Supermassive Black Hole Activity in the Cosmic Evolution Survey

Total Page:16

File Type:pdf, Size:1020Kb

Supermassive Black Hole Activity in the Cosmic Evolution Survey Supermassive Black Hole Activity in the Cosmic Evolution Survey Item Type text; Electronic Dissertation Authors Trump, Jonathan Russell Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 11/10/2021 08:07:30 Link to Item http://hdl.handle.net/10150/194982 SUPERMASSIVE BLACK HOLE ACTIVITY IN THE COSMIC EVOLUTION SURVEY by Jonathan Russell Trump A Dissertation Submitted to the Faculty of the DEPARTMENT OF ASTRONOMY In Partial Fulfillment of the Requirements For the Degree of DOCTOR OF PHILOSOPHY In the Graduate College THE UNIVERSITY OF ARIZONA 2010 2 The University of Arizona Graduate College As members of the Dissertation Committee, we certify that we have read the dis- sertation prepared by Jonathan Russell Trump entitled Supermassive Black Hole Activity in the Cosmic Evolution Survey and recommend that it be accepted as fulfilling the dissertation requirement for the Degree of Doctor of Philosophy. Date: 16 April 2010 Christopher D. Impey Date: 16 April 2010 Romeel Dav´e Date: 16 April 2010 Richard F. Green Date: 16 April 2010 Dennis Zaritsky Final approval and acceptance of this dissertation is contingent upon the candidate’s submission of the final copies of the dissertation to the Graduate College. I hereby certify that I have read this dissertation prepared under my direction and recommend that it be accepted as fulfilling the dissertation requirement. Date: 16 April 2010 Dissertation Director: Christopher D. Impey 3 Statement By Author This dissertation has been submitted in partial fulfillment of requirements for an advanced degree at The University of Arizona and is deposited in the University Library to be made available to borrowers under rules of the Library. Brief quotations from this dissertation are allowable without special permission, provided that accurate acknowledgment of source is made. Requests for permission for extended quotation from or reproduction of this manuscript in whole or in part may be granted by the head of the major department or the Dean of the Graduate College when in his or her judgment the proposed use of the material is in the interests of scholarship. In all other instances, however, permission must be obtained from the author. Signed: Jonathan Russell Trump 4 Acknowledgments I leaned on and learned from a lot of people on the way to my Ph.D., and I’d like to use this space to formally thank them. First, I’d like to thank my parents. I was always lucky to come from a supportive family which highly valued education and encouraged me to succeed. I never lacked for educational opportunities, with my parents offering everything from financial support for academic competitions in high school and college to an always-interested ear throughout my pursuits. I thank them most for their patience: I’ve been in school for 22 straight years, and I think my parents showed a tremendous amount of faith in me to remain so supportive throughout the myriad missteps and dead-ends in such a long path. I’m simply a better human being from their influence, and for that, I am truly thankful. I’d also like to thank all the teachers and mentors of my “formative” years, when I didn’t know starlight from satellites and quasars were just another twinkle in the sky. I owe a great deal to Mr. Moyer, who taught me that everyone has a great talent just waiting to be recognized (and he was somehow able to recognize this in 10-year-olds). I want to thank Mr. Dietrich, who really set me on the path of my first true research projects and taught me about the pride and success that comes from hard work. I’d especially like to thank my uncle, the late Frank Schweingruber, whose contagious enthusiasm led me to love the physics of the universe. I still vividly recall the boundless enthusiasm of my Uncle Frank as he mentored me in designing my senior project in high school: a double-slit experiment demonstrating the wave- particle duality of light. I want to thank my professors at Penn State, especially those who taught me what it is to be an astronomer. Jane Charlton and Caryl Gronwall gave me much- needed advice when it came to choosing a graduate school, and with Niel Brandt, Mike Eracleous, Chris Palma, Larry Ramsey, and Steinn Sigurdsson showed an enthusiasm for astronomy that I can only hope to match. I also want to thank my undergraduate advisor Don Schneider and Gordon Richards (at the time, Don’s postdoc). They gave me a comfortable introduction to the large survey AGN science that I eventually pursued for my thesis (and will continue for as a postdoc). And they were also bold enough to hand a significant project to