American Astronomical Society 2014 Annual Report
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Asian Nobel Prize' for Mapping the Universe 27 May 2010
Scientists win 'Asian Nobel Prize' for mapping the universe 27 May 2010 Three US scientists whose work helped map the category. universe are among the recipients of the one- million-US-dollar Shaw Prize, known as the "Asian (c) 2010 AFP Nobel," the competition's organisers said Thursday. Princeton University professors Lyman Page and David Spergel and Charles Bennett of Johns Hopkins University, won the award for an experiment that helped to determine the "geometry, age and composition of the universe to unprecedented precision." The trio will share the Shaw Prize's award for astronomy, with one-million-US-dollar prizes also awarded in the categories for mathematical sciences and life sciences and medicine. The University of California's David Julius won the award for life sciences and medicine for his "seminal discoveries" of how the skin senses pain and temperature, the organisers' statement said. "(Julius's) work has provided insights into fundamental mechanisms underlying the sense of touch as well as knowledge that opens the door to rational drug design for the treatment of chronic pain," the statement said. Princeton's Jean Bourgain won an award for his "profound work" in mathematical sciences, it said. The Shaw Prize, funded by Hong Kong film producer and philanthropist Run Run Shaw and first awarded in 2004, honours exceptional contributions "to the advancement of civilization and the well-being of humankind." The awards will be presented at a ceremony in Hong Kong on September 28. Last year, two scientists whose work challenged the assumption that obesity is caused by a lack of will power won the life sciences and medicine 1 / 2 APA citation: Scientists win 'Asian Nobel Prize' for mapping the universe (2010, May 27) retrieved 27 September 2021 from https://phys.org/news/2010-05-scientists-asian-nobel-prize-universe.html This document is subject to copyright. -
Professor Peter Goldreich Member of the Board of Adjudicators Chairman of the Selection Committee for the Prize in Astronomy
The Shaw Prize The Shaw Prize is an international award to honour individuals who are currently active in their respective fields and who have recently achieved distinguished and significant advances, who have made outstanding contributions in academic and scientific research or applications, or who in other domains have achieved excellence. The award is dedicated to furthering societal progress, enhancing quality of life, and enriching humanity’s spiritual civilization. Preference is to be given to individuals whose significant work was recently achieved and who are currently active in their respective fields. Founder's Biographical Note The Shaw Prize was established under the auspices of Mr Run Run Shaw. Mr Shaw, born in China in 1907, was a native of Ningbo County, Zhejiang Province. He joined his brother’s film company in China in the 1920s. During the 1950s he founded the film company Shaw Brothers (HK) Limited in Hong Kong. He was one of the founding members of Television Broadcasts Limited launched in Hong Kong in 1967. Mr Shaw also founded two charities, The Shaw Foundation Hong Kong and The Sir Run Run Shaw Charitable Trust, both dedicated to the promotion of education, scientific and technological research, medical and welfare services, and culture and the arts. ~ 1 ~ Message from the Chief Executive I warmly congratulate the six Shaw Laureates of 2014. Established in 2002 under the auspices of Mr Run Run Shaw, the Shaw Prize is a highly prestigious recognition of the role that scientists play in shaping the development of a modern world. Since the first award in 2004, 54 leading international scientists have been honoured for their ground-breaking discoveries which have expanded the frontiers of human knowledge and made significant contributions to humankind. -
David Spergel Is the Director of the Center for Computational Astrophysics and the Charles Young Professor of Astronomy at Princeton University
