through chemical analysis and morphology characterization, strong influence of fireworks on physicochemical characteristics of PM10 and PM2.5 was observed. Concentrations of many species exhibited an increasing trend during heavy-firework period, especially for K+, Mg2+ and Cr; and the results of non-sea-salt ions demonstrated anthropogenic influence on them. Then, source apportionment was conducted by receptor models and Peak Analysis. Total influence of fireworks was quantified by PMF, showing that fireworks contributed rather higher fractions (23.40% to PM10 and 29.66% to PM2.5) during heavy-firework period than those during light-firework period (4.28% to PM10 and 7.18% to PM2.5). Profiles of total fireworks obtained by two independent methods (PMF and Peak Analysis) were consistent, with higher abundances of K+, Al, Si, Ca and OC. Finally, individual contributions of direct and indirect impacts of fireworks were quantified by CMB. The percentage contributions of resuspended dust, biomass combustion and direct-fireworks were 36.82, 14.08 and 44.44% for PM10 and 34.89, 16.60 and 52.54% for PM2.5, in terms of the total fireworks. The quantification of total, direct and indirect impacts of fireworks to ambient PM gives an original contribution to understand the physicochemical characteristics and mechanisms of such high-intensity anthropogenic activities.

  11. The Hubble Ultra Deep Field

    CERN Document Server

    Beckwith, S V W; Koekemoer, A M; Caldwell, J A R; Ferguson, H C; Hook, R; Lucas, R A; Bergeron, L E; Corbin, M; Jogee, S; Panagia, N; Robberto, M; Royle, P; Somerville, R S; Sosey, M; Beckwith, Steven V. W.; Stiavelli, Massimo; Koekemoer, Anton M.; Caldwell, John A. R.; Ferguson, Henry C.; Hook, Richard; Lucas, Ray A.; Bergeron, Louis E.; Corbin, Michael; Jogee, Shardha; Panagia, Nino; Robberto, Massimo; Royle, Patricia; Somerville, Rachel S.; Sosey, Megan

    2006-01-01

    This paper presents the Hubble Ultra Deep Field (HUDF), a one million second exposure of an 11 square minute-of-arc region in the southern sky with the Hubble Space Telescope. The exposure time was divided among four filters, F435W (B435), F606W (V606), F775W (i775), and F850LP (z850), to give approximately uniform limiting magnitudes mAB~29 for point sources. The image contains at least 10,000 objects presented here as a catalog. Few if any galaxies at redshifts greater than ~4 resemble present day spiral or elliptical galaxies. Using the Lyman break dropout method, we find 504 B-dropouts, 204 V-dropouts, and 54 i-dropouts. Using these samples that are at different redshifts but derived from the same data, we find no evidence for a change in the characteristic luminosity of galaxies but some evidence for a decrease in their number densities between redshifts of 4 and 7. The ultraviolet luminosity density of these samples is dominated by galaxies fainter than the characteristic luminosity, and the HUDF reveal...

  12. 77 FR 37604 - Safety Zone; Fourth of July Fireworks, Berkeley Marina, Berkeley, CA

    Science.gov (United States)

    2012-06-22

    ... SECURITY Coast Guard 33 CFR Part 165 Safety Zone; Fourth of July Fireworks, Berkeley Marina, Berkeley, CA... enforce the safety zone for the Berkeley Marina Fourth of July Fireworks display in the Captain of the... Berkeley Pier in position 37 51'40'' N, 122 19'19'' W (NAD 83) from 9:30 p.m. until 10:15 p.m. on July...

  13. Hubble 2008: Science Year in Review

    Science.gov (United States)

    2009-01-01

    Hubbles remarkable mission has now spanned 18 years. During that time, it has been at the nexus of perhaps the most exciting period of discovery in the history of astronomy. Simultaneously, Hubble has offered up some of the most daunting engineering challenges to humans working in space, and success in meeting those challenges has been among NASAs greatest triumphs.

  14. Witnessing entanglement in an undergraduate laboratory

    Science.gov (United States)

    Beck, Marisol N.; Beck, M.

    2016-02-01

    An entangled state of a two-particle system is a quantum state that cannot be separated, meaning it cannot be written as the product of states of the individual particles. One way to tell if a system is entangled is to use it to violate a Bell inequality (such as the Clauser-Horne-Shimony-Holt, CHSH, inequality), because entanglement is necessary for such a violation. However, there are other, easier-to-perform measurements that determine whether or not a system is entangled. An operator that corresponds to such a measurement is referred to as an entanglement witness. Here, we present the theory of witness operators and an undergraduate experiment that measures entanglement witnesses for the joint polarization state of two photons. We are able to produce states for which the expectation value of a witness operator is entangled by more than 300 standard deviations. In order to further examine the performance of these witness operators, we present a simple way to generate states that closely approximate Werner states, which have a controllable degree of entanglement.

  15. 18 CFR 1b.16 - Rights of witnesses.

    Science.gov (United States)

    2010-04-01

    ... the witness and his employer, said counsel shall inform the Investigating Officer and each client of... confidence, upon his initiative or the witness' with respect to any question, and if the witness refuses to... grounds of self-incrimination, the witness must assert the privilege personally. (3) Following...

  16. Modest Witness(ing) and Lively Stories: Paying Attention to Matters of Concern in Early Childhood

    Science.gov (United States)

    Blaise, Mindy; Hamm, Catherine; Iorio, Jeanne Marie

    2017-01-01

    This article considers the role of early childhood education within these uncertain times of human induced climate change. It draws from feminism and environmental humanities to experiment with different ways of becoming-with the world. By bringing together Donna Haraway's figure of the Modest Witness and Deborah Bird Rose's notion of witnessing,…

  17. Modest Witness(ing) and Lively Stories: Paying Attention to Matters of Concern in Early Childhood

    Science.gov (United States)

    Blaise, Mindy; Hamm, Catherine; Iorio, Jeanne Marie

    2017-01-01

    This article considers the role of early childhood education within these uncertain times of human induced climate change. It draws from feminism and environmental humanities to experiment with different ways of becoming-with the world. By bringing together Donna Haraway's figure of the Modest Witness and Deborah Bird Rose's notion of witnessing,…

  18. Unification of witnessing initial system-environment correlations and witnessing non-Markovianity

    CERN Document Server

    Rodríguez-Rosario, César A; Mazzola, Laura; Aspuru-Guzik, Alán

    2012-01-01

    We show the connection between a witness that detects dynamical maps with initial system-environment correlations and a witness that detects non-Markovian open quantum systems. Our analysis is based on studying the role that state preparation plays in witnessing violations of contractivity of open quantum system dynamics. Contractivity is a property of some quantum processes where the trace distance of density matrices decrease with time. From this, we show how a witness of initial-correlations is an upper bound to a witness of non-Markovianity. We discuss how this relationship shows further connections between initial system-environment correlations and non-Markovianity at an instance of time in open quantum systems.

  19. From Entanglement Witness to Generalized Catalan Numbers

    CERN Document Server

    Cohen, Eliahu; Itzhaki, Nissan

    2015-01-01

    The problem of entanglement detection for arbitrary spin systems is analyzed. We demonstrate how a single measurement of the squared total spin can probabilistically discern separable from entangled many-particle states. For achieving this goal, we construct a tripartite analogy between the degeneracy of entanglement witness eigenstates, tensor products of SO(3) representations and classical lattice walks with special constraints. Within this framework, degeneracies are naturally given by generalized Catalan numbers and determine the fraction of states that are decidedly entangled. In addition, we introduce the concept of a "sterile entanglement witness", which detects entanglement without affecting much the system's dynamics. We show that our proposed witness is sterile when the system becomes large enough.

  20. From entanglement witness to generalized Catalan numbers.

    Science.gov (United States)

    Cohen, E; Hansen, T; Itzhaki, N

    2016-07-27

    Being extremely important resources in quantum information and computation, it is vital to efficiently detect and properly characterize entangled states. We analyze in this work the problem of entanglement detection for arbitrary spin systems. It is demonstrated how a single measurement of the squared total spin can probabilistically discern separable from entangled many-particle states. For achieving this goal, we construct a tripartite analogy between the degeneracy of entanglement witness eigenstates, tensor products of SO(3) representations and classical lattice walks with special constraints. Within this framework, degeneracies are naturally given by generalized Catalan numbers and determine the fraction of states that are decidedly entangled and also known to be somewhat protected against decoherence. In addition, we introduce the concept of a "sterile entanglement witness", which for large enough systems detects entanglement without affecting much the system's state. We discuss when our proposed entanglement witness can be regarded as a sterile one.

  1. COSMOS Hubble Space Telescope Observations

    CERN Document Server

    Scoville, N Z; Blain, A W; Calzetti, D; Comastri, A; Capak, P; Carilli, C; Carlstrom, J E; Carollo, C M; Colbert, J; Daddi, E; Ellis, Richard S; Elvis, M; Ewald, S P; Fall, M; Franceschini, A; Giavalisco, M; Green, W; Griffiths, R E; Guzzo, L; Hasinger, G; Impey, C; Kneib, J P; Koda, J; Koekemoer, A; Lefèvre, O; Lilly, S; Liu, C T; McCracken, H J; Massey, R; Mellier, Y; Miyazaki, S; Mobasher, B; Mould, J; Norman, C; Réfrégier, A; Renzini, A; Rhodes, J; Rich, M; Sanders, D B; Schiminovich, D; Schinnerer, E; Scodeggio, M; Sheth, K; Shopbell, P L; Taniguchi, Y; Tyson, N; Urry, C M; Van Waerbeke, L; Vettolani, P; White, S D M; Yan, L

    2006-01-01

    The Cosmic Evolution Survey (COSMOS) was initiated with an extensive allocation (590 orbits in Cycles 12-13) using the Hubble Space Telescope (HST) for high resolution imaging. Here we review the characteristics of the HST imaging with the Advanced Camera for Surveys (ACS) and parallel observations with NICMOS and WFPC2. A square field (1.8$\\sq$\\deg) has been imaged with single-orbit ACS I-F814W exposures with 50% completeness for sources 0.5\\arcsec in diameter at I$_{AB} $ = 26.0 mag. The ACS imaging is a key part of the COSMOS survey, providing very high sensitivity and high resolution (0.09\\arcsec FWHM, 0.05\\arcsec pixels) imaging and detecting a million objects. These images yield resolved morphologies for several hundred thousand galaxies. The small HST PSF also provides greatly enhanced sensitivity for weak lensing investigations of the dark matter distribution.

  2. The Hubble Sphere Hydrogen Survey

    CERN Document Server

    Peterson, J B; Pen, U L; Peterson, Jeffrey B.; Bandura, Kevin; Pen, Ue Li

    2006-01-01

    An all sky redshift survey, using hydrogen 21 cm emission to locate galaxies, can be used to track the wavelength of baryon acoustic oscillations imprints from z ~ 1.5 to z = 0. This will allow precise determination of the evolution of dark energy. A telescope made of fixed parabolic cylindrical reflectors offers substantial benefit for such a redshift survey. Fixed cylinders can be built for low cost, and long cylinders also allow low cost fast fourier transform techniques to be used to define thousands of simultaneous beams. A survey made with fixed reflectors naturally covers all of the sky available from it's site with good uniformity, minimizing sample variance in the measurement of the acoustic peak wavelength. Such a survey will produce about a billion redshifts, nearly a thousand times the number available today. The survey will provide a three dimensional mapping of a substantial fraction of the Hubble Sphere.

  3. The Hubble Tarantula Treasury Project

    Science.gov (United States)

    Sabbi, Elena; Lennon, D. J.; Anderson, J.; Van Der Marel, R. P.; Aloisi, A.; Boyer, M. L.; Cignoni, M.; De Marchi, G.; de Mink, S. E.; Evans, C. J.; Gallagher, J. S.; Gordon, K. D.; Gouliermis, D.; Grebel, E.; Koekemoer, A. M.; Larsen, S. S.; Panagia, N.; Ryon, J. E.; Smith, L. J.; Tosi, M.; Zaritsky, D. F.

    2014-01-01

    The Tarantula Nebula (a.k.a. 30 Doradus) in the Large Magellanic Cloud is one of the most famous objects in astronomy, with first astronomical references being more than 150 years old. Today the Tarantula Nebula and its ionizing cluster R136 are considered one of the few known starburst regions in the Local Group and an ideal test bed to investigate the temporal and spatial evolution of a prototypical starburst on a sub-cluster scale. The Hubble Tarantula Treasury Project (HTTP) is a panchromatic imaging survey of the stellar populations and ionized gas in the Tarantula Nebula that reaches into the sub-solar mass regime (eBook that explains how stars form and evolve using images from HTTP. The eBook utilizes emerging technology that works in conjunction with the built-in accessibility features in the Apple iPad to allow totally blind users to interactively explore complex astronomical images.

  4. The Child Witness in the Courtroom.

    Science.gov (United States)

    Pantell, Robert H

    2017-03-01

    Beginning in the 1980s, children have increasingly served as witnesses in the criminal, civil, and family courts; currently, >100 000 children appear in court each year. This statement updates the 1992 American Academy of Pediatrics (AAP) policy statement "The Child as a Witness" and the subsequent 1999 "The Child in Court: A Subject Review." It also builds on existing AAP policy on adverse life events affecting children and resources developed to understand and address childhood trauma. The purpose of this policy statement is to provide background information on some of the legal issues involving children testifying in court, including the accuracy and psychological impact of child testimony; to provide suggestions for how pediatricians can support patients who will testify in court; and to make recommendations for policy improvements to minimize the adverse psychological consequences for child witnesses. These recommendations are, for the most part, based on studies on the psychological and physiologic consequences of children witnessing and experiencing violence, as well as appearing in court, that have emerged since the previous AAP publications on the subject. The goal is to reduce the secondary traumatization of and long-term consequences for children providing testimony about violence they have experienced or witnessed. This statement primarily addresses children appearing in court as victims of physical or sexual abuse or as witnesses of violent acts; most of the scientific literature addresses these specific situations. It may apply, in certain situations, to children required to provide testimony in custody disputes, child welfare proceedings, or immigration court. It does not address children appearing in court as offenders or as part of juvenile justice proceedings. Copyright © 2017 by the American Academy of Pediatrics.

  5. Hubble Space Telescope-Illustration

    Science.gov (United States)

    1989-01-01

    This illustration depicts a side view of the Hubble Space Telescope (HST). The HST is the product of a partnership between NASA, European Space Agency Contractors, and the international community of astronomers. It is named after Edwin P. Hubble, an American Astronomer who discovered the expanding nature of the universe and was the first to realize the true nature of galaxies. The purpose of the HST, the most complex and sensitive optical telescope ever made, is to study the cosmos from a low-Earth orbit. By placing the telescope in space, astronomers are able to collect data that is free of the Earth's atmosphere. The HST detects objects 25 times fainter than the dimmest objects seen from Earth and provides astronomers with an observable universe 250 times larger than visible from ground-based telescopes, perhaps as far away as 14 billion light-years. The HST views galaxies, stars, planets, comets, possibly other solar systems, and even unusual phenomena such as quasars, with 10 times the clarity of ground-based telescopes. The major elements of the HST are the Optical Telescope Assembly (OTA), the Support System Module (SSM), and the Scientific Instruments (SI). The HST is approximately the size of a railroad car, with two cylinders joined together and wrapped in a silvery reflective heat shield blanket. Wing-like solar arrays extend horizontally from each side of these cylinders, and dish-shaped anternas extend above and below the body of the telescope. The HST was deployed from the Space Shuttle Discovery (STS-31 mission) into Earth orbit in April 1990. The Marshall Space Flight Center had responsibility for design, development, and construction of the HST. The Perkin-Elmer Corporation, in Danbury, Connecticut, developed the optical system and guidance sensors. The Lockheed Missile and Space Company of Sunnyvale, California produced the protective outer shroud and spacecraft systems, and assembled and tested the finished telescope.

  6. The role of the expert witness.

    Science.gov (United States)

    Jerrold, Laurance

    2007-08-01

    The role of expert witnesses in medical malpractice litigation is often misunderstood. Much maligned, the expert has been the subject of castigation by a range of people, from his professional colleagues to the jurists who preside over his testimony. From an academic perspective, the expert witness is a necessary evil, and his denigration is his own doing; for the expert is a neutral character who creates his own professional persona. This purpose of this article is to serve as a primer for those interested in understanding the role that the expert is supposed to play in litigation, and the factors surrounding his activities.

  7. Hubble Gallery of Jupiter's Galilean Satellites

    Science.gov (United States)

    1995-01-01

    This is a Hubble Space Telescope 'family portrait' of the four largest moons of Jupiter, first observed by the Italian scientist Galileo Galilei nearly four centuries ago. Located approximately one-half billion miles away, the moons are so small that, in visible light, they appear as fuzzy disks in the largest ground-based telescopes. Hubble can resolve surface details seen previously only by the Voyager spacecraft in the early 1980s. While the Voyagers provided close-up snapshots of the satellites, Hubble can now follow changes on the moons and reveal other characteristics at ultraviolet and near-infrared wavelengths.Over the past year Hubble has charted new volcanic activity on Io's active surface, found a faint oxygen atmosphere on the moon Europa, and identified ozone on the surface of Ganymede. Hubble ultraviolet observations of Callisto show the presence of fresh ice on the surface that may indicate impacts from micrometeorites and charged particles from Jupiter's magnetosphere.Hubble observations will play a complementary role when the Galileo spacecraft arrives at Jupiter in December of this year.This image and other images and data received from the Hubble Space Telescope are posted on the World Wide Web on the Space Telescope Science Institute home page at URL http://oposite.stsci.edu/pubinfo/

  8. Immodest Witnesses: Reliability and Writing Assessment

    Science.gov (United States)

    Gallagher, Chris W.

    2014-01-01

    This article offers a survey of three reliability theories in writing assessment: positivist, hermeneutic, and rhetorical. Drawing on an interdisciplinary investigation of the notion of "witnessing," this survey emphasizes the kinds of readers and readings each theory of reliability produces and the epistemological grounds on which it…

  9. Textile Exports to Japan Witnessing a Downturn

    Institute of Scientific and Technical Information of China (English)

    2010-01-01

    China textile and apparel exports to Japan was witnessing a downturn in all statistics of China Customs and Japan METI in the Jan.-Apr. 2010 period. Exports to Japan this year later will face more pressure as gains in Japan’s consumption could moderate due to a lackluster jobs market and debt crisis.

  10. Rhetorical Witnessing: Recognizing Genocide in Guatemala

    Science.gov (United States)

    Flynn, Elizabeth A.; Wolf, Rudiger Escobar

    2008-01-01

    The article explores the rhetorical dimensions of witnessing. We concentrate, in particular, on two groups: 1) university students at the University of San Carlos, Quetzaltenango, whose murals are dramatic reminders of the massacres that resulted in the deaths of over 200,000 indigenous people in the 1980s and early 90s and of the corrupt…

  11. 41 CFR 105-70.033 - Witnesses.

    Science.gov (United States)

    2010-07-01

    ... 41 Public Contracts and Property Management 3 2010-07-01 2010-07-01 false Witnesses. 105-70.033 Section 105-70.033 Public Contracts and Property Management Federal Property Management Regulations System (Continued) GENERAL SERVICES ADMINISTRATION Regional Offices-General Services Administration...

  12. Why WITS? Why not a way beyond?

    Directory of Open Access Journals (Sweden)

    Shipra Nagar

    2014-01-01

    Full Text Available Introduction: WITS appraisal is a common parameter in cephalometrics to assess maxillo-mandibular skeletal relationship as an adjunct to angle ANB. The high variability of the WITS appraisal is attributable to difficulties or inaccuracies in identifying the occlusal plane or variations due to tooth eruption, dental development or treatment changes by vertical movement of incisors, molars, or both. Aim: An extracranial reference line common to both denture bases, instead of the occlusal plane is proposed to assess antero-posterior jaw relationships. Materials and Methods: A true vertical obtained by plumb line was recorded, while taking the cephalogram for 40 subjects. A line drawn perpendicular to this true vertical gave a stable and reproducible extracranial true horizontal (HOR reference line. The linear distance between perpendiculars from points A and B was measured as an adjunct to angle ANB. Result: The Pearson′s product moment correlation coefficient calculated for the entire sample indicated higher correlation coefficient (r = 0.8712 for the linear measurements on HOR (AH-BH with respect to the angle ANB when compared with the WITS readings (AO-BO (r = 0.549. Conclusion: The horizontal appraisal method proposed eliminates the demerits of the occlusal plane and has the merits of simplicity and accuracy in comparison to WITS appraisal.

  13. Hubble expansion is not a velocity

    Science.gov (United States)

    Ma, Yin-Zhe; Zhang, Shuang-Nan

    2016-11-01

    In this paper, we clarify the difference between the Hubble expansion and the Doppler shift pedagogically and illustrate both physically and mathematically why the Hubble expansion cannot be regarded as a velocity. Therefore, we suggest to replace the misleading word ‘recession velocity’ to be ‘Hubble recession’ to describe the cosmic expansion. We further derive how the peculiar velocity of a galaxy is related to its observed redshift and proper distance, which has practical use in the galaxy redshift and distance surveys.

  14. 76 FR 41691 - Safety Zone; BGSU Football Gridiron Classic Golf and Dinner Fireworks, Catawba Island Club, Port...

    Science.gov (United States)

    2011-07-15

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; BGSU Football Gridiron Classic Golf and... Lake Erie during the BGSU Football Gridiron Classic Golf and Dinner Fireworks. This temporary safety..., Bowling Green State University will hold its BGSU Football Gridiron Classic Golf and Dinner Fireworks,...

  15. 76 FR 65378 - Safety Zone; The Florida Orchestra Pops in the Park Fireworks Display, Tampa Bay, St. Petersburg, FL

    Science.gov (United States)

    2011-10-21

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; The Florida Orchestra Pops in the Park... vicinity of Spa Beach in St. Petersburg, Florida during The Florida Orchestra Pops in the Park Fireworks... Saturday, October 22, 2011, The Florida Orchestra Pops in the Park Fireworks Display is scheduled to...

  16. 76 FR 48718 - Safety Zones; August Fireworks Displays and Swim Events in the Captain of the Port New York Zone

    Science.gov (United States)

    2011-08-09

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zones; August Fireworks Displays and Swim Events... Guard Captain of the Port (COTP) New York Zone for fireworks displays and swim events. This action is... for the Annual Newburgh to Beacon Swim, Swim Across America, and the Rose Pintoff Centennial...

  17. 78 FR 37966 - Safety Zone; National Cherry Festival Air Show and Fireworks Display, West Grand Traverse Bay...

    Science.gov (United States)

    2013-06-25

    ....regulations.gov , inserting USCG-2013-0189 in the ``SEARCH'' box, and then clicking ``SEARCH.'' They are also... National Cherry Festival Fireworks display over West Grand Traverse Bay within the arc of a circle with a... within the arc of a circle with a 1000- foot radius from the fireworks launch site located on a barge...

  18. THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY

    Energy Technology Data Exchange (ETDEWEB)

    Dalcanton, Julianne J.; Williams, Benjamin F.; Rosenfield, Philip; Weisz, Daniel R.; Gilbert, Karoline M.; Gogarten, Stephanie M. [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195 (United States); Lang, Dustin [Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544 (United States); Lauer, Tod R.; Dong Hui [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Kalirai, Jason S.; Boyer, Martha L.; Gordon, Karl D. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Seth, Anil C. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States); Dolphin, Andrew [Raytheon Company, 1151 East Hermans Road, Tucson, AZ 85756 (United States); Bell, Eric F. [Department of Astronomy, University of Michigan, 500 Church St., Ann Arbor, MI 48109 (United States); Bianchi, Luciana C. [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States); Caldwell, Nelson [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Dorman, Claire E.; Guhathakurta, Puragra [University of California Observatories/Lick Observatory, University of California, 1156 High St., Santa Cruz, CA 95064 (United States); Girardi, Leo [Osservatorio Astronomico di Padova-INAF, Vicolo dell' Osservatorio 5, I-35122 Padova (Italy); and others

    2012-06-01

    The Panchromatic Hubble Andromeda Treasury is an ongoing Hubble Space Telescope Multi-Cycle Treasury program to image {approx}1/3 of M31's star-forming disk in six filters, spanning from the ultraviolet (UV) to the near-infrared (NIR). We use the Wide Field Camera 3 (WFC3) and Advanced Camera for Surveys (ACS) to resolve the galaxy into millions of individual stars with projected radii from 0 to 20 kpc. The full survey will cover a contiguous 0.5 deg{sup 2}area in 828 orbits. Imaging is being obtained in the F275W and F336W filters on the WFC3/UVIS camera, F475W and F814W on ACS/WFC, and F110W and F160W on WFC3/IR. The resulting wavelength coverage gives excellent constraints on stellar temperature, bolometric luminosity, and extinction for most spectral types. The data produce photometry with a signal-to-noise ratio of 4 at m{sub F275W} = 25.1, m{sub F336W} = 24.9, m{sub F475W} = 27.9, m{sub F814W} = 27.1, m{sub F110W} = 25.5, and m{sub F160W} = 24.6 for single pointings in the uncrowded outer disk; in the inner disk, however, the optical and NIR data are crowding limited, and the deepest reliable magnitudes are up to 5 mag brighter. Observations are carried out in two orbits per pointing, split between WFC3/UVIS and WFC3/IR cameras in primary mode, with ACS/WFC run in parallel. All pointings are dithered to produce Nyquist-sampled images in F475W, F814W, and F160W. We describe the observing strategy, photometry, astrometry, and data products available for the survey, along with extensive testing of photometric stability, crowding errors, spatially dependent photometric biases, and telescope pointing control. We also report on initial fits to the structure of M31's disk, derived from the density of red giant branch stars, in a way that is independent of assumed mass-to-light ratios and is robust to variations in dust extinction. These fits also show that the 10 kpc ring is not just a region of enhanced recent star formation, but is instead a dynamical

  19. The Panchromatic Hubble Andromeda Treasury

    CERN Document Server

    Dalcanton, J J; Lang, D; Lauer, T R; Kalirai, J S; Seth, A C; Dolphin, A; Rosenfield, P; Weisz, D R; Bell, E F; Bianchi, L C; Boyer, M L; Caldwell, N; Dong, H; Dorman, C E; Gilbert, K M; Girardi, L; Gogarten, S M; Gordon, K D; Guhathakurta, P; Hodge, P W; Holtzman, J A; Johnson, L; Larsen, S S; Lewis, A; Melbourne, J L; Olsen, K A G; Rix, H -W; Rosema, K; Saha, A; Sarajedini, A; Skillman, E D; Stanek, K Z

    2012-01-01

    The Panchromatic Hubble Andromeda Treasury (PHAT) is an on-going HST Multicycle Treasury program to image ~1/3 of M31's star forming disk in 6 filters, from the UV to the NIR. The full survey will resolve the galaxy into more than 100 million stars with projected radii from 0-20 kpc over a contiguous 0.5 square degree area in 828 orbits, producing imaging in the F275W and F336W filters with WFC3/UVIS, F475W and F814W with ACS/WFC, and F110W and F160W with WFC3/IR. The resulting wavelength coverage gives excellent constraints on stellar temperature, bolometric luminosity, and extinction for most spectral types. The photometry reaches SNR=4 at F275W=25.1, F336W=24.9, F475W=27.9, F814W=27.1, F110W=25.5, and F160W=24.6 for single pointings in the uncrowded outer disk; however, the optical and NIR data are crowding limited, and the deepest reliable magnitudes are up to 5 magnitudes brighter in the inner bulge. All pointings are dithered and produce Nyquist-sampled images in F475W, F814W, and F160W. We describe the...

  20. New Explanation of Hubble's Red Shift

    Science.gov (United States)

    Cao, Dayong

    2016-03-01

    The balance system between dark massenergy (with a spacetime center) and stellar massenergy (with a massenergy center) cause a flat universe. In the flat universe, the Hubble 's redshift is caused by the Lorentz transformation (Einstein transformation). This paper will discuss about the relationship among Einstein transformation, Doppler effect, and Hubble 's redshift under the balanced and flat universe model. http://meetings.aps.org/link/BAPS.2014.APR.Y9.1

  1. Gender, smiling, and witness credibility in actual trials.

    Science.gov (United States)

    Nagle, Jacklyn E; Brodsky, Stanley L; Weeter, Kaycee

    2014-01-01

    It has been acknowledged that females exhibit more smiling behaviors than males, but there has been little attention to this gender difference in the courtroom. Although both male and female witnesses exhibit smiling behaviors, there has been no research examining the subsequent effect of gender and smiling on witness credibility. This study used naturalistic observation to examine smiling behaviors and credibility in actual witnesses testifying in court. Raters assessed the smiling behaviors and credibility (as measured by the Witness Credibility Scale) of 32 male and female witnesses testifying in trials in a mid-sized Southern city. "Credibility raters" rated the perceived likeability, trustworthiness, confidence, knowledge, and overall credibility of the witnesses using the Witness Credibility Scale. "Smile raters" noted smiling frequency and types, including speaking/expressive and listening/receptive smiles. Gender was found to affect perceived trustworthiness ratings, in which male witnesses were seen as more trustworthy than female witnesses. No significant differences were found in the smiling frequency for male and female witnesses. However, the presence of smiling was found to contribute to perceived likeability of a witness. Smiling female witnesses were found to be more likeable than smiling male and non-smiling female witnesses. Copyright © 2014 John Wiley & Sons, Ltd.

  2. CHILD WITNESSES AND THE CONFRONTATION CLAUSE.

    Science.gov (United States)

    Lyon, Thomas D; Dente, Julia A

    2012-01-01

    After the Supreme Court's ruling in Crawford v. Washington that a criminal defendant's right to confront the witnesses against him is violated by the admission of testimonial hearsay that has not been cross-examined, lower courts have overturned convictions in which hearsay from children was admitted after child witnesses were either unwilling or unable to testify. A review of social scientific evidence regarding the dynamics of child sexual abuse suggests a means for facilitating the fair receipt of children's evidence. Courts should hold that defendants have forfeited their confrontation rights if they exploited a child's vulnerabilities such that they could reasonably anticipate that the child would be unavailable to testify. Exploitation includes choosing victims on the basis of their filial dependency, their vulnerability, or their immaturity, as well as taking actions that create or accentuate those vulnerabilities.

  3. [Expert medical witness testimony of maxillofacial injuries].

    Science.gov (United States)

    Orihovac, Zeljko; Macan, Darko

    2008-07-01

    The basic principles of expert medical witness testimony of the maxillofacial region are described. The specific anatomic characteristics of the region are emphasized, especially in view of the fact that face is the most exposed part of the human body. Post-traumatic deformities of the maxillofacial region involve soft tissues of the face and mouth as well as bony structures of the viscerocranium and teeth. Endured physical pain, lessening of life activities, disfigurement and requirement of assistance by third person are separately described as an important part of expert medical witness testimony of the maxillofacial region. The number of lawsuits raised against physicians has significantly increased in the past several years, more often in cases where the patients are dissatisfied with the results of cosmetic surgery, especially when these procedures are performed on the face.

  4. Optimized entanglement witnesses for Dicke states

    Energy Technology Data Exchange (ETDEWEB)

    Bergmann, Marcel; Guehne, Otfried [Naturwissenschaftlich-Technische Fakultaet, Universitaet Siegen, Department Physik, Walter-Flex-Strasse 3, D-57068 Siegen (Germany)

    2013-07-01

    Quantum entanglement is an important resource for applications in quantum information processing like quantum teleportation and cryptography. Moreover, the number of particles that can be entangled experimentally using polarized photons or ion traps has been significantly enlarged. Therefore, criteria to decide the question whether a given multi-particle state is entangled or not have to be improved. Our approach to this problem uses the notion of PPT mixtures which form an approximation to the set of bi-separable states. With this method, entanglement witnesses can be obtained in a natural manner via linear semi-definite programming. In our contribution, we will present analytical results for entanglement witnesses for Dicke states. This allows to overcome the limitations of convex optimization.

  5. Former astronaut Armstrong witnesses STS-83 launch

    Science.gov (United States)

    1997-01-01

    Apollo l1 Commander Neil A. Armstrong and his wife, Carol, were among the many special NASA STS-83 launch guests who witnessed the liftoff of the Space Shuttle Columbia April 4 at the Banana Creek VIP Viewing Site at KSC. Columbia took off from Launch Pad 39A at 2:20:32 p.m. EST to begin the 16-day Microgravity Science Laboratory-1 (MSL-1) mission.

  6. Positive maps, positive polynomials and entanglement witnesses

    CERN Document Server

    Skowronek, Lukasz

    2009-01-01

    We link the study of positive quantum maps, block positive operators, and entanglement witnesses with problems related to multivariate polynomials. For instance, we show how indecomposable block positive operators relate to biquadratic forms that are not sums of squares. Although the general problem of describing the set of positive maps remains open, in some particular cases we solve the corresponding polynomial inequalities and obtain explicit conditions for positivity.

  7. Positive maps, positive polynomials and entanglement witnesses

    Energy Technology Data Exchange (ETDEWEB)

    Skowronek, Lukasz; Zyczkowski, Karol [Institute of Physics, Jagiellonian University, Krakow (Poland)], E-mail: lukasz.skowronek@uj.edu.pl, E-mail: karol@tatry.if.uj.edu.pl

    2009-08-14

    We link the study of positive quantum maps, block positive operators and entanglement witnesses with problems related to multivariate polynomials. For instance, we show how indecomposable block positive operators relate to biquadratic forms that are not sums of squares. Although the general problem of describing the set of positive maps remains open, in some particular cases we solve the corresponding polynomial inequalities and obtain explicit conditions for positivity.

  8. United States Federal Guidance on Witness Protection in Human Trafficking

    Science.gov (United States)

    2015-06-12

    UNITED STATES FEDERAL GUIDANCE ON WITNESS PROTECTION IN HUMAN TRAFFICKING A thesis presented to the Faculty of the U.S. Army...JUN 2015 4. TITLE AND SUBTITLE United States Federal Guidance on Witness Protection in Human Trafficking 5a. CONTRACT NUMBER 5b. GRANT NUMBER...United States needs overarching federal guidance on witness protection for human trafficking victims/witnesses in order to enhance their safety and

  9. Analytical Solutions for Bending Of Fireworks and Similarities with the Solution of Electromagnetic Wave Diffraction

    CERN Document Server

    Akbar, Fathan

    2016-01-01

    In this paper we examine more deeply about the bending mechanism of rod-shaped fireworks which burned from the free end. We derived new analytic equations. Surprisingly, we obtained the bending patterns are similar to the cornu spiral. With a few simple steps we proved that positions of points throughout the fireworks are given by Fresnel integrals, C(x) and S(x), which are generally found in phenomena of electromagnetic wave diffraction. Although we deeply discussed bending of fireworks rods, however the proposed method is likely to explain any phenomena in nature related to an evolving length scale associated with some material that becomes progressively stiff or dry, such as the growth of resin exuded from trees.

  10. 32 CFR 516.54 - Witnesses for the United States.

    Science.gov (United States)

    2010-07-01

    ... 32 National Defense 3 2010-07-01 2010-07-01 true Witnesses for the United States. 516.54 Section 516.54 National Defense Department of Defense (Continued) DEPARTMENT OF THE ARMY AID OF CIVIL AUTHORITIES AND PUBLIC RELATIONS LITIGATION Release of Information and Appearance of Witnesses Scope Status, Travel, and Expenses of Witnesses §...

  11. 39 CFR 955.22 - Examination of witnesses.

    Science.gov (United States)

    2010-07-01

    ... 39 Postal Service 1 2010-07-01 2010-07-01 false Examination of witnesses. 955.22 Section 955.22 Postal Service UNITED STATES POSTAL SERVICE PROCEDURES RULES OF PRACTICE BEFORE THE POSTAL SERVICE BOARD OF CONTRACT APPEALS § 955.22 Examination of witnesses. Witnesses before the Board will be examined...

  12. 29 CFR 18.615 - Exclusion of witnesses.

    Science.gov (United States)

    2010-07-01

    ... 29 Labor 1 2010-07-01 2010-07-01 true Exclusion of witnesses. 18.615 Section 18.615 Labor Office... OFFICE OF ADMINISTRATIVE LAW JUDGES Rules of Evidence Witnesses § 18.615 Exclusion of witnesses. At the... authorize exclusion of a party who is a natural person, or an officer or employee of a party which is not...

  13. 5 CFR 1201.32 - Witnesses; right to representation.

    Science.gov (United States)

    2010-01-01

    ... 5 Administrative Personnel 3 2010-01-01 2010-01-01 false Witnesses; right to representation. 1201.32 Section 1201.32 Administrative Personnel MERIT SYSTEMS PROTECTION BOARD ORGANIZATION AND... § 1201.32 Witnesses; right to representation. Witnesses have the right to be represented when testifying...

  14. 29 CFR 2.15 - Protection of witnesses.

    Science.gov (United States)

    2010-07-01

    ... 29 Labor 1 2010-07-01 2010-07-01 true Protection of witnesses. 2.15 Section 2.15 Labor Office of the Secretary of Labor GENERAL REGULATIONS Audiovisual Coverage of Administrative Hearings § 2.15 Protection of witnesses. A witness has the right, prior to or during his testimony, to exclude...