a fresh-faced student with a lot to learn: with their help, my undergraduate research resulted in a widely cited published paper. Making your student’s research well-known is surely the greatest gift than an advisor can give. It’s also important to me to recognize those friends who encouraged me in my education and research, and made academic life much easier. I’ll start with Amy and Andrew, two of my oldest friends, because it’s friends like these that help you realize it’s perfectly natural to love science. I’d like to thank my study partners and fellow stargazers in college: Shoe, Kimbo, Bragg, Sloan, and Danimal; Nate, Nate, and Seltzer; Rick, Eric, Adam, and Dave. Joe and Megan certainly showed 5 me that it’s far easier to learn with partners like them by your side. Brooklyn, Ben Opp, Jerry, Brandon, Iva, Maggie, the Stephs, James, Suz, Coley, and Boz all made Tucson an easy place to live and work. The Steward Mug Club was the ultimate blessing, because with Brandon, Nopey, and my heterolifemate Aleks as both best friends and my colleagues, the frustrations of graduate school are no more distressing than an empty 25-oz mug. And special thanks go to my brother Ben, who’s always been a far better listener than I, and showed it constantly through my trials even as our lives led us so far apart. I want to thank my partner, Lindsay, for her patience and support through the inevitable stresses of a thesis. Ultimately, this thesis is the product of collaboration with many colleagues. Nick Scoville made the Cosmic Evolution Survey an easy place for a graduate student to succeed, always ensuring that I was comfortable and had a large suite of scientific real estate to explore. Martin Elvis was consistently my go-to pundit when I needed a quasar expert, and originally suggested several of the research paths pursued in this work. I’d like to thank Pat McCarthy for teaching me how to observe, and the staffs at the Magellan and MMT telescopes for making my observations painless. (I should also thank the Chilean weather, with only one night lost over 20 nights of observing.) Knud Jahnke, Anton Koekemoer, Marcella Brusa, Andrea Comastri, Francesca Civano, Patrick Shopbell, and Mara Salvato also helped with guidance and countless discussions. I want to thank Yoshi Taniguchi, Tohru Nagao, and their students at Ehime University for making Matsuyama, Japan like a second home to me while I worked there on research visits. My research was also reliant on financial support from an ARCS fellowship, a NSF/JSPS summer fellowship, NSF/DDEP grant #0943995, NSF grant #NNX08AJ28G, and NASA grant HST-GO-09822. I owe a great deal to my graduate advisor, Chris Impey. I first began this research after Chris sent an email to all students in the department explaining that he needed someone to go observing in Chile. A trip to South America sounded pretty good to me, and five and a half years later I’ve been observing in Chile four times, plus three trips to Japan, two to China, and an observing run in Hawaii. All this because Chris encouraged me to write ambitious proposals, and then had the patience to help mold them into success. And whenever Chris felt he lacked the expertise on an issue, he made sure to send me to a conference full of experts. Chris was patient, but also knew how to push me when I needed that extra motivation. I hope that some day I can give my students all that Chris has given me in my graduate career. Thanks also go to Sandy Faber, David Koo, and Raja Guhathakurta... because it’s far easier to write and defend a thesis when you have an excellent postdoc job waiting for you in Santa Cruz. 6 Dedication For Frank Schweingruber, who taught me that the universe is a beautiful and fasci- nating subject of study. 7 Table of Contents List of Figures ............................... 9 List of Tables ................................ 11 Abstract ................................... 12 Chapter 1 Introduction ........................... 14 Chapter 2 The COSMOS AGN Spectroscopic Survey: XMM Coun- terparts .................................... 20 2.1 ChapterIntroduction. 20 2.2 Observations................................ 25 2.2.1 XMM-Newton........................... 25 2.2.2 Magellan/IMACS. 26 2.2.3 MMT/Hectospec ......................... 36 2.2.4 SDSS................................ 40 2.3 SpectralAnalysis ............................. 40 2.3.1 AGNClassification . 41 2.3.2 AGN, Starbursts, and Quiescent Galaxies . 90 2.4 Completeness ............................... 95 2.4.1 X-rayFluxLimit ......................... 96 2.4.2 OpticalFluxLimit . .. .. 96 2.4.3 Redshift-Dependent Completeness . 98 2.4.4 Characterizing the Low-Confidence Targets . 103 2.5 Discussion .................................106 2.5.1 Demographics.