David Spergel is the director of the Center for Computational Astrophysics and the Charles Young Professor of Astronomy at Princeton University. He is the former chair of the Space Studies Board. Using microwave background observations from the Wilkinson Microwave Anisotropy Probe (WMAP) and the Atacama Cosmology Telescope, Spergel has measured the age, shape and composition of the universe. These observations have played a significant role in establishing the standard model of cosmology. He is one of the leaders of the Simons Observatory, which will include a planned millimeter-wave telescope that will allow us to take the next step in studying the microwave sky and probing the history of the universe. Spergel is currently co-chair of the Wide Field Infrared Survey Telescope (WFIRST) science team. WFIRST will study the nature of dark energy, complete the demographic survey of extrasolar planets, characterize the atmospheres of nearby planets and survey the universe with more than 100 times the field of view of the Hubble Space Telescope. Spergel has played a significant role in designing the coronagraph and in shaping the overall mission. Since completing my Ph.D. work, Spergel has been interested in using laboratory experiments and astronomical observations to probe the nature of dark matter and look for new physics. Recently, Spergel has been active in the exploration of data from the Gaia satellite and observations made by Subaru’s Hyper Suprime-Cam. Spergel serves as co-chair of the Global Coordination of Ground and Space Astrophysics working group of the International Astronomical Union. At Princeton, Spergel was department chair for a decade. -
Stsci Newsletter: 2011 Volume 028 Issue 02
National Aeronautics and Space Administration Interacting Galaxies UGC 1810 and UGC 1813 Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) 2011 VOL 28 ISSUE 02 NEWSLETTER Space Telescope Science Institute We received a total of 1,007 proposals, after accounting for duplications Hubble Cycle 19 and withdrawals. Review process Proposal Selection Members of the international astronomical community review Hubble propos- als. Grouped in panels organized by science category, each panel has one or more “mirror” panels to enable transfer of proposals in order to avoid conflicts. In Cycle 19, the panels were divided into the categories of Planets, Stars, Stellar Rachel Somerville, [email protected], Claus Leitherer, [email protected], & Brett Populations and Interstellar Medium (ISM), Galaxies, Active Galactic Nuclei and Blacker, [email protected] the Inter-Galactic Medium (AGN/IGM), and Cosmology, for a total of 14 panels. One of these panels reviewed Regular Guest Observer, Archival, Theory, and Chronology SNAP proposals. The panel chairs also serve as members of the Time Allocation Committee hen the Cycle 19 Call for Proposals was released in December 2010, (TAC), which reviews Large and Archival Legacy proposals. In addition, there Hubble had already seen a full cycle of operation with the newly are three at-large TAC members, whose broad expertise allows them to review installed and repaired instruments calibrated and characterized. W proposals as needed, and to advise panels if the panelists feel they do not have The Advanced Camera for Surveys (ACS), Cosmic Origins Spectrograph (COS), the expertise to review a certain proposal. Fine Guidance Sensor (FGS), Space Telescope Imaging Spectrograph (STIS), and The process of selecting the panelists begins with the selection of the TAC Chair, Wide Field Camera 3 (WFC3) were all close to nominal operation and were avail- about six months prior to the proposal deadline. -
MATTERS of GRAVITY Contents Editor
MATTERS OF GRAVITY The newsletter of the Topical Group on Gravitation of the American Physical Society Number 17 Spring 2001 Contents APS TGG News: APS Prize on gravitation, by Clifford Will .................. 3 TGG Elections, by David Garfinkle ...................... 3 We hear that, by Jorge Pullin ......................... 3 Research Briefs: Experimental Unruh Radiation?, by Matt Visser ............... 4 Why is the Universe accelerating?, by Beverly Berger ............ 6 The Lazarus Project, by Richard Price .................... 9 LIGO locks its first detector!, by Stan Whitcomb ............... 12 Progress on the nonlinear r-mode problem, by Keith Lockitch ........ 13 Conference Reports Analog Models of General Relativity, by Matt Visser ............. 