  15. Version 1 of the Hubble Source Catalog

    CERN Document Server

    Whitmore, Bradley C; Budavari, Tamas; Casertano, Stefano; Downes, Ronald A; Donaldson, Thomas; Fall, S Michael; Lubow, Stephen H; Quick, Lee; Strolger, Louis-Gregory; Wallace, Geoff; White, Richard L

    2016-01-01

    The Hubble Source Catalog is designed to help optimize science from the Hubble Space Telescope by combining the tens of thousands of visit-based source lists in the Hubble Legacy Archive into a single master catalog. Version 1 of the Hubble Source Catalog includes WFPC2, ACS/WFC, WFC3/UVIS, and WFC3/IR photometric data generated using SExtractor software to produce the individual source lists. The catalog includes roughly 80 million detections of 30 million objects involving 112 different detector/filter combinations, and about 160 thousand HST exposures. Source lists from Data Release 8 of the Hubble Legacy Archive are matched using an algorithm developed by Budavari & Lubow (2012). The mean photometric accuracy for the catalog as a whole is better than 0.10 mag, with relative accuracy as good as 0.02 mag in certain circumstances (e.g., bright isolated stars). The relative astrometric residuals are typically within 10 mas, with a value for the mode (i.e., most common value) of 2.3 mas. The absolute astro...

  16. Testing the Copernican Principle with Hubble Parameter

    CERN Document Server

    Zhang, Tong-Jie; Ma, Cong

    2012-01-01

    By way of expressing the Hubble expansion rate for the general Lema\\^{i}tre-Tolman-Bondi (LTB) metric as a function of cosmic time, we test the scale on which the Copernican Principle holds in the context of a void model. By performing parameter estimation on the CGBH void model, we show the Hubble parameter data favors a void with characteristic radius of $2 \\sim 3$ Gpc. This brings the void model closer, but not yet enough, to harmony with observational indications given by the background kinetic Sunyaev-Zel'dovich effect and the normalization of near-infrared galaxy luminosity function. However, the test of such void models may ultimately lie in the future detection of the discrepancy between longitudinal and transverse expansion rates, a touchstone of inhomogeneous models. With the proliferation of observational Hubble parameter data and future large-scale structure observation, a definitive test could be performed on the question of cosmic homogeneity.

  17. Witnessing the elimination of magic wands.

    Science.gov (United States)

    Blom, Stefan; Huisman, Marieke

    This paper discusses static verification of programs that have been specified using separation logic with magic wands. Magic wands are used to specify incomplete resources in separation logic, i.e., if missing resources are provided, a magic wand allows one to exchange these for the completed resources. One of the applications of the magic wand operator is to describe loop invariants for algorithms that traverse a data structure, such as the imperative version of the tree delete problem (Challenge 3 from the VerifyThis@FM2012 Program Verification Competition), which is the motivating example for our work. Most separation logic-based static verification tools do not provide support for magic wands, possibly because validity of formulas containing the magic wand is, by itself, undecidable. To avoid this problem, in our approach the program annotator has to provide a witness for the magic wand, thus circumventing undecidability due to the use of magic wands. A witness is an object that encodes both instructions for the permission exchange that is specified by the magic wand and the extra resources needed during that exchange. We show how this witness information is used to encode a specification with magic wands as a specification without magic wands. Concretely, this approach is used in the VerCors tool set: annotated Java programs are encoded as Chalice programs. Chalice then further translates the program to BoogiePL, where appropriate proof obligations are generated. Besides our encoding of magic wands, we also discuss the encoding of other aspects of annotated Java programs into Chalice, and in particular, the encoding of abstract predicates with permission parameters. We illustrate our approach on the tree delete algorithm, and on the verification of an iterator of a linked list.

  18. Being an expert witness in geomorphology

    Science.gov (United States)

    Keller, Edward A.

    2015-02-01

    Gathering your own data and coming to your own conclusion through scientific research and discovery is the most important principle to remember when being an expert witness in geomorphology. You can only be questioned in deposition and trial in your area of expertise. You are qualified as an expert by education, knowledge, and experience. You will have absolutely nothing to fear from cross-examination if you are prepared and confident about your work. Being an expert witness requires good communication skills. When you make a presentation, speak clearly and avoid jargon, especially when addressing a jury. Keep in mind that when you take on a case that may eventually go to court as a lawsuit, the entire process, with appeals and so forth, can take several years. Therefore, being an expert may become a long-term commitment of your time and energy. You may be hired by either side in a dispute, but your job is the same - determine the scientific basis of the case and explain your scientific reasoning to the lawyers, the judge, and the jury. Your work, including pre-trial investigations, often determines what the case will be based on. The use of science in the discovery part of an investigation is demonstrated from a California case involving the Ventura River, where building of a flood control levee restricted flow to a narrower channel, increasing unit stream power as well as potential for bank erosion and landsliding.

  19. 75 FR 67618 - Safety Zone: Richardson Ash Scattering by Fireworks, San Francisco, CA

    Science.gov (United States)

    2010-11-03

    ... Sausalito Ferry docks in Sausalito, CA. From 6:15 p.m. until 7 p.m., the area to which the temporary safety... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone: Richardson Ash Scattering by Fireworks, San... establishing a temporary safety zone in the navigable waters of San Francisco Bay 1,500 feet off Yellow Bluff...

  20. 76 FR 64820 - Safety Zone; Mainardi/Kinsey Wedding Fireworks, Lake Erie, Lakewood, OH

    Science.gov (United States)

    2011-10-19

    ... premature detonations, dangerous detonations, dangerous projectiles, and falling or burning debris that may cause death, serious bodily injury or property damage. Discussion of Rule Because of the aforementioned.../Kinsey wedding fireworks display. The safety zone will be in effect on October 22, 2011 from 8:30 p.m....

  1. 33 CFR 100.T05-0443 - Safety Zone; Fireworks Display, Delaware River, New Hope, PA.

    Science.gov (United States)

    2010-07-01

    ..., Delaware River, New Hope, PA. 100.T05-0443 Section 100.T05-0443 Navigation and Navigable Waters COAST GUARD... Safety Zone; Fireworks Display, Delaware River, New Hope, PA. (a) Location. The safety zone will restrict.... Bridge located in New Hope, PA, and 400 ft east of the shoreline of New Hope, PA. (b) Regulations. (1)...

  2. 76 FR 37007 - Safety Zone; Stockton Ports Baseball Club Fourth of July Fireworks Display, Stockton, CA

    Science.gov (United States)

    2011-06-24

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Stockton Ports Baseball Club Fourth of July... Stockton Ports Baseball Club will sponsor the Stockton Ports Baseball Club Fourth of July Fireworks Display... read as follows: Sec. 165.T11-422 Safety Zone; Stockton Ports Baseball Club Fourth of July...

  3. 76 FR 65963 - Safety Zone; Waverly Country Club Fireworks Display on the Willamette River, Portland, OR

    Science.gov (United States)

    2011-10-25

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Waverly Country Club Fireworks Display on...: The Coast Guard is establishing a safety zone on the Willamette River located at the Waverly Country... safety zone covers all waters of the Willamette River in front of the Waverly Country Club...

  4. 75 FR 79085 - Notice and Request for Comments on the Clarification of the Fireworks Approvals Policy

    Science.gov (United States)

    2010-12-17

    ... logistics supply chain comprised of mostly foreign fireworks manufacturers and domestic importers, retailers... pyrotechnic industry regardless of their actual position in the supply chain. It is unclear as to what was the... change to the Federal Docket Management System (FDMS), including any personal information. Docket:...

  5. 76 FR 27251 - Safety Zone; Coughlin Wedding Fireworks, Lake St. Clair, Harrison Township, MI

    Science.gov (United States)

    2011-05-11

    ..., Harrison Township, MI AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a temporary safety zone on Lake St. Clair, Harrison Township, MI. This safety zone is intended to... radius of the fireworks barge launch site located off the shore of Harrison Township, MI at position...

  6. 77 FR 43167 - Safety Zone; Electric Zoo Fireworks, East River, Randall's Island, NY

    Science.gov (United States)

    2012-07-24

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Electric Zoo Fireworks, East River, Randall... prior notice and opportunity to comment when the agency for good cause finds that those procedures are... finds that good cause exists for not publishing a notice of proposed rulemaking (NPRM) with respect...

  7. 77 FR 19573 - Safety Zone; Wedding Fireworks Display, Boston Inner Harbor, Boston, MA

    Science.gov (United States)

    2012-04-02

    ... the January 17, 2008, issue of the Federal Register (73 FR 3316). Public Meeting We do not now plan to... Harbor, Boston, MA AGENCY: Coast Guard, DHS. ACTION: Notice of proposed rulemaking. SUMMARY: The Coast... in the vicinity of Anthony's Pier 4, Boston, MA for a wedding fireworks display. This...

  8. 78 FR 23850 - Safety Zones; Annual Fireworks Events in the Captain of the Port Buffalo Zone

    Science.gov (United States)

    2013-04-23

    ...) Mentor Harbor Yacht Club Fireworks, Mentor Harbor, OH. (i) Location. All U.S. waters of Lake Erie and Mentor Harbor within a 700 foot radius of land position 41 43'36'' N, 081 21'09'' W (NAD 83) in Mentor... necessary to maintain a safe course. (d) Exemption. Public vessels, as defined in paragraph (b) of...

  9. 76 FR 27967 - Safety Zone; Shore Thing and Independence Day Fireworks, Chesapeake Bay, Norfolk, VA

    Science.gov (United States)

    2011-05-13

    ... View Beach Park, Norfolk, VA in support of the Shore Thing and Independence Day Fireworks event. This action is necessary to provide for the safety of life on navigable waters during the Shore Thing and... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Shore Thing and Independence Day...

  10. 77 FR 51475 - Safety Zone; Apache Pier Labor Day Fireworks; Myrtle Beach, SC

    Science.gov (United States)

    2012-08-24

    ... INFORMATION: Table of Acronyms DHS Department of Homeland Security FR Federal Register NPRM Notice of Proposed... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Apache Pier Labor Day Fireworks; Myrtle... establishing a temporary safety zone on the waters of the Atlantic Ocean in the vicinity of Apache Pier...

  11. 76 FR 46626 - Safety Zone; Discovery World Private Wedding Firework Displays, Milwaukee, WI

    Science.gov (United States)

    2011-08-03

    ... From the Federal Register Online via the Government Publishing Office DEPARTMENT OF HOMELAND SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Discovery World Private Wedding Firework Displays, Milwaukee, WI AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard...

  12. 78 FR 29086 - Safety Zone; Discovery World Fireworks, Milwaukee Harbor, Milwaukee, WI

    Science.gov (United States)

    2013-05-17

    ... Acronyms DHS--Department of Homeland Security FR--Federal Register NPRM--Notice of Proposed Rulemaking A... Federal Register (73 FR 3316). 4. Public Meeting We do not now plan to hold a public meeting, but you may... Fireworks, Milwaukee Harbor, Milwaukee, WI AGENCY: Coast Guard, DHS. ACTION: Notice of proposed...

  13. 76 FR 61947 - Safety Zones; Fireworks Displays in Captain of the Port Long Island Sound Zone

    Science.gov (United States)

    2011-10-06

    ... move their event dates for the following reasons. The sponsor for CDM Chamber of Commerce Annual Music... Executive Order 13563, and does not require an assessment of potential costs and benefits under section 6(a....T01-0870 Fireworks display events 1 CDM Chamber of Commerce Annual Music Date: September 24,...

  14. 76 FR 33641 - Safety Zone; The Pacific Grove Feast of Lanterns, Fireworks Display, Pacific Grove, CA

    Science.gov (United States)

    2011-06-09

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; The Pacific Grove Feast of Lanterns... Lovers Point, in Pacific Grove, California in support of the Pacific Grove Feast of Lanterns Fireworks... regulations must be in effect during the event. Basis and Purpose Pacific Grove Feast of Lanterns will...

  15. 78 FR 11798 - Safety Zones; Annual Fireworks Events in the Captain of the Port Buffalo Zone

    Science.gov (United States)

    2013-02-20

    ... coordinates for the safety zones corresponding with the Browns Football Half time Fireworks and the Lorain... Football Half time and the Lorain Port Fest safety zones, to include changing the format of the coordinates... economy, will not interfere with other agencies, will not adversely alter the budget of any grant or loan...

  16. 76 FR 61259 - Safety Zone; Monte Foundation Fireworks Extravaganza, Aptos, CA

    Science.gov (United States)

    2011-10-04

    ..., California in support of the Monte Foundation Fireworks Extravaganza. This safety zone is established to... life, property and the environment; therefore, a 30-day notice is impracticable. Delaying the effective... safety that may disproportionately affect children. Indian Tribal Governments This rule does not...

  17. 78 FR 38584 - Safety Zone; San Diego Symphony Summer POPS Fireworks 2013 Season, San Diego, CA

    Science.gov (United States)

    2013-06-27

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; San Diego Symphony Summer POPS Fireworks 2013 Season, San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a safety zone on the navigable waters of San Diego Bay in support of the San Diego...

  18. 78 FR 10062 - Safety Zone; Sea World San Diego Fireworks, Mission Bay; San Diego, CA

    Science.gov (United States)

    2013-02-13

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Sea World San Diego Fireworks, Mission Bay; San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a safety zone on the navigable waters of Mission Bay in support of the Sea World San Diego...

  19. 77 FR 42647 - Safety Zone: San Diego Symphony POPS Fireworks; San Diego, CA

    Science.gov (United States)

    2012-07-20

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone: San Diego Symphony POPS Fireworks; San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a safety zone on the navigable waters of San Diego Bay in support of the San Diego Symphony POPS...

  20. 77 FR 42649 - Safety Zone: Sea World San Diego Fireworks, Mission Bay; San Diego, CA

    Science.gov (United States)

    2012-07-20

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone: Sea World San Diego Fireworks, Mission Bay; San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is... rule, call or email Petty Officer David Varela, Waterways Management, U.S. Coast Guard Sector San Diego...

  1. 77 FR 60899 - Safety Zone; Sea World San Diego Fireworks, Mission Bay; San Diego, CA

    Science.gov (United States)

    2012-10-05

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Sea World San Diego Fireworks, Mission Bay; San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a safety zone on the navigable waters of Mission Bay in support of the Sea World San Diego...

  2. 77 FR 42638 - Safety Zone: Sea World San Diego Fireworks, Mission Bay; San Diego, CA

    Science.gov (United States)

    2012-07-20

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone: Sea World San Diego Fireworks, Mission Bay; San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a safety zone on the navigable waters of Mission Bay in support of the Sea World San Diego...

  3. 78 FR 29025 - Sea World San Diego Fireworks 2013 Season; Mission Bay, San Diego, CA

    Science.gov (United States)

    2013-05-17

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Sea World San Diego Fireworks 2013 Season; Mission Bay, San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a safety zone on the navigable waters of Mission Bay in support of the Sea World San Diego...

  4. 78 FR 48046 - Safety Zone; Kuoni Destination Management Fireworks; San Diego, CA

    Science.gov (United States)

    2013-08-07

    ... [Docket No. USCG-2013-0666] RIN 1625-AA00 Safety Zone; Kuoni Destination Management Fireworks; San Diego... safety zone on the navigable waters of the San Diego Bay in support of the Kuoni Destination Management... San Diego, Coast Guard; telephone 619-278-7656, email d11marineeventssandiego@uscg.mil . If you have...

  5. 75 FR 77756 - Safety Zone; San Diego Parade of Lights Fireworks, San Diego, CA

    Science.gov (United States)

    2010-12-14

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; San Diego Parade of Lights Fireworks, San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a safety zone upon the navigable water of the San Diego Bay in San Diego, CA in support of the two...

  6. 76 FR 22812 - Safety Zone; Sea World Fireworks; Mission Bay, San Diego, CA

    Science.gov (United States)

    2011-04-25

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Sea World Fireworks; Mission Bay, San Diego... Diego, CA; telephone (619) 278- 7233, e-mail Cody.C.McLaughlin@uscg.mil . If you have questions on...; Mission Bay, San Diego, CA. (a) Location. The safety zone will include the area within 600 feet of the...

  7. 77 FR 35268 - Safety Zone, Fireworks Display, Lake Superior; Cornucopia, WI

    Science.gov (United States)

    2012-06-13

    ... or fatalities. Establishing a safety zone to control vessel movement around the location of the... the fireworks launch site with its center in position 46 51'35'' N, 091 06'10'' W.; at Cornucopia, WI... and the States, or on the distribution of power and responsibilities among the various levels of...

  8. Constructing optimal entanglement witnesses. II. Witnessing entanglement in 4N×4N systems

    Science.gov (United States)

    Chruściński, Dariusz; Pytel, Justyna

    2010-11-01

    We provide a class of optimal nondecomposable entanglement witnesses for 4N×4N composite quantum systems or, equivalently, another construction of nondecomposable positive maps in the algebra of 4N×4N complex matrices. This construction provides natural generalization of the Robertson map. It is shown that their structural physical approximations give rise to entanglement breaking channels.

  9. Delegateable signatures based on non-interactive witness indistinguishable and non-interactive witness hiding proofs

    Institute of Scientific and Technical Information of China (English)

    TANG ChunMing; PEI DingYi; WANG XiaoFeng; LIU ZhuoJun

    2008-01-01

    A delegateable signature scheme (DSS) which was first introduced by Barak is mainly based on the non-interactive zero-knowledge proof (NIZK) for preventing the signing verifier from telling which witness (i.e., restricted subset) is being used. However, the scheme is not significantly efficient due to the difficulty of constructing NIZK. We first show that a non-Interactive witness indistinguishable (NIWI) proof sys-tern and a non-interactive witness hiding (NIWH) proof system are easier and more efficient proof models than NIZK in some cases. Furthermore, the witnesses em-ployed in these two protocols (NIWI and NIWT) cannot also be distinguished by the verifiers. Combined with the Σ-protocol, we then construct NlWl and NIWH proofs for any NP statement under the existence of one-way functions and show that each proof is different from those under the existence of trapdoor permutations. Finally, based on our NIWI and NIWH proofs, we construct delegateable signature schemes under the existence of one-way functions, which are more efficient than Barak's scheme under the existence of trapdoor permutations.

  10. The Hubble Flow of Plateau Inflation

    NARCIS (Netherlands)

    Coone, Dries; Roest, Diederik; Vennin, Vincent

    2015-01-01

    In the absence of CMB precision measurements, a Taylor expansion has often been invoked to parametrize the Hubble flow function during inflation. The standard "horizon flow" procedure implicitly relies on this assumption. However, the recent Planck results indicate a strong preference for plateau

  11. HUBBLE CAPTURES DYNAMICS OF CRAB NEBULA

    Science.gov (United States)

    2002-01-01

    A new sequence of Hubble Space Telescope images of the remnant of a tremendous stellar explosion is giving astronomers a remarkable look at the dynamic relationship between the tiny Crab Pulsar and the vast nebula that it powers. This picture shows a Hubble Space Telescope image of the inner parts of the Crab. The pulsar itself is visible as the left of the pair of stars near the center of the frame. Surrounding the pulsar is a complex of sharp knots and wisp-like features. This image is one of a sequence of Hubble images taken over the course of several months. This sequence shows that the inner part of the Crab Nebula is far more dynamic than previously understood. The Crab literally 'changes it stripes' every few days as these wisps stream away from the pulsar at half the speed of light. The Hubble Space Telescope photo was taken Nov. 5, 1995 by the Wide Field and Planetary Camera 2 at a wavelength of around 550 nanometers, in the middle of the visible part of the electromagnetic spectrum. Credit: Jeff Hester and Paul Scowen (Arizona State University), and NASA

  12. The Hubble Flow of Plateau Inflation

    NARCIS (Netherlands)

    Coone, Dries; Roest, Diederik; Vennin, Vincent

    2015-01-01

    In the absence of CMB precision measurements, a Taylor expansion has often been invoked to parametrize the Hubble flow function during inflation. The standard "horizon flow" procedure implicitly relies on this assumption. However, the recent Planck results indicate a strong preference for plateau in

  13. The Hubble Space Telescope: Problems and Solutions.

    Science.gov (United States)

    Villard, Ray

    1990-01-01

    Presented is the best understanding of the flaw discovered in the optics of the Hubble Space Telescope and the possible solutions to the problems. The spherical aberration in the telescope's mirror and its effect on the quality of the telescope's imaging ability is discussed. (CW)

  14. Hubble Exoplanet Pro/Am Collaboration (Abstract)

    Science.gov (United States)

    Conti, D. M.

    2016-06-01

    (Abstract only) A collaborative effort is being organized between a world-wide network of amateur astronomers and a Hubble Space Telescope (HST) science team. The purpose of this collaboration is to supplement an HST near-infrared spectroscopy survey of some 15 exoplanets with ground-based observations in the visible range.

  15. Dark Energy and the Hubble Law

    Science.gov (United States)

    Chernin, A. D.; Dolgachev, V. P.; Domozhilova, L. M.

    The Big Bang predicted by Friedmann could not be empirically discovered in the 1920th, since global cosmological distances (more than 300-1000 Mpc) were not available for observations at that time. Lemaitre and Hubble studied receding motions of galaxies at local distances of less than 20-30 Mpc and found that the motions followed the (nearly) linear velocity-distance relation, known now as Hubble's law. For decades, the real nature of this phenomenon has remained a mystery, in Sandage's words. After the discovery of dark energy, it was suggested that the dynamics of local expansion flows is dominated by omnipresent dark energy, and it is the dark energy antigravity that is able to introduce the linear velocity-distance relation to the flows. It implies that Hubble's law observed at local distances was in fact the first observational manifestation of dark energy. If this is the case, the commonly accepted criteria of scientific discovery lead to the conclusion: In 1927, Lemaitre discovered dark energy and Hubble confirmed this in 1929.

  16. Local gravitational physics of the Hubble expansion

    CERN Document Server

    Kopeikin, Sergei

    2014-01-01

    We study physical consequences of the Hubble expansion of FLRW manifold on measurement of space, time and light propagation in the local inertial frame. We analyse the solar system radar ranging and Doppler tracking experiments, and time synchronization. FLRW manifold is covered by global coordinates (t,y^i), where t is the cosmic time coinciding with the proper time of the Hubble observers. We introduce local inertial coordinates x^a=(x^0,x^i) in the vicinity of a world line of a Hubble observer with the help of a special conformal transformation. The local inertial metric is Minkowski flat and is materialized by the congruence of time-like geodesics of static observers being at rest with respect to the local spatial coordinates x^i. We consider geodesic motion of test particles and notice that the local coordinate time x^0=x^0(t) taken as a parameter along the world line of particle, is a function of the Hubble's observer time t. This function changes smoothly from x^0=t for a particle at rest (observer's c...

  17. 33 CFR 165.161 - Safety zones: Coast Guard Captain of the Port New York annual fireworks displays.

    Science.gov (United States)

    2010-07-01

    ... following New Year's Eve. (b) Regulations. (1) The general regulations contained in 33 CFR 165.23 apply. (2... following Labor Day. (5) Deepavali Festival fireworks, East River, NY: (i) Location. All waters of the...

  18. 76 FR 38015 - Safety Zones; July 4th Weekend Fireworks Displays Within the Captain of the Port St. Petersburg...

    Science.gov (United States)

    2011-06-29

    ... fireworks will be launched, located on the Gulf of Mexico just offshore of Sand Bar Restaurant in Anna Maria... safety zone will be enforced for a maximum of two hours and 15 minutes; (2) vessel traffic in the...

  19. 78 FR 34577 - Safety Zone; Ad Club's 100th Anniversary Gala Fireworks Display, Boston Inner Harbor, Boston, MA.

    Science.gov (United States)

    2013-06-10

    ... Anniversary Gala celebration being held at The Institute Of Contemporary Art in conjunction with the fireworks... 100th Anniversary Gala celebration at The Institute of Contemporary Art. The COTP Boston has...

  20. [Influence of Burning Fireworks on Air Quality During the Spring Festival in the Pearl River Delta].

    Science.gov (United States)

    Zhao, Wei; Fan, Shao-jia; Xie, Wen-zhang; Sun, Jia-ren

    2015-12-01

    Based on data from the air quality monitoring stations in the Pearl River Delta during the 2015 Spring Festival, the regional air quality was investigated and the impact of burning fireworks on urban air quality was assessed. The results showed that: Zhaoqing was the worst polluted city in PM₁₀, PM₂.₅, SO₂ and CO in terms of concentrations in the region during the period, Huizhou was the worst polluted city in O₃ and Guangzhou was the most polluted city in NO₂ at the same time. Compared to the data of last year, the SO₂, NO₂, CO, PM₁₀ and PM₂.₅ concentrations had decreased significantly, but the O₃ concentration had increased during the Spring Festival. Burning fireworks during the Spring Festival were mainly concentrated in the suburbs. The concentrated discharge of fireworks made the SO₂, PM₁₀ and PM₂.₅ concentrations increased significantly in the New Year's Eve night, even multiplied, but had no significant effect on CO, O₃ and NO₂. The rapid decline in PM₂.₅/PM₁₀ proportion was caused by the discharge of fireworks, and the ratio of PM₂.₅/PM₁₀ reached the minimum when concentration of particles reached the peak. By assessing, the maximum contribution of hourly concentration from burning fireworks in each city was between 16 µg · m⁻³ and 65 µg · m⁻³ for PM₂.₅, between 28 µg · m⁻³ and 138 µg · m⁻³ for PM₁₀ and between 9 µg · m⁻³ and 43 µg · m⁻³ for SO₂.

  1. Chemical speciation of respirable suspended particulate matter during a major firework festival in India.

    Science.gov (United States)

    Sarkar, Sayantan; Khillare, Pandit S; Jyethi, Darpa S; Hasan, Amreen; Parween, Musarrat

    2010-12-15

    Ambient respirable particles (PM ≤ 10 μm, denoted by PM(10)) were characterized with respect to 20 elements, 16 polycyclic aromatic hydrocarbons (PAHs), elemental and organic carbon (EC and OC) during a major firework event-the "Diwali" festival in Delhi, India. The event recorded extremely high 24-h PM(10) levels (317.2-616.8 μg m(-3), 6-12 times the WHO standard) and massive loadings of Ba (16.8 μg m(-3), mean value), K (46.8 μg m(-3)), Mg (21.3 μg m(-3)), Al (38.4 μg m(-3)) and EC (40.5 μg m(-3)). Elemental concentrations as high as these have not been reported previously for any firework episode. Concentrations of Ba, K, Sr, Mg, Na, S, Al, Cl, Mn, Ca and EC were higher by factors of 264, 18, 15, 5.8, 5, 4, 3.2, 3, 2.7, 1.6 and 4.3, respectively, on Diwali as compared to background values. It was estimated that firework aerosol contributed 23-33% to ambient PM(10) on Diwali. OC levels peaked in the post-Diwali samples, perhaps owing to secondary transformation processes. Atmospheric PAHs were not sourced from fireworks; instead, they correlated well with changes in traffic patterns indicating their primary source in vehicular emissions. Overall, the pollutant cocktail generated by the Diwali fireworks could be best represented with Ba, K and Sr as tracers. It was also found that chronic exposure to Diwali pollution is likely to cause at least a 2% increase in non-carcinogenic hazard index (HI) associated with Al, Mn and Ba in the exposed population. Copyright © 2010 Elsevier B.V. All rights reserved.

  2. The air pollution caused by the burning of fireworks during the lantern festival in Beijing

    Science.gov (United States)

    Wang, Ying; Zhuang, Guoshun; Xu, Chang; An, Zhisheng

    The effects of the burning of fireworks on air quality in Beijing was firstly assessed from the ambient concentrations of various air pollutants (SO 2, NO 2, PM 2.5, PM 10 and chemical components in the particles) during the lantern festival in 2006. Eighteen ions, 20 elements, and black carbon were measured in PM 2.5 and PM 10, and the levels of organic carbon could be well estimated from the concentrations of dicarboxylic acids. Primary components of Ba, K, Sr, Cl -, Pb, Mg and secondary components of C 5H 6O 42-, C 3H 2O 42-, C 2O 42-, C 4H 4O 42-, SO 42-, NO 3- were over five times higher in the lantern days than in the normal days. The firework particles were acidic and of inorganic matter mostly with less amounts of secondary components. Primary aerosols from the burning of fireworks were mainly in the fine mode, while secondary formation of acidic anions mainly took place on the coarse particles. Nitrate was mainly formed through homogeneous gas-phase reactions of NO 2, while sulfate was largely from heterogeneous catalytic transformations of SO 2. Fe could catalyze the formation of nitrate through the reaction of α-Fe 2O 3 with HNO 3, while in the formation of sulfate, Fe is not only the catalyst, but also the oxidant. A simple method using the concentration of potassium and a modified method using the ratio of Mg/Al have been developed to quantify the source contribution of fireworks. It was found that over 90% of the total mineral aerosol and 98% of Pb, 43% of total carbon, 28% of Zn, 8% of NO 3-, and 3% of SO 42- in PM 2.5 were from the emissions of fireworks on the lantern night.

  3. Estimation of the direct and indirect impacts of fireworks on the physicochemical characteristics of atmospheric PM10 and PM2.5

    Science.gov (United States)

    Tian, Y. Z.; Wang, J.; Peng, X.; Shi, G. L.; Feng, Y. C.

    2014-09-01

    To quantify the total, direct and indirect impacts of fireworks individually, size-resolved PM samples were collected before, during and after a Chinese folk festival (Chinese New Year) in a megacity in China. Through chemical analysis and morphological characterisation, a strong influence of fireworks on the physicochemical characteristics of PM10 and PM2.5 was observed. The concentrations of many species exhibited an increasing trend during the heavy-firework period, especially for K+, Mg2+ and Cr; the results of the non-sea-salt ions demonstrated an anthropogenic influence on K+ and Mg2+. Then, source apportionment was conducted by receptor models and peak analysis (PA). The total influence of the fireworks was quantified by positive matrix factorisation (PMF), showing that the fireworks contributed higher fractions (23.40% for PM10 and 29.66% for PM2.5) during the heavy-firework period than during the light-firework period (4.28% for PM10 and 7.18% for PM2.5). The profiles of the total fireworks obtained by two independent methods (PMF and peak analysis) were consistent, with higher abundances of K+, Al, Si, Ca and organic carbon (OC). Finally, the individual contributions of the direct and indirect impacts of fireworks were quantified by chemical mass balance (CMB). The percentage contributions of resuspended dust, biomass combustion and direct fireworks were 36.8 ± 8.37%, 14.1 ± 2.82% and 44.4 ± 8.26%, respectively, for PM10 and 34.9 ± 4.19%, 16.6 ± 3.05% and 52.5 ± 9.69%, respectively, for PM2.5, in terms of the total fireworks. The quantification of the total, direct and indirect impacts of fireworks in the ambient PM gives a original contribution for understanding the physicochemical characteristics and mechanisms of such high-intensity anthropogenic activities.

  4. Implementation of a measurement-device-independent entanglement witness.

    Science.gov (United States)

    Xu, Ping; Yuan, Xiao; Chen, Luo-Kan; Lu, He; Yao, Xing-Can; Ma, Xiongfeng; Chen, Yu-Ao; Pan, Jian-Wei

    2014-04-11

    Entanglement, the essential resource in quantum information processing, should be witnessed in many tasks such as quantum computing and quantum communication. The conventional entanglement witness method, relying on an idealized implementation of measurements, could wrongly conclude a separable state to be entangled due to imperfect detections. Inspired by the idea of a time-shift attack, we construct an attack on the conventional entanglement witness process and demonstrate that a separable state can be falsely identified to be entangled. To close such detection loopholes, based on a recently proposed measurement-device-independent entanglement witness method, we design and experimentally demonstrate a measurement-device-independent entanglement witness for a variety of two-qubit states. By the new scheme, we show that an entanglement witness can be realized without detection loopholes.

  5. HUBBLE SEES A VAST 'CITY' OF STARS

    Science.gov (United States)

    2002-01-01

    In these pictures, a 'city' of a million stars glitters like a New York City skyline. The images capture the globular cluster 47 Tucanae, located 15,000 light-years from Earth in the southern constellation Tucana. Using NASA's Hubble Space Telescope, astronomers went hunting in this large city for planetary companions: bloated gaseous planets that snuggle close to their parent stars, completing an orbit in a quick three to five days. To their surprise, they found none. This finding suggests that the cluster's environment is too hostile for breeding planets or that it lacks the necessary elements for making them. The picture at left, taken by a terrestrial telescope, shows most of the cluster, a tightly packed group of middle-aged stars held together by mutual gravitational attraction. The box near the center represents the Hubble telescope's view. The image at right shows the Hubble telescope's close-up look at a swarm of 35,000 stars near the cluster's central region. The stars are tightly packed together: They're much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle-aged Sun. Most of the stars in the cluster are believed to have formed about 10 billion years ago. The bright, blue stars -- thought to be remnants of stellar collisions and mergers -- provide a few rejuvenated, energetic stars in an otherwise old system. The Hubble picture was taken in July 1999. Credits for Hubble image: NASA and Ron Gilliland (Space Telescope Science Institute) Credits for ground-based image: David Malin, c Anglo-Australian Observatory

  6. Influence of variable heat transfer coefficient of fireworks and crackers on thermal explosion critical ambient temperature and time to ignition

    OpenAIRE

    Guo Zerong; Xia Quan; Yan Peiyu; Du Zhiming

    2016-01-01

    To study the effect of variable heat transfer coefficient of fireworks and crackers on thermal explosion critical ambient temperature and time to ignition, considering the heat transfer coefficient as the power function of temperature, mathematical thermal explosion steady state and unsteady-state model of finite cylindrical fireworks and crackers with complex shell structures are established based on two-dimensional steady state thermal explosion theory. T...

  7. Effect of relativistic motion on witnessing nonclassicality of quantum states

    Science.gov (United States)

    Checińska, Agata; Lorek, Krzysztof; Dragan, Andrzej

    2017-01-01

    We show that the operational definition of nonclassicality of a quantum state depends on the motion of the observer. We use the relativistic Unruh-DeWitt detector model to witness nonclassicality of the probed field state. It turns out that the witness based on the properties of the P representation of the quantum state depends on the trajectory of the detector. Inertial and noninertial motion of the device have qualitatively different impact on the performance of the witness.

  8. Murder, insanity, and medical expert witnesses.

    Science.gov (United States)

    Ciccone, J R

    1992-06-01

    Recent advances in the ability to study brain anatomy and function and attempts to link these findings with human behavior have captured the attention of the legal system. This had led to the increasing use of the "neurological defense" to support a plea of not guilty by reason of insanity. This article explores the history of the insanity defense and explores the role of the medical expert witnesses in integrating clinical and laboratory findings, eg, computed tomographic scans, magnetic resonance scans, and single-photon emission computed tomographic scans. Three cases involving murder and brain dysfunction are discussed: the first case involves a subarachnoid hemorrhage resulting in visual perceptual and memory impairment; the second case, a diagnosis of Alzheimer's disease; and the third case, the controverted diagnosis of complex partial seizures in a serial killer.

  9. Entanglement witness derived from NMR superdense coding

    Energy Technology Data Exchange (ETDEWEB)

    Rahimi, Robabeh [Graduate School of Engineering Science, Osaka University, 1-3 Machikaneyama, Toyonaka, Osaka 560-8531 (Japan); Takeda, Kazuyuki [Graduate School of Engineering Science, Osaka University, 1-3 Machikaneyama, Toyonaka, Osaka 560-8531 (Japan); Ozawa, Masanao [Graduate School of Information Sciences, Tohoku University, Aoba-ku, Sendai 980-8579 (Japan); Kitagawa, Masahiro [Graduate School of Engineering Science, Osaka University, 1-3 Machikaneyama, Toyonaka, Osaka 560-8531 (Japan)

    2006-03-03

    It is shown that superdense coding (SDC) experiments by means of nuclear magnetic resonance (NMR) can show non-classical efficiency gain over classical communication only for nuclear spin polarization beyond a certain threshold, and this threshold coincides with that for non-separability of the density matrix. It is also claimed that transfer of two-bit information mediated by a single qubit in the previous NMR SDC experiments with low nuclear spin polarization is not ascribed to the non-classical effect induced by entanglement, but merely to a statistical effect in an ensemble system having a large number of molecules. Towards experimental detection of entanglement, a new class of entanglement witnesses is proposed, which is based on the measurement of nuclear spin magnetizations in the Bell basis and is suitable for actual NMR experiments.