Recommended publications
  • The Cosmic Evolution Survey (Cosmos): Overview1 N
    The Astrophysical Journal Supplement Series, 172:1Y8, 2007 September # 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE COSMIC EVOLUTION SURVEY (COSMOS): OVERVIEW1 N. Scoville,2,3 H. Aussel,4 M. Brusa,5 P. Capak,2 C. M. Carollo,6 M. Elvis,7 M. Giavalisco,8 L. Guzzo,9 G. Hasinger,5 C. Impey,10 J.-P. Kneib,11 O. LeFevre,11 S. J. Lilly,6 B. Mobasher,8 A. Renzini,12,13 R. M. Rich,14 D. B. Sanders,15 E. Schinnerer,16,17 D. Schminovich,18 P. Shopbell,2 Y. Taniguchi,19 and N. D. Tyson20 Received 2006 April 25; accepted 2006 June 28 ABSTRACT The Cosmic Evolution Survey (COSMOS) is designed to probe the correlated evolution of galaxies, star formation, active galactic nuclei (AGNs), and dark matter (DM) with large-scale structure (LSS) over the redshift range z > 0:5Y6. The survey includes multiwavelength imaging and spectroscopy from X-rayYtoYradio wavelengths covering a 2 deg2 area, including HST imaging. Given the very high sensitivity and resolution of these data sets, COSMOS also provides unprecedented samples of objects at high redshift with greatly reduced cosmic variance, compared to earlier surveys. Here we provide a brief overview of the survey strategy, the characteristics of the major COSMOS data sets, and a summary the science goals. Subject headinggs: cosmology: observations — dark matter — galaxies: evolution — galaxies: formation — large-scale structure of universe — surveys 1. INTRODUCTION multiband imaging and spectroscopy provide redshifts and hence cosmic ages for these populations. Most briefly, the early universe Our understanding of the formation and evolution of galaxies and their large-scale structures (LSSs) has advanced enormously galaxies were more irregular/interacting than at present and the overall cosmic star formation rate probably peaked at z 1Y3 over the last decade—a result of a phenomenal synergy between with 10Y30 times the current rates (Lilly et al.
    [Show full text]
  • HEIC0701: for IMMEDIATE RELEASE 19:30 (CET)/01:30 PM EST 7 January, 2007
    HEIC0701: FOR IMMEDIATE RELEASE 19:30 (CET)/01:30 PM EST 7 January, 2007 http://www.spacetelescope.org/news/html/heic0701.html News release: First 3D map of the Universe’s Dark Matter scaffolding 7-January-2007 By analysing the COSMOS survey – the largest ever survey undertaken with Hubble – an international team of scientists has assembled one of the most important results in cosmology: a three-dimensional map that offers a first look at the web-like large-scale distribution of dark matter in the Universe. This historic achievement accurately confirms standard theories of structure formation. For astronomers, the challenge of mapping the Universe has been similar to mapping a city from night-time aerial snapshots showing only streetlights. These pick out a few interesting neighbourhoods, but most of the structure of the city remains obscured. Similarly, we see planets, stars and galaxies in the night sky; but these are constructed from ordinary matter, which accounts in total for only one sixth of the total mass in the Universe. The remainder is a mysterious component - dark matter - that neither emits nor reflects light. An international team of astronomers led by Richard Massey of the California Institute of Technology (Caltech), USA, has made a three-dimensional map that offers a first look at the web-like large-scale distribution of dark matter in the Universe in unprecedented detail. This new map is equivalent to seeing a city, its suburbs and surrounding country roads in daylight for the first time. Major arteries and intersections are revealed and the variety of different neighbourhoods becomes evident.
