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Rediscovering Our Galaxy Edited By
IAU IAU Symposium Proceedings of the International Astronomical Union IAU Symposium No. 334 Symposium 10–14 July 2017 Astronomers are at a crucial point in our understanding of the Milky Way. Deciphering the assembly history of our galaxy requires 334 Potsdam, Germany detailed mapping of the structure, dynamics, chemical composition, and age distribution of its stellar populations. In the last decade, astrometric, spectroscopic, photometric, and asteroseismic surveys have started to unveil the inner- and 10–14 July 2017 334 Rediscovering 10–14 July 2017 outermost regions of the Milky Way. IAU Symposium 334 explores Potsdam, Germany Our Galaxy the still open questions and focusses on the concepts emerging Potsdam, Germany Rediscovering from the analysis of these large, new, and complex datasets. This volume presents a summary of these topics, including the current novel data and the challenges they already pose to modeling, Our Galaxy before Gaia end-of-mission, PLATO, and large spectroscopic surveys such as WEAVE and 4MOST are about to start. Graduate students and researchers will learn that, in this golden era of Galactic Archaeology, we are about to rediscover our galaxy. Proceedings of the International Astronomical Union Editor in Chief: Dr Piero Benvenuti This series contains the proceedings of major scientifi c meetings held by the International Astronomical Union. Each volume contains a series of articles on a topic of current interest in astronomy, giving a timely overview of research in the fi eld. With contributions by leading -
IAU Symp 269, POST MEETING REPORTS
IAU Symp 269, POST MEETING REPORTS C.Barbieri, University of Padua, Italy Content (i) a copy of the final scientific program, listing invited review speakers and session chairs; (ii) a list of participants, including their distribution on gender (iii) a list of recipients of IAU grants, stating amount, country, and gender; (iv) receipts signed by the recipients of IAU Grants (done); (v) a report to the IAU EC summarizing the scientific highlights of the meeting (1-2 pages). (vi) a form for "Women in Astronomy" statistics. (i) Final program Conference: Galileo's Medicean Moons: their Impact on 400 years of Discovery (IAU Symposium 269) Padova, Jan 6-9, 201 Program Wednesday 6, location: Centro San Gaetano, via Altinate 16.0 0 – 18.00 meeting of Scientific Committee (last details on the Symp 269; information on the IYA closing ceremony program) 18.00 – 20.00 welcome reception Thursday 7, morning: Aula Magna University 8:30 – late registrations 09.00 – 09.30 Welcome Addresses (Rector of University, President of COSPAR, Representative of ESA, President of IAU, Mayor of Padova, Barbieri) Session 1, The discovery of the Medicean Moons, the history, the influence on human sciences Chair: R. Williams Speaker Title 09.30 – 09.55 (1) G. Coyne Galileo's telescopic observations: the marvel and meaning of discovery 09.55 – 10.20 (2) D. Sobel Popular Perceptions of Galileo 10.20 – 10.45 (3) T. Owen The slow growth of human humility (read by Scott Bolton) 10.45 – 11.10 (4) G. Peruzzi A new Physics to support the Copernican system. Gleanings from Galileo's works 11.10 – 11.35 Coffee break Session 1b Chair: T. -
December2009
December2009 On the cover: Saturn and its moon Director s Message “Wild Youth” of Titan obtained using 4 ’ 27 adaptive optics Doug Simons on the Gemini Massive Galaxies North telescope. Mariska Kriek For more details on this image and the Titan Monitoring & Pieter van Dokkum related discovery of 7 unexpected weather on Henry Roe & Emily Schaller Titan see the article by High-Z Band-Shuffling Henry Roe and Emily 30 Schaller starting on Most Distant Known page 7. 