  10. HUBBLE SPIES HUGE CLUSTERS OF STARS FORMED

    Science.gov (United States)

    2002-01-01

    BY ANCIENT ENCOUNTER This stunningly beautiful image [right] taken with the NASA Hubble Space Telescope shows the heart of the prototypical starburst galaxy M82. The ongoing violent star formation due to an ancient encounter with its large galactic neighbor, M81, gives this galaxy its disturbed appearance. The smaller picture at upper left shows the entire galaxy. The image was taken in December 1994 by the Kitt Peak National Observatory's 0.9-meter telescope. Hubble's view is represented by the white outline in the center. In the Hubble image, taken by the Wide Field and Planetary Camera 2, the huge lanes of dust that crisscross M82's disk are another telltale sign of the flurry of star formation. Below the center and to the right, a strong galactic wind is spewing knotty filaments of hydrogen and nitrogen gas. More than 100 super star clusters -- very bright, compact groupings of about 100,000 stars -- are seen in this detailed Hubble picture as white dots sprinkled throughout M82's central region. The dark region just above the center of the picture is a huge dust cloud. A collaboration of European and American scientists used these clusters to date the ancient interaction between M82 and M81. About 600 million years ago, a region called 'M82 B' (the bright area just below and to the left of the central dust cloud) exploded with new stars. Scientists have discovered that this ancient starburst was triggered by the violent encounter with M81. M82 is a bright (eighth magnitude), nearby (12 million light-years from Earth) galaxy in the constellation Ursa Major (the Great Bear). The Hubble picture was taken Sept. 15, 1997. The natural-color composite was constructed from three Wide Field and Planetary Camera 2 exposures, which were combined in chromatic order: 4,250 seconds through a blue filter (428 nm); 2,800 seconds through a green filter (520 nm); and 2,200 seconds through a red (820 nm) filter. Credits for Hubble image: NASA, ESA, R. de Grijs (Institute of

  11. From expert witness to defendant: abolition of expert witness protection and its implications.

    Science.gov (United States)

    Mendelson, Danuta

    2012-12-01

    In Jones v Kaney [2011] 2 AC 398, the United Kingdom Supreme Court held that in England and Wales (but not in Scotland), clients can sue expert witnesses in negligence and/or contract for work performed under their retainer, whether in civil or criminal trials. The duties of expert witnesses in England are regulated by the Civil Procedure Rules and Protocols; the former also regulate the conduct of cases involving expert opinions. The legal context that led to the litigation is examined in the light of these rules, in particular, the nature of the allegations against Dr Kaney, a psychologist retained to provide psychiatric opinion. Jones v Kaney, as a decision of the United Kingdom Supreme Court, is not a binding precedent in Australia. However, unlike statutory enactments, common law judgments are retrospective in their operation, which means that health care practitioners who follow a generally accepted practice today may still be sued for damages by their patients or clients in the future. By definition, the future, including the refusal by the Australian High Court to follow Kaney's abolition of expert witnesses' immunity from suit for breach of duty to their clients, cannot be predicted with certainty. Consequently, health care practitioners in Australia and other countries should be aware of the case, its jurisprudential and practical ramifications.

  12. Frames of most uniform Hubble flow

    CERN Document Server

    Kraljic, David

    2016-01-01

    It has been observed that the locally measured Hubble parameter converges quickest to the background value and the dipole structure of the velocity field is smallest in the reference frame of the Local Group of galaxies. We study the statistical properties of Lorentz boosts with respect to the Cosmic Microwave Background frame which make the Hubble flow look most uniform around a particular observer. We use a very large N-Body simulation to extract the dependence of the boost velocities on the local environment such as underdensities, overdensities, and bulk flows. We find that the observation is not unexpected if we are located in an underdensity, which is indeed the case for our position in the universe. The amplitude of the measured boost velocity for our location is consistent with the expectation in the standard cosmology.

  13. Hubble parameter data constraints on dark energy

    Energy Technology Data Exchange (ETDEWEB)

    Chen Yun, E-mail: chenyun@mail.bnu.edu.cn [Department of Astronomy, Beijing Normal University, Beijing 100875 (China); Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, KS 66506 (United States); Ratra, Bharat, E-mail: ratra@phys.ksu.edu [Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, KS 66506 (United States)

    2011-09-20

    We use Hubble parameter versus redshift data from Stern et al. (2010) and Gaztanaga et al. (2009) to place constraints on model parameters of constant and time-evolving dark energy cosmological models. These constraints are consistent with (through not as restrictive as) those derived from supernova Type Ia magnitude-redshift data. However, they are more restrictive than those derived from galaxy cluster angular diameter distance, and comparable with those from gamma-ray burst and lookback time data. A joint analysis of the Hubble parameter data with more restrictive baryon acoustic oscillation peak length scale and supernova Type Ia apparent magnitude data favors a spatially-flat cosmological model currently dominated by a time-independent cosmological constant but does not exclude time-varying dark energy.

  14. Hubble space telescope onboard battery performance

    Science.gov (United States)

    Rao, Gopalakrishna M.; Wajsgras, Harry; Vaidyanathan, Hari; Armontrout, Jon D.

    1996-01-01

    The performance of six 88 Ah Nickel-Hydrogen (Ni-H2) batteries that are used onboard in the Hubble Space Telescope (Flight Spare Module (FSM) and Flight Module 2 (FM2)) is discussed. These batteries have 22 series cells per battery and a common bus that would enable them to operate at a common voltage. It is launched on April 24, 1990. This paper reviews: the cell design, battery specification, system constraints, operating parameters, onboard battery management, and battery performance.

  15. Development of a Portable Muon Witness System

    Energy Technology Data Exchange (ETDEWEB)

    Aguayo Navarrete, Estanislao; Kouzes, Richard T.; Orrell, John L.

    2011-01-01

    Since understanding and quantifying cosmic ray induced radioactive backgrounds in copper and germanium are important to the MAJORANA DEMONSTRATOR, methods are needed for monitoring the levels of such backgrounds produced in materials being transported and processed for the experiment. This report focuses on work conducted at Pacific Northwest National Laboratory to develop a muon witness system as a one way of monitoring induced activities. The operational goal of this apparatus is to characterize cosmic ray exposure of materials. The cosmic ray flux at the Earth’s surface is composed of several types of particles, including neutrons, muons, gamma rays and protons. These particles induce nuclear reactions, generating isotopes that contribute to the radiological background. Underground, the main mechanism of activation is by muon produced spallation neutrons since the hadron component of cosmic rays is removed at depths greater than a few tens of meters. This is a sub-dominant contributor above ground, but muons become predominant in underground experiments. For low-background experiments cosmogenic production of certain isotopes, such as 68Ge and 60Co, must be accounted for in the background budgets. Muons act as minimum ionizing particles, depositing a fixed amount of energy per unit length in a material, and have a very high penetrating power. Using muon flux measurements as a “witness” for the hadron flux, the cosmogenic induced activity can be quantified by correlating the measured muon flux and known hadronic production rates. A publicly available coincident muon cosmic ray detector design, the Berkeley Lab Cosmic Ray Detector (BLCRD), assembled by Juniata College, is evaluated in this work. The performance of the prototype is characterized by assessing its muon flux measurements. This evaluation is done by comparing data taken in identical scenarios with other cosmic ray telescopes. The prototype is made of two plastic scintillator paddles with

  16. 22 CFR 903.10 - Access to witnesses.

    Science.gov (United States)

    2010-04-01

    ... given access to witnesses employed by the foreign affairs agencies. In the event that the agency of the... 22 Foreign Relations 2 2010-04-01 2010-04-01 true Access to witnesses. 903.10 Section 903.10 Foreign Relations FOREIGN SERVICE GRIEVANCE BOARD INITIATION AND DOCUMENTATION OF CASES § 903.10 Access to...

  17. Through the (In)visible Witness in "Through the Wire"

    Science.gov (United States)

    Wake, Caroline

    2008-01-01

    This essay analyses "Through the Wire", an Australian verbatim play by and about asylum seekers, in order to investigate both the figure of the performing witness and the function of performing witness in and through theatre. It suggests that while the characters, actors and spectators involved in the play are all "performing…

  18. Repeated Witnessing of Conspecifics in Pain : Effects on Emotional Contagion

    NARCIS (Netherlands)

    Carrillo, Maria; Migliorati, Filippo; Bruls, Rune; Han, Yingying; Heinemans, Mirjam; Pruis, Ilanah; Gazzola, V.; Keysers, C.

    2015-01-01

    Witnessing of conspecifics in pain has been shown to elicit socially triggered freezing in rodents. It is unknown how robust this response is to repeated exposure to a cage-mate experiencing painful stimulation. To address this question, shock-experienced Observer rats repeatedly witnessed familiar

  19. 31 CFR 103.75 - Examination of witnesses and records.

    Science.gov (United States)

    2010-07-01

    ... 31 Money and Finance: Treasury 1 2010-07-01 2010-07-01 false Examination of witnesses and records. 103.75 Section 103.75 Money and Finance: Treasury Regulations Relating to Money and Finance FINANCIAL RECORDKEEPING AND REPORTING OF CURRENCY AND FOREIGN TRANSACTIONS Summons § 103.75 Examination of witnesses...

  20. Indigenous Digital Storytelling in Video: Witnessing with Alma Desjarlais

    Science.gov (United States)

    Iseke, Judy M.

    2011-01-01

    Indigenous digital storytelling in video is a way of witnessing the stories of Indigenous communities and Elders, including what has happened and is happening in the lives and work of Indigenous peoples. Witnessing includes acts of remembrance in which we look back to reinterpret and recreate our relationship to the past in order to understand the…

  1. 29 CFR 18.605 - Competency of judge as witness.

    Science.gov (United States)

    2010-07-01

    ... 29 Labor 1 2010-07-01 2010-07-01 true Competency of judge as witness. 18.605 Section 18.605 Labor Office of the Secretary of Labor RULES OF PRACTICE AND PROCEDURE FOR ADMINISTRATIVE HEARINGS BEFORE THE OFFICE OF ADMINISTRATIVE LAW JUDGES Rules of Evidence Witnesses § 18.605 Competency of judge as...

  2. 13 CFR 142.24 - Can witnesses be subpoenaed?

    Science.gov (United States)

    2010-01-01

    ... 13 Business Credit and Assistance 1 2010-01-01 2010-01-01 false Can witnesses be subpoenaed? 142.24 Section 142.24 Business Credit and Assistance SMALL BUSINESS ADMINISTRATION PROGRAM FRAUD CIVIL REMEDIES ACT REGULATIONS Hearing Provisions § 142.24 Can witnesses be subpoenaed? A party seeking...

  3. Cosmic Supernova Rates and the Hubble Sequence

    CERN Document Server

    Calura, F

    2006-01-01

    We compute the type Ia, Ib/c and II supernova (SN) rates as functions of the cosmic time for galaxies of different morphological types. We use four different chemical evolution models, each one reproducing the features of a particular morphological type: E/S0, S0a/b, Sbc/d and Irr galaxies. We essentially describe the Hubble sequence by means of decreasing efficiency of star formation and increasing infall timescale. These models are used to study the evolution of the SN rates per unit luminosity and per unit mass as functions of cosmic time and as functions of the Hubble type. Our results indicate that: (i) the observed increase of the SN rate per unit luminosity and unit mass from early to late galaxy types is accounted for by our models. Our explanation of this effect is related to the fact that the latest Hubble types have the highest star formation rate per unit mass; (ii) By adopting a Scalo (1986) initial mass function in spiral disks, we find that massive single stars ending their lives as Wolf-Rayet ...

  4. Witness self-efficacy: development and validation of the construct.

    Science.gov (United States)

    Cramer, Robert J; Neal, Tess M S; DeCoster, Jamie; Brodsky, Stanley L

    2010-01-01

    Despite the application of Self-Efficacy Theory (Bandura, 1977, 2000) to many areas of psychology, there is a lack of research on self-efficacy in the ability to testify in court. The present study fills this gap by incrementally developing the construct of Witness Self-Efficacy and establishing its psychometric properties. Study I features exploratory and confirmatory factor analyses yielding a two-factor Witness Self-Efficacy Scale (WSES). The two components are Poise and Communication Style. Study II uses a second data collection to show that both WSES domains possess convergent, divergent, and predictive validity relations consistent with those expected using an SET framework. Notably, WSES components predicted perceptions of witness credibility and sentencing outcomes above and beyond witness extraversion, general self-efficacy, and general self-confidence. Implications for SET and witness preparation training are discussed. Copyright © 2010 John Wiley & Sons, Ltd.

  5. Global solution to the Cauchy problem on a universe fireworks model

    CERN Document Server

    Zhenglu Jiang

    2008-01-01

    We prove existence and uniqueness of the global solution to the Cauchy problem on a universe fireworks model with finite total mass at the initial state when the ratio of the mass surviving the explosion, the probability of the explosion of fragments and the probability function of the velocity change of a surviving particle satisfy the corresponding physical conditions. Although the nonrelativistic Boltzmann-like equation modeling the universe fireworks is mathematically easy, this paper leads rather theoretically to an understanding of how to construct contractive mappings in a Banach space for the proof of the existence and uniqueness by means of methods taken from the famous work by DiPerna & Lions about the Boltzmann equation. We also show both the regularity and the time-asymptotic behavior of solution to the Cauchy problem.

  6. Advanced Fireworks Algorithm and Its Application Research in PID Parameters Tuning

    Directory of Open Access Journals (Sweden)

    Jun-jie Xue

    2016-01-01

    Full Text Available Proportional-Integral-Derivative (PID controller is one of the most widely used controllers for its property of simplicity and practicability. In order to design high-quality performances PID controllers, an Advanced Fireworks (AFW algorithm based on self-adaption principle and bimodal Gaussian function is proposed, which is built to optimize the PID controller by parameters tuning. Firstly, a compound index of optimization performance is formulated, and then the extremal optimization method of PID control system is proposed. Secondly, a PID parameters tuning model combined with AFW is built. At last, 5 typical transfer functions are simulated to obtain optimal parameters by AFW and contrast tuning method, such as Ziegler-Nichols method, Enhanced Fireworks (EFW algorithm, and Particle Swarm Optimization (PSO. Simulation results show that AFW are effective and are easily implemented methods to solve PID control problems of different transfer functions.

  7. A Study on the Optimization Performance of Fireworks and Cuckoo Search Algorithms in Laser Machining Processes

    Science.gov (United States)

    Goswami, D.; Chakraborty, S.

    2014-11-01

    Laser machining is a promising non-contact process for effective machining of difficult-to-process advanced engineering materials. Increasing interest in the use of lasers for various machining operations can be attributed to its several unique advantages, like high productivity, non-contact processing, elimination of finishing operations, adaptability to automation, reduced processing cost, improved product quality, greater material utilization, minimum heat-affected zone and green manufacturing. To achieve the best desired machining performance and high quality characteristics of the machined components, it is extremely important to determine the optimal values of the laser machining process parameters. In this paper, fireworks algorithm and cuckoo search (CS) algorithm are applied for single as well as multi-response optimization of two laser machining processes. It is observed that although almost similar solutions are obtained for both these algorithms, CS algorithm outperforms fireworks algorithm with respect to average computation time, convergence rate and performance consistency.

  8. Federal and State Laws and Safety Considerations Relating to Fireworks in the United States.

    Science.gov (United States)

    1982-05-01

    Circular No. 230) if he prepared, in triplicate, a complete transcript of has otherwise complied with the applicable the record of the proceedings. The...be, will certify to the correctness of sioner may be represented in proceedings un- such transcript of the record, forward one der Section 181.73 abd...CLAss B FiRIvoRI~s. Mecans fireworks designed primarily to pro- duce visible or auiclible effects by comnbustion, deflagration or deton- ation. Class H

  9. Radiative Impact of Fireworks at a Tropical Indian Location: A Case Study

    Directory of Open Access Journals (Sweden)

    B. P. Singh

    2014-01-01

    Full Text Available During Diwali festival, extensive burning of crackers and fireworks is made. Weeklong intensive observational campaign for aerosol study was carried out at a representative urban location in the eastern Indo-Gangetic Plain (IGP, Varanasi (25.3°N, 83.0°E, from October 29 to November 04, 2005 (Diwali on November 01, 2005, to investigate behavioral change of aerosol properties and radiative forcing between firework affected and nonaffected periods. Results show a substantial increase (~27% in aerosol optical depth, aerosol absorption coefficients, and aerosol scattering coefficients during affected period as compared to non-affected periods. Magnitudes of radiative forcing at top of atmosphere during affected and non-affected periods are found to be +10 ± 1 and +12 ± 1 Wm−2, respectively, which are −31 ± 7 and −17 ± 5 Wm−2, respectively, at surface. It suggests an additional cooling of ~20% at top of atmosphere, ~45% cooling at surface, and additional atmospheric heating of 0.23 Kday−1 during fireworks affected period, which is ~30% higher than the non-affected period average.

  10. Perchlorate contamination of groundwater from fireworks manufacturing area in South India.

    Science.gov (United States)

    Isobe, Tomohiko; Ogawa, Shohei P; Sugimoto, Rina; Ramu, Karri; Sudaryanto, Agus; Malarvannan, Govindan; Devanathan, Gnanasekaran; Ramaswamy, Babu Rajendran; Munuswamy, Natesan; Ganesh, Deavaraj Sankar; Sivakumar, Jeyaraj; Sethuraman, A; Parthasarathy, V; Subramanian, Annamalai; Field, Jennifer; Tanabe, Shinsuke

    2013-07-01

    Perchlorate contamination was investigated in groundwater and surface water from Sivakasi and Madurai in the Tamil Nadu State of South India. Sensitive determination of perchlorate (LOQ = 0.005 μg/L) was achieved by large-volume (500 μL) injection ion chromatography coupled with tandem mass spectrometry. Concentrations of perchlorate were <0.005-7,690 μg/L in groundwater (n = 60), <0.005-30.2 μg/L in surface water (n = 11), and 0.063-0.393 μg/L in tap water (n = 3). Levels in groundwater were significantly higher in the fireworks factory area than in the other locations, indicating that the fireworks and safety match industries are principal sources of perchlorate pollution. This is the first study that reports the contamination status of perchlorate in this area and reveals firework manufacture to be the pollution source. Since perchlorate levels in 17 out of 57 groundwater samples from Sivakasi, and none from Madurai, exceeded the drinking water guideline level proposed by USEPA (15 μg/L), further investigation on human health is warranted.

  11. College students' behavioral reactions upon witnessing relational peer aggression.

    Science.gov (United States)

    You, Ji-In; Bellmore, Amy

    2014-01-01

    With a sample of 228 college students (82.5% females) from the Midwestern United States, individual factors that contribute to emerging adults' behavioral responses when witnessing relational aggression among their peers were explored. The experience of witnessing relational aggression was found to be systematically associated with college students' behavioral responses to relational aggression through two social cognitive processes: normative beliefs about relational aggression and susceptibility to peer influence. The experience of witnessing relational aggression was associated with defending behavior through normative beliefs about relational aggression and both assisting and reinforcing behavior through normative beliefs about relational aggression and susceptibility to peer influence. The experience of witnessing relational aggression was also associated with onlooking behavior through normative beliefs about relational aggression. The findings indicate that exposure to relational aggression as a witness may influence witness responses because of the way such exposure may shape specific social cognitions. The potential for using the study findings for promoting effective witness interventions among college students is discussed.

  12. Circumstances and witness characteristics associated with overdose fatality.

    Science.gov (United States)

    Bohnert, Amy S B; Tracy, Melissa; Galea, Sandro

    2009-10-01

    Emergency physicians have an opportunity to provide overdose fatality prevention interventions to individuals at risk for experiencing or witnessing an overdose to reduce fatality. The present study uses data about the most recent overdose observed by a sample of inner-city drug users to determine the circumstances of overdose that are associated with overdose fatality. Participants (n=690) aged 18 years or older were recruited with targeted street outreach. All participants had used heroin or cocaine in the previous 2 months and had witnessed at least 1 overdose. Survey data included the circumstances of the last overdose witnessed, including actions taken, drug use behavior, the location of the event, and whether or not the overdose was fatal (the outcome measure). One hundred fifty-two (21.7%) of the witnessed overdoses were fatal. Witness powdered cocaine use (adjusted odds ratio=1.6; 95% confidence interval [CI] 1.0 to 2.6) and injection drug history (adjusted odds ratio=0.5; 95% CI 0.3 to 0.9) were associated with the last witnessed overdose being fatal. Witnessed overdoses that occurred in public or abandoned buildings compared with homes were more likely to be fatal (adjusted odds ratio=1.9; 95% CI 1.0 to 3.5), as were overdoses in which witnesses sought outside medical help (adjusted odds ratio=1.5; 95% CI 1.0 to 2.1). Future prevention interventions may fruitfully target users of powdered cocaine, drug users without a history of injecting, and individuals who use drugs in public or abandoned buildings for brief interventions on responding when witnessing an overdose to reduce mortality.

  13. The type Ia supernovae and the Hubble's constant

    OpenAIRE

    2004-01-01

    The Hubble's constant is usually surmised to be a constant; but the experiments show a large spread and conflicting estimates. According to the plasma-redshift theory, the Hubble's constant varies with the plasma densities along the line of sight. It varies then slightly with the direction and the distance to a supernova and a galaxy. The relation between the magnitudes of type Ia supernovae and their observed redshifts results in an Hubble's constant with an average value in intergalactic sp...

  14. Evaluating population exposure to environmental pollutants during Deepavali fireworks displays using air quality measurements of the SAFAR network.

    Science.gov (United States)

    Beig, G; Chate, D M; Ghude, Sachin D; Ali, K; Satpute, Trupti; Sahu, S K; Parkhi, Neha; Trimbake, H K

    2013-06-01

    Indian government has implemented a state of art project "System of Air quality Forecasting And Research (SAFAR)" for assessing the air-quality scenario in Delhi during "Commonwealth Games-2010" which is operational in Delhi. Using a high resolution data of the SAFAR network, we estimate the excess numbers of cases for total, cardiovascular and respiratory mortalities and hospital admissions with the air-quality response to population attributable-risks due to emissions from fireworks displays (Deepavali-2010). The ratios of numbers of excess cases for fireworks displays (Deepavali) to those of non-Deepavali period (CWG-2010) vary from 1.75 to 3.5 for PM(2.5) and from 3 to 8 for PM(10) at monitoring stations in study area except in an airport. These ratios approach to 1 for PM(2.5) or PM(10) in airport area which can be attributed to restrictions on fireworks displays and eventually a very low population exposure. The numbers of excess cases for PM(2.5) and PM(10) during extreme emissions by fireworks displays are about 2-fold to those of non-Deepavali period. The SAFAR is recognized by the Global Urban Research Meteorology and Environment of the World Meteorological Organization and thus results would likely to provide episodic limits for developing countries in common line with the air-quality standards set for developed world for pollutant levels due to emissions from the fireworks displays when population of country celebrates traditional festivals collectively.

  15. An assessment of firework particle persistence on the hands and related police force practices in relation to GSR evidence.

    Science.gov (United States)

    Grima, Matthew; Hanson, Robert; Tidy, Helen

    2014-06-01

    In a previous study by Grima et al. Sci. Justice 52 (1) (2012) 49, it was shown that background particles can aid in the exclusion of firework particles which are indistinguishable from GSR. Issues relating to the persistence of such particle populations were presented. The scope of this project was to examine persistence on the hands in the context of possible post-display scene contamination and how this can affect GSR evidence, especially in light of possible GSR/firework mixtures. Persistence was investigated by recovering firework residues eight hours post-display following contact of the hands with bedding. In addition, particle profiling was carried out using SEM-EDX. Firework particle populations exhibited strong persistence in all displays, with not less than 667 particles persisting in each scenario. This factor challenges GSR evidence, especially if personnel stationed at display sites enter scenes of crime or come into contact with suspects after a display. A survey of UK police force practices following firework displays showed that authorities are not aware of the impact particle transfer may have on GSR evidence. Recommendations for the implementation of basic hygiene practices for particle transfer control have also been made. Copyright © 2014 Elsevier Ireland Ltd. All rights reserved.

  16. Post STS-134 Evaluation of Main Flame Deflector Witness Materials

    Science.gov (United States)

    Long, Victoria

    2011-01-01

    NASA and USA design engineers submitted witness materials from the solid rocket booster (SRB) main flame deflector for evaluation after the launch of STS-134. The following items were submitted for analysis: 1018 steel witness rods 304 stainless steel caps, tungsten pistons, and A-286 piston sleeves. All of the items were photographed in order to document their condition after the launch of STS-134. All of the items were dimensionally measured in order to determine the amount of material lost during launch. Microstructural changes were observed in the 1018 witness rod metallographic samples due to the heat of the launch

  17. Hubble Deep Fever A faint galaxy diagnosis

    CERN Document Server

    Driver, S P

    1998-01-01

    The longstanding faint blue galaxy problem is gradually subsiding as a result of technological advancement, most notably from high-resolution Hubble Space Telescope imaging. In particular two categorical facts have recently been established, these are: 1) The excess faint blue galaxies are of irregular morphologies, and, 2) the majority of these irregulars occur at redshifts 1 2. Taking these facts together we favour a scenario where the faint blue excess is primarily due to the formation epoch of spiral systems via merging at redshifts 1 < z < 2. The final interpretation now awaits refinements in our understanding of the local galaxy population !

  18. Hubble Parameter in Bulk Viscous Cosmology

    CERN Document Server

    Tawfik, A; Wahba, M

    2009-01-01

    We discuss influences of bulk viscosity on the Early Universe, which is modeled by Friedmann-Robertson-Walker metric and Einstein field equations. We assume that the matter filling the isotropic and homogeneous background is relativistic viscous characterized by ultra-relativistic equations of state deduced from recent lattice QCD simulations. We obtain a set of complicated differential equations, for which we suggest approximate solutions for Hubble parameter $H$. We find that finite viscosity in Eckart and Israel-Stewart fluids would significantly modify our picture about the Early Universe.

  19. Hubble Parameter Corrected Interactions in Cosmology

    Directory of Open Access Journals (Sweden)

    J. Sadeghi

    2014-01-01

    character opening a room for different kinds of manipulations. In this paper we will consider a modification of an interaction Q, where we accept that interaction parameter b1 (order of unity in Q=3Hb1ρ is time dependent and presented as a linear function of Hubble parameter H of the form b0+btH, where b and b0 are constants. We consider two different models including modified Chaplygin gas and polytropic gas which have bulk viscosity. Then, we investigate problem numerically and analyze behavior of different cosmological parameters concerning fluids and behavior of the universe.

  20. Spectral conditions for entanglement witnesses versus bound entanglement

    Science.gov (United States)

    Chruściński, Dariusz; Kossakowski, Andrzej; Sarbicki, Gniewomir

    2009-10-01

    It is shown that entanglement witnesses constructed via the family of spectral conditions are decomposable, i.e., cannot be used to detect bound entanglement. It supports several observations that bound entanglement reveals highly nonspectral features.

  1. Spectral conditions for entanglement witnesses vs. bound entanglement

    CERN Document Server

    Chruscinski, Dariusz; Sarbicki, Gniewomir

    2009-01-01

    It is shown that entanglement witnesses constructed via the family of spectral conditions are decomposable, i.e. cannot be used to detect bound entanglement. It supports several observations that bound entanglement reveals highly non-spectral features.

  2. A class of Bell diagonal states and entanglement witnesses

    CERN Document Server

    Chruscinski, D; Mlodawski, K; Matsuoka, T

    2010-01-01

    We analyze special class of bipartite states - so called Bell diagonal states. In particular we provide new examples of bound entangled Bell diagonal states and construct the class of entanglement witnesses diagonal in the magic basis.

  3. Resource-Efficient Measurement-Device-Independent Entanglement Witness

    Science.gov (United States)

    Verbanis, E.; Martin, A.; Rosset, D.; Lim, C. C. W.; Thew, R. T.; Zbinden, H.

    2016-05-01

    Imperfections in experimental measurement schemes can lead to falsely identifying, or over estimating, entanglement in a quantum system. A recent solution to this is to define schemes that are robust to measurement imperfections—measurement-device-independent entanglement witness (MDI-EW). This approach can be adapted to witness all entangled qubit states for a wide range of physical systems and does not depend on detection efficiencies or classical communication between devices. Here we extend the theory to remove the necessity of prior knowledge about the two-qubit states to be witnessed. Moreover, we tested this model via a novel experimental implementation for MDI-EW that significantly reduces the experimental complexity. By applying it to a bipartite Werner state, we demonstrate the robustness of this approach against noise by witnessing entanglement down to an entangled state fraction close to 0.4.

  4. Post STS-133 Evaluation of Main Flame Deflector Witness Materials

    Science.gov (United States)

    Long, Victoria

    2011-01-01

    NASA and USA Structures engineers submitted main flame deflector witness materials for evaluation after the launch of STS-133. The following items were submitted for analysis: HY-80 steel witness rods, 304 stainless steel caps, tungsten pistons, 17-4 precipitation hardened (PH) stainless steel and A-286 piston sleeves, Medtherm Corporation calorimeters, and Nanmac Corporation thermocouples. All of the items were photographed in order to document their condition after the launch of STS-133, and before they were reinstalled at the launch pad for future launches. The HY -80 witness rods, 304 stainless steel caps, and the piston sleeves were dimensionally measured in order to determine the amount of material lost during launch. Microstructural changes were observed in the HY-80 witness rod and 304 stainless steel cap metallographic samples due to the heat of the launch.

  5. Comparisons of different witnesses of non-Markovianity

    Science.gov (United States)

    Zuo, Wei; Qian, Xiao-Qing; Liang, Xian-Ting

    2017-01-01

    In this paper, the evolutions of two kinds of witnesses of the non-Markovianity and their rates of changes with time are investigated and compared. Four definitions, the trace distance, fidelity, quantum relative entropy, and quantum Fisher information are used for the first kind of witnesses which are based on the completely positive maps (CPM). Three definitions, the quantum entanglement, quantum mutual information, and quantum discord are used for the second kind of witnesses, and they are based on the local completely positive maps (LCPM). An open two-level quantum system model and a numerically quantum dissipative dynamics method, hierarchy equation of motion (HEM) are used in the investigations. It is shown that the evolutions of the witnesses and their rates of the changes calculated with different definitions clearly show the characteristics of the non-Markovianity and they are in agreement with each other.

  6. Constructing entanglement witnesses for infinite-dimensional systems

    CERN Document Server

    Hou, Jinchuan

    2010-01-01

    It is shown that, every entangled state in an infinite-dimensional composite system has an entanglement witness of simpler form $\\alpha I+T$ with $\\alpha$ a nonnegative number and $T$ a finite rank self-adjoint operator. We also provide two method of constructing entanglement witness and apply them to obtain some entangled states that cannot be detected by the PPT criterion and the realignment criterion.

  7. Globular Cluster Systems along the Hubble Sequence

    Science.gov (United States)

    Huizinga, Edwin

    1996-07-01

    Globular Cluster Systems {GCSs} provide a powerful tool to differentiate between competing galaxy formation- and evolution scenarios. However, our current knowledge of GCS in spiral galaxies is based mainly on studies of the Galaxy and M31. Even though GCSs have been detected in other spiral galaxies, ground-based observations barely reach the peak of the Globular-Cluster luminosity function, and do not provide accurate colors. We propose a systematic study of the GCSs in 6 edge-on L* spiral galaxies beyond the Local Group, using WFPC2. These galaxies were carefully selected to meet several stringent criteria. With the new dithering techniques, it will be possible to resolve any faint background galaxies and obtain a clean sample of globular clusters for all galaxies in our sample. This will allow us to study the complete luminosity functions, {V-I} color distributions, and GCS richness for L* galaxies as a function of Hubble type {Sa, Sb, Sc}. These data will be used to study the relations between the galaxies' bulge and {thin/thick} disk properties and their GCSs. If, for example, GCS properties correlate with bulge properties, this will rule out any strong evolution along the Hubble Sequence towards earlier type spirals, from Sc to Sa, as has recently been proposed by Pfenniger et al. {1994}.

  8. Is Hubble's Expansion due to Dark Energy

    CERN Document Server

    Gupta, R C

    2010-01-01

    {\\it The universe is expanding} is known (through Galaxy observations) since 1929 through Hubble's discovery ($V = H D$). Recently in 1999, it is found (through Supernovae observations) that the universe is not simply expanding but is accelerating too. We, however, hardly know only $4\\%$ of the universe. The Wilkinson Microwave Anisotropy Probe (WMAP) satellite observational data suggest $73\\%$ content of the universe in the form of dark-energy, $23\\%$ in the form of non-baryonic dark-matter and the rest $4\\%$ in the form of the usual baryonic matter. The acceleration of the universe is ascribed to this dark-energy with bizarre properties (repulsive-gravity). The question is that whether Hubble's expansion is just due to the shock of big-bang & inflation or it is due to the repulsive-gravity of dark-energy? Now, it is believed to be due to dark-energy, say, by re-introducing the once-discarded cosmological-constant $\\Lambda$. In the present paper, it is shown that `the formula for acceleration due to dark...

  9. Cosmological test with the QSO Hubble diagram

    CERN Document Server

    Lopez-Corredoira, M; Lusso, E; Risaliti, G

    2016-01-01

    A Hubble diagram (HD) has recently been constructed in the redshift range 099% C.L. The Quasi-Steady State Model is excluded at >95% C.L. The remaining four models (Lambda-CDM/wCDM, the R_h=ct Universe, the Friedmann open universe and a Static universe with a linear Hubble law) all pass the test. However, only Lambda-CDM/wCDM and $R_{\\rm h}=ct$ also pass the Alcock-Paczynski (AP) test. The optimized parameters in Lambda-CDM/wCDM are Omega_m=0.20^{+0.24}_{-0.20} and w_{de}=-1.2^{+1.6}_{-infinity} (the dark-energy equation-of-state). Combined with the AP test, these values become Omega_m=0.38^{+0.20}_{-0.19} and w_{de}=-0.28^{+0.52}_{-0.40}. But whereas this optimization of parameters in Lambda-CDM/wCDM creates some tension with their concordance values, the $R_{\\rm h}=ct$ Universe has the advantage of fitting the QSO and AP data without any free parameters.

  10. Inverse Hubble Flows in Molecular Clouds

    CERN Document Server

    Toalá, Jesús A; Colín, Pedro; Gómez, Gilberto C

    2014-01-01

    Motivated by recent numerical simulations of molecular cloud (MC)evolution, in which the clouds engage in global gravitational contraction, and local collapse events culminate significantly earlier than the global collapse, we investigate the growth of density perturbations embedded in a collapsing background, to which we refer as an Inverse Hubble Flow (IHF). We use the standard procedure for the growth of perturbations in a universe that first expands (the usual Hubble Flow) and then recollapses (the IHF). We find that linear density perturbations immersed in an IHF grow faster than perturbations evolving in a static background (the standard Jeans analysis). A fundamental distinction between the two regimes is that, in the Jeans case, the time $\\tau_\\mathrm{nl}$ for a density fluctuation to become nonlinear increases without limit as its initial value approaches zero, while in the IHF case $\\tau_\\mathrm{nl} \\le \\tau_\\mathrm{ff}$ always, where $\\tau_\\mathrm{ff}$ is the free-fall time of the background densit...

  11. HUBBLE SNAPSHOT CAPTURES LIFE CYCLE OF STARS

    Science.gov (United States)

    2002-01-01

    NASA's Hubble Space Telescope has snapped a nearly face-on view of a swirling disk of dust and gas surrounding a developing star called AB Aurigae. The Hubble telescope image, taken in visible light by the Space Telescope Imaging Spectrograph, shows unprecedented detail in the disk, including clumps of dust and gas that may be the seeds of planet formation. Normally, a young star's bright light prevents astronomers from seeing material closer to it. That's why astronomers used a coronograph in these two images of AB Aurigae to block most of the light from the star. The rest of the disk material is illuminated by light reflected from the gas and dust surrounding the star. The image on the left represents the best ground-based coronographic observation of AB Aurigae. Paul Kalas of the Space Telescope Science Institute took the image with the University of Hawaii's 2.2-meter telescope. The telescope's coronograph eclipsed a 33.5-billion-mile (53.6-billion-kilometer) area centered on the star. This area is nine times larger than our solar system. The picture shows that the star resides in a region of dust clouds - the semicircular-shaped material to the left of the star. The Hubble telescope image on the right shows a windowpane-shaped occulting bar -- the dark bands running vertically through the middle of the image and horizontally across the upper part of it. The occulting bar covers the innermost part of the disk and star, about 7.1 billion miles (11.5 billion kilometers) or 1.4 times our solar system's diameter. The diagonal lines are the remnants of the diffraction spikes produced in Hubble telescope images of bright stars. The disk is extremely wide: its diameter is roughly 1,300 times Earth's distance from the Sun. The disk material seen in this image is at a distance equivalent to well beyond Pluto's orbit. One faint background star is visible at 5 o'clock. The star's disk shows a wealth of structure, with bright spiral-shaped bands from 9 o'clock to 6 o

  12. Astronauts give Hubble a new lease of life

    Science.gov (United States)

    Banks, Michael

    2009-06-01

    Astronauts successfully repaired and upgraded the Hubble Space Telescope last month by performing five space walks each lasting more than six hours. The mission will improve Hubble's "observational power" by up to a factor of 100. The upgrade will also enable the 19-year-old instrument to carry on obtaining images of the early universe until 2014.

  13. Laryngeal findings and acoustic changes in hubble-bubble smokers.

    Science.gov (United States)

    Hamdan, Abdul-latif; Sibai, Abla; Oubari, Dima; Ashkar, Jihad; Fuleihan, Nabil

    2010-10-01

    The purpose of our investigation was to evaluate the laryngeal findings and acoustic changes in hubble-bubble smokers. A total of 42 subjects with history of hubble-bubble smoking were recruited for this study. A corresponding group with a history of cigarette smoking and controls were matched. All subjects underwent laryngeal video-endostroboscopic evaluation and acoustic analysis. In the hubble-bubble smoking group, 61.9% were males. The average age was 30.02 +/- 9.48 years and the average number of years of smoking was 8.09 +/- 6.45 years. Three subjects had dysphonia at the time of examination. The incidence of benign lesions of the vocal folds in the hubble-bubble group was 21.5%, with edema being the most common at 16.7% followed by cyst at 4.8%. The incidence of laryngeal findings was significantly higher in the hubble-bubble group compared to controls. In the cigarette-smoking group, the most common finding was vocal fold cyst in 14.8% followed by polyps in 7.4%, and edema, sulcus vocalis and granuloma. These findings were not significantly different from the hubble-bubble group except for the thick mucus, which was significantly higher in the latter. There were no significant changes in any of the acoustic parameters between hubble-bubble smokers and controls except for the VTI and MPT, which were significantly lower in the hubble-bubble group. In comparison with the cigarette-smoking group, hubble-bubble smokers had significantly higher Fundamental frequency and habitual pitch (p value 0.042 and 0.008, respectively). The laryngeal findings in hubble-bubble smokers are comparable to cigarette smokers. These laryngeal findings are not translated acoustically, as all the acoustic parameters are within normal range compared to controls.