    [Show full text]
  • Astronomy 2008 Index
    Astronomy Magazine Article Title Index 10 rising stars of astronomy, 8:60–8:63 1.5 million galaxies revealed, 3:41–3:43 185 million years before the dinosaurs’ demise, did an asteroid nearly end life on Earth?, 4:34–4:39 A Aligned aurorae, 8:27 All about the Veil Nebula, 6:56–6:61 Amateur astronomy’s greatest generation, 8:68–8:71 Amateurs see fireballs from U.S. satellite kill, 7:24 Another Earth, 6:13 Another super-Earth discovered, 9:21 Antares gang, The, 7:18 Antimatter traced, 5:23 Are big-planet systems uncommon?, 10:23 Are super-sized Earths the new frontier?, 11:26–11:31 Are these space rocks from Mercury?, 11:32–11:37 Are we done yet?, 4:14 Are we looking for life in the right places?, 7:28–7:33 Ask the aliens, 3:12 Asteroid sleuths find the dino killer, 1:20 Astro-humiliation, 10:14 Astroimaging over ancient Greece, 12:64–12:69 Astronaut rescue rocket revs up, 11:22 Astronomers spy a giant particle accelerator in the sky, 5:21 Astronomers unearth a star’s death secrets, 10:18 Astronomers witness alien star flip-out, 6:27 Astronomy magazine’s first 35 years, 8:supplement Astronomy’s guide to Go-to telescopes, 10:supplement Auroral storm trigger confirmed, 11:18 B Backstage at Astronomy, 8:76–8:82 Basking in the Sun, 5:16 Biggest planet’s 5 deepest mysteries, The, 1:38–1:43 Binary pulsar test affirms relativity, 10:21 Binocular Telescope snaps first image, 6:21 Black hole sets a record, 2:20 Black holes wind up galaxy arms, 9:19 Brightest starburst galaxy discovered, 12:23 C Calling all space probes, 10:64–10:65 Calling on Cassiopeia, 11:76 Canada to launch new asteroid hunter, 11:19 Canada’s handy robot, 1:24 Cannibal next door, The, 3:38 Capture images of our local star, 4:66–4:67 Cassini confirms Titan lakes, 12:27 Cassini scopes Saturn’s two-toned moon, 1:25 Cassini “tastes” Enceladus’ plumes, 7:26 Cepheus’ fall delights, 10:85 Choose the dome that’s right for you, 5:70–5:71 Clearing the air about seeing vs.
    [Show full text]
  • The Zcosmos Redshift Survey
    Reports from Observers The zCOSMOS Redshift Survey Simon Lilly (ETH, Zürich, Switzerland) that have been developed, using almost are the product of the gravitational growth and the zCOSMOS team* all of the most powerful observing facil- of initially tiny density fluctuations in the ities in the world. This next step is called distribution of dark matter in the Universe COSMOS and the ESO VLT will make a – fluctuations which likely arise from quan- The last ten years have seen the open- major enabling contribution to this pro- tum processes in the earliest moments ing up of dramatic new vistas of the fur- gramme through the zCOSMOS survey of the Big Bang, τ ~10–35 s. These densi- thest reaches of space and time – an being carried out with the VIMOS spec- ty fluctuations eventually collapse to make exploration in which the VLT has played trograph. gravitationally-bound dark matter struc- a major role. However, the work so far tures within which the baryonic material has been exploratory, and sampled only cools, concentrating at the bottom of the small and possibly unrepresentative vol- It is well known that the finite speed gravitational potential wells where it forms umes of the distant Universe. The next of light enables us to observe very distant the visible components of galaxies. step is to bring to bear on a single large objects as they were when the Universe area of sky the full range of techniques as a whole was much younger, and there- In many respects, the Λ-CDM paradigm by to directly observe the evolving prop- is strikingly successful, especially in de- erties of the galaxy population over cos- scribing large-scale structure.