10 with GMOS Object in Universe Adam Muzzin & Howard Yee Edo Berger 34 AO Open-Loop Guiding 13 Z~5 Star-forming with Galactic Centers Galaxy with NIFS/IFU Richard McDermid, Davor Krajnović Mark Swinbank & Michele Cappellari IFU Wiki 17 39 Science Highlights Mark Westmoquette & Millicent Maier Nancy A. Levenson 19 Mid-IR Observations 43 Exoplanet Imaging of Seyfert Galaxies Christian Marois & Michael Liu Cristina Ramos Almeida & Chris Packham 47 Time-Sharing 23 Globulars in M31 Programs Dennis Crabtree & Tom Geballe Dougal Mackey, Annette Ferguson & Avon Huxor 2 GeminiFocus Exploring the Universe, Sharing its Wonders 52 Kyoto Science Meeting 77 Introducing Jean-René Roy, Atsuko Nitta Nancy A. Levenson & Nancy A. Levenson Joy Pollard On-site Observing 55 78 Profile: François Rigaut Dennis Crabtree María Antonieta García Planning for Future 57 82 Profile: Dolores Coulson Instruments Peter Michaud Eric Tollestrup 86 Hawai‘i & Chile 60 MCAO Progress Nature Pictures by Staff François Rigaut & Céline D’orgeville Joy Pollard & Manuel Paredes 62 Greening of Gemini Sarah Blanchard Broadening Participation Managing Editor, Peter Michaud 67 Associate Editor, Carolyn Collins Petersen Neil Barker Proof Reader, Stephen James O’Meara Designer, Kirk Pu‘uohau-Pummill 70 GeminiFocus Reader’s Survey Peter Michaud Any opinions, findings, and conclusions or recommendations expressed in this material are PIO Activities those of the author(s) and do not necessarily reflect 72 the views of the National Science Foundation. -
The Cycle 11 Review Process
VOL 19 ISSUE 01 Space Telescope Science Institute The Cycle 11 Review Process Duccio Macchetto, [email protected], Georges Meylan, [email protected], Letizia Stanghellini, [email protected], Roeland van der Marel, [email protected], Robert Williams, [email protected], Brett Blacker, [email protected] Laguerra sort through Lorretta Willers, Victoria Horne, and Tania Cycle 11 proposals during the afternoon proposal-processing shift. New Science Opportunities in Cycle 11 There were other novelties in Cycle 11. Given the rate of increase in the size of the Hubble data archive and the value of large, homogeneous data he Hubble Telescope Allocation Committee (TAC) and panels met sets, we wished to stimulate a more ambitious Archival Research (AR) in Baltimore between November 12 and 17, 2001, to select and program by creating the new AR Legacy Program. Selected Legacy recommend to the Director the suite of programs to be programs will perform a homogeneous analysis of a well-defined dataset in executed in Cycle 11. the Hubble archive and will generate data products of use to the scientific TCycle 11 will provide the most powerful combination of instruments since community (catalogs, software tools, web interfaces, etc.), which will allow the launch of the Hubble Space Telescope. Hubble’s scientific capabilities a variety of new investigations. will be greatly enhanced by upgrades during the next servicing mission, cur- Another important change in Cycle 11 was the start of the Hubble Theory rently scheduled for February 2002. The Advanced Camera for Surveys Program, funded as part of the Hubble AR program. The Theory Program is (ACS) will provide a large increase in sensitivity and field of view, and the in line with recommendations in the report from the Astronomy and installation of a cryocooler will revive the Near Infrared Camera and Astrophysics Survey Committee of the National Research Council, which Multi-Object Spectrometer (NICMOS). -
第 28 届国际天文学联合会大会 Programme Book
IAU XXVIII GENERAL ASSEMBLY 20-31 AUGUST, 2012 第 28 届国际天文学联合会大会 PROGRAMME BOOK 1 Table of Contents Welcome to IAU Beijing General Assembly XXVIII ........................... 4 Welcome to Beijing, welcome to China! ................................................ 6 1.IAU EXECUTIVE COMMITTEE, HOST ORGANISATIONS, PARTNERS, SPONSORS AND EXHIBITORS ................................ 8 1.1. IAU EXECUTIVE COMMITTEE ..................................................................8 1.2. IAU SECRETARIAT .........................................................................................8 1.3. HOST ORGANISATIONS ................................................................................8 1.4. NATIONAL ADVISORY COMMITTEE ........................................................9 1.5. NATIONAL ORGANISING COMMITTEE ..................................................9 1.6. LOCAL ORGANISING COMMITTEE .......................................................10 1.7. ORGANISATION SUPPORT ........................................................................ 