17 Astrophysical Sources of Gravitational radiation, by Joan Centrella ..... 19 Numerical relativity at the 20th Texas meeting, by Pablo Laguna ...... 21 Editor Jorge Pullin Center for Gravitational Physics and Geometry The Pennsylvania State University University Park, PA 16802-6300 Fax: (814)863-9608 Phone (814)863-9597 Internet: [email protected] WWW: http://www.phys.psu.edu/~pullin ISSN: 1527-3431 1 Editorial Not much to report here. If you are burning to have Matters of Gravity with you all the time, the newsletter is now available for Palm Pilots, Palm PC's and web-enabled cell phones as an Avantgo channel. Check out http://www.avantgo.com under technology science. The next newsletter is due September 1st. If everything goes well this newsletter should! be available in the gr-qc Los Alamos archives (http://xxx.lanl.gov) under number gr-qc/yymmnnn. To retrieve it send email to [email protected] with Subject: get yymmnnn (numbers 2-16 are also available in gr-qc). -
Durham E-Theses
Durham E-Theses Probing the nature of dark matter with small-scale cosmology: A new estimate of the satellite galaxy complement of the Milky Way NEWTON, OLIVER,JAMES How to cite: NEWTON, OLIVER,JAMES (2019) Probing the nature of dark matter with small-scale cosmology: A new estimate of the satellite galaxy complement of the Milky Way, Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/13312/ Use policy This work is licensed under a Creative Commons Attribution Share Alike 3.0 (CC BY-SA) Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk 2 Probing the nature of dark matter with small-scale cosmology A new estimate of the satellite galaxy complement of the Milky Way Oliver Newton A Thesis presented for the degree of Doctor of Philosophy Institute for Computational Cosmology Ogden Centre for Fundamental Physics Department of Physics Durham University United Kingdom August 2019 Probing the nature of dark matter with small-scale cosmology A new estimate of the satellite galaxy complement of the Milky Way Oliver Newton Submitted for the degree of Doctor of Philosophy August 2019 Abstract: The standard model of cosmology has been enormously successful both at reproducing many observed properties of the Universe, and at predicting others. Despite this success one of its key components, a dark matter particle, has not been observed in targeted searches or indirect detection experiments. In addition, a number of discrepancies have arisen between observational proxies of DM structure and the small-scale predictions of this leading cosmological model, challenging its status as the standard paradigm. -
08-20-PPC.Pdf
WELCOME TO THE PPC 2018: XII INTERNATIONAL CONFERENCE ON INTERCONNECTIONS BETWEEN PARTICLE PHYSICS AND COSMOLOGY August 20, 2018 2 / 9 Conference scientific programme A venue to discuss particle physics, cosmology and astrophysics: 1 Gravitational waves: Monday August 20 – 24, 2018, Zurich, Switzerland 2 Early Universe cosmology: Monday PPC 2018 XIIth International Workshop on the Interconnection between Particle Physics and Cosmology 3 Late Universe cosmology: Monday and Tuesday The objectives of PPC 2018 are to analyze the connection between dark matter and particle physics models, discuss the connections among dark matter, grand unification models and recent neutrino results, explore predictions for ongoing and forthcoming experiments, and to provide a stimulating venue for exchange of scientific ideas among experts in these areas. 4 Low energy precision experiments: Monday International Program Advisory Committee Ben Allanach (Cambridge) John Ellis (King’s College London/CERN) Vernon Barger (Wisconsin) V.A. Bednyakov (JINR) Wim de Boer (Karlsruhe) 5 Dark matter: Tuesday and Thursday Joel Butler (FNAL/CERN) Tiziano Camporesi (CERN) Johnathan Ellis (CERN) JoAnne Hewett (SLAC) Ian Hinchliffe (LBL) Fabio Iocco (ICTP-SAIFR & IFT-UNESP) Karl Jakobs (U. Freiburg) Gordon Kane (Michigan) 6 Neutrinos: Tuesday Dmitri I. Kazakov (JINR, Dubna) Robert Kirshner (Harvard) Tomio Kobayashi (Tokyo) Pran Nath (NEU) Mihoko Nojiri (KEK) Frank Paige (BNL) Saul Perlmutter (LBNL) Michael Peskin (SLAC) 7 Collider physics: Wednesday and Thursday Adam Riess (Johns -
Annual Report 2010 Report Annual IPMU ANNUAL REPORT 2010 April 2010 April – March 2011March