    [Show full text]
  • Kipac Annual Report 2017
    KIPAC ANNUAL REPORT 2017 KAVLI INSTITUTE FOR PARTICLE ASTROPHYSICS AND COSMOLOGY Contents 2 10 LZ Director 11 3 Deputy Maria Elena Directors Monzani 4 12 BICEP Array SuperCDMS 5 13 Zeeshan Noah Ahmed Kurinisky 6 14 COMAP Athena 7 15 Dongwoo Dan Wilkins Chung Adam Mantz 8 16 LSST Camera Young scientists 9 20 Margaux Lopez Solar eclipse Unless otherwise specified, all photographs credit of KIPAC. 22 Research 28 highlights Blinding it for science 22 EM counterparts 29 to gravity waves An X-ray view into black holes 23 30 Hidden knots of Examining where dark matter planets form 24 32 KIPAC together 34 Publications Galaxy dynamics and dark matter 36 KIPAC members 25 37 Awards, fellowships and doctorates H0LiCOW 38 KIPAC visitors and speakers 26 39 KIPAC alumni Simulating jets 40 Research update: DM Radio 27 South Pole 41 On the cover Telescope Pardon our (cosmic) dust We’re in the midst of exciting times here at the Kavli Institute for Particle Astro- physics and Cosmology. We’ve always managed to stay productive, with contri- butions big and small to a plethora of projects like the Fermi Gamma-ray Space Telescope, the Dark Energy Survey, the Nuclear Spectroscopic Telescope Array, the Gemini Planet Imager and many, many more—not to mention theory and data analysis, simulations, and research with publicly available data. We have no shortage of scientific topics to keep us occupied. But we are currently hard at work building a variety of new experimental instru- ments, and preparing to reap the benefits of some very long-range planning that will keep KIPAC scientists busy studying our universe in almost every wavelength and during almost every major epoch of the evolution of the universe, into the late 2020s and beyond.
    [Show full text]
  • Arxiv:Astro-Ph/0612305V1 12 Dec 2006 Giavalisco .Scoville N
    The Cosmic Evolution Survey (COSMOS) – Overview N. Scoville1,2, H. Aussel17, M. Brusa5, P. Capak1, C. M. Carollo8, M. Elvis3, M. Giavalisco4, L. Guzzo15, G. Hasinger5, C. Impey6, J.-P. Kneib7, O. LeFevre7, S. J. Lilly8, B. Mobasher4, A. Renzini9,19, R. M. Rich18, D. B. Sanders10, E. Schinnerer11,12, D. Schminovich13, P. Shopbell1, Y. Taniguchi14, N. D. Tyson16 arXiv:astro-ph/0612305v1 12 Dec 2006 –2– ⋆Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by AURA Inc, under NASA contract NAS 5-26555; also based on data collected at : the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan; the XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA; the European Southern Observatory under Large Program 175.A-0839, Chile; Kitt Peak National Observatory, Cerro Tololo Inter-American Observatory, and the National Optical As- tronomy Observatory, which are operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation; the National Radio Astronomy Observatory which is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc ; and the Canada-France-Hawaii Telescope with MegaPrime/MegaCam operated as a joint project by the CFHT Corporation, CEA/DAPNIA, the NRC and CADC of Canada, the CNRS of France, TERAPIX and the Univ. of Hawaii.
    [Show full text]
  • COSMOS-21 COSMIC EVOLUTION SURVEY COSMOS 2-Sq
    COSMIC EVOLUTION SURVEY COSMOS 2-sq. degree survey COSMOS-21 COSMOS Status Subaru S05B-S06A Previous S-cam Runs Intensive Program Taniguchi et al. COSMOS-21 KeyKey IssuesIssues && KeyKey WordsWords Extragalactic Astronomy Observational Cosmology Evolution of Galaxies, AGNs, & DM as a function of Large Scale Structure Evolution MultiMulti--λλ StrategyStrategy w/w/ GreatGreat ObservatoriesObservatories CurrentCurrent StatusStatus ofof thethe COSMOSCOSMOS •• HSTHST (I814):(I814): donedone •• Subaru:Subaru: COSMOSCOSMOS--77 •• VLTVLT zz--COSMOS:COSMOS: ~5,000~5,000 objectobject •• XMM,XMM, VLA,VLA, GALEX:GALEX: donedone •• SSTSST ss--COSMOS:COSMOS: goinggoing onon (GO2)(GO2) •• HSTHST (g(g’’),), CXO:CXO: notnot yetyet •• 11st YearYear PhotoPhoto--zz CatalogCatalog releasedreleased !! •• ApJApJ SpecialSpecial IssueIssue (submit(submit byby Sep)Sep) ScienceScience SteeringSteering CommiteeCommitee •• NickNick Scoville,Scoville, •• AlvioAlvio Renzini,Renzini, •• DaveDave SandersSanders ,, •• MauroMauro Giavalisco,Giavalisco, •• OlivierOlivier LeFevreLeFevre,, •• YoshiYoshi Taniguchi,Taniguchi, •• ChrisChris Impey,Impey, •• MartinMartin Elvis,Elvis, •• SimonSimon Lilly,Lilly, •• MikeMike Rich,Rich, •• EvaEva SchinnerrerSchinnerrer COSMOSCOSMOS WorkingWorking GroupsGroups •• DataData ProductsProducts •• LargeLarge ScaleScale StructureStructure •• StarStar FormationFormation •• AGNAGN •• MorphologyMorphology •• LensingLensing •• HighHigh--zz 11stst YearYear PhotoPhoto--zz CatalogCatalog [1][1] SS--camcam rr ’’--selectedselected catalogcatalog (r(r
    [Show full text]
  • Cosmological Evolution of the Galaxy Merger Rate from MUSE Deep Fields Emmy Ventou
    Cosmological evolution of the galaxy merger rate from MUSE deep fields Emmy Ventou To cite this version: Emmy Ventou. Cosmological evolution of the galaxy merger rate from MUSE deep fields. Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]. Université Paul Sabatier - Toulouse III, 2018. English. NNT : 2018TOU30323. tel-02475982 HAL Id: tel-02475982 https://tel.archives-ouvertes.fr/tel-02475982 Submitted on 12 Feb 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. THÈSE En vue de l’obtention du DOCTORAT DE L’UNIVERSITÉ DE TOULOUSE Délivré par l'Université Toulouse 3 - Paul Sabatier Présentée et soutenue par Emmy VENTOU Le 21 décembre 2018 Evolution cosmologique du taux de fusion des galaxies à partir des champs profonds MUSE Ecole doctorale : SDU2E - Sciences de l'Univers, de l'Environnement et de l'Espace Spécialité : Astrophysique, Sciences de l'Espace, Planétologie Unité de recherche : IRAP - Institut de Recherche en Astrophysique et Planetologie Thèse dirigée par Thierry CONTINI et Benoît EPINAT Jury M. Olivier LE FèVRE, Rapporteur M. Christopher CONSELICE, Rapporteur Mme Anne VERHAMME, Examinatrice M. Nicolas BOUCHE, Examinateur Mme Genevieve SOUCAIL, Examinatrice M. Carlos LOPEZ SAN JUAN, Examinateur M.
    [Show full text]
  • COSMOS (Cosmic Evolution Survey)
    COSMOS (cosmic evolution survey) Richard Massey with Nick Scoville, Roberto Abraham, Masaru Ajiki, Justin Alpert, Herve Aussel, Josh Barnes, Andrew Blain, Daniela Calzetti, Peter Capak, John Weak lensing results fromCarlstrom, the ChrisHST Carilli, Andrea Cimatti, Andrea Comastri, Marcella Corollo, Emannuel Daddi, Richard Ellis, Martin Elvis, COSMOS survey Amr El Zant, Shawn Ewald, Mike Fall, Alexis Finoguenov, Alberto Franceschini, Mauro Giavalisco, Richard Griffiths, Gigi Guzzo, Gunther Hasinger, Catherine Heymans, Chris Impey, Jean- Paul Kneib, Karel Nel, Jeyhan Kartaltepe, Jin Koda, Anton Koekemoer, Lisa Kewley, Alexie Leauthaud, Olivier LeFevre, Ingo Lehmann, Simon Lilly, Thorsten Lisker, Charles Liu, Henry McCracken, Yannick Mellier, Satoshi Miyazaki, Bahram Mobasher, Takashi Murayama, Colin Norman, Alex Refregier, Alvio Renzini, Jason Rhodes, Mike Rich, Dimitra Rigopoulou, Dave Sanders, Shunji Sasaki, Dave Schminovich, Eva Schinnerer, Marco Scodeggio, Kartik Sheth, Patrick Shopbell, Jason Surace, Yoshi Taniguchi, James Taylor, Dave Thompson, Neil Tyson, Meg Urry, Ludovic Van Waerbeke, Paolo Vettolani, Simon White, Lin Yan The view from Hubble QuickTime™ and a decompressor are needed to see this picture. Hubble Space Telescope data N. Scoville et al. (ApJ 2007) Largest ever HST survey • 577 contiguous ACS pointings • 1.6 square degrees in IF814W band (VSDSS at z=1) • Depth IF814W<26.6 (at 5) • 2 million galaxies • ~80 resolved galaxies/arcmin2 http://irsa.ipac.caltech.edu/Missions/cosmos.html Multicolour followup of COSMOS field P. Capak et al. (ApJ 2007), B. Mobasher et al. (ApJ 2007) Radio Δz/(1+z)= 0.05 , 0.15 X-ray Large-scale distribution of baryonic material N. Scoville et al. (ApJ 2007) Large-scale distribution of baryonic material QuickTime™ and a QuickTime™ and a YUV420 codec decompressor YUV420 codec decompressor are needed to see this picture.