11 1.8. PARTNERS, SPONSORS AND EXHIBITORS ........................................... 11 2.IAU XXVIII GENERAL ASSEMBLY INFORMATION ............... 14 2.1. LOCAL ORGANISING COMMITTEE OFFICE .......................................14 2.2. IAU SECRETARIAT .......................................................................................14 2.3. REGISTRATION DESK – OPENING HOURS ...........................................14 2.4. ON SITE REGISTRATION FEES AND PAYMENTS ................................14 -
Stsci Newsletter: 2017 Volume 034 Issue 02
2017 - Volume 34 - Issue 02 Emerging Technologies: Bringing the James Webb Space Telescope to the World Like the rest of the Institute, excitement is building in the Office of Public Outreach (OPO) as the clock winds down for the launch of the James Webb Space Telescope. Our task is translating and sharing this excitement over groundbreaking engineering—and the scientific discoveries to come—with the public. Webb @ STScI In the lead-up to Webb’s launch in Spring 2019, the Institute continues its work as the science and operations center for the mission. The Institute has played a critical role in a number of recent Webb mission milestones. Updates on Hubble Operation at the Institute Observations with the Hubble Space Telescope continue to be in great demand. This article discusses Cycle 24 observing programs and scheduling efficiency, maintaining COS productivity into the next decade, keeping Hubble operations smooth and efficient, and ensuring the freshness of Hubble archive data. Hubble Cycle 25 Proposal Selection Hubble is in high demand and continues to add to our understanding of the universe. The peer-review proposal selection process plays a fundamental role in establishing a merit-based science program, and that is only possible thanks to the work and integrity of all the Time Allocation Committee (TAC) and review panel members, and the external reviewers. We present here the highlights of the Cycle 25 selection process. Using Gravity to Measure the Mass of a Star In a reprise of the famous 1919 solar eclipse experiment that confirmed Einstein's general relativity, the nearby white dwarf, Stein 2051 B, passed very close to a background star in March 2014. -
Deep Photometry in a Remote M31 Major Axis Field Near G1
Deep Photometry in a Remote M31 Major Axis Field Near G11 R. Michael Rich [email protected] David B. Reitzel [email protected] Department of Physics and Astronomy, University of California at Los Angeles, Math-Sciences 8979, Los Angeles, CA 90095-1562, USA Puragra Guhathakurta UCO/Lick Observatory, University of California at Santa Cruz, 1156 High Street, Santa Cruz, CA 95064, USA [email protected] Karl Gebhardt Department of Astronomy, University of Texas at Austin, C1400, Austin, TX 78712, USA [email protected] and Luis C. Ho The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91109 [email protected] ABSTRACT arXiv:astro-ph/0309296v3 6 Jan 2004 We present photometry from Hubble Space Telescope (HST )/Wide Field Planetary Camera 2 parallel imagery of a remote M31 field at a projected distance of ∼ 34 kpc from the nucleus near the SW major axis. This field is near the globular cluster G1, and near one of the candidate tidal plumes identified by Ferguson et al. (2002). The F606W (V ) and F814W (I) images were obtained in parallel with Space Telescope Imaging Spectrograph spectroscopy of G1 (GO-9099) and total 7.11 hours of integration time — the deepest HST field in the outer disk of M31 to date, reaching to V ∼ 28. The color-magnitude diagram of the field shows a clearly-defined red clump at V = 25.25 and a red giant branch consistent with [Fe/H] ≈ −0.7. The lack of a blue horizontal branch contrasts with other M31 halo fields, the Andromeda dwarf spheroidals, and with the nearby globular cluster G1. -
Rosemary F.G. Wyse Curriculum Vitae