  14. Automation of Hubble Space Telescope Mission Operations

    Science.gov (United States)

    Burley, Richard; Goulet, Gregory; Slater, Mark; Huey, William; Bassford, Lynn; Dunham, Larry

    2012-01-01

    On June 13, 2011, after more than 21 years, 115 thousand orbits, and nearly 1 million exposures taken, the operation of the Hubble Space Telescope successfully transitioned from 24x7x365 staffing to 815 staffing. This required the automation of routine mission operations including telemetry and forward link acquisition, data dumping and solid-state recorder management, stored command loading, and health and safety monitoring of both the observatory and the HST Ground System. These changes were driven by budget reductions, and required ground system and onboard spacecraft enhancements across the entire operations spectrum, from planning and scheduling systems to payload flight software. Changes in personnel and staffing were required in order to adapt to the new roles and responsibilities required in the new automated operations era. This paper will provide a high level overview of the obstacles to automating nominal HST mission operations, both technical and cultural, and how those obstacles were overcome.

  15. From Hubble's NGSL to Absolute Fluxes

    Science.gov (United States)

    Heap, Sara R.; Lindler, Don

    2012-01-01

    Hubble's Next Generation Spectral Library (NGSL) consists of R-l000 spectra of 374 stars of assorted temperature, gravity, and metallicity. Each spectrum covers the wavelength range, 0.18-1.00 microns. The library can be viewed and/or downloaded from the website, http://archive.stsci.edu/prepds/stisngsll. Stars in the NGSL are now being used as absolute flux standards at ground-based observatories. However, the uncertainty in the absolute flux is about 2%, which does not meet the requirements of dark-energy surveys. We are therefore developing an observing procedure that should yield fluxes with uncertainties less than 1 % and will take part in an HST proposal to observe up to 15 stars using this new procedure.

  16. The Gamma Ray Bursts Hubble diagram

    CERN Document Server

    Capozziello, S; Dainotti, M G; De Laurentis, M; Izzo, L; Perillo, M

    2011-01-01

    Thanks to their enormous energy release, Gamma Rays Bursts (GRBs) have recently attracted a lot of interest to probe the Hubble diagram (HD) deep into the matter dominated era and hence complement Type Ia Supernovae (SNeIa). We consider here three different calibration methods based on the use of a fiducial LCDM model, on cosmographic parameters and on the local regression on SNeIa to calibrate the scaling relations proposed as an equivalent to the Phillips law to standardize GRBs finding any significant dependence. We then investigate the evolution of these parameters with the redshift to obtain any statistical improvement. Under this assumption, we then consider possible systematics effects on the HDs introduced by the calibration method, the averaging procedure and the homogeneity of the sample arguing against any significant bias.

  17. Disk heating agents across the Hubble sequence

    CERN Document Server

    Gerssen, J

    2012-01-01

    We measure the shape of the velocity ellipsoid in two late-type spiral galaxies (Hubble types Sc and Scd) and combine these results with our previous analyses of six early-type spirals (Sa to Sbc) to probe the relation between galaxy morphology and the ratio of the vertical and radial dispersions. We confirm at much higher significance (99.9 percent) our prior detection of a tight correlation between these quantities. We explore the trends of the magnitude and shape of the velocity ellipsoid axes with galaxy properties (colour, gas surface mass density, and spiral arm structure). The observed relationships allow for an observational identification of the radial and vertical disk heating agents in external disk galaxies.

  18. The Hubble Deep Field South STIS Imaging

    CERN Document Server

    Gardner, J P; Brown, T M; Carollo, C M; Christensen, J; Dashevsky, I; Dickinson, M E; Espey, B R; Ferguson, H C; Fruchter, A S; Gonnella, A M; González-Lopezlira, R A; Hook, R N; Kaiser, M E; Martin, C L; Sahu, K C; Savaglio, S; Smith, T E; Teplitz, H I; Williams, R E; Wilson, J

    1999-01-01

    We present the imaging observations made with the Space Telescope Imaging Spectrograph of the Hubble Deep Field - South. The field was imaged in 4 bandpasses: a clear CCD bandpass for 156 ksec, a long-pass filter for 22-25 ksec per pixel typical exposure, a near-UV bandpass for 23 ksec, and a far-UV bandpass for 52 ksec. The clear visible image is the deepest observation ever made in the UV-optical wavelength region, reaching a 10 sigma AB magnitude of 29.4 for an object of area 0.2 square arcseconds. The field contains QSO J2233-606, the target of the STIS spectroscopy, and extends 50"x50" for the visible images, and 25"x25" for the ultraviolet images. We present the images, catalog of objects, and galaxy counts obtained in the field.

  19. Bianchi I meets the Hubble diagram

    CERN Document Server

    Schucker, Thomas; Valent, Galliano

    2014-01-01

    We improve existing fits of the Bianchi I metric to the Hubble diagram of supernovae and find an intriguing yet non-significant signal for anisotropy that should be verified or falsified in the near future by the Large Synoptic Survey Telescope. Since the literature contains two different formulas for the apparent luminosity as a function of time of flight in Bianchi I metrics, we present an independent derivation confirming the result by Saunders (1969). The present fit differs from earlier ones by Koivisto & Mota and by Campanelli et al. in that we use Saunders' formula, a larger sample of supernovae, Union 2 and JLA, and we use the general Bianchi I metric with three distinct eigenvalues.

  20. Hubble Space Telescope: A cosmic time machine

    Science.gov (United States)

    Westphal, J. A.; Harms, R. J.; Brandt, J. C.; Bless, R. C.; Macchetto, F. D.; Jefferys, W. H.

    1991-01-01

    The mission of the Hubble Space Telescope (HST) is to explore the expanding and evolving universe. During the 3,000 operating hours every year for the next 15 years or more, the HST will be used to study: galaxies; pulsars; globular clusters; neighboring stars where planets may be forming; binary star systems; condensing gas clouds and their chemical composition; and the rings of Saturn and the swirling ultraviolet clouds of Venus. The major technical achievements - its nearly perfect mirrors, its precise guidance system of rate gyroscopes, reaction wheels, star trackers, and fine guidance sensors are briefly discussed. The scientific instruments on board HST are briefly described. The integration of the equipment and instruments is outlined. The Space Telescope Science Institute (STScI) has approved time for 162 observations from among 556 proposals. The mission operation and data flow are explained.

  1. Hubble Space Telescope Battery Capacity Update

    Science.gov (United States)

    Hollandsworth, Roger; Armantrout, Jon; Rao, Gopalakrishna M.

    2007-01-01

    Orbital battery performance for the Hubble Space Telescope is discussed and battery life is predicted which supports decision to replace orbital batteries by 2009-2010 timeframe. Ground characterization testing of cells from the replacement battery build is discussed, with comparison of data from battery capacity characterization with cell studies of Cycle Life and 60% Stress Test at the Naval Weapons Surface Center (NWSC)-Crane, and cell Cycle Life testing at the Marshal Space Flight Center (MSFC). The contents of this presentation includes an update to the performance of the on-orbit batteries, as well as a discussion of the HST Service Mission 4 (SM4) batteries manufactured in 1996 and activated in 2000, and a second set of SM4 backup replacement batteries which began manufacture Jan 11, 2007, with delivery scheduled for July 2008.

  2. Perchlorate in dust fall and indoor dust in Malta: An effect of fireworks.

    Science.gov (United States)

    Vella, Alfred J; Chircop, Cynthia; Micallef, Tamara; Pace, Colette

    2015-07-15

    We report on the presence of perchlorate in the settleable dust of Malta, a small central Mediterranean island. Both dust fall collected directly as it precipitated from atmosphere over a period of one month and deposited indoor dust from domestic residences were studied. Perchlorate was determined by ion chromatography of water extracts of the collected dusts. Dust fall was collected from 43 towns during 2011 to 2013 and indoor dust was sampled from homes in the same localities. Perchlorate was detected in 108 of 153 samples of dust fall (71%) and in 28 of 37 indoor dust samples (76%). Detectable perchlorate in dust fall ranged from 0.52μgg(-1) to 561μgg(-1) with a median value of 6.2μgg(-1); in indoor dust, levels were from 0.79μgg(-1) to 53μgg(-1) with a median value of 7.8μgg(-1), the highest recorded anywhere to date. Statistical analysis suggested that there was no significant difference in perchlorate content of indoor dust and dust fall. Perchlorate levels in dust fall escalate during the summer in response to numerous religious feasts celebrated with fireworks and perchlorate persists at low μgg(-1) concentrations for several months beyond the summer festive period. In Malta, perchlorate derives exclusively from KClO4, imported for fireworks manufacture. Its residue in dust presents an exposure risk to the population, especially via ingestion by hand to mouth transfer. Our results suggest that wherever intensive burning of fireworks takes place, the environmental impact may be much longer lived than realised, mainly due to re-suspension and deposition of contaminated settled dust in the urban environment.

  3. HUBBLE WATCHES STAR TEAR APART ITS NEIGHBORHOOD

    Science.gov (United States)

    2002-01-01

    NASA's Hubble Space Telescope has snapped a view of a stellar demolition zone in our Milky Way Galaxy: a massive star, nearing the end of its life, tearing apart the shell of surrounding material it blew off 250,000 years ago with its strong stellar wind. The shell of material, dubbed the Crescent Nebula (NGC 6888), surrounds the 'hefty,' aging star WR 136, an extremely rare and short-lived class of super-hot star called a Wolf-Rayet. Hubble's multicolored picture reveals with unprecedented clarity that the shell of matter is a network of filaments and dense knots, all enshrouded in a thin 'skin' of gas [seen in blue]. The whole structure looks like oatmeal trapped inside a balloon. The skin is glowing because it is being blasted by ultraviolet light from WR 136. Hubble's view covers a small region at the northeast tip of the structure, which is roughly three light-years across. A picture taken by a ground-based telescope [lower right] shows almost the entire nebula. The whole structure is about 16 light-years wide and 25 light-years long. The bright dot near the center of NGC 6888 is WR 136. The white outline in the upper left-hand corner represents Hubble's view. Hubble's sharp vision is allowing scientists to probe the intricate details of this complex system, which is crucial to understanding the life cycle of stars and their impact on the evolution of our galaxy. The results of this study appear in the June issue of the Astronomical Journal. WR 136 created this web of luminous material during the late stages of its life. As a bloated, red super-giant, WR 136 gently puffed away some of its bulk, which settled around it. When the star passed from a super-giant to a Wolf-Rayet, it developed a fierce stellar wind - a stream of charged particles released from its surface - and began expelling mass at a furious rate. The star began ejecting material at a speed of 3.8 million mph (6.1 million kilometers per hour), losing matter equal to that of our Sun's every 10

  4. The experience of the child witness: Legal and psychological issues.

    Science.gov (United States)

    Robinson, Jana

    2015-01-01

    The increasing presence of child witnesses in the courtroom has brought with it a host of challenges and dilemmas. Related concerns include whether children may be deemed incompetent solely because of their age, whether their testimony is reliable and accurate in light of their allegedly suggestible nature, and whether the experience of testifying may re-traumatize witnesses who are also victims. A growing body of multidisciplinary research continues to address the legal and clinical implications of permitting children to testify in open court. Numerous guidelines have been promulgated that contain recommendations for protecting children's best interests as they journey through the criminal justice system. Related courtroom procedures vary greatly among American jurisdictions, and innovations in other countries--for example, the United Kingdom's Youth Justice and Criminal Evidence Act of 1999, and similar legislation in Israel and in Norway--have introduced a range of alternative measures that can be employed with young witnesses, depending primarily on whether the child witness is ultimately deemed either "vulnerable" or "intimidated." This article incorporates legal and psychological studies--from geographically diverse perspectives--that focus upon the courtroom experiences of child witnesses in criminal proceedings, including determinations of testimonial capacity and other matters unique to this population. Copyright © 2015 Elsevier Ltd. All rights reserved.

  5. APPLYING ARTIFICIAL NEURAL NETWORK OPTIMIZED BY FIREWORKS ALGORITHM FOR STOCK PRICE ESTIMATION

    Directory of Open Access Journals (Sweden)

    Khuat Thanh Tung

    2016-04-01

    Full Text Available Stock prediction is to determine the future value of a company stock dealt on an exchange. It plays a crucial role to raise the profit gained by firms and investors. Over the past few years, many methods have been developed in which plenty of efforts focus on the machine learning framework achieving the promising results. In this paper, an approach based on Artificial Neural Network (ANN optimized by Fireworks algorithm and data preprocessing by Haar Wavelet is applied to estimate the stock prices. The system was trained and tested with real data of various companies collected from Yahoo Finance. The obtained results are encouraging.

  6. Experience in working with volunteers as providers of support to victims and witnesses in victim and witness support departments at the courts

    National Research Council Canada - National Science Library

    Hamer-Vidmar Nikica; Bajto Martina

    2015-01-01

    The aim of this paper is to present the results of a survey on the experience of engaging volunteers as providers of support for victims and witnesses in Victim and Witness Support Departments at the courts...

  7. Experimental realization of dimension witnesses based on quantum state discrimination

    Science.gov (United States)

    Sun, Yong-Nan; Liu, Zhao-Di; Sun, Jun; Chen, Geng; Xu, Xiao-Ye; Wu, Yu-Chun; Tang, Jian-Shun; Han, Yong-Jian; Li, Chuan-Feng; Guo, Guang-Can

    2016-11-01

    The dimension witness is an important concept in fundamental physics and quantum information processing which allows one to test the dimension of an unknown physical system in a device independent manner. Here, we report an experimental test of classical and quantum dimensions in a prepare and measure scenario through dimension witnesses based on quantum state discrimination. In our work, we have not only distinguished between quantum and classical systems of the same dimension (two, three, and four dimensions) but also distinguished between real and complex two-level quantum systems. We have also shown the strong link between dimension witnesses and quantum state discrimination which was introduced in N. Brunner, M. Navascués, and T. Vértesi [Phys. Rev. Lett. 110, 150501 (2013), 10.1103/PhysRevLett.110.150501].

  8. 78 FR 53677 - Safety Zone; Battle of Lake Erie Fireworks, Lake Erie, Put-In-Bay, OH

    Science.gov (United States)

    2013-08-30

    ..., Put-In- Bay, OH AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing temporary safety zone in the waters of Lake Erie, Put-In-Bay, Ohio. This zone is intended to... the launching of fireworks in the vicinity of Put-In-Bay, OH on September 1, 2013. The Captain of...

  9. Influence of variable heat transfer coefficient of fireworks and crackers on thermal explosion critical ambient temperature and time to ignition

    Directory of Open Access Journals (Sweden)

    Guo Zerong

    2016-01-01

    Full Text Available To study the effect of variable heat transfer coefficient of fireworks and crackers on thermal explosion critical ambient temperature and time to ignition, considering the heat transfer coefficient as the power function of temperature, mathematical thermal explosion steady state and unsteady-state model of finite cylindrical fireworks and crackers with complex shell structures are established based on two-dimensional steady state thermal explosion theory. The influence of variable heat transfer coefficient on thermal explosion critical ambient temperature and time to ignition are analyzed. When heat transfer coefficient is changing with temperature and in the condition of natural convection heat transfer, critical ambient temperature lessen, thermal explosion time to ignition shorten. If ambient temperature is close to critical ambient temperature, the influence of variable heat transfer coefficient on time to ignition become large. For firework with inner barrel in example analysis, the critical ambient temperature of propellant is 463.88 K and the time to ignition is 4054.9s at 466 K, 0.26 K and 450.8s less than without considering the change of heat transfer coefficient respectively. The calculation results show that the influence of variable heat transfer coefficient on thermal explosion time to ignition is greater in this example. Therefore, the effect of variable heat transfer coefficient should be considered into thermal safety evaluation of fireworks to reduce potential safety hazard.

  10. 75 FR 34374 - Safety Zone; Stockton Ports Baseball Club/City of Stockton, 4th of July Fireworks Display...

    Science.gov (United States)

    2010-06-17

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Stockton Ports Baseball Club/City of... Ports Baseball Club and the City of Stockton will sponsor the Stockton Ports Baseball Club/City of... Ports Baseball Club/City of Stockton 4th of July Fireworks Display, Stockton, CA. (a) Location....

  11. 78 FR 62293 - Safety Zone, Oyster Festival 30th Anniversary Fireworks Display, Oyster Bay; Oyster Bay, NY

    Science.gov (United States)

    2013-10-15

    ... CFR Part 165 RIN 1625-AA00 Safety Zone, Oyster Festival 30th Anniversary Fireworks Display, Oyster Bay; Oyster Bay, NY AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a temporary safety zone on the navigable waters of Oyster Bay near Oyster Bay, NY for the...

  12. 76 FR 33155 - Safety Zones; Multiple Firework Displays in Captain of the Port, Puget Sound Area of Responsibility

    Science.gov (United States)

    2011-06-08

    ... the Port, Puget Sound Area of Responsibility AGENCY: Coast Guard, DHS. ACTION: Temporary final rule..., or on the distribution of power and responsibilities between the Federal Government and Indian tribes...; Multiple Firework Displays in Captain of the Port, Puget Sound Area of Responsibility (a) Location. The...

  13. 76 FR 50124 - Safety Zones; August and September Fireworks and Swimming Events in Captain of the Port Boston Zone

    Science.gov (United States)

    2011-08-12

    ... Swimming Events in Captain of the Port Boston Zone AGENCY: Coast Guard, DHS. ACTION: Temporary final rule... navigable waters from the hazardous nature of swimming and fireworks events. Sponsors stated they are... and swimming events. Basis and Purpose The legal basis for the temporary rule is 33 U.S.C. 1226, 1231...

  14. 33 CFR 165.T11-304 - Safety zone; Sea World Summer Nights Fireworks; Mission Bay, San Diego, California.

    Science.gov (United States)

    2010-07-01

    ... Nights Fireworks; Mission Bay, San Diego, California. 165.T11-304 Section 165.T11-304 Navigation and...; Mission Bay, San Diego, California. (a) Location. The limits of the safety zone will include a 600 foot... prohibited unless authorized by the Captain of the Port of San Diego or his designated on-scene...

  15. 75 FR 17329 - Safety Zone; Big Bay Fourth of July Fireworks, San Diego Bay, San Diego, CA

    Science.gov (United States)

    2010-04-06

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Big Bay Fourth of July Fireworks, San Diego Bay, San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Notice of proposed rulemaking. SUMMARY: The Coast Guard proposes establishing a temporary safety zone on the navigable waters of the San Diego Bay in...

  16. 78 FR 48044 - Safety Zone; San Diego International Airport Terminal Two West Grand Opening Fireworks; San Diego...

    Science.gov (United States)

    2013-08-07

    ... [Docket No. USCG-2013-0637] RIN 1625-AA00 Safety Zone; San Diego International Airport Terminal Two West Grand Opening Fireworks; San Diego, CA AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The Coast Guard is establishing a safety zone on the navigable waters of the San Diego Bay in support...

  17. 75 FR 81854 - Safety Zone; New Year's Celebration for the City of San Francisco, Fireworks Display, San...

    Science.gov (United States)

    2010-12-29

    .... SUMMARY: The Coast Guard is establishing a temporary safety zone in support of the New Year's Eve... Year's Eve Celebration for the City of San Francisco Fireworks Display from 11:45 p.m. on December 31... Standards The National Technology Transfer and Advancement Act (NTTAA) (15 U.S.C. 272 note) directs...

  18. PLANCK and WMAP constraints on generalised Hubble flow inflationary trajectories

    Energy Technology Data Exchange (ETDEWEB)

    Contaldi, Carlo R.; Horner, Jonathan S., E-mail: c.contaldi@imperial.ac.uk, E-mail: j.horner11@imperial.ac.uk [Theoretical Physics Group, Blackett Laboratory, Imperial College London, South Kensington, London, SW7 2BZ (United Kingdom)

    2014-08-01

    We use the Hamilton-Jacobi formalism to constrain the space of possible single field, inflationary Hubble flow trajectories when compared to the WMAP and PLANK satellites Cosmic Microwave Background (CMB) results. This method yields posteriors on the space of Hubble Slow Roll (HSR) parameters that uniquely determine the history of the Hubble parameter during the inflating epoch. The trajectories are used to numerically determine the observable primordial power spectrum and bispectra that can then be compared to observations. Our analysis is used to infer the most likely shape of the inflaton potential V(φ) and also yields a prediction for, B, the dimensionless amplitude of the non-Gaussian bispectrum.

  19. A Scientific Revolution: the Hubble and James Webb Space Telescopes

    Science.gov (United States)

    Gardner, Jonathan P.

    2012-01-01

    Astronomy is going through a scientific revolution, responding to a flood of data from the Hubble Space Telescope, other space missions, and large telescopes on the ground. In this talk, I will discuss some of the most important astronomical discoveries of the last IO years, and the role that space telescopes have played in those discoveries. The next decade looks equally bright with the newly refurbished Hubble and the promise of its successor, the James Webb Space Telescope. I will describe how Hubble was upgraded and how and why we are building Webb.

  20. Macroscooic inequivalent entanglement witness in Heisenberg spin Chain

    Institute of Scientific and Technical Information of China (English)

    Zhang Ting; Chen Ping-Xing; Li Cheng-Zu

    2009-01-01

    Motivated by the wise idea of entanglement witness(EW),we present an inequivalent entanglement witness(IEEW)that can analogously classify certain eigenstates entangled in inequivalent ways under stochastic local operations and classical communication(SLOCC)in the Heisenberg spin chain.Since the IEEW is the absolute value of magnetization |M| that is a macroscopically measurable quantity,our conclusions provide a macroscopic method to detect incquivalent entanglement between microscopic spins,on the one hand,and clearly show that inequivalent entanglement can yield different macroscopic effects,on the other hand.

  1. Entanglement Observables and Witnesses for Interacting Quantum Spin Systems

    CERN Document Server

    Wu, L A; Sarandy, M S; Lidar, D A

    2004-01-01

    We discuss the detection of entanglement in interacting quantum spin systems. First, thermodynamic Hamiltonian-based witnesses are computed for a general class of one-dimensional spin-1/2 models. Second, we introduce optimal bipartite entanglement observables. We show that a bipartite entanglement measure can generally be associated to a set of independent two-body spin observables whose expectation values can be used to witness entanglement. The number of necessary observables is ruled by the symmetries of the model. Illustrative examples are presented.

  2. Post STS-135 Evaluation of Main Flame Deflector Witness Materials

    Science.gov (United States)

    Long, Victoria

    2011-01-01

    NASA and USA design engineers submitted witness materials from the solid rocket booster (SRB) main flame deflector for evaluation after the launch of STS-135. The following items were submitted for analysis: HY-80 steel witnes rods, 304 sta inles steel caps, and tungsten pistons. All of the items were photographed in order to document their condition after the launch of STS-135. The submitted samples were dimensionally measured in order to determine the amount of material lost during launch. Microstructural changes were observed in the HY-80 witness rod metallographic samples due to the heat of the launch.

  3. A Unique test for Hubble's new Solar Arrays

    Science.gov (United States)

    2000-10-01

    In mid-October, a team from the European Space Agency (ESA) and NASA will perform a difficult, never-before-done test on one of the Hubble Space Telescope's new solar array panels. Two of these panels, or arrays, will be installed by astronauts in November 2001, when the Space Shuttle Columbia visits Hubble on a routine service mission. The test will ensure that the new arrays are solid and vibration free before they are installed on orbit. The test will be conducted at ESA's European Space Research and Technology Center (ESTEC) in Noordwijk, The Netherlands. Because of the array's size, the facility's special features, and ESA's longstanding experience with Hubble's solar arrays, ESTEC is the only place in the world the test can be performed. This test is the latest chapter in a longstanding partnership between ESA and NASA on the Hubble Space Telescope. The Large Space Simulator at ESTEC, ESA's world-class test facility, features a huge vacuum chamber containing a bank of extremely bright lights that simulate the Sun's intensity - including sunrise and sunset. By exposing the solar wing to the light and temperature extremes of Hubble's orbit, engineers can verify how the new set of arrays will act in space. Hubble orbits the Earth once every 90 minutes. During each orbit, the telescope experiences 45 minutes of searing sunlight and 45 minutes of frigid darkness. This test will detect any tiny vibrations, or jitters, caused by these dramatic, repeated changes. Even a small amount of jitter can affect Hubble's sensitive instruments and interfere with observations. Hubble's first set of solar arrays experienced mild jitter and was replaced in 1993 with a much more stable pair. Since that time, advances in solar cell technology have led to the development of even more efficient arrays. In 2001, NASA will take advantage of these improvements, by fitting Hubble with a third-generation set of arrays. Though smaller, this new set generates more power than the previous

  4. HUBBLE CAPTURES THE HEART OF STAR BIRTH

    Science.gov (United States)

    2002-01-01

    NASA Hubble Space Telescope's Wide Field and Planetary Camera 2 (WFPC2) has captured a flurry of star birth near the heart of the barred spiral galaxy NGC 1808. On the left are two images, one superimposed over the other. The black-and-white picture is a ground-based view of the entire galaxy. The color inset image, taken with the Hubble telescope's Wide Field and Planetary Camera 2 (WFPC2), provides a close-up view of the galaxy's center, the hotbed of vigorous star formation. The ground-based image shows that the galaxy has an unusual, warped shape. Most spiral galaxies are flat disks, but this one has curls of dust and gas at its outer spiral arms (upper right-hand corner and lower left-hand corner). This peculiar shape is evidence that NGC 1808 may have had a close interaction with another nearby galaxy, NGC 1792, which is not in the picture Such an interaction could have hurled gas towards the nucleus of NGC 1808, triggering the exceptionally high rate of star birth seen in the WFPC2 inset image. The WFPC2 inset picture is a composite of images using colored filters that isolate red and infrared light as well as light from glowing hydrogen. The red and infrared light (seen as yellow) highlight older stars, while hydrogen (seen as blue) reveals areas of star birth. Colors were assigned to this false-color image to emphasize the vigorous star formation taking place around the galaxy's center. NGC 1808 is called a barred spiral galaxy because of the straight lines of star formation on both sides of the bright nucleus. This star formation may have been triggered by the rotation of the bar, or by matter which is streaming along the bar towards the central region (and feeding the star burst). Filaments of dust are being ejected from the core into a faint halo of stars surrounding the galaxy's disk (towards the upper left corner) by massive stars that have exploded as supernovae in the star burst region. The portion of the galaxy seen in this 'wide-field' image is

  5. Hubble Case Studies of Transiting Giant Exoplanets

    Science.gov (United States)

    Wilkins, Ashlee N.; Deming, Drake; Barker, Adrian; Benneke, Björn; Delrez, Laetitia; Gillon, Michaël; Hamilton, Douglas P.; Jehin, Emmanuel; Knutson, Heather; Lewis, Nikole K.; Madhusudhan, Nikku; Mandell, Avi; McCullough, Peter R.; Wakeford, Hannah R.

    2017-01-01

    The study of planets around other stars has entered a science-rich era of characterization, in which detailed information about individual planets can be inferred from observations beyond mere detection, which only yields bulk properties like mass or radius. Characterization probes more revealing quantities such as chemical abundances, albedo, and temperature/pressure profiles, which allow us to address larger questions of planet formation mechanisms, planetary evolution, and, eventually, habitability and presence of biosignature gases. The primary method for characterization of close-in planets is transit spectroscopy. This dissertation talk will focus on transiting exoplanet case studies with the Hubble Space Telescope’ Wide-Field Camera-3 (WFC-3) as a tool of exoplanet characterization in a near-infrared band dominated by strong water features. I will first present a characterization the WFC-3 systematic effects that must be mitigated to extract the incredibly small (tens to 200 parts per million) signals, and then a study of four transiting giant planets (HATS-7b, HAT-p-3b, HD 149026b, and WASP-18b) in transmission, and two (WASP-18b and CoRoT-2b) in eclipse. Finally, I will discuss the role of transit timing monitoring of WASP-18b with HST and other observatories as another clue to its evolution as a close-in, massive planet. The five planets range from Neptune-class to Super-Jupiter-class in size/mass. Though these planets may be relatively rare, their observability represents a unique opportunity to probe planet formation and evolution, as well as atmospheric structures in a high-irradiation environment. These observations also yield insights into aerosols (i.e. clouds/hazes) in the atmosphere; clouds and/or hazes should significantly impact atmospheric chemistry and observational signatures, and we as a community must get a better handle on the phenomenon of aerosols in advance of the next generation of space observatories, including JWST and WFIRST

  6. Weary Astronauts Return From Hubble Mission

    Institute of Scientific and Technical Information of China (English)

    Broward; Liston; 姜其宝

    2002-01-01

    在完成了对“哈勃”太空望远镜大修后,“带病”工作的美国“哥伦比亚”号航天飞机3月12日安全返回肯尼迪航天中心。在“哥伦比亚”号为期11天的飞行期间,宇航员为“哈勃”更换了电池板、电力控制装置等,并给望远镜装上功能更强的照相机。他们还创造了航天飞机一次飞行中,宇航员太空行走总时间最长的新记录。本文有两句写得颇有诗意: As Columbia’s wheels touched down on the three - mile landing strip(飞机的起落跑道) at Florida’s Kennedy Space Center, Hubble was flying more than 350miles above the Pacific Ocean, its systems performing well, NASA said。 译文:当“哥伦比亚”号航天飞机的轮子接触在佛罗里达州的肯尼迪航天中心3英里长的起落跑道时,哈勃望远镜正在太平洋上空350英里处飞行,它的系统工作正常。美国国家航空和宇宙航行局如是说。 注:上句所以如此具有文采,是因为使用了“对照”(contrast)的修辞手法。特别是其中两个数字的运用,真可咀嚼! 另一处是: Hubble has really opened our eyes to what the universe is made of , its struc-ture, and has helped us learn how little we know about the universe。 佳句!又使用了“对照”(contrast)的修辞手法!且更具哲理,发?

  7. The Characteristics of Air Pollutants during Two Distinct Episodes of Fireworks Burning in a Valley City of North China

    Science.gov (United States)

    Song, Yang; Wan, Xiaoming; Bai, Shuoxin; Guo, Dong; Ren, Ci; Zeng, Yu; Li, Yirui; Li, Xuewen

    2017-01-01

    Background The elevation and dissipation of pollutants after the ignition of fireworks in different functional areas of a valley city were investigated. Methods The Air Quality Index (AQI) as well as inter-day and intra-day concentrations of various air pollutants (PM10, PM2.5, SO2, NO2, CO, O3) were measured during two episodes that took place during Chinese New Year festivities. Results For the special terrain of Jinan, the mean concentrations of pollutants increased sharply within 2–4 h of the firework displays, and concentrations were 4–6 times higher than the usual levels. It took 2–3 d for the pollutants to dissipate to background levels. Compared to Preliminary Eve (more fireworks are ignited on New Year’s Eve, but the amounts of other human activities are also lesser), the primary pollutants PM2.5, PM10, and CO reached higher concentrations on New Year’s Eve, and the highest concentrations of these pollutants were detected in living quarters. All areas suffered from serious pollution problems on New Year’s Eve (rural = urban for PM10, but rural > urban for PM2.5). However, SO2 and NO2 levels were 20%–60% lower in living quarters and industrial areas compared to the levels in these same areas on Preliminary Eve. In contrast to the other pollutants, O3 concentrations fell instead of rising with the firework displays. Conclusion Interactions between firework displays and other human activities caused different change trends of pollutants. PM2.5 and PM10 were the main pollutants, and the rural living quarter had some of the highest pollution levels. PMID:28045925

  8. The Characteristics of Air Pollutants during Two Distinct Episodes of Fireworks Burning in a Valley City of North China.

    Science.gov (United States)

    Song, Yang; Wan, Xiaoming; Bai, Shuoxin; Guo, Dong; Ren, Ci; Zeng, Yu; Li, Yirui; Li, Xuewen

    2017-01-01

    The elevation and dissipation of pollutants after the ignition of fireworks in different functional areas of a valley city were investigated. The Air Quality Index (AQI) as well as inter-day and intra-day concentrations of various air pollutants (PM10, PM2.5, SO2, NO2, CO, O3) were measured during two episodes that took place during Chinese New Year festivities. For the special terrain of Jinan, the mean concentrations of pollutants increased sharply within 2-4 h of the firework displays, and concentrations were 4-6 times higher than the usual levels. It took 2-3 d for the pollutants to dissipate to background levels. Compared to Preliminary Eve (more fireworks are ignited on New Year's Eve, but the amounts of other human activities are also lesser), the primary pollutants PM2.5, PM10, and CO reached higher concentrations on New Year's Eve, and the highest concentrations of these pollutants were detected in living quarters. All areas suffered from serious pollution problems on New Year's Eve (rural = urban for PM10, but rural > urban for PM2.5). However, SO2 and NO2 levels were 20%-60% lower in living quarters and industrial areas compared to the levels in these same areas on Preliminary Eve. In contrast to the other pollutants, O3 concentrations fell instead of rising with the firework displays. Interactions between firework displays and other human activities caused different change trends of pollutants. PM2.5 and PM10 were the main pollutants, and the rural living quarter had some of the highest pollution levels.

  9. The Hubble Relation for a Comprehensive Sample of QSOs

    Indian Academy of Sciences (India)

    D. Basu

    2003-03-01

    A correlation between redshifts () and apparent magnitudes () (Hubble relation) of Quasi Stellar Objects (QSOs) has long been sought. Such a correlation exists for galaxies whose redshifts are of cosmological origin. However, a plot of the two quantities representing the Hubble diagram for QSOs exhibits, in general, a wild scatter. This raises the question whether redshifts of QSOs are cosmological. On the other hand, most luminous QSOs in groups, and subsamples with particular properties, have been reported to show the Hubble relation. In the present paper, we analyse all optically non-variable QSOs in a comprehensive sample. In our analysis we grouped the objects into certain intervals of apparent magnitudes. Correlations obtained between redshifts and magnitudes are all statistically robust. Also, the Hubble relation in the usual form = 5 log +C is obeyed very convincingly for QSOs with < 19.5.

  10. How Long Can the Hubble Space Telescope Operate Reliably?

    Science.gov (United States)

    Xapsos, M. A.; Stauffer, C.; Jordan, T.; Poivey, C.; Lum, G.; Haskins, D. N.; Pergosky, A. M.; Smith, D. C.; LaBel, K. A.

    2014-01-01

    Total ionizing dose exposure of electronic parts in the Hubble Space Telescope is analyzed using 3-D ray trace and Monte Carlo simulations. Results are discussed along with other potential failure mechanisms for science operations.

  11. Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant

    Science.gov (United States)

    Freedman, Wendy L.; Madore, Barry F.; Scowcroft, Victoria; Burns, Chris; Monson, Andy; Persson, S. Eric; Seibert, Mark; Rigby, Jane

    2012-01-01

    Using a mid-infrared calibration of the Cepheid distance scale based on recent observations at 3.6 micrometers with the Spitzer Space Telescope, we have obtained a new, high-accuracy calibration of the Hubble constant. We have established the mid-IR zero point of the Leavitt law (the Cepheid period-luminosity relation) using time-averaged 3.6 micrometers data for 10 high-metallicity, MilkyWay Cepheids having independently measured trigonometric parallaxes. We have adopted the slope of the PL relation using time-averaged 3.6micrometers data for 80 long-period Large Magellanic Cloud (LMC) Cepheids falling in the period range 0.8 Hubble Space Telescope Key Project has decreased by over a factor of three. Applying the Spitzer calibration to the Key Project sample, we find a value of H(sub 0) = 74.3 with a systematic uncertainty of +/-2.1 (systematic) kilometers per second Mpc(sup -1), corresponding to a 2.8% systematic uncertainty in the Hubble constant. This result, in combination with WMAP7measurements of the cosmic microwave background anisotropies and assuming a flat universe, yields a value of the equation of state for dark energy, w(sub 0) = -1.09 +/- 0.10. Alternatively, relaxing the constraints on flatness and the numbers of relativistic species, and combining our results with those of WMAP7, Type Ia supernovae and baryon acoustic oscillations yield w(sub 0) = -1.08 +/- 0.10 and a value of N(sub eff) = 4.13 +/- 0.67, mildly consistent with the existence of a fourth neutrino species.

  12. Featured Image: Mapping Jupiter with Hubble

    Science.gov (United States)

    Kohler, Susanna

    2016-07-01

    Zonal wind profile for Jupiter, describing the speed and direction of its winds at each latitude. [Simon et al. 2015]This global map of Jupiters surface (click for the full view!) was generated by the Hubble Outer Planet Atmospheres Legacy (OPAL) program, which aims to createnew yearly global maps for each of the outer planets. Presented in a study led by Amy Simon (NASA Goddard Space Flight Center), the map above is the first generated for Jupiter in the first year of the OPAL campaign. It provides a detailed look at Jupiters atmospheric structure including the Great Red Spot and allowed the authors to measure the speed and direction of the wind across Jupiters latitudes, constructing an updated zonal wind profile for Jupiter.In contrast to this study, the Juno mission (which will be captured into Jupiters orbit today after a 5-year journey to Jupiter!) will be focusing more on the features below Jupiters surface, studying its deep atmosphere and winds. Some of Junos primary goals are to learn about Jupiters composition, gravitational field, magnetic field, and polar magnetosphere. You can follow along with the NASATV livestream as Juno arrives at Jupiter tonight; orbit insertion coverage starts at 10:30 EDT.CitationAmy A. Simon et al 2015 ApJ 812 55. doi:10.1088/0004-637X/812/1/55

  13. Hubble Space Telescope Crew Rescue Analysis

    Science.gov (United States)

    Hamlin, Teri L.; Canga, Michael A.; Cates, Grant R.