IPMU April 2010–March 2011 Annual Report 2010 IPMU ANNUAL REPORT 2010 April 2010 – March 2011 World Premier International Institute for the Physics and Mathematics of the Universe (IPMU) Research Center Initiative Todai Institutes for Advanced Study Todai Institutes for Advanced Study The University of Tokyo 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan TEL: +81-4-7136-4940 FAX: +81-4-7136-4941 http://www.ipmu.jp/ History (April 2010–March 2011) April • Workshop “Recent advances in mathematics at IPMU II” • Press Release “Shape of dark matter distribution” • Mini-Workshop “Cosmic Dust” May • Shaw Prize to David Spergel • Press Release “Discovery of the most distant cluster of galaxies” • Press Release “An unusual supernova may be a missing link in stellar evolution” June • CL J2010: From Massive Galaxy Formation to Dark Energy • Press Conference “Study of type Ia supernovae strengthens the case for the dark energy” July • Institut d’Astrophysique de Paris Medal (France) to Ken’ichi Nomoto • IPMU Day of Extra-galactic Astrophysics Seminars: Chemical Evolution August • Workshop “Galaxy and cosmology with Thirty Meter Telescope (TMT)” September • Subaru Future Instrumentation Workshop • Horiba International Conference COSMO/CosPA October • The 3rd Anniversary of IPMU, All Hands Meeting and Reception • Focus Week “String Cosmology” • Nishinomiya-Yukawa Memorial Prize to Eiichiro Komatsu • Workshop “Evolution of massive galaxies and their AGNs with the SDSS-III/BOSS survey” • Open Campus Day: Public lecture, mini-lecture and exhibits November -
Astro2020 Science White Paper Probing Feedback in Galaxy Formation with Millimeter-Wave Observations
Astro2020 Science White Paper Probing Feedback in Galaxy Formation with Millimeter-wave Observations Thematic Areas: Planetary Systems Star and Planet Formation Formation and Evolution of Compact Objects 3 Cosmology and Fundamental Physics Stars and Stellar Evolution Resolved Stellar Populations and their Environments 3 Galaxy Evolution Multi-Messenger Astronomy and Astrophysics Principal Authors: Names: Nicholas Battaglia, J. Colin Hill Institutions: Cornell University, Institute for Advanced Study Emails: [email protected], [email protected] Phones: (607)-255-3735, (509)-220-8589 Co-authors: Stefania Amodeo (Cornell), James G. Bartlett (APC/U. Paris Diderot), Kaustuv Basu (Uni- versity of Bonn), Jens Erler (University of Bonn), Simone Ferraro (Lawrence Berkeley Na- tional Laboratory), Lars Hernquist (Harvard), Mathew Madhavacheril (Princeton), Matthew McQuinn (University of Washington), Tony Mroczkowski (European Southern Observatory), Daisuke Nagai (Yale), Emmanuel Schaan (Lawrence Berkeley National Laboratory), Rachel Somerville (Rutgers/Flatiron Institute), Rashid Sunyaev (MPA), Mark Vogelsberger (MIT), Jessica Werk (University of Washington) Endorsers: James Aguirre (University of Pennsylvania), Zeeshan Ahmed (SLAC), Marcelo Alvarez arXiv:1903.04647v1 [astro-ph.CO] 11 Mar 2019 (UC–Berkeley), Daniel Angles-Alcazar (Flatiron Institute), Chetan Bavdhankar (National Center for Nuclear Physics), Eric Baxter (University of Pennsylvania), Andrew Benson (Carnegie Observatories), Bradford Benson (Fermi National Accelerator Laboratory/ Uni- versity of Chicago), Paolo de Bernardis (Sapienza Università di Roma), Frank Bertoldi (Uni- versity of Bonn), Fredirico Bianchini (University of Melbourne), Colin Bischoff (University of Cincinnati), Lindsey Bleem (Argonne National Laboratory/KICP), J. Richard Bond (Uni- versity of Toronto/ CITA), Greg Bryan (Columbia/Flatiron Institute), Erminia Calabrese (Cardiff), John E. Carlstrom (University of Chicago/Argonne National Laboratory/KICP), Joanne D. -
Advanced Dark Energy Physics Telescope