Rosemary F.G. Wyse Curriculum Vitae Positions Held: Jul 1993 - present Full Professor, The Johns Hopkins University Jul 1990 - Jun 1993 Associate Professor, The Johns Hopkins University Jan 1988 - Jun 1990 Assistant Professor, The Johns Hopkins University Aug 1986 - Jan 1988 University of California President's Fellow, UC Berkeley Jan - July 1986 Postdoctoral Fellow, SpaceTelescope Science Institute Aug - Dec 1985 University of California President's Fellow, UC Berkeley Sep 1983 - Jul 1985 Parisot Postdoctoral Fellow at UC Berkeley Sep1982 - Aug 1983 Lindemann Fellow of the English Speaking Union of the Commonwealth; Princeton University and UC Berkeley Education 1978-82: University of Cambridge, Institute of Astronomy. Degree : Ph.D. (Supervisor : Bernard Jones); awarded April 1983. 1977-78: University of Cambridge, Department of Applied Mathematics. Degree : Part Three of the Mathematics Tripos (with Distinction). 1974-77: University of London, Queen Mary College, Physics Department. Degree : B.Sc (First Class Honours) in Physics with Astrophysics. Prizes & Honors 2017 • Elected Fellow of the American Physical Society 2016: • Elected Fellow of the American Association for the Advancement of Science • Dirk Brouwer award from the Division of Dynamical Astronomy, AAS • Blauuw Professor and Lecturer, University of Groningen (The Netherlands) • Visiting Professor, Leverhulme Trust, held at University of Edinburgh (UK) 2015: • Distinguished Visitor, Australia National University, Canberra (Australia) • Hunstead Visitor, University of Sydney, Institute for Astronomy 2009: • Distinguished Visitor, Scottish Universities Physics Alliance 2002: • Hilary term. Elected Visiting Fellow of New College, Oxford (UK) • Trinity term. Elected Keeley Fellow, Wadham College, Oxford (UK) 1990-1992: • Fellowship from the Alfred P. Sloan Foundation. 1989: • Teaching Fellowship from the Eli Lilly Foundation. -
IAU Volume 5 Issue S262 Front Matter
STELLAR POPULATIONS – PLANNING FOR THE NEXT DECADE IAU SYMPOSIUM No. 262 COVER ILLUSTRATION: ARP 147 Arp 147 appears in the Arp Atlas of Peculiar Galaxies, compiled by Halton Arp in the 1960s and published in 1966. Arp 147 lies in the constellation Cetus, and it is more than 400 million light-years away from Earth. The two galaxies happen to be oriented so that they appear to mark the number 10. The left-most galaxy, or the “one” in this image, is relatively undisturbed apart from a smooth ring of starlight. It appears nearly on edge to our line of sight. The right-most galaxy, resembling a zero, exhibits a clumpy, blue ring of intense star formation. The blue ring was most probably formed after the galaxy on the left passed through the galaxy on the right. Just as a pebble thrown into a pond creates an outwardly moving circular wave, a propagating density wave was generated at the point of impact and spread outward. As this density wave collided with material in the target galaxy that was moving inward due to the gravitational pull of the two galaxies, shocks and dense gas were produced, stimulating star formation. The dusty reddish knot at the lower left of the blue ring probably marks the location of the original nucleus of the galaxy that was hit. The galaxy pair was photographed on October 27–28, 2008, to test the performance of the WFPC2 after being brought back on line a few days before. This picture was assembled from WFPC2 images taken with three separates filters. -
Aas Newsletter
AASAAS NNEWSLETTEREWSLETTER August 2003 A Publication for the members of the American Astronomical Society Issue 116 development of the new statement. Both the DPS President’s Column and the SPD have suggested names of scientists to Caty Pilachowski, [email protected] serve on the AGU panel. When the AGU statement is drafted, the Society can then consider whether we Inside The AAS and Public Policy wish to endorse or even co-sign a joint statement on The AAS efforts in public policy on behalf of the climate change. Members in Nashville strongly 3 astronomical community are increasingly Council supported this direction for the Society, and the important to the Society and to its members. As Actions dialogue will continue as the AGU statement is