    2010-01-01

    In the aftermath of the 2003 Columbia accident, NASA removed the Hubble Space Telescope (HST) Servicing Mission 4 (SM4) from the Space Shuttle manifest. Reasons cited included concerns that the risk of flying the mission would be too high. The HST SM4 was subsequently reinstated and flown as Space Transportation System (STS)-125 because of improvements in the ascent debris environment, the development of techniques for astronauts to perform on orbit repairs to damaged thermal protection, and the development of a strategy to provide a viable crew rescue capability. However, leading up to the launch of STS-125, the viability of the HST crew rescue capability was a recurring topic. For STS-125, there was a limited amount of time available to perform a crew rescue due to limited consumables (power, oxygen, etc.) available on the Orbiter. The success of crew rescue depended upon several factors, including when a problem was identified; when and what actions, such as powering down, were begun to conserve consumables; and where the Launch on Need (LON) vehicle was in its ground processing cycle. Crew rescue success also needed to be weighed against preserving the Orbiter s ability to have a landing option in case there was a problem with the LON vehicle. This paper focuses on quantifying the HST mission loss of crew rescue capability using Shuttle historical data and various power down strategies. Results from this effort supported NASA s decision to proceed with STS-125, which was successfully completed on May 24th 2009.

  14. UV/Visible Telescope with Hubble Disposal

    Science.gov (United States)

    Benford, Dominic J.

    2013-01-01

    Submission Overview: Our primary objective is to convey a sense of the significant advances possible in astrophysics investigations for major Cosmic Origins COR program goals with a 2.4m telescope asset outfitted with one or more advanced UV visible instruments. Several compelling science objectives were identified based on community meetings these science objectives drove the conceptual design of instruments studied by the COR Program Office during July September 2012. This RFI submission encapsulates the results of that study, and suggests that a more detailed look into the instrument suite should be conducted to prove viability and affordability to support the demonstrated scientific value. This study was conducted in the context of a larger effort to consider the options available for a mission to dispose safely of Hubble hence, the overall architecture considered for the mission we studied for the 2.4m telescope asset included resource sharing. This mitigates combined cost and risk and provides naturally for a continued US leadership role in astrophysics with an advanced, general-purpose UV visible space telescope.

  15. Type Ia Supernovae and the Hubble Constant

    CERN Document Server

    Branch, D

    1998-01-01

    The focus of this review is the work that has been done during the 1990s on using Type Ia supernovae (SNe Ia) to measure the Hubble constant ($H_0$). SNe Ia are well suited for measuring $H_0$. A straightforward maximum-light color criterion can weed out the minority of observed events that are either intrinsically subluminous or substantially extinguished by dust, leaving a majority subsample that has observational absolute-magnitude dispersions of less than $\\sigma_{obs}(M_B) \\simeq \\sigma_{obs}(M_V) \\simeq 0.3$ mag. Correlations between absolute magnitude and one or more distance-independent SN Ia or parent-galaxy observables can be used to further standardize the absolute magnitudes to better than 0.2 mag. The absolute magnitudes can be calibrated in two independent ways --- empirically, using Cepheid-based distances to parent galaxies of SNe Ia, and physically, by light curve and spectrum fitting. At present the empirical and physical calibrations are in agreement at $M_B \\simeq M_V \\simeq -19.4$ or -19....

  16. The Hubble Deep Field South Flanking Fields

    CERN Document Server

    Lucas, R A; Brown, T M; Casertano, S; Conselice, C J; De Mello, D F; Dickinson, M E; Ferguson, H C; Fruchter, A S; Gardner, J P; Gilmore, D; González-Lopezlira, R A; Heyer, I; Hook, R N; Kaiser, M E; Mack, J; Makidon, R B; Martin, C L; Mutchler, M Y; Smith, T E; Stiavelli, M; Teplitz, H I; Wiggs, M S; Williams, R E; Zurek, D R; Lucas, Ray A.; Baum, Stefi A.; Brown, Thomas M.; Casertano, Stefano; Conselice, Chris; Mello, Duilia de; Dickinson, Mark E.; Ferguson, Henry C.; Fruchter, Andrew S.; Gardner, Jonathan P.; Gilmore, Diane; Gonzalez-Lopezlira, Rosa A.; Heyer, Inge; Hook, Richard N.; Kaiser, Mary Elizabeth; Mack, Jennifer; Makidon, Russell; Martin, Crystal L.; Mutchler, Max; Stiavelli, Massimo; Teplitz, Harry I.; Wiggs, Michael S.; Williams, Robert E.; Zurek, David R.

    2003-01-01

    As part of the Hubble Deep Field South program, a set of shorter 2-orbit observations were obtained of the area adjacent to the deep fields. The WFPC2 flanking fields cover a contiguous solid angle of 48 square arcminutes. Parallel observations with the STIS and NICMOS instruments produce a patchwork of additional fields with optical and near-infrared (1.6 micron) response. Deeper parallel exposures with WFPC2 and NICMOS were obtained when STIS observed the NICMOS deep field. These deeper fields are offset from the rest, and an extended low surface brightness object is visible in the deeper WFPC2 flanking field. In this data paper, which serves as an archival record of the project, we discuss the observations and data reduction, and present SExtractor source catalogs and number counts derived from the data. Number counts are broadly consistent with previous surveys from both ground and space. Among other things, these flanking field observations are useful for defining slit masks for spectroscopic follow-up o...

  17. HUBBLE PARAMETER MEASUREMENT CONSTRAINTS ON DARK ENERGY

    Energy Technology Data Exchange (ETDEWEB)

    Farooq, Omer; Mania, Data; Ratra, Bharat, E-mail: omer@phys.ksu.edu, E-mail: mania@phys.ksu.edu, E-mail: ratra@phys.ksu.edu [Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, KS 66506 (United States)

    2013-02-20

    We use 21 Hubble parameter versus redshift data points from Simon et al., Gaztanaga et al., Stern et al., and Moresco et al. to place constraints on model parameters of constant and time-evolving dark energy cosmologies. The inclusion of the eight new measurements results in H(z) constraints more restrictive than those derived by Chen and Ratra. These constraints are now almost as restrictive as those that follow from current Type Ia supernova (SNIa) apparent magnitude versus redshift data, which now more carefully account for systematic uncertainties. This is a remarkable result. We emphasize, however, that SNIa data have been studied for a longer time than the H(z) data, possibly resulting in a better estimate of potential systematic errors in the SNIa case. A joint analysis of the H(z), baryon acoustic oscillation peak length scale, and SNIa data favors a spatially flat cosmological model currently dominated by a time-independent cosmological constant but does not exclude slowly evolving dark energy.

  18. Hubble parameter measurement constraints on dark energy

    CERN Document Server

    Farooq, Omer; Ratra, Bharat

    2012-01-01

    We use 21 Hubble parameter versus redshift data points, from Gazta\\~{n}aga et al. (2009), Stern et al. (2010), and Moresco et al. (2012), to place constraints on model parameters of constant and time-evolving dark energy cosmologies. This is the largest set of H(z) data considered to date. The inclusion of the 8 new Moresco et al. (2012) measurements results in H(z) constraints more restrictive than those derived by Chen & Ratra (2011b). These constraints are now almost as restrictive as those that follow from current Type Ia supernova (SNIa) apparent magnitude versus redshift data (Suzuki et al. 2012), which now more carefully account for systematic uncertainties. This is a remarkable result. We emphasize however that SNIa data have been studied for a longer time than the H(z) data, possibly resulting in a better estimate of potential systematic errors in the SNIa case. A joint analysis of the H(z), baryon acoustic oscillation peak length scale, and SNIa data favors a spatially-flat cosmological model cu...

  19. Determination of the Hubble Constant Using Cepheids

    CERN Document Server

    Abdel-Sabour, Mohamed; Issa, Issa Ali; El-Nawawy, Mohamed Saleh; Kordi, Ayman; Almostafa, Zaki; El-Said, Ahmad Essam; Ali, Gamal Bakr

    2014-01-01

    This paper introduces a statistical treatment to use Cepheid variable stars as distance indicators. The expansion rate of the Universe is also studied here through deriving the value of the Hubble constant H0. A Gaussian function approximation is proposed to fit the absolute magnitude and period of Cepheid variables in our galaxy. The calculations are carried out on samples of Cepheids observed in 23 galaxies to derive the distance modulus (DM) of these galaxies based on the frequency distributions of their periods and intrinsic apparent magnitudes. The DM is the difference between the apparent magnitude for extragalactic Cepheids and the absolute magnitude of the galactic Cepheids at maximum number. It is calculated by using the comparison of the period distribution of Cepheids in our galaxy and in other galaxies. This method is preferred due to its simplicity to use and its efficiency in providing reliable DM. A linear fit with correlation coefficient of 99.68% has been found between the published distance ...

  20. Spectral conditions for positive maps and entanglement witnesses

    Science.gov (United States)

    Chruściński, Dariusz; Kossakowski, Andrzej

    2011-03-01

    We provide partial classification of entanglement witnesses and positive maps which is based on a family of spectral conditions. Interestingly many well known examples of positive maps (e.g. transposition, reduction map, the family of Choi maps) belong to the class constructed via spectral conditions.

  1. Optimal entanglement witnesses from generalized reduction and Robertson maps

    Energy Technology Data Exchange (ETDEWEB)

    Chruscinski, Dariusz; Pytel, Justyna, E-mail: darch@fizyka.umk.pl [Institute of Physics, Nicolaus Copernicus University, Grudziadzka 5/7, 87-100 Torun (Poland)

    2011-04-22

    We provide a generalization of the reduction and Robertson positive maps in matrix algebras. They give rise to a new class of optimal entanglement witnesses. Their structural physical approximation is analyzed. As a byproduct we provide new examples of PPT (positive partial transpose) entangled states.

  2. Optimal entanglement witnesses from generalized reduction and Robertson maps

    CERN Document Server

    Chruściński, Dariusz

    2010-01-01

    We provide a generalization of the reduction and Robertson positive maps in matrix algebras. They give rise to a new class of optimal entanglement witnesses. Their structural physical approximations is analyzed. As a byproduct we provide a new examples of PPT (Positive Partial Transpose) entangled states.

  3. Optimal entanglement witnesses from generalized reduction and Robertson maps

    Science.gov (United States)

    Chruściński, Dariusz; Pytel, Justyna

    2011-04-01

    We provide a generalization of the reduction and Robertson positive maps in matrix algebras. They give rise to a new class of optimal entanglement witnesses. Their structural physical approximation is analyzed. As a byproduct we provide new examples of PPT (positive partial transpose) entangled states.

  4. 40 CFR 164.71 - Fees of witnesses.

    Science.gov (United States)

    2010-07-01

    ... 40 Protection of Environment 23 2010-07-01 2010-07-01 false Fees of witnesses. 164.71 Section 164.71 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY (CONTINUED) PESTICIDE PROGRAMS RULES OF PRACTICE GOVERNING HEARINGS, UNDER THE FEDERAL INSECTICIDE, FUNGICIDE, AND RODENTICIDE ACT, ARISING...

  5. Children Who Witness Domestic Violence: A Review of Empirical Literature.

    Science.gov (United States)

    Kolbo, Jerome R.; And Others

    1996-01-01

    Presents a review of the empirical literature examining the initial effects of witnessing domestic violence on children's functioning. Although results are somewhat inconclusive regarding children's social, cognitive, and physical development, findings of recently conducted investigations, when combined and compared with the previously reviewed…

  6. Anderson-Witting transport coefficients for flows in general relativity

    CERN Document Server

    Ambrus, Victor E

    2016-01-01

    The transport coefficients induced by the Anderson-Witting approximation of the collision term in the relativistic Boltzmann equation are derived for close to equilibrium flows in general relativity. Using the tetrad formalism, it is shown that the expression for these coefficients is the same as that obtained on flat space-time, in agreement with the generalized equivalence principle.

  7. 14 CFR 77.55 - Examination of witnesses.

    Science.gov (United States)

    2010-01-01

    ... 14 Aeronautics and Space 2 2010-01-01 2010-01-01 false Examination of witnesses. 77.55 Section 77.55 Aeronautics and Space FEDERAL AVIATION ADMINISTRATION, DEPARTMENT OF TRANSPORTATION (CONTINUED) AIRSPACE OBJECTS AFFECTING NAVIGABLE AIRSPACE Rules of Practice for Hearings Under Subpart D § 77.55...

  8. Instability of a witness bunch in a plasma bubble

    Energy Technology Data Exchange (ETDEWEB)

    Burov, A. [Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Lebedev, V. [Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Nagaitsev, S. [Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

    2016-02-16

    The stability of a trailing witness bunch, accelerated by a plasma wake accelerator (PWA) in a blow-out regime, is discussed. The instability growth rate as well as the energy spread, required for BNS damping, are obtained. A relationship between the PWA power efficiency and the BNS energy spread is derived.

  9. Properties of dimension witnesses and their semidefinite programming relaxations

    Science.gov (United States)

    Mironowicz, Piotr; Li, Hong-Wei; Pawłowski, Marcin

    2014-08-01

    In this paper we develop a method for investigating semi-device-independent randomness expansion protocols that was introduced in Li et al. [H.-W. Li, P. Mironowicz, M. Pawłowski, Z.-Q. Yin, Y.-C. Wu, S. Wang, W. Chen, H.-G. Hu, G.-C. Guo, and Z.-F. Han, Phys. Rev. A 87, 020302(R) (2013), 10.1103/PhysRevA.87.020302]. This method allows us to lower bound, with semi-definite programming, the randomness obtained from random number generators based on dimension witnesses. We also investigate the robustness of some randomness expanders using this method. We show the role of an assumption about the trace of the measurement operators and a way to avoid it. The method is also generalized to systems of arbitrary dimension and for a more general form of dimension witnesses than in our previous paper. Finally, we introduce a procedure of dimension witness reduction, which can be used to obtain from an existing witness a new one with a higher amount of certifiable randomness. The presented methods find an application for experiments [J. Ahrens, P. Badziag, M. Pawlowski, M. Zukowski, and M. Bourennane, Phys. Rev. Lett. 112, 140401 (2014), 10.1103/PhysRevLett.112.140401].

  10. Witnesses to Political Violence in Guatemala. Facts for Action #5.

    Science.gov (United States)

    Marchant, Fred; Wunder, Haleh

    The sources of political violence against Guatemala's rural poor are traced in this document for high school global education classes. The paper summarizes "Witness to Political Violence in Guatemala: The Suppression of a Rural Development Movement" (Oxfam America's Impact Audit No. 2). The study was based on 115 respondents, both…

  11. Witness for the Innocent: Children's Literature and the Vietnam War.

    Science.gov (United States)

    Saul, E. Wendy

    1985-01-01

    Presents findings from a study of treatment of the Vietnam war in children's literature. Found that there have not been a large number of books published on subject. Those dealing with subject witness the horrors of the war while treating the conflict as an isolated incident, without a past, and having only a tenuous relationship to our national…

  12. Local Hubble Expansion: Current State of the Problem

    CERN Document Server

    Dumin, Yurii V

    2016-01-01

    We present a brief qualitative overview of the current state of the problem of Hubble expansion at the sufficiently small scales (e.g., in planetary systems or local intergalactic volume). The crucial drawbacks of the available theoretical treatments are emphasized, and the possible ways to avoid them are outlined. Attention is drawn to a number of observable astronomical phenomena that could be naturally explained by the local Hubble expansion.

  13. Replacement vs. Renovation: The Reincarnation of Hubble Middle School

    Science.gov (United States)

    Ogurek, Douglas J.

    2010-01-01

    At the original Hubble Middle School, neither the views (a congested Roosevelt Road and glimpses of downtown Wheaton) nor the century-old facility that offered them was very inspiring. Built at the start of the 20th century, the 250,000-square-foot building was converted from Wheaton Central High School to Hubble Middle School in the early 1980s.…

  14. Psychological expert witness testimony and judicial decision making trends.

    Science.gov (United States)

    Shapiro, David L; Mixon, LeKisha; Jackson, Melissa; Shook, Jonathan

    2015-01-01

    Despite the establishment of the Daubert standard in 1993, the evidentiary criteria are rarely used as a basis for admissibility of expert witness testimony in the behavioral sciences. Ever since the promulgation of Frye and the Federal Rules of Evidence, controversy has surrounded the admissibility of expert testimony in courtrooms. There appears to be no existing uniform application of standards governing the admissibility of psychological expert witness testimony. Therefore, it is essential for the psycho-legal communities to explore judicial decision-making trends regarding psychological expert witness evidence. In this current research, psychological expert witness testimony and judicial decision-making will be explored. In preliminary examination, 97 criminal and civil case summaries from the LexisNexis Academic Database involved issues of admissibility. Analyses conducted by eight trained and paired coders revealed that reliability and assistance to the trier of fact were the most often cited reasons for admissibility in courts. Consistent with prior studies, it was also found that the most applied standards for admissibility of psychological evidence were the Federal Rules of Evidence. Interestingly, while the Daubert scientific criteria for admission of scientific testimony were mentioned, they were rarely utilized. A secondary analysis of 167 civil and criminal appellate cases indicated that the reliability of testimony (18% of all cases), ability to assist the trier of fact (17%), the expert witness' qualifications (17%), and the relevance of the testimony (16%) were the most commonly cited reasons for determining admissibility. A tertiary qualitative analysis focusing on these four categories then revealed eight major trends in admissibility of psychological expert evidence.

  15. Observations of the Hubble Deep Field with the Infrared Space Observatory .4. Association of sources with Hubble Deep Field galaxies

    DEFF Research Database (Denmark)

    Mann, R.G.; Oliver, S.J.; Serjeant, S.B.G.

    1997-01-01

    We discuss the identification of sources detected by the Infrared Space Observatory (ISO) at 6.7 and 15 mu m in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming...... these results (and, in one case, clarifying them) with independent visual searches, We find 15 ISO sources to be reliably associated with bright [I-814(AB) Hubble Flanking Fields (10 galaxies...

  16. Observations of the Hubble Deep Field with the Infrared Space Observatory .4. Association of sources with Hubble Deep Field galaxies

    DEFF Research Database (Denmark)

    Mann, R.G.; Oliver, S.J.; Serjeant, S.B.G.;

    1997-01-01

    We discuss the identification of sources detected by the Infrared Space Observatory (ISO) at 6.7 and 15 mu m in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming...... these results (and, in one case, clarifying them) with independent visual searches, We find 15 ISO sources to be reliably associated with bright [I-814(AB) Hubble Flanking Fields (10 galaxies...

  17. Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant

    CERN Document Server

    Freedman, Wendy L; Scowcroft, Victoria; Burns, Chris; Monson, Andy; Persson, S Eric; Seibert, Mark; Rigby, Jane

    2012-01-01

    Using a mid-infrared calibration of the Cepheid distance scale based on recent observations at 3.6 um with the Spitzer Space Telescope, we have obtained a new, high-accuracy calibration of the Hubble constant. We have established the mid-IR zero point of the Leavitt Law (the Cepheid Period-Luminosity relation) using time-averaged 3.6 um data for ten high-metallicity, Milky Way Cepheids having independently-measured trigonometric parallaxes. We have adopted the slope of the PL relation using time-averaged 3.6 um data for 80 long-period Large Magellanic Cloud (LMC) Cepheids falling in the period range 0.8 < log(P) < 1.8. We find a new reddening-corrected distance to the LMC of 18.477 +/- 0.033 (systematic) mag. We re-examine the systematic uncertainties in H0, also taking into account new data over the past decade. In combination with the new Spitzer calibration, the systematic uncertainty in H0 over that obtained by the Hubble Space Telescope (HST) Key Project has decreased by over a factor of three. App...

  18. HUBBLE PROVIDES COMPLETE VIEW OF JUPITER'S AURORAS

    Science.gov (United States)

    2002-01-01

    NASA's Hubble Space Telescope has captured a complete view of Jupiter's northern and southern auroras. Images taken in ultraviolet light by the Space Telescope Imaging Spectrograph (STIS) show both auroras, the oval- shaped objects in the inset photos. While the Hubble telescope has obtained images of Jupiter's northern and southern lights since 1990, the new STIS instrument is 10 times more sensitive than earlier cameras. This allows for short exposures, reducing the blurring of the image caused by Jupiter's rotation and providing two to five times higher resolution than earlier cameras. The resolution in these images is sufficient to show the 'curtain' of auroral light extending several hundred miles above Jupiter's limb (edge). Images of Earth's auroral curtains, taken from the space shuttle, have a similar appearance. Jupiter's auroral images are superimposed on a Wide Field and Planetary Camera 2 image of the entire planet. The auroras are brilliant curtains of light in Jupiter's upper atmosphere. Jovian auroral storms, like Earth's, develop when electrically charged particles trapped in the magnetic field surrounding the planet spiral inward at high energies toward the north and south magnetic poles. When these particles hit the upper atmosphere, they excite atoms and molecules there, causing them to glow (the same process acting in street lights). The electrons that strike Earth's atmosphere come from the sun, and the auroral lights remain concentrated above the night sky in response to the 'solar wind,' as Earth rotates underneath. Earth's auroras exhibit storms that extend to lower latitudes in response to solar activity, which can be easily seen from the northern U. S. But Jupiter's auroras are caused by particles spewed out by volcanoes on Io, one of Jupiter's moons. These charged particles are then magnetically trapped and begin to rotate with Jupiter, producing ovals of auroral light centered on Jupiter's magnetic poles in both the day and night skies

  19. Turning noise into signal: Learning from the scatter in the Hubble diagram

    Science.gov (United States)

    Castro, Tiago; Quartin, Miguel; Benitez-Herrera, Sandra

    2016-09-01

    The supernova (SN) Hubble diagram residual contains valuable information on both the present matter power spectrum and its growth history. In this paper we show that this information can be retrieved with precision by combining both peculiar velocity and weak-lensing analysis on the data. To wit, peculiar velocity induces correlations on the nearby SN while lensing induces a non-Gaussian dispersion in faraway objects. We show that both effects have almost orthogonal degeneracies and discuss how they can be extracted simultaneously from the data. We analyze the JLA supernova catalog in a 14-dimensional parameter space, assuming a flexible growth-rate index γ. We arrive at the following marginalized constraints: σ8 = 0.65-0.37+0.23 and γ = 1.38-0.65+1.7. Assuming instead GR as the correct gravitation theory (and thus γ ≡ 0.55), the constraints in σ8 tighten further: σ8 = 0.40-0.23+0.21. We show that these constraints complement well the ones obtained from other datasets and that they could improve substantially with more SNe.

  20. Turning noise into signal: learning from the scatter in the Hubble diagram

    CERN Document Server

    Castro, Tiago; Benitez-Herrera, Sandra

    2015-01-01

    The supernova Hubble diagram residual contains valuable information on both the present matter power spectrum and its growth history. In this paper we show that this information can be retrieved with precision by combining both peculiar velocity and weak-lensing analysis on the data. To wit, peculiar velocity induces correlations on the nearby supernovae while lensing induces a non-Gaussian dispersion in faraway objects. We show that both effects have almost orthogonal degeneracies and discuss how they can be extracted simultaneously from the data. We analyze the JLA supernova catalog in a 14-dimensional parameter space, assuming a flexible growth-rate index gamma. We arrive at the following marginalized constraints: sigma8 = $1.16^{+0.23}_{-0.47}$ and gamma = $0.80^{+0.29}_{-0.34}$. We note that these constraints complement well the ones obtained from other data sets. Assuming instead GR as the correct gravitation theory (and thus gamma = 0.55), the constraints in sigma8 tighten further: sigma8 = $0.89^{+0.1...

  1. Global Electrophonic Fireball Survey a review of witness reports - I

    CERN Document Server

    Vinkovic, D; Lim, P L; Kovacic, D; Zgrablic, G; Andreic, Z

    2002-01-01

    Despite more than 300 years since its first scientific description, the phenomenon of electrophonic sounds from meteors are still eluding complete physical explanation. According to the accepted knowledge, the sound itself is created by strong electric fields on the ground induced by the meteor. Nonetheless, there is no convincing theory that can fully explain how a meteor can generate such a strong electric field. Extreme rareness of the phenomenon has prevented a substantial experimental work so far; thus, consequently, it remains on the margins of scientific interest. This is quite unfortunate since these electric fields suggest existence of a highly complex electromagnetic coupling and charge dynamics between the meteors and the ionosphere. Therefore, the existing theoretical work relies mostly on the witness reports. The Global Electrophonic Fireball Survey (GEFS) is the first systematic survey of witness reports of these sounds with a standardized questionnaire designed exclusively for this phenomenon. ...

  2. Manipulating Multi-qudit Entanglement Witnesses by Using Linear Programming

    CERN Document Server

    Jafarizadeh, M A; Najarbashi, G

    2006-01-01

    A new class of entanglement witnesses (EWs) called reduction type entanglement witnesses is introduced, which can detect some multi-qudit entangeled states including PPT ones with Hilbert space of dimension $d_{_{1}}\\otimes d_{_{2}}\\otimes...\\otimes d_{_{n}}$. The novelty of this work comes from the fact that the feasible regions turn out to be convex polygons, hence the manipulation of these EWs reduces to linear programming which can be solved \\emph{exactly} by using simplex method. The decomposability and non-decomposability of these EWs are studied and it is shown that it has a close connection with eigenvalues and optimality of EWs. Also using the Jamio\\l kowski isomorphism, the corresponding possible positive maps, including the generalized reduction maps of Ref. \\cite{Hall1}, are obtained.

  3. CRIMINAL LEGAL PROTECTION OF CHILD VICTIMS AND WITNESSES OF CRIMES

    Directory of Open Access Journals (Sweden)

    Monika Mushevska

    2016-01-01

    Full Text Available The term victim indicates a natural person that underwent some kind of crime, including psychological and mental disorder, and emotional suffering or monetary loss, that were caused by accomplishing or not accomplishing a certain kind of activity that violates the law in one state. The term Victim also includes the close members of the victim’s family that depend on the victim. “Kids, victims and witnesses of crimes” indicates kids and adolescents under 18 years of age, which are victims of different kinds of crime or witnesses of different kinds of crime, in spite of the role that they have in the crime act. In all proceedings that directly or indirectly child victims involved it is important to act in a way that is the best and most appropriate for the child.

  4. Repeated Witnessing of Conspecifics in Pain: Effects on Emotional Contagion.

    Directory of Open Access Journals (Sweden)

    Maria Carrillo

    Full Text Available Witnessing of conspecifics in pain has been shown to elicit socially triggered freezing in rodents. It is unknown how robust this response is to repeated exposure to a cage-mate experiencing painful stimulation. To address this question, shock-experienced Observer rats repeatedly witnessed familiar Demonstrators receive painful footshocks (six sessions. Results confirm that Observers freeze during the first testing session. The occurrence of this behaviour however gradually diminished as the experimental sessions progressed, reaching minimal freezing levels by the end of the experiments. In contrast, the appearance and continuous increase in the frequency of yawning, a behavior that was inhibited by metyrapone (i.e,. a glucocorticoid synthesis blocker, might represent an alternative coping strategy, suggesting that the observer's reduced freezing does not necessarily indicate a disappearance in the affective response to the Demonstrator's distress.

  5. Bearing witness to suffering in AIDS: constructing meaning from loss.

    Science.gov (United States)

    Hall, V P

    2001-01-01

    The phenomenon of AIDS volunteerism has been described as an act of bearing witness. It has been suggested that bearing witness assists individuals affected by the suffering in HIV/AIDS to heal. The purpose of this research was to explore AIDS volunteerism as a potentially healing phenomenon. Using grounded theory methodology, open-ended interviews were conducted with 17 participants over a 7-month period of time. The constant comparative method was used for data analysis. A substantive theory was generated that identified the basic sociological process as constructing meaning from loss and described the transformative psychosocial and spiritual healing process individuals undergo as they volunteer. Constructing meaning from loss is described within the following three major stages: (a) experiencing suffering, (b) containing suffering, and (c) transforming suffering. Characteristics within each stage are described. Suffering and complex loss are major issues in HIV/AIDS. Interventions are recommended for nurses who care for those affected by HIV disease.

  6. Witnessing Quantum Coherence: from solid-state to biological systems

    CERN Document Server

    Li, Che-Ming; Chen, Yueh-Nan; Chen, Guang-Yin; Nori, Franco; 10.1038/srep00885

    2012-01-01

    Quantum coherence is one of the primary non-classical features of quantum systems. While protocols such as the Leggett-Garg inequality (LGI) and quantum tomography can be used to test for the existence of quantum coherence and dynamics in a given system, unambiguously detecting inherent "quantumness" still faces serious obstacles in terms of experimental feasibility and efficiency, particularly in complex systems. Here we introduce two "quantum witnesses" to efficiently verify quantum coherence and dynamics in the time domain, without the expense and burden of non-invasive measurements or full tomographic processes. Using several physical examples, including quantum transport in solid-state nanostructures and in biological organisms, we show that these quantum witnesses are robust and have a much finer resolution in their detection window than the LGI has. These robust quantum indicators may assist in reducing the experimental overhead in unambiguously verifying quantum coherence in complex systems.

  7. Forensic physicians and written evidence: witness statements v. expert reports.

    Science.gov (United States)

    Choong, Kartina A; Barrett, Martin

    2014-02-01

    When assisting the courts in criminal proceedings, the work of forensic physicians are leaning more towards the preparation of written evidence rather than the giving of oral evidence in person. For this, they may be asked to serve either as professional witnesses or expert witnesses. These 2 roles have nevertheless been a constant source of confusion among forensic physicians. In view of this, the article aims to highlight the similarities and differences between these 2 roles particularly in relation to the preparation of written evidence. It will take a close look at the forms of written evidence which forensic physicians are expected to produce in those distinct capacities and the attending duties, evidentiary rules and legal liabilities. Through this, the work aspires to assist forensic physicians undertake those responsibilities on a more informed footing.

  8. CRIMINAL LEGAL PROTECTION OF CHILD VICTIMS AND WITNESSES OF CRIMES

    OpenAIRE

    Monika Mushevska

    2016-01-01

    The term victim indicates a natural person that underwent some kind of crime, including psychological and mental disorder, and emotional suffering or monetary loss, that were caused by accomplishing or not accomplishing a certain kind of activity that violates the law in one state. The term Victim also includes the close members of the victim’s family that depend on the victim. “Kids, victims and witnesses of crimes” indicates kids and adolescents under 18 years of ...

  9. China Witnesses Great Growth with Major Trade Partners

    Institute of Scientific and Technical Information of China (English)

    2006-01-01

    @@ China, in 2005, had gone through a year of trade disputes with some major trade partners such as the United States of America, the European,etc..But what was the impact of the disputes on China's trade relations with them? The documents of the China Ministry of Commerce show that all the relations had witnessed a optimistic development, with active fruits ahieved as well.

  10. China Witnesses Great Growth with Major Trade Partners

    Institute of Scientific and Technical Information of China (English)

    2006-01-01

      China, in 2005, had gone through a year of trade disputes with some major trade partners such as the United States of America, the European,etc..But what was the impact of the disputes on China's trade relations with them? The documents of the China Ministry of Commerce show that all the relations had witnessed a optimistic development, with active fruits ahieved as well.……

  11. Did Franz Boas witness an act of cannibalism?

    Science.gov (United States)

    Maud, R

    1986-01-01

    Franz Boas has been used as an authority for the existence of cannibalism among the Kwakiutl of British Columbia, as cited in Patterns of Culture. There is reason to think, however, that all his evidence is hearsay, and that he himself never witnessed an act of cannibalism. One indication is that he eliminated all references to such acts in his final overview, published posthumously as Kwakiutl Ethnology.

  12. The Hubble Space Telescope Frontier Fields Program

    Science.gov (United States)

    Koekemoer, Anton M.; Mack, Jennifer; Lotz, Jennifer M.; Borncamp, David; Khandrika, Harish G.; Lucas, Ray A.; Martlin, Catherine; Porterfield, Blair; Sunnquist, Ben; Anderson, Jay; Avila, Roberto J.; Barker, Elizabeth A.; Grogin, Norman A.; Gunning, Heather C.; Hilbert, Bryan; Ogaz, Sara; Robberto, Massimo; Sembach, Kenneth; Flanagan, Kathryn; Mountain, Matt

    2017-08-01

    The Hubble Space Telescope Frontier Fields program is a large Director's Discretionary program of 840 orbits, to obtain ultra-deep observations of six strong lensing clusters of galaxies, together with parallel deep blank fields, making use of the strong lensing amplification by these clusters of distant background galaxies to detect the faintest galaxies currently observable in the high-redshift universe. The entire program has now completed successfully for all 6 clusters, namely Abell 2744, Abell S1063, Abell 370, MACS J0416.1-2403, MACS J0717.5+3745 and MACS J1149.5+2223,. Each of these was observed over two epochs, to a total depth of 140 orbits on the main cluster and an associated parallel field, obtaining images in ACS (F435W, F606W, F814W) and WFC3/IR (F105W, F125W, F140W, F160W) on both the main cluster and the parallel field in all cases. Full sets of high-level science products have been generated for all these clusters by the team at STScI, including cumulative-depth data releases during each epoch, as well as full-depth releases after the completion of each epoch. These products include all the full-depth distortion-corrected drizzled mosaics and associated products for each cluster, which are science-ready to facilitate the construction of lensing models as well as enabling a wide range of other science projects. Many improvements beyond default calibration for ACS and WFC3/IR are implemented in these data products, including corrections for persistence, time-variable sky, and low-level dark current residuals, as well as improvements in astrometric alignment to achieve milliarcsecond-level accuracy. The full set of resulting high-level science products and mosaics are publicly delivered to the community via the Mikulski Archive for Space Telescopes (MAST) to enable the widest scientific use of these data, as well as ensuring a public legacy dataset of the highest possible quality that is of lasting value to the entire community.

  13. Icing Forecasting of High Voltage Transmission Line Using Weighted Least Square Support Vector Machine with Fireworks Algorithm for Feature Selection

    Directory of Open Access Journals (Sweden)

    Tiannan Ma

    2016-12-01

    Full Text Available Accurate forecasting of icing thickness has great significance for ensuring the security and stability of the power grid. In order to improve the forecasting accuracy, this paper proposes an icing forecasting system based on the fireworks algorithm and weighted least square support vector machine (W-LSSVM. The method of the fireworks algorithm is employed to select the proper input features with the purpose of eliminating redundant influence. In addition, the aim of the W-LSSVM model is to train and test the historical data-set with the selected features. The capability of this proposed icing forecasting model and framework is tested through simulation experiments using real-world icing data from the monitoring center of the key laboratory of anti-ice disaster, Hunan, South China. The results show that the proposed W-LSSVM-FA method has a higher prediction accuracy and it may be a promising alternative for icing thickness forecasting.

  14. Among School Teachers: Bearing Witness as an Orientation in Educational Inquiry

    Science.gov (United States)

    Hansen, David T.

    2017-01-01

    In this writing, David Hansen illuminates the aesthetic, moral, and epistemic meaning of bearing witness to teaching and teachers by drawing upon a recently completed field-based endeavor that included extensive school visits. Hansen shows how bearing witness can bring the inquirer close to the truth of teaching. However, the witness must…

  15. The Kitty Genovese Murder and the Social Psychology of Helping: The Parable of the 38 Witnesses

    Science.gov (United States)

    Manning, Rachel; Levine, Mark; Collins, Alan

    2007-01-01

    This article argues that an iconic event in the history of helping research--the story of the 38 witnesses who remained inactive during the murder of Kitty Genovese--is not supported by the available evidence. Using archive material, the authors show that there is no evidence for the presence of 38 witnesses, or that witnesses observed the murder,…

  16. PACMan to Help Sort Hubble Proposals

    Science.gov (United States)

    Kohler, Susanna

    2017-04-01

    Every year, astronomers submit over a thousand proposals requesting time on the Hubble Space Telescope (HST). Currently, humans must sort through each of these proposals by hand before sending them off for review. Could this burden be shifted to computers?A Problem of VolumeAstronomer Molly Peeples gathered stats on the HST submissions sent in last week for the upcoming HST Cycle 25 (the deadline was Friday night), relative to previous years. This years proposal round broke the record, with over 1200 proposals submitted in total for Cycle 25. [Molly Peeples]Each proposal cycle for HST time attracts on the order of 1100 proposals accounting for far more HST time than is available. The proposals are therefore carefully reviewed by around 150 international members of the astronomy community during a six-month process to select those with the highest scientific merit.Ideally, each proposal will be read by reviewers that have scientific expertise relevant to the proposal topic: if a proposal requests HST time to study star formation, for instance, then the reviewers assigned to it should have research expertise in star formation.How does this matching of proposals to reviewers occur? The current method relies on self-reported categorization of the submitted proposals. This is unreliable, however; proposals are often mis-categorized by submitters due to misunderstanding or ambiguous cases.As a result, the Science Policies Group at the Space Telescope Science Institute (STScI) which oversees the review of HST proposals must go through each of the proposals by hand and re-categorize them. The proposals are then matched to reviewers with self-declared expertise in the same category.With the number of HST proposals on the rise and the expectation that the upcoming James Webb Space Telescope (JWST) will elicit even more proposals for time than Hubble scientists at STScI and NASA are now asking: could the human hours necessary for this task be spared? Could a computer program

  17. 33 CFR 165.1315 - Safety Zones: Fireworks displays in the Captain of the Port Portland Zone.