JDEM/JDEM/ADEPTADEPT AADVANCEDDVANCED DDARKARK EENERGYNERGY PPHYSICSHYSICS TTELESCOPEELESCOPE HEPAP Feb 24, 2005 C. Bennett (Johns Hopkins Univ) ADEPT-1 ADEPT Science Team JHU Goddard Jonathan Bagger Gary Hinshaw Chuck Bennett Harvey Moseley Holland Ford Bill Oegerle Warren Moos Adam Riess Arizona Daniel Eisenstein Princeton Chris Hirata STScI David Spergel Harry Ferguson Swinburne Hawaii Chris Blake John Tonry Karl Glazebrook Penn U British Columbia Licia Verde Catherine Heymans HEPAP Feb 24, 2005 C. Bennett (Johns Hopkins Univ) ADEPT-2 Dark Energy Overview Dark energy equation of state: P = w ρ Options have HUGE implications for fundamental physics w = w0 (constant) ? w = w(z) (not constant) ? w is irrelevant, because GR is wrong ? Complementary space-based and ground-based measurements are both needed ADEPT is designed to do from space what needs to be done from space in a cost-controlled manner HEPAP Feb 24, 2005 C. Bennett (Johns Hopkins Univ) ADEPT-3 What is ADEPT? A dark energy probe, primarily Baryon Acoustic Oscillations (BAO) Redshift survey of 100 million galaxies 1 ≤ z ≤2 Slitless spectroscopy 1.3 − 2.0 µm Hα Nearly cosmic variance limited over nearly the full sky (28,600 deg2) First and final generation 1 ≤ z ≤2BAO measurement A dark energy probe, also using Type Ia Supernovae (SNe Ia) ∼1000 SNe Ia 0.8 ≤ z ≤1.3with no additional hardware or operating modes Products: ≡ δθ DA=angular diameter distance DA l / ≡ ()π 1/2 DL = luminosity distance DL Lf/4 H(z) expansion rate Galaxy redshift survey (power spectrum shape, tests of modified gravity w/CMB) HEPAP Feb 24, 2005 C. -
Newton Advanced Fellowships 2015
Newton Advanced Fellowships 2015 The full list of recipients and their UK partners is as follows: Brazil Dr Henrique de Melo Jorge Barbosa, University of Sao Paulo and Professor Gordon McFiggans, University of Manchester Measurements and modelling of anthropogenic pollution effects on clouds in the Amazon Professor Marilia Buzalaf, Bauru School of Dentistry, University of São Paulo and Professor John Michael Edwardson, University of Cambridge Identification of proteins conferring protection against dental erosion Dr Helena Cimarosti, Universidade Federal de Santa Catarina and Professor Jeremy Henley, University of Bristol SUMOylation: novel neuroprotective approach for Alzheimer’s disease? Professor Fernanda das Neves Costa, Federal University of Rio de Janeiro and Dr Svetlana Ignatova, Brunel University Countercurrent chromatography coupled with MS detection: tracking the large-scale isolation of target bioactive compounds to be used as starting material for the synthesis of new drug candidates Professor Pedro Duarte, University of Sao Paulo and Professor Sir David Hendry, Nuffield College Recent History of Macroeconomics and the Large-Scale Macroeconometric Models Dr Cristina Eluf, State University of Bahia and Dr Vander Viana, University of Stirling Corpus linguistics and teacher education: New perspectives for Brazilian pre-service teachers of English to speakers of other languages Dr Fernanda Estevan, University of Sao Paulo and Dr Thomas Gall, University of Southampton Affirmative Action in College Admission: Encouragement, Discouragement, -
Numerical Cosmology & Galaxy Formation
Numerical Cosmology & Galaxy Formation Lecture 1: Motivation and Historical Overview Benjamin Moster 1 About this lecture • Lecture slides will be uploaded to www.usm.lmu.de/people/moster/Lectures/NC2016.html • Exercises will be lead by Dr. Remus 1st exercise will be next week (20.04.16, 12-14, USM Hörsaal) • Goal of exercises: run your own simulations Code: Gadget-2 available at http://www.mpa-garching.mpg.de/gadget/ • Evaluation: - Exercise sheets and tutorials: 50% - Project with oral presentation (to be chosen individually): 50% 2 Numerical Cosmology & Galaxy Formation 1 13.04.2016 Literature • Textbooks: - Mo, van den Bosch, White: Galaxy Formation and Evolution, 2010 - Schneider: Extragalactic Astronomy and Cosmology, 2006 - Padmanabhan: Structure Formation in the Universe, 1993 - Hockney, Eastwood: Computer Simulation Using Particles, 1988 • Reviews: - Trenti, Hut: Gravitational N-Body Simulations, 2008 - Dolag: Simulation Techniques for Cosmological Simulations, 2008 - Klypin: Numerical Simulations in Cosmology, 2000 - Bertschinger: Simulations of Structure Formation in the Universe, 1998 3 Numerical Cosmology & Galaxy Formation 1 13.04.2016 Outline of the lecture course • Lecture 1: Motivation & Historical Overview • Lecture 2: Review of Cosmology • Lecture 3: Generating initial conditions • Lecture 4: Gravity algorithms • Lecture 5: Time integration & parallelization • Lecture 6: Hydro schemes - Grid codes • Lecture 7: Hydro schemes - Particle codes • Lecture 8: Radiative cooling, photo heating • Lecture 9: Subresolution physics