the participation of the astronomical community brought to Council and to members for discussion. in the public policy arena has grown, so has the As that time draws nearer, we will seek further input range of activities and services coordinated or 4 and guidance from members on this important issue. Prize organized by the Society. Nomination Form Much of the Society’s public policy initiatives are Given the importance of the Society’s public policy overseen by the Committee on Astronomy and statements, Council also initiated and approved a 5 Public Policy (CAPP), currently chaired by Sidney continued on page 3 Membership Wolff. CAPP provides guidance to the AAS Dues & Council on public policy questions, as well as Subscription brings to Council issues that require the Society’s Rates attention. CAPP was established nearly 25 years 2003 AAS Elections ago, and members are appointed by the President, with the approval of the AAS Council. -
Rpt All Pis W/Juniors by MOA
rpt_All PIs w/Juniors by MOA MOAName PI Name and Science Interest Institution ScienceCollaboration Australia/AAL MOA PI Scientists: 10 Brough, Sarah University of New South Wales Galaxies Galaxy surveys; galaxy clusters; brightest cluster galaxies; intracluster light Davis, Tamara University of Queensland Dark Energy Cosmology; dark energy; large scale structure; weak lensing; supernovae; AGN de Grijs, Richard Macquarie University Stars, Milky Way, and Local Volume Star clusters, Local Group, Magellanic Clouds Driver, Simon University of Western Australia Galaxies Multiwavelength galaxy surveys; galaxy evolution; low surface brightness galaxies Galloway, Duncan Monash University Transients/Variable Stare Gravitational waves; transients Glazebrook, Karl Swinburne University of Technology Dark Energy, Strong Lensing Gravitational lensing; multiwavelength galaxy surveys; galaxy evolution Jerjen, Helmut Australian National University Galaxies Dwarf galaxies, Milky Way satellites, galaxy formation Martell, Sarah University of New South Wales Stars, Milky Way, and Local Volume Chemical tagging; Milky Way; satellites and streams Meurer, Gerhardt University of Western Australia Stars, Milky Way, and Local Volume; Galaxies Nearby galaxies Webster, Rachel University of Melbourne Active Galactic Nuclei; Strong Lensing Gravitational lensing; AGN; quasars Tuesday, March 09, 2021 Page 1 of 77 MOAName PI Name and Science Interest Institution ScienceCollaboration MOAName Institution Scientist Name Status MentorName Australia/AAL University of New South -
Post%Meeting+Report+
Post%Meeting+Report+ ++ IAU$Symposium$321$ Formation$and$evolution$of$galaxy$outskirts$ Toledo$(Spain),$March$14E18th$2016E04E06$ $ $ 1.! Meeting$number:$IAU$Symposium$321$ $ 2.! Meeting$title:$“Formation$and$evolution$of$galaxy$outskirts”$ $ 3.! Coordinating$division:$J$(Galaxies$and$Cosmology)$ $ 4.! Dedication$of$meeting:$None$ $ 5.! Location:$Toledo$(Spain)$ $ 6.! Dates$of$meeting:$March$14E18th$2016$ $ 7.! Number$of$participants:$210$ $ 8.! List$of$represented$countries:$ $ Argentina$ Finland$ Portugal$ Armenia$ France$ Russia$ Australia$ Germany$ South$Africa$ Austria$ Greece$ South$Korea$ Brazil$ India$ Spain$ Canada$ Israel$ Sweden$ Chile$ Italy$ Switzerland$ China$ Japan$ United$Kingdom$ Denmark$ Mexico$ United$States$ Ecuador$ Netherlands$ Vietnam$ Estonia$ Poland$ $ $ 9.! Report$submitted$by:$Armando$Gil$de$Paz$(Universidad$Complutense$de$ Madrid,$Spain)$–$Symposium$chairperson,$SOC$chair$and$LOC$coEchair$(jointly$ with$Ainhoa$SáncheZ$Penim;$Universidad$Complutense$de$Madrid).$ $ 10.!Date$and$place:$April$8th$2016$ $ 11.!Signature$of$SOC$Chairperson:$ $ $ MONDAY March 14th, 2016 S 08:00-09:00 Registration 09:00-09:30 Opening ceremony s Resolved Stellar Populations in galaxy outskirts (I) – The Milky Way (chair: Lia Athanassoula) 09:30-09:50 Invited: Outskirts of the Milky Way (Francesca Figueras, University of Barcelona) 09:50-10:05 Extended Structure of the Milky Way (Carl Grillmair, California Institute of Technology) 10:05-10:20 The radial extent and scale-length of the Galactic thick disk (Thomas Bensby, Lund Observatory)