    Science.gov (United States)

    2010-07-01

    ... waters of Grays Harbor encompassed in a 600 foot radius around position 46°54′14″ N 124°06′08″ W. (ii... week of June or the first week of July each year. (16) East County 4th of July Fireworks, Gresham, OR..., Washington: from the northern shore of the Columbia River at 45°33′50″ N 122°20′16″ W, thence to 45°33′42″...

  18. Final Environmental Assessment for Fireworks Display and Cleanup for the Luke Air Force Base, Arizona, Fourth of July Celebrations

    Science.gov (United States)

    2015-04-21

    fireworks for recreational purposes or pyrotechnics for musical or cinematic/theatrical functions." Other Regulatory Requirements The EA...would be projected from the stage that is erected at Fowler Park as the venue for live music that occurs as part of the Freedom Fest celebration...for irrigation requirements. The greatest declines occurred west, north, and south of Luke AFB. A large area of depression has existed southwest of

  19. Hubble Parameter in QCD Universe for finite Bulk Viscosity

    CERN Document Server

    Tawfik, A; Mansour, H; Harko, T

    2010-01-01

    The influence of perturbative bulk viscosity on the evolution of Hubble parameter in the QCD era of the early Universe has been analyzed, where Friedmann-Robertson-Walker metric and Einstein field equations are utilized. Homogeneous and isotropic background matter is assumed to be characterized by barotropic equations of state deduced from recent lattice QCD simulations and heavy--ion collisions. Taking into account perturbative bulk viscosity coefficient, an estimation for the evolution of the Hubble parameter has been introduced and compared with its evolution in a non--viscous matter. A numerical solution for finite viscous Israel-Stewart background matter is also worked out. Both methods qualitatively agree in reproducing viscous Hubble parameter that turns to be slightly different from the non--viscous one. This treatment is strictly limited within a very narrow temperature-- or time--interval in QCD era, where the QGP matter is likely dominant.

  20. Planck and WMAP constraints on generalised Hubble flow inflationary trajectories

    CERN Document Server

    Contaldi, Carlo R

    2013-01-01

    We use the Hamilton--Jacobi formalism to constrain the space of possible single field, inflationary Hubble flow trajectories when compared to the WMAP and Planck satellites Cosmic Microwave Background (CMB) results. This method yields posteriors on the space of Hubble Slow Roll (HSR) parameters that uniquely determine the history of the Hubble parameter during the inflating epoch. The trajectories are used to numerically determine the observable primordial power spectrum and bispectra that can then be compared to observations. Our analysis is used to infer the most likely shape of the inflaton potential $V(\\phi)$ and also yields a prediction for, $f_{\\rm NL}$, the dimensionless amplitude of the non-Gaussian bispectrum.

  1. Hubble's Law Implies Benford's Law for Distances to Galaxies

    Science.gov (United States)

    Hill, Theodore P.; Fox, Ronald F.

    2016-03-01

    A recent article by Alexopoulos and Leontsinis presented empirical evidence that the first digits of the distances from the Earth to galaxies are a reasonably good fit to the probabilities predicted by Benford's law, the well known logarithmic statistical distribution of significant digits. The purpose of the present article is to give a theoretical explanation, based on Hubble's law and mathematical properties of Benford's law, why galaxy distances might be expected to follow Benford's law. The new galaxy-distance law derived here, which is robust with respect to change of scale and base, to additive and multiplicative computational or observational errors, and to variability of the Hubble constant in both time and space, predicts that conformity to Benford's law will improve as more data on distances to galaxies becomes available. Conversely, with the logical derivation of this law presented here, the recent empirical observations may be viewed as independent evidence of the validity of Hubble's law.

  2. Hubble's Law Implies Benford's Law for Distances to Stars

    CERN Document Server

    Fox, Ronald F

    2014-01-01

    A recent article by Alexopoulos and Leontsinis presented empirical evidence that the distances to stars listed in the 2011 HYG database "follow well the probabilities predicted by Benford's law", the well known logarithmic statistical distribution of significant digits. The purpose of the present article is to give a theoretical explanation, based on Hubble's law and mathematical properties of Benford's law, why star distances might be expected to follow Benford's law. Conversely, with the logical derivation given here, the empirical observations may be viewed as new independent evidence of the validity of Hubble's law.

  3. Constraining Ω with the fluctuation of the local Hubble flow

    Institute of Scientific and Technical Information of China (English)

    Quan Guo; Huan-Yuan Shan

    2009-01-01

    We present an analysis of the fluctuation of the local Hubble flow using 350 galaxies in the Local Volume (D<5 Mpc, hereafter LV) with accurate measurements of distances, positions and radial velocities, and compare the results with the theoretical prediction of the local Hubble flow induced by density perturbations. This allows us to set a useful constraint on the local Ω parameters: ΩM~0.6 and ΩΛ~0.7, which may serve as compelling evidence for the existence of dark energy in the local Universe.

  4. Hubble Space Telescope: Latest citations from the EI Compendex*Plus Database

    Science.gov (United States)

    1996-02-01

    The bibliography contains citations concerning the Hubble Space Telescope and its mission. Topics include design changes, flight performance, and initial problems encountered. The Hubble's solar arrays and observations of space are discussed.

  5. Analysis of Interplanetary Dust Experiment Detectors and Other Witness Plates

    Science.gov (United States)

    Griffis, D. P.; Wortman, J. J.

    1992-01-01

    The development of analytical procedures for identifying the chemical composition of residue from impacts that occurred on the Interplanetary Dust Experiment (IDE) detectors during the flight of Long Duration Exposure Facility (LDEF) and the carrying out of actual analysis on IDE detectors and other witness plates are discussed. Two papers on the following topics are presented: (1) experimental analysis of hypervelocity microparticle impact sites on IDE sensor surfaces; and (2) contaminant interfaces with secondary Ion Mass Spectrometer (SIMS) analysis of microparticle impactor residues on LDEF surfaces.

  6. Entanglement Witnesses and Characterizing Entanglement Properties of Some PPT States

    CERN Document Server

    Jafarizadeh, M A; Akbari, Y

    2010-01-01

    On the basis of linear programming, new sets of entanglement witnesses (EWs) for 3x3 and 4x4 systems are constructed. In both cases, the constructed EWs correspond to the hyperplanes contacting, without intersecting, the related feasible regions at line segments and restricted planes respectively. Due to the special property of the contacting area between the hyper-planes and the feasible regions, the corresponding hyper-planes can be turned around the contacting area throughout a bounded interval and hence create an infinite number of EWs. As these EWs are able to detect entanglement of some PPT states, they are non-decomposable (nd-EWs).

  7. Blood transfusion in jehovah's witnesses, a dilemma in medicine?

    Directory of Open Access Journals (Sweden)

    Rafael Gutierrez-Vega

    2014-10-01

    Full Text Available The provision of health services should be carried attached to the scientific and ethical principles of medicine. The negative to accept blood transfusion by Jehovah's Witnesses, when indicated, determines a conflict and a challenge for physicians. We discuss concepts related to this complex situation, including: Freedom of religion and belief, patients’ rights, regulatory framework that applies to providers of health services and medical rights. Which should be taken into account in these situations to make an informed decision from the legal and ethical point of view.

  8. High Redshift Galaxies in the Hubble Ultra Deep Field

    CERN Document Server

    Hathi, Nimish P

    2008-01-01

    My dissertation presents results from three recent investigations in the Hubble Ultra Deep Field (HUDF) focusing on understanding structural and physical properties of high redshift galaxies. Here I summarize results from these studies. This thesis work was conducted at Arizona State University under the guidance of Prof. Rogier Windhorst and Prof. Sangeeta Malhotra.

  9. WSRT observations of the Hubble Deep Field region

    NARCIS (Netherlands)

    Garrett, MA; de Bruyn, AG; Giroletti, M; Baan, WA; Schilizzi, RT

    We present deep WSRT 1.4 GHz observations of the Hubble Deep Field region. At the 5 sigma level, the WSRT clearly detects 85 regions of radio emission in a 10' x 10' field centred on the HDF Eight of these regions fall within the HDF itself, four of these are sources that have not previously been

  10. Dynamical decomposition of galaxies across the Hubble sequence

    NARCIS (Netherlands)

    Zhu, L.; van den Bosch, R. C. E.; van de Ven, G.; Falcón-Barroso, J.; Lyubenova, M.; Meidt, S. E.; Martig, M.; Yildirim, A.

    2016-01-01

    Ongoing and upcoming integral-field spectroscopic surveys will provide stellar kinematic maps of thousands of nearby galaxies across the Hubble sequence. For the first time, we have been able to construct Schwarzschild dynamical models that fit in detail elliptical through spiral galaxies from the

  11. Hubble: Linked Data Hub for Clinical Decision Support

    NARCIS (Netherlands)

    Hoekstra, R.; Magliacane, S.; Rietveld, L.; de Vries, G.; Wibisono, A.; Schlobach, S.; Simperl, E.; Norton, B.; Mladenic, D.; Della Valle, E.; Fundulaki, I.; Passant, A.; Troncy, R.

    2015-01-01

    The AERS datasets is one of the few remaining, large publicly available medical data sets that until now have not been published as Linked Data. It is uniquely positioned amidst other medical datasets. This paper describes the Hubble prototype system for clinical decision support that demonstrates

  12. A Guided Inquiry on Hubble Plots and the Big Bang

    Science.gov (United States)

    Forringer, Ted

    2014-01-01

    In our science for non-science majors course "21st Century Physics," we investigate modern "Hubble plots" (plots of velocity versus distance for deep space objects) in order to discuss the Big Bang, dark matter, and dark energy. There are two potential challenges that our students face when encountering these topics for the…

  13. Early Scientific Results from the Rejuvenated Hubble Space Telescope

    Science.gov (United States)

    Niedner, Malcolm

    2010-01-01

    With the complete success of Servicing Mission 4 (SM4) to the Hubble Space Telescope in May, 2009, the Observatory's capabilities are extremely broad and beyond anything it has previously been equipped with. I will present results on the important early science corning out of the telescope and discuss prospects for the future."

  14. Angular Momentum across the Hubble sequence from the CALIFA survey

    NARCIS (Netherlands)

    Falcón-Barroso, Jesús; Lyubenova, Mariya; van de Ven, Glenn

    We investigate the stellar angular momentum of galaxies across the Hubble sequence from the CALIFA survey. The distribution of CALIFA elliptical and lenticular galaxies in the λRe - ɛe diagram is consistent with that shown by the Atlas3D survey. Our data, however, show that the location of spiral

  15. Short term effect of hubble-bubble smoking on voice.

    Science.gov (United States)

    Hamdan, A-L; Sibai, A; Mahfoud, L; Oubari, D; Ashkar, J; Fuleihan, N

    2011-05-01

    To investigate the short term effect of hubble-bubble smoking on voice. Prospective study. Eighteen non-dysphonic subjects (seven men and 11 women) with a history of hubble-bubble smoking and no history of cigarette smoking underwent acoustic analysis and laryngeal video-stroboscopic examination before and 30 minutes after hubble-bubble smoking. On laryngeal video-stroboscopy, none of the subjects had vocal fold erythema either before or after smoking. Five patients had mild vocal fold oedema both before and after smoking. After smoking, there was a slight increase in the number of subjects with thick mucus between the vocal folds (six, vs four before smoking) and with vocal fold vessel dilation (two, vs one before smoking). Acoustic analysis indicated a drop in habitual pitch, fundamental frequency and voice turbulence index after smoking, and an increase in noise-to-harmonics ratio. Even 30 minutes of hubble-bubble smoking can cause a drop in vocal pitch and an increase in laryngeal secretions and vocal fold vasodilation.

  16. Kennedy Educate to Innovate (KETI) Hubble Powerpoint Presentation

    Science.gov (United States)

    Paglialonga, Jessica

    2011-01-01

    The presentation describes the Hubble Space Telescope and it's contributions to astronomy. Also discussed are the James Webb Space Telescope and the kinds of careers that relate to STEM (science, technology, engineering, and mathematics) that students can pursue in fields related to space telescopes.

  17. HUBBLE FINDS A BARE BLACK HOLE POURING OUT LIGHT

    Science.gov (United States)

    2002-01-01

    NASA's Hubble Space Telescope has provided a never-before-seen view of a warped disk flooded with a torrent of ultraviolet light from hot gas trapped around a suspected massive black hole. [Right] This composite image of the core of the galaxy was constructed by combining a visible light image taken with Hubble's Wide Field Planetary Camera 2 (WFPC2), with a separate image taken in ultraviolet light with the Faint Object Camera (FOC). While the visible light image shows a dark dust disk, the ultraviolet image (color-coded blue) shows a bright feature along one side of the disk. Because Hubble sees ultraviolet light reflected from only one side of the disk, astronomers conclude the disk must be warped like the brim of a hat. The bright white spot at the image's center is light from the vicinity of the black hole which is illuminating the disk. [Left] A ground-based telescopic view of the core of the elliptical galaxy NGC 6251. The inset box shows Hubble Space Telescope's field of view. The galaxy is 300 million light-years away in the constellation Ursa Minor. Photo Credit: Philippe Crane (European Southern Observatory), and NASA

  18. A Guided Inquiry on Hubble Plots and the Big Bang

    Science.gov (United States)

    Forringer, Ted

    2014-01-01

    In our science for non-science majors course "21st Century Physics," we investigate modern "Hubble plots" (plots of velocity versus distance for deep space objects) in order to discuss the Big Bang, dark matter, and dark energy. There are two potential challenges that our students face when encountering these topics for the…

  19. Hubble Space Telescope On-orbit Transfer Function Test

    Science.gov (United States)

    Vadlamudi, N.; Blair, M. A.; Clapp, B. R.

    1992-01-01

    The paper describes the On-orbit Transfer Function Test (TFT) designed for on-orbit vibration testing of the Hubble Space Telescope (HST). The TFT provides means for extracting accurate on-orbit characteristics of HST flexible body dynamics, making it possible to check periodically the state of the vehicle on-orbit and to assess changes in modal parameters.

  20. Kennedy Educate to Innovate (KETI) Hubble Powerpoint Presentation

    Science.gov (United States)

    Paglialonga, Jessica

    2011-01-01

    The presentation describes the Hubble Space Telescope and it's contributions to astronomy. Also discussed are the James Webb Space Telescope and the kinds of careers that relate to STEM (science, technology, engineering, and mathematics) that students can pursue in fields related to space telescopes.

  1. The voices of victims and witnesses of school bullying

    Directory of Open Access Journals (Sweden)

    C. de Wet

    2005-07-01

    Full Text Available There has never been a stronger demand from the South African public to reduce school violence than at present. The demand for safe schools cannot be achieved unless the issue of bullying is adequately addressed. However, it appears from newspaper reports that some of the role players are not willing to listen to the victims of bullying. The aim of this article is to give a voice to some of the victims, as well as those witnessing school bullying. This article reports on findings from an investigation of the experiences of a group of Free State learners who were witnesses and victims of bullying. The research instrument was the Delaware Bullying Questionnaire. The first important conclusion from this study was that bullying was a serious problem in some Free State schools. Secondly, it was found that the respondents were more often the victims of male than of female bullies. Thirdly, the quantitative data indicated that the majority of victims were bullied by learners who were in the same grade as they were. The qualitative data, however, revealed that the bullying of Grade 8 learners by Grade 12 learners seems to be a fairly common occurrence. Finally, some comments and recommendations are made.

  2. Trauma, forgiveness and the witnessing dance: making public spaces intimate.

    Science.gov (United States)

    Gobodo-Madikizela, Pumla

    2008-04-01

    In this paper I explore the concept of forgiveness as a response to gross human rights violations. I present a conceptual examination of the effects of massive trauma in relation to what I refer to as the 'unfinished business' of trauma. Using a psychoanalytic framework, I consider the process of 'bearing witness' about trauma and examine how this process opens up the possibility of reciprocal expressions of empathy between victim and perpetrator. I then argue that, in this context of trauma testimony and witnessing, empathy is essential for the development of remorse on the part of perpetrators, and of forgiveness on the part of victims. Using a case study from South Africa's Truth and Reconciliation Commission (TRC) I clarify the relationship between empathy and forgiveness, and show how the restorative model of the TRC can open up an ethical space and create the possibility of transformation for victims, perpetrators and bystanders. In my conclusion I suggest that forgiveness in politics is the only action that holds promise for the repair of brokenness in post-conflict societies, particularly if, as in South Africa, victims have to live together with perpetrators and beneficiaries in the same country.

  3. The impact of ground-level fireworks (13 km long) display on the air quality during the traditional Yanshui Lantern Festival in Taiwan.

    Science.gov (United States)

    Chang, Shuenn-Chin; Lin, Ta-Hsiung; Young, Chea-Yuan; Lee, Chung-Te

    2011-01-01

    In this study, the concentrations of CO, non-methane hydrocarbons, NO(X), SO(2), benzene, toluene, ethylbenzene, xylene (BTEX), PM₁₀, and PM₂.₅ were continuously monitored before and after the fireworks display during the traditional Lantern Festival from March 2-7, 2007 in Yanshui Town, Taiwan. Major roads in Yanshui Town were surrounded by fireworks 13 km in length, with the display lasting for 45 min. More than 200 small firecracker towers popped up randomly in town, resulting in exceedingly inhomogeneous air quality until the end of display at 03:00 the next day, March 5. During the fireworks display, the hourly concentration of PM₁₀ and PM₂.₅ at Yanshui Primary School reached about 429 and 250 μg m⁻³, respectively, which is 10 times the normal level, and 6 s values even went as high as 1,046 and 842 μg m⁻³, respectively. Similarly, BTEX concentration went up to about five to 10 times its normal value during the fireworks display. As indicated by the distribution of submicron particle sizes, the number of particles with a diameter less than 100 nm increased abruptly during the event period. Metal components with concentrations of more than 10 times higher than the normal value at Yanshui Primary School were Sr, K, Ba, Pb, Al, Mg, and Cu, in sequence. Among water-soluble ions, the content of K( + ), Mg²( + ), and Cl( - ) increased the most, all of which were related to the materials used in the fireworks. The results of this study indicate that fireworks can cause an abrupt increase in the concentration of trace substances in the air within a short period. Although the risks of these trace substances on public health remain to be further assessed, the study results can be utilized in the management of folk events.

  4. HUBBLE VIEWS ANCIENT STORM IN THE ATMOSPHERE OF JUPITER

    Science.gov (United States)

    2002-01-01

    When 17th-century astronomers first turned their telescopes to Jupiter, they noted a conspicuous reddish spot on the giant planet. This Great Red Spot is still present in Jupiter's atmosphere, more than 300 years later. It is now known that it is a vast storm, spinning like a cyclone. Unlike a low-pressure hurricane in the Caribbean Sea, however, the Red Spot rotates in a counterclockwise direction in the southern hemisphere, showing that it is a high-pressure system. Winds inside this Jovian storm reach speeds of about 270 mph. The Red Spot is the largest known storm in the Solar System. With a diameter of 15,400 miles, it is almost twice the size of the entire Earth and one-sixth the diameter of Jupiter itself. The long lifetime of the Red Spot may be due to the fact that Jupiter is mainly a gaseous planet. It possibly has liquid layers, but lacks a solid surface, which would dissipate the storm's energy, much as happens when a hurricane makes landfall on the Earth. However, the Red Spot does change its shape, size, and color, sometimes dramatically. Such changes are demonstrated in high-resolution Wide Field and Planetary Cameras 1 and 2 images of Jupiter obtained by NASA's Hubble Space Telescope, and presented here by the Hubble Heritage Project team. The mosaic presents a series of pictures of the Red Spot obtained by Hubble between 1992 and 1999. Astronomers study weather phenomena on other planets in order to gain a greater understanding of our own Earth's climate. Lacking a solid surface, Jupiter provides us with a laboratory experiment for observing weather phenomena under very different conditions than those prevailing on Earth. This knowledge can also be applied to places in the Earth's atmosphere that are over deep oceans, making them more similar to Jupiter's deep atmosphere. The Hubble images were originally collected by Amy Simon (Cornell U.), Reta Beebe (NMSU), Heidi Hammel (Space Science Institute, MIT), and their collaborators, and have been

  5. Differences between accounts provided by witnesses and alleged victims of child sexual abuse.

    Science.gov (United States)

    Lamb, Michael E; Sternberg, Kathleen J; Orbach, Yael; Hershkowitz, Irit; Horowitz, Dvora

    2003-09-01

    To determine whether child witnesses of sexual abuse were more or less informative about the alleged incidents than alleged victims when interviewed similarly. Twenty-six alleged victims of child sexual abuse (aged 5 to 14 years; M=9.8 years) and 26 children who had witnessed but not experienced similar events were interviewed by experienced youth investigators about the alleged abuse. Children in the two groups were matched with respect to their age, relationships with the alleged perpetrator, and seriousness of the alleged offenses. All children were interviewed using the NICHD investigative interview protocol. Witnesses and victims provided similar amounts of information about the incidents of abuse. Interviewers used more open-ended invitations and elicited more information using open-ended prompts from witnesses than from victims, whereas they used more risky (including suggestive) prompts when interviewing victims. These results confirm that young children can be informative witnesses about events that they have either experienced or witnessed.

  6. Parametric optimization of ultrasonic machining process using gravitational search and fireworks algorithms

    Directory of Open Access Journals (Sweden)

    Debkalpa Goswami

    2015-03-01

    Full Text Available Ultrasonic machining (USM is a mechanical material removal process used to erode holes and cavities in hard or brittle workpieces by using shaped tools, high-frequency mechanical motion and an abrasive slurry. Unlike other non-traditional machining processes, such as laser beam and electrical discharge machining, USM process does not thermally damage the workpiece or introduce significant levels of residual stress, which is important for survival of materials in service. For having enhanced machining performance and better machined job characteristics, it is often required to determine the optimal control parameter settings of an USM process. The earlier mathematical approaches for parametric optimization of USM processes have mostly yielded near optimal or sub-optimal solutions. In this paper, two almost unexplored non-conventional optimization techniques, i.e. gravitational search algorithm (GSA and fireworks algorithm (FWA are applied for parametric optimization of USM processes. The optimization performance of these two algorithms is compared with that of other popular population-based algorithms, and the effects of their algorithm parameters on the derived optimal solutions and computational speed are also investigated. It is observed that FWA provides the best optimal results for the considered USM processes.

  7. Psychological and behavioral correlates of family violence in child witnesses and victims.

    Science.gov (United States)

    Hughes, Honore M

    1988-01-01

    Abused and nonabused child witnesses to parental violence temporarily residing in a battered women's shelter were compared to children from a similar economic background on measures of self-esteem, anxiety, depression, and behavior problems, using mothers' and self-reports. Results indicated significantly more distress in the abused-witness children than in the comparison group, with nonabused witness children's scores falling between the two. Age of child and types of violence were mediating factors. Implications of the findings are discussed.

  8. Witnessing effective entanglement over a 2km fiber channel

    CERN Document Server

    Wittmann, Christoffer; Wiechers, Carlos; Elser, Dominique; Häseler, Hauke; Lütkenhaus, Norbert; Leuchs, Gerd

    2009-01-01

    We present a fiber-based continuous-variable quantum key distribution system. In the scheme, a quantum signal of two non-orthogonal weak optical coherent states is sent through a fiber-based quantum channel. The receiver simultaneously measures conjugate quadratures of the light using two homodyne detectors. From the measured Q-function of the transmitted signal, we estimate the attenuation and the excess noise caused by the channel. The estimated excess noise originating from the channel and the channel attenuation including the quantum efficiency of the detection setup is investigated with respect to the detection of effective entanglement. The local oscillator is considered in the verification. We witness effective entanglement with a channel length of up to 2km.

  9. Witness to 30 Years of China-U.S. Relations

    Institute of Scientific and Technical Information of China (English)

    2009-01-01

    Jan Carol Berris has witnessed a series of events that made history for China-U.S. relations, including ping-pong diplomacy, the exchange of ping-pong players in the 1970s that eased the way for higher-level contact. She has overseen hundreds of American delegations to China and met many from China. She has traveled to China about 100 times with groups and individuals as diverse as a tennis team and a Supreme Court Justice. She is popular among different groups of people in China, who better recognize her Chinese name, Bai Lijuan. As both countries celebrate the 30th anniversary of normalization of China-U.S. diplomatic relations, Berris, Vice President of the National Committee on United States-China Relations, talks to Beijing Review reporter Chen Wen about her special experience of that particular period of history.

  10. Graphic Evolution Witness the Development of Lung Cancer Translational Research

    Directory of Open Access Journals (Sweden)

    Chao ZHANG

    2016-06-01

    Full Text Available Lung cancer treatment has altered from conventional chemotherapy to targeted treatment, which now has been turned to the immunotherapy. Translational research has played an irreplaceable role during this progression which graphic evolution has witnessed. The evolution has gone through forest plot, KM-curve, waterfall plot, spider plot and timeline-area, showing us the refining concept and gradual process of lung cancer treatment undergoing from community towards individual. Even though the latest immunotherapy is getting increasingly hot, the result isn’t quite expected. Meanwhile, the limitations of conventional treatment still exist which require further research. This article will primarily illustrate the development of translational research of lung cancer via the aspect of curve evolution and analysis some abortive clinical trials in lung cancer surgery for inspiring the next graphic style and lung cancer treatment.

  11. Molecules as Drives and Witnesses of Star Formation

    Science.gov (United States)

    Shustov, B. M.

    2017-07-01

    The progress in understanding the role of molecules in star formation is discussed. After very brief introduction which we note in that no star formation would be possible without molecules at the dawn of the Universe and that molecules are important drivers and witnesses of star formation in the current epoch, we consider observational technologies and emphasize the prospective role of UV observations. Special attention is paid to possibilities of UV spectroscopy with coming space observatory Spektr-UF (World Space Observatory - Ultraviolet; WSO-UV). Only one example (observations of CO-dark clouds) from vast scientific program of the WSO-UV is mentioned. Also very briefly disclosed is a model approach to study complex evolution of very young (prestellar) object focusing on chemical (molecular) evolution.

  12. Witnessing Macroscopic Entanglement in a Staggered Magnetic Field

    CERN Document Server

    Hide, J; Son, W; Vedral, V; Hide, Jenny; Lawrie, Ian; Son, Wonmin; Vedral, Vlatko

    2007-01-01

    We investigate macroscopic entanglement in an infinite XX spin-1/2 chain with staggered magnetic field, $B_l=B+e^{-i\\pi l}b$. Using single-site entropy and by constructing an entanglement witness, we search for the existence of entanglement when the system is at absolute zero, as well as in thermal equilibrium. Although the role of the alternating magnetic field $b$ is, in general, to suppress entanglement as do $B$ and $T$, we find that when T=0, introducing $b$ allows the existence of entanglement even when the uniform magnetic field $B$ is arbitrarily large. We find that the region and the amount of entanglement in the spin chain can be enhanced by a staggered magnetic field.

  13. Witness to Change: A Tibetan Woman Recalls Her Life

    Directory of Open Access Journals (Sweden)

    Nangchukja

    2015-07-01

    Full Text Available Nangchukja. 2015. Witness to Change: A Tibetan Woman Recalls Her Life in Gerald Roche, Keith Dede, Fernanda Pirie, and Benedict Copps (eds Asian Highlands Perspectives 37 Centering the Local, A Festschrift for Dr. Charles Kevin Stuart on the Occasion of his Sixtieth Birthday, 250-278. Women play a critical role in rural Tibetan households. As youths and adults, they engage in labor-intensive chores, including farming, herding, fetching water, cooking, tailoring, cleaning, collecting fuel, and child care. In their old age, most Tibetan women dedicate themselves to chanting, prostrating, going on pilgrimage, and meditating. Prior to the early twenty-first century, in such areas as Mang ra County in A mdo, women seldom traveled away from their family and community for work, though nomadic women seasonally traveled long distances between summer and winter camps with their family's livestock. Farming and herding have sustained life on the Tibetan Plateau for millennia. These traditional lifestyles have been changing in most Tibetan communities today in China's rapidly urbanizing society. Despite the massive transformations that have taken place in A mdo over the last sixty years, much continuity remains in how Tibetan women in A mdo spend their time. In 2015, average women in their forties and above are still actively engaged in such religious practices as chanting, prostrating, going on pilgrimage, and meditating. This paper presents the life-story of an elder Tibetan woman, Lha mtsho (b. 1946. Similar to many other Tibetan women born in the late 1940s, she was witness to the chaos of 1958, the Great Leap Forward (1958-1961, the Cultural Revolution (1966-1976, and also saw China's economic reform and development from the late 1970s up until today.

  14. The Web Interface Template System (WITS), a software developer`s tool

    Energy Technology Data Exchange (ETDEWEB)

    Lauer, L.J.; Lynam, M.; Muniz, T. [Sandia National Labs., Albuquerque, NM (United States). Financial Systems Dept.

    1995-11-01

    The Web Interface Template System (WITS) is a tool for software developers. WITS is a three-tiered, object-oriented system operating in a Client/Server environment. This tool can be used to create software applications that have a Web browser as the user interface and access a Sybase database. Development, modification, and implementation are greatly simplified because the developer can change and test definitions immediately, without writing or compiling any code. This document explains WITS functionality, the system structure and components of WITS, and how to obtain, install, and use the software system.

  15. Children who witness violence: what services do they need to heal?

    Science.gov (United States)

    Willis, Danny; Hawkins, Joellen W; Pearce, Carole W; Phalen, Jaime; Keet, Meredith; Singer, Cristen

    2010-09-01

    Children are witnesses to violence far too often in their daily lives. To elicit information on the needs of children and adolescents living in the United States who have witnessed violence in their homes, neighborhoods, or communities, we held focus groups with mothers who have survived interpersonal violence and whose family included child witnesses to violence (CWV), professionals who work with families affected by violence, and with adolescents who have witnessed violence. Based on four separate focus group discussions held in Massachusetts, involving a total of 45 participants, recommendations for screening, programming, and the development of healing interventions are offered to mental health professionals.

  16. Determinants of witnessed parental physical violence among university students in transitional Albania

    National Research Council Canada - National Science Library

    Burazeri, Genc; Qirjako, Gentiana; Roshi, Enver; Brand, Helmut

    2011-01-01

    We aimed to assess the extent and the socioeconomic correlates of witnessed parental physical violence among university students in Albania, a country in transition from rigidly structured socialism...

  17. Children's memory distortions following social contact with a co-witness: disentangling social and cognitive mechanisms.

    Science.gov (United States)

    Bright-Paul, Alexandra; Jarrold, Christopher; Wright, Daniel B; Guillaume, Stephanie

    2012-01-01

    This study examined whether recalling an event with a co-witness influences children's recall. Individual 3-5-year-olds (n = 48) watched a film with a co-witness. Unbeknown to participants, the co-witness was watching an alternative version of the film. Afterwards both the co-witness and the participant answered questions about the film together (public recall), and the degree to which children conformed to the co-witness's alternative version of events was measured. Subsequently participants were questioned again individually (private recall). Children also completed false belief and inhibitory control tasks. By separating errors made in public and private, the results indicated that both social conformity (32% of errors) and memory distortion (68% of errors) played a role in co-witness influence. Inhibitory control predicted the likelihood of retracting errors in private, but only for children who failed (r = .66) rather than passed false belief tasks (r = -.10). The results suggest that children with a theory of mind conform in the company of the co-witness to avoid social embarrassment, while those a poor theory of mind conform on the basis of an inability to inhibit the co-witness's response. The findings contribute to our understanding of the motivations responsible for co-witness conformity across early childhood.

  18. Witnessing Interparental Violence and Acceptance of Dating Violence as Predictors for Teen Dating Violence Victimization.

    Science.gov (United States)

    Karlsson, Marie E; Temple, Jeff R; Weston, Rebecca; Le, Vi Donna

    2016-04-01

    We examined the association between witnessing interparental violence, attitudes about dating violence, and physical and psychological teen dating violence (TDV) victimization. Participants were 918 teens with dating experience. Witnessing interparental violence and acceptance of dating violence were significant predictors of TDV victimization. Acceptance of dating violence was also a partial mediator between witnessing interparental violence and TDV victimization. Witnessing mother-to-father violence and acceptance of female-perpetrated violence were the most consistent predictors. TDV programs aiming to prevent victimization could benefit from targeting youth exposed to father-to-mother and mother-to-father violence, targeting attitudes about violence, and tailoring interventions to gender-specific risk factors.

  19. A nuclear data approach for the Hubble constant measurements

    Directory of Open Access Journals (Sweden)

    Pritychenko Boris

    2017-01-01

    Full Text Available An extraordinary number of Hubble constant measurements challenges physicists with selection of the best numerical value. The standard U.S. Nuclear Data Program (USNDP codes and procedures have been applied to resolve this issue. The nuclear data approach has produced the most probable or recommended Hubble constant value of 67.2(69 (km/sec/Mpc. This recommended value is based on the last 20 years of experimental research and includes contributions from different types of measurements. The present result implies (14.55 ± 1.51 × 109 years as a rough estimate for the age of the Universe. The complete list of recommended results is given and possible implications are discussed.

  20. A nuclear data approach for the Hubble constant measurements

    Science.gov (United States)

    Pritychenko, Boris

    2017-09-01

    An extraordinary number of Hubble constant measurements challenges physicists with selection of the best numerical value. The standard U.S. Nuclear Data Program (USNDP) codes and procedures have been applied to resolve this issue. The nuclear data approach has produced the most probable or recommended Hubble constant value of 67.2(69) (km/sec)/Mpc. This recommended value is based on the last 20 years of experimental research and includes contributions from different types of measurements. The present result implies (14.55 ± 1.51) × 109 years as a rough estimate for the age of the Universe. The complete list of recommended results is given and possible implications are discussed.

  1. A nuclear data approach for the Hubble constant measurements

    Energy Technology Data Exchange (ETDEWEB)

    Pritychenko, B. [Brookhaven National Laboratory (BNL), Upton, NY (United States)

    2015-06-09

    An extraordinary number of Hubble constant measurements challenges physicists with selection of the best numerical value. The standard U.S. Nuclear Data Program (USNDP) codes and procedures have been applied to resolve this issue. The nuclear data approach has produced the most probable or recommended Hubble constant value of 67.00(770) (km/sec)/Mpc. This recommended value is based on the last 25 years of experimental research and includes contributions from different types of measurements. The present result implies (14.6±1.7) x 109 years as a rough estimate for the age of the Universe. The complete list of recommended results is given and possible implications are discussed.

  2. A nuclear data approach for the Hubble constant measurements

    Energy Technology Data Exchange (ETDEWEB)

    Pritychenko, B. [Brookhaven National Laboratory (BNL), Upton, NY (United States)

    2015-06-09

    An extraordinary number of Hubble constant measurements challenges physicists with selection of the best numerical value. The standard U.S. Nuclear Data Program (USNDP) codes and procedures have been applied to resolve this issue. The nuclear data approach has produced the most probable or recommended Hubble constant value of 67.00(770) (km/sec)/Mpc. This recommended value is based on the last 25 years of experimental research and includes contributions from different types of measurements. The present result implies (14.6±1.7) x 109 years as a rough estimate for the age of the Universe. The complete list of recommended results is given and possible implications are discussed.

  3. HUBBLE PEEKS INTO A STELLAR NURSERY IN A NEARBY GALAXY

    Science.gov (United States)

    2002-01-01

    HUBBLE PEEKS INTO A STELLAR NURSERY IN A NEARBY GALAXY NASA's Hubble Space Telescope has peered deep into a neighboring galaxy to reveal details of the formation of new stars. Hubble's target was a newborn star cluster within the Small Magellanic Cloud, a small galaxy that is a satellite of our own Milky Way. The new images show young, brilliant stars cradled within a nebula, or glowing cloud of gas, cataloged as N 81. These massive, recently formed stars inside N 81 are losing material at a high rate, sending out strong stellar winds and shock waves and hollowing out a cocoon within the surrounding nebula. The two most luminous stars, seen in the Hubble image as a very close pair near the center of N 81, emit copious ultraviolet radiation, causing the nebula to glow through fluorescence. Outside the hot, glowing gas is cooler material consisting of hydrogen molecules and dust. Normally this material is invisible, but some of it can be seen in silhouette against the nebular background, as long dust lanes and a small, dark, elliptical-shaped knot. It is believed that the young stars have formed from this cold matter through gravitational contraction. Few features can be seen in N 81 from ground-based telescopes, earning it the informal nick-name 'The Blob.' Astronomers were not sure if just one or a few hot stars were embedded in the cloud, or if it was a stellar nursery containing a large number of less massive stars. Hubble's high-resolution imaging shows the latter to be the case, revealing that numerous young, white-hot stars---easily visible in the color picture---are contained within N 81. This crucial information bears strongly on theories of star formation, and N 81 offers a singular opportunity for a close-up look at the turbulent conditions accompanying the birth of massive stars. The brightest stars in the cluster have a luminosity equal to 300,000 stars like our own Sun. Astronomers are especially keen to study star formation in the Small Magellanic

  4. European astronaut selected for the third Hubble Space Telescope

    Science.gov (United States)

    1998-08-01

    The STS-104 crew will rendezvous with the orbiting Hubble Space Telescope, which is the size of a city bus, capture it using the Shuttle's Canadian robot arm and secure it in Columbia's payload bay. Then, working in teams of two, the four astronauts will leave the Shuttle's pressurised cabin and venture into the payload bay, performing a variety of tasks that will improve the productivity and reliability of the telescope. The four astronauts will perform a series of six "extravehicular" activities in the open space environment. Such activities are commonly called spacewalks, but this term does little justice to the considerable physical and mental efforts that astronauts need to make in doing the very demanding work involved. The Shuttle commander and pilot for this flight have not yet been appointed, but the four designated mission specialists begin training for the STS-104 mission immediately. "The ambitious nature of this mission, with its six spacewalks, made it important for the payload crew to begin training as early as possible," said David C. Leestma, NASA Director of Flight Crew Operations at the Johnson Space Center in Houston, to which Claude Nicollier is on resident assignment from ESA's European Astronaut Centre in Cologne, Germany, the home base of the European astronaut corps. The Hubble Space Telescope was launched into orbit in April 1990. It is one of the most capable optical telescopes available to astronomers today, producing images and spectral observations at the forefront of astronomy. The European Space Agency contributed a 15 share to the development of Hubble. One of the five scientific instruments on board, the Faint Object Camera, was built by a European industrial consortium made up of British Aerospace, Dornier and Matra under a contract with the European Space Agency. The solar arrays which provide Hubble with electrical power were manufactured by British Aerospace and Dornier. In its eight years of operation, the telescope has not

  5. Astrometry with Hubble Space Telescope Fine Guidance Sensors - A Review

    CERN Document Server

    Benedict, G Fritz; Nelan, Edmund P; Harrison, Thomas E

    2016-01-01

    Over the last 20 years Hubble Space Telescope Fine Guidance Sensor interferometric astrometry has produced precise and accurate parallaxes of astrophysical interesting stars and mass estimates for stellar companions. We review parallax results, and binary star and exoplanet mass determinations, and compare a subset of these parallaxes with preliminary Gaia results. The approach to single-field relative astrometry described herein may continue to have value for targets fainter than the Gaia limit in the coming era of 20-30m telescopes.

  6. Telescope simulators for Hubble - An overview of optical designs

    Science.gov (United States)

    Davilla, Pam; Wood, H. J.; Atcheson, Paul D.; Saunders, Renee; Sullivan, Joe; Vaughan, Arthur H.; Saisse, Michel

    1993-01-01

    This paper briefly describes optical design of the Hubble Space Telescope (HST) and overviews three optical design simulators for HST which have been proposed for use as verification tools to characterize the performance of second-generation instruments during ground testing. These simulators are: the Refractive Aberrated Simulator developed at Ball Aerospace, the Optical Simulator developed at Laboratoire Astronomie Spatiale, and the Jet Propulsion Laboratory Stimulus. Relative advantages and disadvantages of each optical configuration are discussed.

  7. Bayesian Approach to the Best Estimate of the Hubble Constant

    Institute of Scientific and Technical Information of China (English)

    王晓峰; 陈黎; 李宗伟

    2001-01-01

    A Bayesian approach is used to derive the probability distribution (PD) of the Hubble constant H0 from recent measurements including supernovae Ia, the Tully-Fisher relation, population Ⅱ and physical methods. The discrepancies among these PDs are briefly discussed. The combined value of all the measurements is obtained,with a 95% confidence interval of 58.7 < Ho < 67.3 (km·s-1.Mpc-1).

  8. Hubble Constant, Lensing, and Time Delay in Relativistic MOND

    OpenAIRE

    2012-01-01

    Time delay in galaxy gravitational lensing systems has been used to determine the value of Hubble constant. As in other dynamical phenomena at the scale of galaxy, dark matter is often invoked in gravitational lensing to account for the "missing mass" (the apparent discrepancy between the dynamical mass and the luminous mass). Alternatively, modified gravity can be used to explain the discrepancy. In this paper we adopt the Tensor-Vector-Scalar gravity (TeVeS), a relativistic version of MOdif...

  9. Type Ia supernova Hubble residuals and host-galaxy properties

    Energy Technology Data Exchange (ETDEWEB)

    Kim, A. G.; Aldering, G.; Aragon, C.; Bailey, S.; Fakhouri, H. K. [Physics Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720 (United States); Antilogus, P.; Bongard, S.; Canto, A.; Cellier-Holzem, F.; Fleury, M.; Guy, J. [Laboratoire de Physique Nucléaire et des Hautes Énergies, Université Pierre et Marie Curie Paris 6, Université Paris Diderot Paris 7, CNRS-IN2P3, 4 place Jussieu, F-75252 Paris Cedex 05 (France); Baltay, C. [Department of Physics, Yale University, New Haven, CT 06250-8121 (United States); Buton, C.; Feindt, U.; Greskovic, P.; Kowalski, M. [Physikalisches Institut, Universität Bonn, Nußallee 12, D-53115 Bonn (Germany); Childress, M. [Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611 (Australia); Chotard, N.; Copin, Y.; Gangler, E. [Université de Lyon, F-69622 Lyon (France); Université de Lyon 1, Villeurbanne (France); CNRS/IN2P3, Institut de Physique Nucléaire de Lyon (France); and others

    2014-03-20

    Kim et al. introduced a new methodology for determining peak-brightness absolute magnitudes of type Ia supernovae from multi-band light curves. We examine the relation between their parameterization of light curves and Hubble residuals, based on photometry synthesized from the Nearby Supernova Factory spectrophotometric time series, with global host-galaxy properties. The K13 Hubble residual step with host mass is 0.013 ± 0.031 mag for a supernova subsample with data coverage corresponding to the K13 training; at <<1σ, the step is not significant and lower than previous measurements. Relaxing the data coverage requirement of the Hubble residual step with the host mass is 0.045 ± 0.026 mag for the larger sample; a calculation using the modes of the distributions, less sensitive to outliers, yields a step of 0.019 mag. The analysis of this article uses K13 inferred luminosities, as distinguished from previous works that use magnitude corrections as a function of SALT2 color and stretch parameters: steps at >2σ significance are found in SALT2 Hubble residuals in samples split by the values of their K13 x(1) and x(2) light-curve parameters. x(1) affects the light-curve width and color around peak (similar to the Δm {sub 15} and stretch parameters), and x(2) affects colors, the near-UV light-curve width, and the light-curve decline 20-30 days after peak brightness. The novel light-curve analysis, increased parameter set, and magnitude corrections of K13 may be capturing features of SN Ia diversity arising from progenitor stellar evolution.

  10. Technicians assembly the Hubble Space Telescope (HST) mockup at JSC

    Science.gov (United States)

    1989-01-01

    At JSC's Mockup and Integration Laboratory (MAIL) Bldg 9A, technicians install a high gain antenna (HGA) on the Hubble Space Telescope (HST) mockup. On the ground a technician operates the controls for the overhead crane that is lifting the HGA into place on the Support System Module (SSM) forward shell. Others in a cherry picker basket wait for the HGA to near its final position so they can secure it on the mockup.

  11. The Hubble party balloon and the expanding universe

    Science.gov (United States)

    Zendri, G.; Rosi, T.; Oss, S.

    2016-09-01

    We show that the metaphor of the inflated balloon used to describe expanding space-time according to the Hubble law can be transformed into a simple laboratory experiment. We obtain, in terms of measured recession speeds and distances of ink dots drawn on a party balloon, easy renditions of various cosmological models, such as the static one and the Einstein-De Sitter universe.

  12. Type Ia Supernova Hubble Residuals and Host-Galaxy Properties

    Energy Technology Data Exchange (ETDEWEB)

    Nearby Supernova Factory; Kim, A. G.; Aldering, G.; Antilogus, P.; Aragon, C.; Bailey, S.; Baltay, C.; Bongard, S.; Buton, C.; Canto, A.; Cellier-Holzem, F.; Childress, M.; Chotard, N.; Copin, Y.; Fakhouri, H. K.; Feindt, U.; Fleury, M.; Gangler, E.; Greskovic, P.; Guy, J.; Kowalski, M.; Lombardo, S.; Nordin, J.; Nugent, P.; Pain, R.; Pecontal, E.; Pereira, R.; Perlmutter, S.; Rabinowitz, D.; Rigault, M.; Runge, K.; Saunders, C.; Scalzo, R.; Smadja, G.; Tao, C.; Thomas, R. C.; Weaver, B. A.

    2014-01-17

    Kim et al. (2013) [K13] introduced a new methodology for determining peak- brightness absolute magnitudes of type Ia supernovae from multi-band light curves. We examine the relation between their parameterization of light curves and Hubble residuals, based on photometry synthesized from the Nearby Supernova Factory spec- trophotometric time series, with global host-galaxy properties. The K13 Hubble residual step with host mass is 0.013 ? 0.031 mag for a supernova subsample with data coverage corresponding to the K13 training; at ? 1?, the step is not significant and lower than previous measurements. Relaxing the data coverage requirement the Hubble residual step with host mass is 0.045 ? 0.026 mag for the larger sample; a calculation using the modes of the distributions, less sensitive to outliers, yields a step of 0.019 mag. The analysis of this article uses K13 inferred luminosities, as distinguished from previous works that use magnitude corrections as a function of SALT2 color and stretch param- eters: Steps at> 2? significance are found in SALT2 Hubble residuals in samples split by the values of their K13 x(1) and x(2) light-curve parameters. x(1) affects the light- curve width and color around peak (similar to the∆m15 and stretch parameters), and x(2) affects colors, the near-UV light-curve width, and the light-curve decline 20 to 30 days after peak brightness. The novel light-curve analysis, increased parameter set, and magnitude corrections of K13 may be capturing features of SN Ia diversity arising from progenitor stellar evolution.

  13. Near-real-time trace element measurements in a rural, traffic-influenced environment with some fireworks

    Science.gov (United States)

    Furger, Markus; Slowik, Jay G.; Cruz Minguillón, María; Hueglin, Christoph; Koch, Chris; Prévôt, André S. H.; Baltensperger, Urs

    2016-04-01

    Aerosol-bound trace elements can affect the environment in significant ways especially when they are toxic. Characterizing the trace element spatial and temporal variability is a prerequisite for human exposure studies. The requirement for high time resolution and consequently the low sample masses asked for analysis methods not easily accessible, such as synchrotron radiation-induced X-ray fluorescence spectrometry (SR-XRF). In recent years, instrumentation that samples and analyzes airborne particulate matter with time resolutions of less than an hour in near real time has entered the market. We present the results of a three-week campaign in a rural environment close to a freeway. The measurement period included the fireworks of the Swiss National Day. The XRF instrument was set up at the monitoring station Härkingen of the Swiss Monitoring Network for Air Pollution (NABEL). It was configured to sample and analyze ambient PM10 aerosols in 1-hour intervals. Sample analysis with XRF was performed by the instrument immediately after collection, i.e. during the next sampling interval. 24 elements were analyzed and quantified (Si, S, Cl, K, Ca, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, As, Se, Cd, Sn, Sb, Ba, Pt, Hg, Pb, Bi). The element concentrations obtained by the XRF instrument were compared to those determined by ICP-AES and ICP-MS in PM10 samples collected by NABEL high volume samplers. The results demonstrate the capability of the instrument to measure over a wide range of concentrations, from a few ng m-3 to μg m-3, under ambient conditions. The time resolution allows for the characterization of diurnal variations of element concentrations, which provides information on the contribution of emission sources, such as road traffic, soil, or fireworks. Some elements (V, Co, As, Pt) were below their detection limit during most of the time, but As could be quantified during the fireworks. Transition metals Cr, Mn, Fe, Cu, Zn could be attributed to freeway traffic. K, S

  14. Hubble parameter in QCD Universe for finite bulk viscosity

    Energy Technology Data Exchange (ETDEWEB)

    Tawfik, A.; Wahba, M. [Egyptian Center for Theoretical Physics (ECTP), MTI University, Al Mukattam, Cairo 11212 (Egypt); Mansour, H. [Department of Physics, Cairo University, Giza (Egypt); Harko, T. [Department of Physics and Center for Theoretical and Computational Physics, The University of Hong Kong, Pok Fu Lam Road, Hong Kong (China)

    2010-12-01

    We consider the influence of the perturbative bulk viscosity on the evolution of the Hubble parameter in the QCD era of the early Universe. For the geometry of the Universe we assume the homogeneous and isotropic Friedmann-Lemaitre-Robertson-Walker metric, while the background matter is assumed to be characterized by barotropic equations of state, obtained from recent lattice QCD simulations, and heavy-ion collisions, respectively. Taking into account a perturbative form for the bulk viscosity coefficient, we obtain the evolution of the Hubble parameter, and we compare it with its evolution for an ideal (non-viscous) cosmological matter. A numerical solution for the viscous QCD plasma in the framework of the causal Israel-Stewart thermodynamics is also obtained. Both the perturbative approach and the numerical solution qualitatively agree in reproducing the viscous corrections to the Hubble parameter, which in the viscous case turns out to be slightly different as compared to the non-viscous case. Our results are strictly limited within a very narrow temperature- or time-interval in the QCD era, where the quark-gluon plasma is likely dominant. (Copyright copyright 2010 WILEY-VCH Verlag GmbH and Co. KGaA, Weinheim)

  15. A Toy Cosmology Using a Hubble-Scale Casimir Effect

    Directory of Open Access Journals (Sweden)

    Michael E. McCulloch

    2014-02-01

    Full Text Available The visible mass of the observable universe agrees with that needed for a flat cosmos, and the reason for this is not known. It is shown that this can be explained by modelling the Hubble volume as a black hole that emits Hawking radiation inwards, disallowing wavelengths that do not fit exactly into the Hubble diameter, since partial waves would allow an inference of what lies outside the horizon. This model of “horizon wave censorship” is equivalent to a Hubble-scale Casimir effect. This incomplete toy model is presented to stimulate discussion. It predicts a minimum mass and acceleration for the observable universe which are in agreement with the observed mass and acceleration, and predicts that the observable universe gains mass as it expands and was hotter in the past. It also predicts a suppression of variation on the largest cosmic scales that agrees with the low-l cosmic microwave background anomaly seen by the Planck satellite.

  16. How was the Hubble sequence 6 Gyrs ago?

    CERN Document Server

    Delgado-Serrano, R; Yang, Y B; Puech, M; Flores, H; Rodrigues, M

    2009-01-01

    The way galaxies assemble their mass to form the well-defined Hubble sequence is amongst the most debated topic in modern cosmology. One difficulty is to link distant galaxies to those at present epoch. We aim at establishing how were the galaxies of the Hubble sequence, 6 Gyrs ago. We intend to derive a past Hubble sequence that can be causally linked to the present-day one. We selected samples of nearby galaxies from the SDSS and of distant galaxies from the GOODS survey. We verified that each sample is representative of galaxies. We further showed that the observational conditions necessary to retrieve their morphological classification are similar in an unbiased way. Morphological analysis has been done in an identical way for all galaxies in the two samples. We found an absence of number evolution for elliptical and lenticular galaxies, which strikingly contrasts with the strong evolution of spiral and peculiar galaxies. Spiral galaxies were 2.3 times less abundant in the past, that is exactly compensate...

  17. The local Hubble flow a manifestation of dark energy

    CERN Document Server

    Baryshev, Yu V; Teerikorpi, P; Baryshev, Yurij; Chernin, Arthur; Teerikorpi, Pekka

    2000-01-01

    Our local environment at $r<10$ Mpc expands linearly and smoothly, as if ruled by a uniform matter distribution, while observations show the very clumpy local universe. This is a long standing enigma in cosmology. We argue that the recently discovered vacuum or quintessence (dark energy (DE) component with the equation of state $p_Q = w \\rho_Q c^2$, $w \\in [-1,0)$) from observations of the high-redshift universe may also manifest itself in the properties of the very local Hubble flow. We introduce the concept of the critical distance $r_Q$ where the repulsive force of dark energy starts to dominate over the gravity of a mass concentration. For the Local Group $r_Q$ is about 1.5 Mpc. Intriguingly, at the same distance 1.5 Mpc the linear and very "cold" Hubble flow emerges, with about the global Hubble constant. We also consider the critical epoch $t_Q$, when the DE antigravity began to dominate over the local matter gravity for a galaxy which at the present epoch is in the local DE dominated region. Our mai...

  18. Gravitational-wave cosmography with LISA and the Hubble tension

    Science.gov (United States)

    Kyutoku, Koutarou; Seto, Naoki

    2017-04-01

    We propose that stellar-mass binary black holes like GW150914 will become a tool to explore the local Universe within ˜100 Mpc in the era of the Laser Interferometer Space Antenna (LISA). High calibration accuracy and annual motion of LISA could enable us to localize up to ≈60 binaries more accurately than the error volume of ≈100 Mpc3 without electromagnetic counterparts under moderately optimistic assumptions. This accuracy will give us a fair chance to determine the host object solely by gravitational waves. By combining the luminosity distance extracted from gravitational waves with the cosmological redshift determined from the host, the local value of the Hubble parameter will be determined up to a few % without relying on the empirically constructed distance ladder. Gravitational-wave cosmography would pave the way for resolution of the disputed Hubble tension, where the local and global measurements disagree in the value of the Hubble parameter at 3.4 σ level, which amounts to ≈9 %.

  19. Type Ia Supernova Hubble Residuals and Host-Galaxy Properties

    CERN Document Server

    Kim, A G; Antilogus, P; Aragon, C; Bailey, S; Baltay, C; Bongard, S; Buton, C; Canto, A; Cellier-Holzem, F; Childress, M; Chotard, N; Copin, Y; Fakhouri, H K; Feindt, U; Fleury, M; Gangler, E; Greskovic, P; Guy, J; Kowalski, M; Lombardo, S; Nordin, J; Nugent, P; Pain, R; Pecontal, E; Pereira, R; Perlmutter, S; Rabinowitz, D; Rigault, M; Runge, K; Saunders, C; Scalzo, R; Smadja, G; Tao, C; Thomas, R C; Weaver, B A

    2014-01-01

    Kim et al. (2013) [K13] introduced a new methodology for determining peak-brightness absolute magnitudes of type Ia supernovae from multi-band light curves. We examine the relation between their parameterization of light curves and Hubble residuals, based on photometry synthesized from the Nearby Supernova Factory spectrophotometric time series, with global host-galaxy properties. The K13 Hubble residual step with host mass is $0.013\\pm 0.031$ mag for a supernova subsample with data coverage corresponding to the K13 training; at $\\ll 1\\sigma$, the step is not significant and lower than previous measurements. Relaxing the data coverage requirement the Hubble residual step with host mass is $0.045\\pm 0.026$ mag for the larger sample; a calculation using the modes of the distributions, less sensitive to outliers, yields a step of 0.019 mag. The analysis of this article uses K13 inferred luminosities, as distinguished from previous works that use magnitude corrections as a function of SALT2 color and stretch para...

  20. Observations of the Hubble Deep Field with the Infrared Space Observatory; 4, Association of sources with Hubble Deep Field Galaxies

    CERN Document Server

    Mann, B M

    1997-01-01

    We discuss the identification of sources detected by ISO at 6.7 and 15 micron in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming these results (and, in one case, clarifying them) with independent visual searches. We find fifteen ISO sources to be reliably associated with bright [I(AB) < 23] galaxies in the HDF, and one with an I(AB)=19.9 star, while a further eleven are associated with objects in the Hubble Flanking Fields (ten galaxies and one star). Amongst optically bright HDF galaxies, ISO tends to detect luminous, star-forming galaxies at fairly high redshift and with disturbed morphologies, in preference to nearby ellipticals.

  1. 76 FR 31851 - Safety Zone; Put-in-Bay Fireworks, Fox's the Dock Pier; South Bass Island, Put-in-Bay, OH

    Science.gov (United States)

    2011-06-02

    ... SECURITY Coast Guard 33 CFR Part 165 RIN 1625-AA00 Safety Zone; Put-in-Bay Fireworks, Fox's the Dock Pier; South Bass Island, Put-in-Bay, OH AGENCY: Coast Guard, DHS. ACTION: Temporary final rule. SUMMARY: The..., Put-in-Bay, Ohio. This Zone is intended to restrict vessels from portions of Lake Erie for the...

  2. Experience in working with volunteers as providers of support to victims and witnesses in victim and witness support departments at the courts

    Directory of Open Access Journals (Sweden)

    Hamer-Vidmar Nikica

    2015-01-01

    Full Text Available The aim of this paper is to present the results of a survey on the experience of engaging volunteers as providers of support for victims and witnesses in Victim and Witness Support Departments at the courts. The Independent Service for Victim and Witness Support in Ministry of Justice is responsible for the development of the victim and witness support system in Croatia. The Independent Service also coordinates the work of Victim and Witness Support Departments and develops and provides training programs and supervision for support officers and volunteers. A survey was conducted in order to determine volunteer motivation, assess the volunteers’ required qualities, their educational needs, the emotional impact arising from the work with victims and witnesses and the volunteers‘ assessment of the level of acceptance by court officials. In order to improve the level of safety of volunteers and the organization itself, the selection and educational processes for volunteers have been improved, according to both the experience achieved by working with volunteers and the results of the aforementioned survey. Engaging volunteers in the judicial system is a large step forward in the field of co-operation between the judiciary and the community.

  3. School Counseling Prevention and Intervention for Child Witnesses of Intimate Partner Violence

    Science.gov (United States)

    Buser, Juleen K.; Saponara, Erin

    2011-01-01

    Children who witness intimate partner violence (IPV) often suffer a range of physical, behavioral, emotional, and familial consequences (Holt, Buckley, & Whelan, 2008). School counselors may be in a key position to implement prevention programs around this issue, identify children who have witnessed IPV, and to engage in intervention efforts.…

  4. Women, Wit, and Witchcraft: The Burden of Stereotypes. Working Paper No. 193.

    Science.gov (United States)

    Levy, Barbara

    This paper examines the negative stereotypes so long foisted on witty women and the move of contemporary witty women writers into a comic vision beyond the imposed connection of female wit to sly cleverness and witchcraft. To illustrate how the woman writer had to cope with a prejudice against and a fear of her wit, the paper considers three…

  5. Child-Witnesses of Domestic Violence: The Evolution of a Counseling Group

    Science.gov (United States)

    Thompson, Elizabeth Heather

    2009-01-01

    A qualitative research design was used to explore the processes by which four child-witnesses of domestic violence made meaning of their experiences in a counseling group. A specific aim of this study was to determine if there were stages of group development that occurred in the counseling group with four young child-witnesses of domestic…

  6. Maternal Mortality and Serious Maternal Morbidity in Jehovah's Witnesses in The Netherlands EDITORIAL COMMENT

    NARCIS (Netherlands)

    Van Wolfswinkel, M. E.; Zwart, J. J.; Schutte, J. M.; Duvekot, J. J.; Pel, M.; Van Roosmalen, J.

    2009-01-01

    Refusal of blood by women with major obstetric hemorrhage who are Jehovah's witnesses increases their risk of maternal death. This retrospective study of case notes assessed the risk of maternal morbidity and mortality from major obstetric hemorrhage in Jehovah's witnesses. The data was obtained fro

  7. 40 CFR 209.21 - Primary discovery (exchange of witness lists and documents).

    Science.gov (United States)

    2010-07-01

    ... Act § 209.21 Primary discovery (exchange of witness lists and documents). (a) At a prehearing... 40 Protection of Environment 24 2010-07-01 2010-07-01 false Primary discovery (exchange of witness lists and documents). 209.21 Section 209.21 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY...

  8. Poor agreement among expert witnesses in bile duct injury malpractice litigation: an expert panel survey.

    NARCIS (Netherlands)

    Reuver, PR de; Dijkgraaf, M.G.; Gevers, S.K.; Gouma, D.J.; Bleichrodt, R.P.; Cuesta, M.A.; Erp, W.F. van; Gerritsen, J.; Hesselink, E.J.; Laarhoven, C.J.H.M. van; Lange, J. de; Obertop, H.; Stassen, L.P.; Terpstra, O.T.; Tilanus, H.W.; Vroonhoven, T.J.; Wit, L. de

    2008-01-01

    OBJECTIVE: To determine the inter-rater agreement of expert witness testimonies in bile duct injury malpractice litigation. BACKGROUND DATA: Malpractice litigation is an increasing concern in modern surgical practice. As most of the lawyers are not educated in medicine, expert witnesses are asked to

  9. 26 CFR 301.7602-1 - Examination of books and witnesses.

    Science.gov (United States)

    2010-04-01

    ... 26 Internal Revenue 18 2010-04-01 2010-04-01 false Examination of books and witnesses. 301.7602-1... Examination and Inspection § 301.7602-1 Examination of books and witnesses. (a) In general. For the purpose of... officer or employee of the Internal Revenue Service may examine any books, papers, records or other...

  10. Witnessing Domestic Abuse in Childhood as an Independent Risk Factor for Depressive Symptoms in Young Adulthood

    Science.gov (United States)

    Russell, David; Springer, Kristen W.; Greenfield, Emily A.

    2010-01-01

    Objective: This study addresses the relationship between retrospective reports of witnessing domestic abuse in childhood and levels of depressive symptoms in young adulthood. We examine whether the association between having witnessed violence in childhood and depression is independent of having been the direct target of sexual and/or physical…

  11. Maternal Mortality and Serious Maternal Morbidity in Jehovah's Witnesses in The Netherlands EDITORIAL COMMENT

    NARCIS (Netherlands)

    Van Wolfswinkel, M. E.; Zwart, J. J.; Schutte, J. M.; Duvekot, J. J.; Pel, M.; Van Roosmalen, J.

    2009-01-01

    Refusal of blood by women with major obstetric hemorrhage who are Jehovah's witnesses increases their risk of maternal death. This retrospective study of case notes assessed the risk of maternal morbidity and mortality from major obstetric hemorrhage in Jehovah's witnesses. The data was obtained

  12. 13 CFR 142.25 - Can a party or witness object to discovery?

    Science.gov (United States)

    2010-01-01

    ... 13 Business Credit and Assistance 1 2010-01-01 2010-01-01 false Can a party or witness object to discovery? 142.25 Section 142.25 Business Credit and Assistance SMALL BUSINESS ADMINISTRATION PROGRAM FRAUD CIVIL REMEDIES ACT REGULATIONS Hearing Provisions § 142.25 Can a party or witness object to...

  13. 13 CFR 142.29 - Are witness lists exchanged before the hearing?

    Science.gov (United States)

    2010-01-01

    ... 13 Business Credit and Assistance 1 2010-01-01 2010-01-01 false Are witness lists exchanged before the hearing? 142.29 Section 142.29 Business Credit and Assistance SMALL BUSINESS ADMINISTRATION PROGRAM FRAUD CIVIL REMEDIES ACT REGULATIONS Hearing Provisions § 142.29 Are witness lists...

  14. 28 CFR 21.4 - Fees and allowances of fact witnesses.

    Science.gov (United States)

    2010-07-01

    ... transportation expenses. A witness shall be entitled to transportation expenses based on the means of transportation reasonably utilized (based on the nature, duration, location and distance of travel) and the... single items costing more than $25. (4) First-class travel by witnesses requires the same...

  15. Aerosol composition and sources during the Chinese Spring Festival: fireworks, secondary aerosol, and holiday effects

    Science.gov (United States)

    Jiang, Q.; Sun, Y. L.; Wang, Z.; Yin, Y.

    2015-06-01

    Aerosol particles were characterized by an Aerodyne aerosol chemical speciation monitor along with various collocated instruments in Beijing, China, to investigate the role of fireworks (FW) and secondary aerosol in particulate pollution during the Chinese Spring Festival of 2013. Three FW events, exerting significant and short-term impacts on fine particles (PM2.5), were observed on the days of Lunar New Year, Lunar Fifth Day, and Lantern Festival. The FW were shown to have a large impact on non-refractory potassium, chloride, sulfate, and organics in submicron aerosol (PM1), of which FW organics appeared to be emitted mainly in secondary, with its mass spectrum resembling that of secondary organic aerosol (SOA). Pollution events (PEs) and clean periods (CPs) alternated routinely throughout the study. Secondary particulate matter (SPM = SOA + sulfate + nitrate + ammonium) dominated the total PM1 mass on average, accounting for 63-82% during nine PEs in this study. The elevated contributions of secondary species during PEs resulted in a higher mass extinction efficiency of PM1 (6.4 m2 g-1) than during CPs (4.4 m2 g-1). The Chinese Spring Festival also provides a unique opportunity to study the impact of reduced anthropogenic emissions on aerosol chemistry in the city. Primary species showed ubiquitous reductions during the holiday period with the largest reduction being in cooking organic aerosol (OA; 69%), in nitrogen monoxide (54%), and in coal combustion OA (28%). Secondary sulfate, however, remained only slightly changed, and the SOA and the total PM2.5 even slightly increased. Our results have significant implications for controlling local primary source emissions during PEs, e.g., cooking and traffic activities. Controlling these factors might have a limited effect on improving air quality in the megacity of Beijing, due to the dominance of SPM from regional transport in aerosol particle composition.

  16. Fireworks-Related Injuries in Iran: A Survey Following the 2014 New Year’s Festival in Tabriz

    Science.gov (United States)

    Shams Vahdati, Samad; Hemmate Gadim, Jamil; Mazouchian, Hossein

    2016-01-01

    Background Iranian people celebrate the last Wednesday eve of the year as Chaharshanbe Suri and use explosives and firecrackers as part of this festival. Objectives This study concerned fireworks injuries related to the Chaharshanbe Suri festival in Tabriz, a provincial capital in East Azerbaijan, Iran, to evaluate the epidemiology and provide data to prevent and manage these accidents. Patients and Methods This study was comprised of patients who were treated at the emergency department of Tabriz Sina hospital with burn injuries related to fireworks. The patients’ demographics, time of the accidents, locations of the burns, and the type of explosive were recorded. Descriptive statistics were used to analyze the data. Results Forty-nine patients were seen in the emergency department. The mean age was 17.16 ± 9.1, ranged from 3 to 36. Forty patients were male (81.6%) and 9 were female (18.4%). Twenty-one patients had second degree burns (47.7%), 10 patients had first degree burns (22.7%), 9 patients had third degree burns (20.5%), and 4 patients had first and second degree burns (9.1%). Conclusions The study shows that walking in the streets or driving with open windows can be dangerous in Iran during Charshanbe suri. PMID:27921014

  17. The impact of witnessing athletic injury: a qualitative examination of vicarious trauma in artistic gymnastics.

    Science.gov (United States)

    Day, Melissa C; Schubert, Nina

    2012-01-01

    We explored how athletes respond and cope after witnessing athletic injury in others participating in the same sport. Participants were eight competitive female artistic gymnasts aged 21-25 years. In the previous 3 years, participants had witnessed a serious athletic injury of another gymnast that had required hospital treatment. Participants took part in semi-structured interviews in which they were asked to discuss their experiences of witnessing injury, including descriptions of the injury's occurrence. Data were analysed using hierarchical content analysis. Following acute reactions to witnessing injury, participants reported experiencing intrusive cognitions and engaged in avoidance coping strategies. Participants reported gradually engaging in more approach coping strategies which served to lower their perceptions of vulnerability to injury. Despite the complex nature of trauma, suggestions may be made to assist applied sport psychologists working with athletes who have witnessed athletic injury.

  18. I-Witnessing; Reflections on Cosmopolitanism in Kigali

    Directory of Open Access Journals (Sweden)

    Hilary Yerbury

    2011-11-01

    Full Text Available Starting from the classic view of cosmopolitanism, this paper uses personal experiences gained during a six-week stay in Rwanda with a family affected by the genocide to explore the disjuncts which emerge in trying to understand the concept. In this process of exploration, it considers conceptions of the guest, the stranger and what Geertz terms the ‘cosmopolite’. Taking a reflexive position, it explores what it means to be a witness to events in someone else’s life, with a focus on post-genocide reconciliation that took place in the family in January and February 2011. In this context, it introduces the notions of cosmopolitan curiosity (Appiah and cosmopolitan tolerance (Beck and finds each of them affected by structural imbalances which render them potentially inadequate in practice. The paper concludes that, from a reflexive point of view, an understanding of cosmopolitanism is a work in progress, and that it is much more difficult to sustain as a lived reality than it is as an abstraction.

  19. The emotional child witness: effects on juror decision-making.

    Science.gov (United States)

    Cooper, Alexia; Quas, Jodi A; Cleveland, Kyndra C

    2014-01-01

    Despite wide variations in child witness behavior while on the stand, little research has focused on how that behavior influences jurors' perceptions of the child's credibility or the case itself. In the current study, the impact of a child's emotional displays on credibility judgments and verdict preferences was examined in jury-eligible college students and jurors released from jury duty. No significant differences emerged in perceptions or verdicts based on whether a child was shown as crying or not while participants read a transcript of the child's testimony. However, participants who rated the child as more emotional (regardless of whether the image showed a crying child) were more likely to render guilty verdicts, were more certain of guilt, and found the child more credible and the defendant less credible than participants who rated the child as less emotional. Also, when the child was perceived as low in emotion, older children were rated as less credible than younger children. The results have implications for understanding how children's emotional displays and jurors' perceptions of children's emotionality influence decisions in sexual abuse cases.

  20. The Problems of Expert Witness in Criminal Law

    Directory of Open Access Journals (Sweden)

    Rafiqa Qurrata A'yun

    2014-12-01

    Full Text Available The expert testimony is a potential problem in the future due to the impact of the advancement of science and technology. These progressions have an impact on the quality of the crime methods, thus it must be balanced with improving the quality and method of evidence evaluation that requires knowledge and expertise. This paper examines the place of expert witness to be considered as one of the evidence in criminal case investigation and criminal court. I argue that expert qualifications should be determined based on formal education, professional experiences, and the relevance of his expertise with the case. The Criminal Procedure Code (KUHAP does not restrict the necessary knowledge, so that the expert testimony about criminal law can also become evidence. However, as one of the evidence that can punish or relieve someone, a testimony stated by an expert should be neutral and objective. This objectivity should be based on scientific arguments, not based on the interests of the party who summoned him/her. This study is descriptive analytic using normative juridical literature and empirical data. It also uses the primary data through guided in-depth interview to the judges, public prosecutors, lawyers, and criminal law experts.

  1. Trauma and the state with Sigmund Freud as witness.

    Science.gov (United States)

    Danto, Elizabeth Ann

    Just before and after the end of World War I, Sigmund Freud took on an activist role and in his writings and speeches, redirected the concept of war trauma from individual failure to a larger issue of community responsibility. Testifying in Vienna as an expert witness for the state, Freud said that the military psychiatrists-not the soldiers-had "acted like machine guns behind the front" and were the "immediate cause of all war neurosis." Freud was called on by the legal community when Julius Wagner-Jauregg, a future Nobel Prize winner (and also future Nazi Party adherent), head of the municipal Clinic for Psychiatry and Nervous Diseases, was accused of the lethal use of electrotherapy on shell-shocked soldiers. As sociological as psychoanalytic in his responses, Freud's withering critique came just 2years after he avowed that "it is possible to foresee that the conscience of society will awake." That speech on the human right to mental health care affirmed Freud's alliance to the social democratic position and inspired the second generation of psychoanalysts to develop community-based clinics throughout Europe where treatment was free of cost, for war neurosis and beyond. Copyright © 2016 Elsevier Ltd. All rights reserved.

  2. Hypothetical constructs, hypothetical questions, and the expert witness.

    Science.gov (United States)

    Brodsky, Stanley L; Titcomb, Caroline; Sams, David M; Dickson, Kara; Benda, Yves

    2012-01-01

    Professor John Henry Wigmore in 1940 described the hypothetical question as an intolerable obstruction of truth. Since that time, the nature and application of the hypothetical question in the courtroom, as well as responses to this line of questioning during expert testimony, have been sources of controversy. Governed by legal philosophical foundations, the hypothetical construct addresses what there is, in a general sense, and what can or ought to be. Alexy (2004) has described the nature of legal philosophy as the epistemological question of what we can know. This article begins by examining the philosophical underpinnings, legal parameters, and teaching purposes of posing hypothetical queries. A social-psychological backdrop for the use of hypothetical questions is then discussed followed by a broader discussion of the hypothetical question's role in court procedures. This paper identifies hypothetical questions used in court as devices to elicit information, or as predictions that potentially change underlying factual interpretations of evidence. In particular, on cross examination hypothetical questions seek to make opposing experts assume facts that are incongruent with their conclusions or opinions. Sometimes in these situations, experts are led to re-evaluate opinions based on alternative understandings of events and behaviors. Thus, this paper's final aim is to explore a foundational understanding of hypothetical questions asked of expert witnesses with special reference to mental health issues. Options for responding to hypothetical questions on the stand are considered along the dimensions of assertiveness-passivity, compliance-resistance, and possible redefinitions of the hypothetical issues.

  3. Characteristics of drug users who witness many overdoses: implications for overdose prevention.

    Science.gov (United States)

    Bohnert, Amy S B; Tracy, Melissa; Galea, Sandro

    2012-01-01

    Programs to improve response of drug users when witnessing an overdose can reduce overdose mortality. Characteristics of drug users may be associated with the number of overdoses ever witnessed. This information could inform overdose prevention programs. Participants in New York City, who were age 18 and older with heroin and/or cocaine use in the past two months, were administered structured interviews (n=1184). Survey topics included overdose response, drug use behavior, treatment history, and demographic information. In a multivariable negative binomial regression model, those persons who were male (IRR [Incidence Rate Ratio]=1.7, CI [95% Confidence Interval]=1.4,2.2), had experienced homelessness (IRR=1.9, CI=1.4,2.6), had used heroin (IRR=2.0, CI=1.3,3.2), had overdosed themselves (IRR=1.9, CI=1.6,2.4), or had attended Narcotics Anonymous (IRR=1.3, CI=1.1,1.6) witnessed a greater count of overdoses in their lifetime. Those persons who have witnessed more overdoses were less likely to have sought medical assistance (OR [Odds Ratio]=0.7) and more likely to report counter-productive or ineffective actions (ORs between 1.9 and 2.4) at the last overdose they witnessed compared to persons who had only ever witnessed one or two overdoses. Persons at high risk for overdose are likely to witness more overdoses. Persons who had witnessed more overdoses were more likely to report taking ineffective action at the last overdose witnessed. Individuals who have witnessed many overdoses are likely key targets of overdose response training. Published by Elsevier Ireland Ltd.

  4. The Hubble constant from galaxy lenses: impacts of triaxiality and model degeneracies

    OpenAIRE

    2008-01-01

    The Hubble constant can be constrained using the time delays between multiple images of gravitationally lensed sources. In some notable cases, typical lensing analyses assuming isothermal galaxy density profiles produce low values for the Hubble constant, inconsistent with the result of the HST Key Project (72 +- 8 km/s/Mpc). Possible systematics in the values of the Hubble constant derived from galaxy lensing systems can result from a number of factors, e.g. neglect of environmental effects,...

  5. Hubble Views Ancient Storm in the Atmosphere of Jupiter - Montage

    Science.gov (United States)

    1999-01-01

    When 17th-century astronomers first turned their telescopes to Jupiter, they noted a conspicuous reddish spot on the giant planet. This Great Red Spot is still present in Jupiter's atmosphere, more than 300 years later. It is now known that it is a vast storm, spinning like a cyclone. Unlike a low-pressure hurricane in the Caribbean Sea, however, the Red Spot rotates in a counterclockwise direction in the southern hemisphere, showing that it is a high-pressure system. Winds inside this Jovian storm reach speeds of about 270 mph.The Red Spot is the largest known storm in the Solar System. With a diameter of 15,400 miles, it is almost twice the size of the entire Earth and one-sixth the diameter of Jupiter itself.The long lifetime of the Red Spot may be due to the fact that Jupiter is mainly a gaseous planet. It possibly has liquid layers, but lacks a solid surface, which would dissipate the storm's energy, much as happens when a hurricane makes landfall on the Earth. However, the Red Spot does change its shape, size, and color, sometimes dramatically. Such changes are demonstrated in high-resolution Wide Field and Planetary Cameras 1 & 2 images of Jupiter obtained by NASA's Hubble Space Telescope, and presented here by the Hubble Heritage Project team. The mosaic presents a series of pictures of the Red Spot obtained by Hubble between 1992 and 1999 (see PIA01594 thru PIA01599 and PIA02400 thru PIA02402 for individual images).Astronomers study weather phenomena on other planets in order to gain a greater understanding of our own Earth's climate. Lacking a solid surface, Jupiter provides us with a laboratory experiment for observing weather phenomena under very different conditions than those prevailing on Earth. This knowledge can also be applied to places in the Earth's atmosphere that are over deep oceans, making them more similar to Jupiter's deep atmosphere.

  6. Enhancing Science with the Hubble Legacy Archive (HLA)

    Science.gov (United States)

    Whitmore, Bradley C.

    2009-01-01

    The Space Telescope Science Institute (STScI), in collaboration with the Space Telescope - European Coordinating Facility (ST-ECF) and the Canadian Astronomy Data Centre (CADC), is developing an enhanced archive for the Hubble Space Telescope (HST). The goal of the HLA is to optimize the science coming from the Hubble Space Telescope by providing better browsing capabilities and easy access to both standard and enhanced Hubble products. Some of the primary enhancements include: 1) providing "real time" access to the data (i.e., having the data online), 2) adding a footprint service to make it easier to browse and download images, 3) providing more extensive "composite images" (e.g., stacked images, mosaics, color images etc.), 4) improving absolute astrometry (i.e., from 1-2" to 0.3"), 5) extracting spectra from slitless spectroscopic data (from ST-ECF), and 6) developing source lists for applicable datasets. The HLA entered its Data Release 2 (DR2) phase of operation in September, 2008. The highlight of DR2 is the inclusion of enhanced WFPC2 images produced by CADC. This more than triples the number of enhanced HLA images. In addition, the number of ACS source lists has more than tripled, with 70 % of the ACS images having both DAOphot and SExtractor lists. The HLA currently contains enhanced products for ACS, WFPC2, and NICMOS GRISM extractions (from ST-ECF), and provides access to standard products for NICMOS, STIS, FOS, and GHRS via MAST. Demonstrations will be provided at the Space Telescope Science Institute booth during the conference and people will have the opportunity to use the system interactively. The url is http://hla.stsci.edu .

  7. SPRINGTIME ON MARS: HUBBLE'S BEST VIEW OF THE RED PLANET

    Science.gov (United States)

    2002-01-01

    This NASA Hubble Space Telescope view of the planet Mars is the clearest picture ever taken from Earth, surpassed only by close-up shots sent back by visiting space probes. The picture was taken on February 25, 1995, when Mars was at a distance of approximately 65 million miles (103 million km) from Earth. Because it is spring in Mars' northern hemisphere, much of the carbon dioxide frost around the permanent water-ice cap has sublimated, and the cap has receded to a core of solid water-ice several hundred miles across. Towering 16 miles (25 km) above the surrounding plains, volcano Ascraeus Mons pokes above the cloud deck near the western or limb. This extinct volcano, measuring 250 miles (402 km) across, was discovered in the early 1970s by Mariner 9 spacecraft. Other key geologic features include (lower left) the Valles Marineris, an immense rift valley the length of the continental United States. Near the center of the disk lies the Chryse basin made up of cratered and chaotic terrain. The oval-looking Argyre impact basin (bottom), appears white due to clouds or frost. Seasonal winds carry dust to form striking linear features reminiscent of the legendary martian 'canals.' Many of these 'wind streaks' emanate from the bowl of these craters where dark coarse sand is swept out by winds. Hubble resolves several dozen impact craters down to 30-mile diameter. The dark areas, once misinterpreted as regions of vegetation by several early Mars watchers, are really areas of coarse sand that is less reflective than the finer, lighter dust. Seasonal changes in the surface appearance occur as winds move the dust and sand around. This picture was taken with Hubble's Wide Field Planetary Camera 2 in PC mode. The pictures were map-projected onto a sphere for accurate registration and perspective. Credit: Philip James (University of Toledo), Steven Lee (University of Colorado), NASA

  8. Direct Determination of Hubble Parameter Using Type IIn Supernovae

    CERN Document Server

    Blinnikov, Sergei; Baklanov, Petr; Dolgov, Alexander

    2012-01-01

    We introduce a novel approach, a Dense Shell Method (DSM), for measuring distances for cosmology. It is based on original Baade idea to relate absolute difference of photospheric radii with photospheric velocity. We demonstrate that this idea works: the new method does not rely on the Cosmic Distance Ladder and gives satisfactory results for the most luminous Type IIn Supernovae. This allows one to make them good primary distance indicators for cosmology. Fixing correction factors for illustration, we obtain with this method the median distance of 68^{+19}_{-15} (68%CL) Mpc to SN 2006gy and median Hubble parameter 79^{+23}_{-17} (68%CL) km/s/Mpc.

  9. Electrostatic Studies for the 2008 Hubble Service Repair Mission

    Science.gov (United States)

    Buhler, C. R.; Clements, J. S.; Calle, C. I.

    2012-01-01

    High vacuum triboelectric testing of space materials was required to identify possible Electrostatic Discharge (ESD) concerns for the astronauts in space during electronics board replacement on the Hubble Space Telescope. Testing under high vacuum conditions with common materials resulted in some interesting results. Many materials were able to charge to high levels which did not dissipate quickly even when grounded. Certain materials were able to charge up in contact with grounded metals while others were not. An interesting result was that like materials did not exchange electrostatic charge under high vacuum conditions. The most surprising experimental result is the lack of brush discharges from charged insulators under high vacuum conditions.

  10. 18 years of science with the Hubble Space Telescope.

    Science.gov (United States)

    Dalcanton, Julianne J

    2009-01-01

    After several decades of planning, the Hubble Space Telescope (HST) was launched in 1990 as the first of NASA's Great Observatories. After a rocky start arising from an error in the fabrication of its main mirror, it went on to change forever many fields of astronomy, and to capture the public's imagination with its images. An ongoing programme of servicing missions has kept the telescope on the cutting edge of astronomical research. Here I review the advances made possible by the HST over the past 18 years.

  11. Felinic principle and measurement of the Hubble parameter

    CERN Document Server

    Piškur, Yodovina

    2013-01-01

    Intelligent life can only appear in Universes, whose physical laws support sufficient complexity to make evolution of intelligent beings possible. Even inside those Universes, intelligent life does not appear randomly, but in parts with realized complexity, e.g. around stars in our Universe. As a consequence, the observational point of an intelligent observer cannot be assumed to be random and one must correct for this selection effect. In this paper we calculate how direct measurements of the Hubble parameter are affected when subject to the condition that they are observed from a Milky Way-like galaxy.

  12. Hubble Space Telescope spectroscopy of OB stars in M31

    Science.gov (United States)

    Hutchings, J. B.; Bianchi, L.; Lamers, H. J. G. L. M.; Massey, P.; Morris, S. C.

    1992-01-01

    We have obtained UV spectra of two luminous hot stars in M31 with the Hubble Space Telescope. The stars are of late O and WN spectral type and lie on opposite sides of M31. We derive UV extinction curves for M31 which differ from both the Galaxy and the LMC. We find differences between the IS absorbers in both lines of sight in M31 and in the Galactic halo. The stellar wind-driven mass loss of the stars is found to be 10 times lower than in similar Galactic stars. One star appears to be an eclipsing W-R binary.

  13. HUBBLE SPACE TELESCOPE Photometry of the Globular Cluster M4

    Science.gov (United States)

    Ibata, Rodrigo A.; Richer, Harvey B.; Fahlman, Gregory G.; Bolte, Michael; Bond, Howard E.; Hesser, James E.; Pryor, Carlton; Stetson, Peter B.

    1999-02-01

    This paper presents a detailed description of the acquisition and processing of a large body of imaging data for three fields in the globular cluster M4 taken with the Wide Field and Planetary Camera 2 aboard the Hubble Space Telescope. Analysis with the ALLFRAME package yielded the deepest photometry yet obtained for this cluster. The resulting data set for 4708 stars (positions and calibrated photometry in V, I, and, in two fields, U) spanning approximately six cluster core radii is presented. The scientific analysis is deferred to three companion papers, which investigate the significant white dwarf population discovered and the main-sequence population.

  14. The very local Hubble flow: computer simulations of dynamical history

    CERN Document Server

    Chernin, A D; Valtonen, M J; Dolgachev, V P; Domozhilova, L M; Makarov, D I

    2003-01-01

    The phenomenon of the very local ($\\le3$ Mpc) Hubble flow is studied on the basis of the data of recent precision observations. A set of computer simulations is performed to trace the trajectories of the flow galaxies back in time to the epoch of the formation of the Local Group. It is found that the `initial conditions' of the flow are drastically different from the linear velocity-distance relation. The simulations enable also to recognize the major trends of the flow evolution and identify the dynamical role of universal antigravity produced by cosmic vacuum.

  15. HUBBLE SPIES HUGE CLUSTERS OF STARS FORMED BY ANCIENT ENCOUNTER

    Science.gov (United States)

    2002-01-01

    NASA's Hubble Space Telescope snapped these two views of the heart of the galaxy M82. The image at left was taken in visible light; the picture at right, in infrared light. In the infrared view, the telescope's Near Infrared Camera and Multi-Object Spectrometer peered through thick dust lanes to find some of the galaxy's more than 100 super star clusters. The clusters are the larger pink and yellow dots scattered throughout the picture. They were formed during a violent collision with the galaxy M81 about 600 million years ago. The galaxy is 12 million light-years from Earth in the constellation Ursa Major. The pictures were taken Sept. 15, 1997. Credits: NASA, ESA, R. de Grijs (Institute of Astronomy, Cambridge, UK) NOTE TO EDITORS: For additional information, please contact Richard de Grijs, Institute of Astronomy, Cambridge University, Madingley Road, Cambridge CB3 0HA, UK, +44(0)1223-337528 (phone), +44(0)1223-337523 (fax), grijs@ast.cam.ac.uk (e-mail). The Space Telescope Science Institute (STScI) is operated by the Association of Universities for Research in Astronomy, Inc. (AURA), for NASA, under contract with the Goddard Space Flight Center, Greenbelt, MD. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency (ESA). This image is issued jointly by NASA and ESA. Electronic images, animation and additional information are available at: http://oposite.stsci.edu/pubinfo/pr/2001/08 and via links in http://oposite.stsci.edu/pubinfo/latest.html http://oposite.stsci.edu/pubinfo/pictures.html http://hubble.stsci.edu/go/news http://hubble.esa.int To receive STScI press releases electronically, send an Internet electronic mail message to public-request@stsci.edu. Leave the subject line blank, and type the word subscribe in the body of the message. The system will respond with a confirmation of the subscription, and you will receive new press releases as they are issued. Please subscribe using the email account

  16. Differences in posttraumatic stress reactions between witnesses and direct victims of motor vehicle accidents.

    Science.gov (United States)

    Tierens, Marlies; Bal, Sarah; Crombez, Geert; Loeys, Tom; Antrop, Inge; Deboutte, Dirk

    2012-06-01

    The present study describes posttraumatic stress reactions in young witnesses of motor vehicle accidents (MVAs). This study investigated (a) whether witnesses of MVAs report fewer trauma symptoms than direct victims, but more than adolescents who were never exposed to an MVA; and (b) whether individual differences in sex, negative appraisal, avoidant coping, and social support account for variability in trauma symptoms beyond status as a witness as compared to a victim. Self-report data came from a community-based sample of 3,007 adolescents with an average age of 14.6 years and comprising 53% boys. Compared to direct victims of an MVA in which someone was injured, witnesses of MVAs with injury reported significantly less internalizing symptoms, such as symptoms of posttraumatic stress (d = 0.25), fear (d = 0.21), and depression (d = 0.17). Compared to adolescents who were never exposed to an MVA with injury, witnesses reported significantly more externalizing symptoms (d = 0.24). In multiple regression analyses the significant difference between witnesses and victims disappeared when sex, other stressful events, appraisals, and coping were added to the model. These findings suggest that adolescent witnesses, as well as direct victims, may be at risk for posttraumatic reactions. Copyright © 2012 International Society for Traumatic Stress Studies.

  17. Evaluation of PADUA score as predictor of Warm Ischemia Time (WIT) during Laparoscopic Partial Nephrectomy (LPN).

    Science.gov (United States)

    Ricciardulli, Stefano; Ding, Qiang; Zhang, Xu; Li, Hongzhao; Wang, Baojun; Yang, Guoqiang; Wang, Xiyou; Zhang, Peng; Ma, Xin; Breda, Alberto

    2016-11-18

    To evaluate the efficacy of Preoperative Aspects and Dimension Used for an Anatomical (PADUA) classification in the prediction of Warm Ischemia Time (WIT) during Laparoscopic Partial Nephrectomy (LPN). Single centre retrospective study on 402 patients who underwent LPN between January 2011 and October 2013. WIT was correlated with each characteristics of the PADUA classification. Univariate and multivariate analysis were used to evaluated the independent predictive risk factors of WIT >20 minutes. The median WIT was 19.8 minutes (IQR 15-25). The PADUA risk groups (High vs Low: OR: 2.804; 95% CI 1.155-6.806; p-value <0.001; Intermediate vs Low: OR 0.971; 95% CI 0.185-5.092 p-value <0.001) and PADUA score as continuous variable (OR: 1.512; 95% CI 1.043-2.194; p-value <0.001) were the best independent risk factors of WIT >20 minutes. Another important factor related with WIT >20 minutes was a CKD stage 3 (p-value: 0.047; OR: 0.528; 95% CI:0.282-0.990). This study reveal that tumor' anatomical aspects may influence the WIT. The use of the nephrometry scoring systems should to be use by the surgeon in the planning of nephron sparing surgery (NSS) and should be considered for its inclusion in international guidelines.

  18. Cosmic variance and the measurement of the local Hubble parameter.

    Science.gov (United States)

    Marra, Valerio; Amendola, Luca; Sawicki, Ignacy; Valkenburg, Wessel

    2013-06-14

    There is an approximately 9% discrepancy, corresponding to 2.4 σ, between two independent constraints on the expansion rate of the Universe: one indirectly arising from the cosmic microwave background and baryon acoustic oscillations and one more directly obtained from local measurements of the relation between redshifts and distances to sources. We argue that by taking into account the local gravitational potential at the position of the observer this tension--strengthened by the recent Planck results--is partially relieved and the concordance of the Standard Model of cosmology increased. We estimate that measurements of the local Hubble constant are subject to a cosmic variance of about 2.4% (limiting the local sample to redshifts z > 0.010) or 1.3% (limiting it to z > 0.023), a more significant correction than that taken into account already. Nonetheless, we show that one would need a very rare fluctuation to fully explain the offset in the Hubble rates. If this tension is further strengthened, a cosmology beyond the Standard Model may prove necessary.

  19. Feasibility of Exoplanet Coronagraphy with the Hubble Space Telescope

    Science.gov (United States)

    Lyon, Richard G.; Woodruff, Robert A.; Brown, Robert; Noecker, M. Charley; Cheng, Edward

    2010-01-01

    Herein we report on a preliminary study to assess the use of the Hubble Space Telescope (HST) for the direct detection and spectroscopic characterization of exoplanets and debris disks - an application for which HST was not originally designed. Coronagraphic advances may enable the design of a science instrument that could achieve limiting contrasts approx.10deg beyond 275 milli-arcseconds (4 lambda/D at 800 nm) inner working angle, thereby enabling detection and characterization of several known jovian planets and imaging of debris disks. Advantages of using HST are that it already exists in orbit, it's primary mirror is thermally stable and it is the most characterized space telescope yet flown. However there is drift of the HST telescope, likely due to thermal effects crossing the terminator. The drift, however, is well characterized and consists of a larger deterministic components and a smaller stochastic component. It is the effect of this drift versus the sensing and control bandwidth of the instrument that would likely limit HST coronagraphic performance. Herein we discuss the science case, quantifY the limiting factors and assess the feasibility of using HST for exoplanet discovery using a hypothetical new instrument. Keywords: Hubble Space Telescope, coronagraphy, exoplanets, telescopes

  20. NASA's Hubble Space Telescope: Presentation to the Freedom Museum

    Science.gov (United States)

    Leete, Stephen

    2017-01-01

    The Freedom Museum, located in Manassas, VA, requested a speaker through the NASA Speakers Bureau, on the topic of the Hubble Space Telescope. A public outreach presentation has been prepared. Many of the facts are drawn from a public source, the Wikipedia article on the Hubble Space Telescope. This covers the history of the development of the HST, as well as the initial flaw and its repair, and the subsequent series of servicing missions, for which I was involved in the last three. This has been the topic of numerous books. This has been supplemented mostly by facts known to the author, such as names of individuals who played key roles, but not any technical information. Because the reqeustor asked for a significant part of the talk to address major science findings and discoveries, significant portions of a public presentation on this topic developed by Kenneth Carpenter of GSFC were obtained and incorporated, with credit. I have confirmed that this material is also available through public sources.

  1. ESA's new European Hubble Science Archive at ESAC

    Science.gov (United States)

    Baines, Deborah

    2015-12-01

    ESA's European Space Astronomy Centre (ESAC) has recently launched a new version of the European Hubble Space Telescope science archive. The new and enhanced archive offers several new features, some of which are not available anywhere else. The new web-based archive has been completely re-engineered and is now faster, more accurate and more robust than ever. Several of its unique features will be presented: the possibility of seeing the exact footprint of each observations on top of an optical all-sky image, the online visualization and inspection of FITS headers, imaging and spectral observation previews without downloading files or the possibility to search for data that has not yet been published in refereed journals. This state-of-the-art science data archive will be the new main access point to HST data for the European astronomical community and will be enhanced in the near-future to include the Hubble Source Catalogue or other high-level data products as required.

  2. Evolution of Cold Streams and Emergence of the Hubble Sequence

    CERN Document Server

    Cen, Renyue

    2014-01-01

    A new physical framework for the emergence of the Hubble sequence is outlined, based on novel analyses performed to quantify the evolution of cold streams of a large sample of galaxies from a state-of-the-art ultra-high resolution, large-scale adaptive mesh-refinement hydrodynamic simulation in a fully cosmological setting. It is found that the following three key physical variables of galactic cold inflows crossing the virial sphere substantially decrease with decreasing redshift: the number of streams N_{90} that make up 90% of concurrent inflow mass flux, average inflow rate per stream dot M_{90} and mean (mass flux weighted) gas density in the streams n_{gas}. Another key variable, the stream dimensionless angular momentum parameter lambda, instead is found to increase with decreasing redshift. Assimilating these trends and others leads naturally to a physically coherent scenario for the emergence of the Hubble sequence, including the following expectations: (1) the predominance of a mixture of disproport...

  3. The Hubble series: Convergence properties and redshift variables

    CERN Document Server

    Cattoen, Celine

    2007-01-01

    In cosmography, cosmokinetics, and cosmology it is quite common to encounter physical quantities expanded as a Taylor series in the cosmological redshift z. Perhaps the most well-known exemplar of this phenomenon is the Hubble relation between distance and redshift. However, we now have considerable high-z data available, for instance we have supernova data at least back to redshift z=1.75. This opens up the theoretical question as to whether or not the Hubble series (or more generally any series expansion based on the z-redshift) actually converges for large redshift? Based on a combination of mathematical and physical reasoning, we argue that the radius of convergence of any series expansion in z is less than or equal to 1, and that z-based expansions must break down for z>1, corresponding to a universe less than half its current size. Furthermore, we shall argue on theoretical grounds for the utility of an improved parameterization y=z/(1+z). In terms of the y-redshift we again argue that the radius of con...

  4. The Hubble series: convergence properties and redshift variables

    Energy Technology Data Exchange (ETDEWEB)

    Cattoen, Celine; Visser, Matt [School of Mathematics, Statistics, and Computer Science, Victoria University of Wellington, PO Box 600, Wellington (New Zealand)

    2007-12-07

    In cosmography, cosmokinetics and cosmology, it is quite common to encounter physical quantities expanded as a Taylor series in the cosmological redshift z. Perhaps the most well-known exemplar of this phenomenon is the Hubble relation between distance and redshift. However, we now have considerable high-z data available; for instance, we have supernova data at least back to redshift z {approx} 1.75. This opens up the theoretical question as to whether or not the Hubble series (or more generally any series expansion based on the z-redshift) actually converges for large redshift. Based on a combination of mathematical and physical reasonings, we argue that the radius of convergence of any series expansion in z is less than or equal to 1, and that z-based expansions must break down for z > 1, corresponding to a universe less than half of its current size. Furthermore, we shall argue on theoretical grounds for the utility of an improved parametrization y = z/(1 + z). In terms of the y-redshift, we again argue that the radius of convergence of any series expansion in y is less than or equal to 1, so that y-based expansions are likely to be good all the way back to the big bang (y = 1), but that y-based expansions must break down for y < -1, now corresponding to a universe more than twice its current size.

  5. The Hubble Space Telescope Education and Public Outreach Program

    Science.gov (United States)

    Teays, T. J.; Eisenhamer, B.; Eisenhamer, J.; Amazing Space Team

    2001-05-01

    The Hubble Space Telescope has conducted a long-standing and vigorous program in education and public outreach. This program uses a variety of methods to reach a broad spectrum of audiences. Education products are developed in a team environment that partners educators, curriculum experts, scientists, and production experts, such as graphic artists, Web designers, programmers, and education evaluators. A popular Web site is maintained, and has been substantially augmented in the past year. The Amazing Space program consists of a suite of online, interactive modules for use in the kindergarten through 12th grade classroom. The program is rooted in the national education standards and benefits from a robust evaluation process. The HST images and data are used to engage students in learning basic science and mathematics concepts. The activity/lessons include extensive, online assistance for educators, so that they can be readily used in the classroom. Hardcopy products such as posters, lithographs, teacher guides, and trading cards are generally tied to online products, to provide multiple entries to the material. We also provide training for teachers in the use of our products, as appropriate. Informal science education is supported by providing services to museums, planetariums, libraries and related institutions. The very popular ViewSpace, a computer-based video service is being used by many informal science facilities. In addition, HST has supported the creation of both permanent and traveling exhibits about HST. The Space Telescope Science Institute operates the Hubble Space Telescope for NASA.

  6. Radio Emission from Galaxies In The Hubble Deep Field

    CERN Document Server

    Richards, E A; Fomalont, E B; Windhorst, R A; Partridge, R B

    1998-01-01

    We report on sensitive radio observations made with the VLA at 8.5 GHz, centered on the Hubble Deep Field (HDF). We collected data in the A, CnB, C, DnC, and D configurations, corresponding to angular resolutions ranging from 0.3" to 10". We detected 29 radio sources in a complete sample within 4.6' of the HDF center and above a flux density limit of 9.0 microjy (5 sigma). Seven of these sources are located within the HDF itself, while the remaining 22 sources are covered by the Hubble Flanking Fields (HFFs) or ground based optical images. All of the sources in the HDF are identified with galaxies with a mean magnitude R = 21.7, while the mean magnitude of the identifications outside the HDF is R = 22.1. Three radio sources have no optical counterparts to R = 27. Based on a radio and optical positional coincidence, we detected an additional 19 radio sources in this field (seven of which are contained in the HDF) with 6.3 microjy < S < 9.0 (3.5 sigma < S < 5 sigma) and and R < 25, but which are ...

  7. Relationship between Hubble type and spectroscopic class in local galaxies

    CERN Document Server

    Almeida, J Sanchez; Munoz-Tunon, C; Huertas-Company, M

    2011-01-01

    We compare the Hubble type and the spectroscopic class of the galaxies with spectra in SDSS/DR7. As it is long known, elliptical galaxies tend to be red whereas spiral galaxies tend to be blue, however, this relationship presents a large scatter, which we measure and quantify in detail. We compare the Automatic Spectroscopic K-means based classification (ASK) with most of the commonly used morphological classifications. All of them provide consistent results. Given a spectral class, the morphological type wavers with a standard deviation between 2 and 3 T types, and the same large dispersion characterizes the variability of spectral classes fixed the morphological type. The distributions of Hubble types given an ASK class are very skewed -- they present long tails that go to the late morphological types for the red galaxies, and to the early morphological types for the blue spectroscopic classes. The scatter is not produced by problems in the classification, and it remains when particular subsets are consider...

  8. Towards a Cosmological Hubble Diagram for Type II-PSupernovae

    Energy Technology Data Exchange (ETDEWEB)

    Nugent, Peter; Sullivan, Mark; Ellis, Richard; Gal-Yam, Avishay; Leonard, Douglas C.; Howell, D. Andrew; Astier, Pierre; Carlberg, RaymondG.; Conley, Alex; Fabbro, Sebastien; Fouchez, Dominique; Neill, James D.; Pain, Reynald; Perrett, Kathy; Pritchet, Chris J; Regnault, Nicolas

    2006-03-20

    We present the first high-redshift Hubble diagram for Type II-P supernovae (SNe II-P) based upon five events at redshift upto z {approx}0.3. This diagram was constructed using photometry from the Canada-France-Hawaii Telescope Supernova Legacy Survey and absorption line spectroscopy from the Keck observatory. The method used to measure distances to these supernovae is based on recent work by Hamuy&Pinto (2002) and exploits a correlation between the absolute brightness of SNeII-P and the expansion velocities derived from the minimum of the Fe II 516.9 nm P-Cygni feature observed during the plateau phases. We present three refinements to this method which significantly improve the practicality of measuring the distances of SNe II-P at cosmologically interesting redshifts. These are an extinction correction measurement based on the V-I colors at day 50, across-correlation measurement for the expansion velocity and the ability to extrapolate such velocities accurately over almost the entire plateau phase. We apply this revised method to our dataset of high-redshift SNe II-P and find that the resulting Hubble diagram has a scatter of only 0.26 magnitudes, thus demonstrating the feasibility of measuring the expansion history, with present facilities, using a method independent of that based upon supernovae of Type Ia.

  9. Constraining The Hubble Parameter Using Distance Modulus - Redshift Relation

    CERN Document Server

    Onuchukwu, C C

    2015-01-01

    Using the relation between distance modulus (m-M) and redshift (z), deduced from Friedman-Robertson-Walker (FRW) metric and assuming different values of deceleration parameter (q0). We constrained the Hubble parameter (h). The estimates of the Hubble parameters we obtained using the median values of the data obtained from NASA Extragalactic Database (NED), are: h=0.7+/-0.3 for q0=0, h=0.6+/-0.3, for q0=1 and h=0.8+/-0.3, for q0=-1. The corresponding age ({\\tau}) and size (R) of the observable universe were also estimated as: {\\tau}=15+/-1 Gyrs, R=(5+/-2)x10^3 Mpc, {\\tau}=18+/-1 Gyrs, R=(6+/-2)x10^3 Mpc and {\\tau}=13+/-1 Gyrs, R=(4+/-2)x10^3 Mpc for q0=0, q0=1 and q0=-1 respectively.

  10. Determining the Hubble constant using HII regions and HII galaxies

    CERN Document Server

    Chavez, Ricardo; Terlevich, Roberto; Plionis, Manolis; Bresolin, Fabio; Basilakos, Spyros; Melnick, Jorge

    2012-01-01

    We report the first results of a long term program aiming to provide accurate independent estimates of the Hubble constant (H0) and the Dark Energy equation of state parameter (w) using the L(Hbeta)-velocity dispersion (sigma) distance estimator for Giant HII regions and HII galaxies. We have used VLT and Subaru high dispersion spectroscopic observations of a local sample of HII galaxies, identified in the SDSS DR7 catalogue in order to re-define and improve the L(Hbeta) - sigma distance indicator and to determine the Hubble constant. To this end we used as local calibration or 'anchor' of this correlation, giant HII regions in nearby galaxies which have accurate distance measurements determined via primary indicators. Using our best sample of 89 nearby HII galaxies and 23 Giant HII regions in 9 galaxies we obtain H0 = 73.9+- 2.7 (statistical)+- 2.9 (systematic) km s-1 Mpc-1, in excellent agreement with, and independently confirming, the most recent SNe Ia based results.

  11. Galaxies at z > 1: Shaping the Hubble sequence

    CERN Document Server

    Talia, M; Mignoli, M; Pozzetti, L; Renzini, A; Kurk, J; Halliday, C

    2013-01-01

    We investigate the morphological properties of 494 galaxies at z>1 from the GMASS survey, in their optical rest-frame, using HST/WFC3-IR images from CANDELS. The fractions of ellipticals and disks decline between z=1 to z=3, while at higher z the galaxy population is dominated by irregulars. Ellipticals have the highest concentration and Gini values, while irregulars assume the lowest ones. However, at 1Hubble types as they are at low z. No significant morphological k-correction was found to be required for the Hubble type classification. From a quantitative point of view, however, there are some differences between the optical and UV morphologies. Different morphological types occupy the two peaks of the (U-B) colour distribution: the majority of irregulars are found in the blue peak, while ellipticals mainly populate the red one. Disks have a smoother colour distribution. We also found that, in an UVJ diagram, the quie...

  12. Let's not, and say we would: imagined and actual responses to witnessing homophobia.

    Science.gov (United States)

    Crosby, Jennifer Randall; Wilson, Johannes

    2015-01-01

    We compared imagined versus actual affective and behavioral responses to witnessing a homophobic slur. Participants (N = 72) witnessed a confederate using a homophobic slur, imagined the same scenario, or were not exposed to the slur. Those who imagined hearing the slur reported significantly higher levels of negative affect than those who actually witnessed the slur, and nearly one half of them reported that they would confront the slur, whereas no participants who actually heard the slur confronted it. These findings reveal a discrepancy between imagined and real responses to homophobic remarks, and they have implications for the likelihood that heterosexuals will actually confront homophobic remarks.

  13. Of puppets and puppeteers: the role of the expert witness in a criminal prosecution in Canada.

    Science.gov (United States)

    Manarin, B

    1999-01-01

    This article explores the issue of reciprocal disclosure of expert evidence in Canada and the attendant responsibility of the expert witness to remain true to his or her own science. Two recent recommendations made to the government of Ontario in this regard are closely scrutinized. The author is critical of those who advocate the concealment of the existence of an expert witness until the last possible moment at trial and of those experts who are content to lie in wait. Additionally, the role of the expert witness in a criminal prosecution is examined to see if standard retainer agreements tend to stifle the quest for the truth.

  14. Jehovah's Witness parents' refusal of blood transfusions: Ethical considerations for psychologists.

    Science.gov (United States)

    Hoffman, Anna

    2016-08-01

    Psychologists in medical settings may be confronted with Jehovah's Witness parents refusing blood transfusions for their children as an ethical dilemma. The purpose of this discussion is to help psychologists provide informed, ethical consultations and support by investigating the values of the Jehovah's Witness community and the origin of the blood transfusion taboo, how medical and legal professionals have approached this dilemma, exploring relevant ethical principles and standards for psychologists, and suggestions for how to move toward a better understanding of harm with Jehovah's Witness families.

  15. European astronomers' successes with the Hubble Space Telescope*

    Science.gov (United States)

    1997-02-01

    [Figure: Laguna Nebula] Their work spans all aspects of astronomy, from the planets to the most distant galaxies and quasars, and the following examples are just a few European highlights from Hubble's second phase, 1994-96. A scarcity of midget stars Stars less massive and fainter than the Sun are much numerous in the Milky Way Galaxy than the big bright stars that catch the eye. Guido De Marchi and Francesco Paresce of the European Southern Observatory as Garching, Germany, have counted them. With the wide-field WFPC2 camera, they have taken sample censuses within six globular clusters, which are large gatherings of stars orbiting independently in the Galaxy. In every case they find that the commonest stars have an output of light that is only one-hundredth of the Sun's. They are ten times more numerous than stars like the Sun. More significant for theories of the Universe is a scarcity of very faint stars. Some astronomers have suggested that vast numbers of such stars could account for the mysterious dark matter, which makes stars and galaxies move about more rapidly than expected from the mass of visible matter. But that would require an ever-growing count of objects at low brightnesses, and De Marchi and Paresce find the opposite to be the case -- the numbers diminish. There may be a minimum size below which Nature finds starmaking difficult. The few examples of very small stars seen so far by astronomers may be, not the heralds of a multitude of dark-matter stars, but rareties. Unchanging habits in starmaking Confirmation that very small stars are scarce comes from Gerry Gilmore of the Institute of Astronomy in Cambridge (UK). He leads a European team that analyses long-exposure images in the WFPC2 camera, obtained as a by-product when another instrument is examining a selected object. The result is an almost random sample of well-observed stars and galaxies. The most remarkable general conclusion is that the make-up of stellar populations never seems to

  16. Nuclei of nearby disk galaxies .1. A Hubble Space Telescope imaging survey

    NARCIS (Netherlands)

    Phillips, AC; Illingworth, GD; MacKenty, JW; Franx, M

    We present deconvolved images of the central regions of 20 nearby disk galaxies, obtained with the original Planetary Camera of the Hubble Space Telescope. The galaxies span a range in Hubble type from SO to Sm. We have measured surface brightness profiles, and inverted these to estimate

  17. Galaxy Zoo Hubble: Crowdsourced Morphologies for 169,944 Galaxies at 0

    Science.gov (United States)

    Willett, Kyle; Galloway, Melanie; Fortson, Lucy; Bamford, Steven; Masters, Karen; Lintott, Chris; Simmons, Brooke; Cheung, Edmond; Schawinski, Kevin; Scarlata, Claudia; Beck, Melanie; Galaxy Zoo volunteers

    2016-01-01

    The Galaxy Zoo project uses crowdsourced visual classifications to create large and statistically robust catalogs of detailed galaxy morphology. We present initial results for the Galaxy Zoo: Hubble dataset, which includes 169,944 images of galaxies selected from the AEGIS, COSMOS, GEMS, and GOODS surveys. The galaxies span a redshift range of 0Zoo: Hubble catalog.

  18. Transitional Justice: History-Telling, Collective Memory, and the Victim-Witness

    National Research Council Canada - National Science Library

    Chrisje Brants; Katrien Klep

    2013-01-01

    .... It explores tensions between history-telling and the normative goals of truth commissions and international criminal courts, taking into account the increasing importance attributed to victims as witnesses of history...

  19. A Bermuda Triangle? Balancing protection, participation and proof in criminal proceedings affecting child victims and witnesses

    National Research Council Canada - National Science Library

    Beijer, A; Liefaard, T

    2011-01-01

    .... It adds a new dimension to the existing and already problematic balance between the protection of the child victim and witness on the one hand and the fairness of the criminal proceedings on the other...

  20. Cross sectional survey of perpetrators, victims, and witnesses of violence in Bogotá, Colombia

    OpenAIRE

    Duque, L.; Klevens, J; Ramirez, C.

    2003-01-01

    Objectives: To establish the prevalence and distribution of witnesses, victims, and perpetrators of different types of violence in the general population and the proportion of victims consulting health services or reporting the incident to authorities.