    [Show full text]
  • Curriculum Vitae Jonathan R. Trump
    Curriculum Vitae Jonathan R. Trump Dept of Physics (860) 486-6310 (office) University of Connecticut (520) 260-4633 (cell) 2152 Hillside Rd, U-3046 (860) 486-3346 (FAX) Storrs, CT 06269 [email protected] http://phys.uconn.edu/∼jtrump/ Professional Appointments 8/2016-current Assistant Professor, Dept of Physics, University of Connecticut 9/2013-8/2016 Hubble Fellow, Penn State University 9/2010-8/2013 DEEP Postdoctoral Scholar, UC Santa Cruz 7/2004-8/2010 Graduate Researcher, University of Arizona 6/2008-8/2008 NSF/JSPS Summer Research Fellow, Ehime University 1/2002-6/2004 Undergraduate Researcher, Penn State University Education 2010 Ph.D University of Arizona, Astronomy, Thesis: Supermassive Black Hole Ac- tivity in the Cosmic Evolution Survey (advisor: Chris Impey) 2004 B.S. Penn State University, Astronomy, summa cum laude, Honors Thesis: Broad Absorption Line Quasars in the Sloan Digital Sky Survey 2004 B.S. Penn State University, Physics, summa cum laude Successful Proposals (selected) - $1.5M in active grants 2020 PI, NSF CAREER: Echo Mapping the Census of Supermassive Black Hole Mass, Accretion, and Spin, $740k 2019 PI, NASA ADAP: Spectral Energy Distributions of Echo-Mapped Quasars, $540k 2018 PI, HST proposal: Ultraviolet Echoes of Quasar Accretion Disks, 40 orbits, $208k 2017 co-I, JWST ERS proposal: The Cosmic Evolution Early Release Science Survey, 63 hrs, $130k (as co-I) 2017 PI, HST proposal: Ultraviolet Echoes of Quasar Accretion Disks, 32 orbits, $135k 2015 co-PI, NSF AAG: The First Multi-Object Reverberation Mapping
    [Show full text]
  • The ASTRONET Infrastructure Roadmap
    The ASTRONET Infrastructure Roadmap: A Strategic Plan for European Astronomy The ASTRONET Infrastructure Roadmap: A Strategic Plan for European Astronomy European for Plan A Strategic Roadmap: Infrastructure The ASTRONET The ASTRONET Infrastructure Roadmap This document has been created by the Infrastructure Roadmap Working Group and Panels under the auspices of ASTRONET, acting on behalf of the following member agencies: ARRS (SI), BMBF and PT-DESY (DE), IA CAS (CZ), CNRS/INSU (FR), DFG (DE), ESA (INT), ESO (INT), ESF (EE), FWF (AT), GNCA (GR), HAS (HU), SAS (SK), INAF (IT), LAS (LT), MICINN (ES), MPG (DE), NCBiR (PL), NOTSA (Nordic), NWO (NL), RSA (RO), SER (CH), SRC (SE), STFC (UK), UAS (UA). Editors: Michael F. Bode, Maria J. Cruz & Frank J. Molster ISBN: 978-3-923524-63-1 Acknowledgments: The ASTRONET project has been made possible via the generous support of the European Commission through Framework Programme 6. We gratefully acknowledge the tremendous amount of work that has been undertaken by the total of over 60 scientists and programme managers from across Europe who have given their time to the formulation of the Infrastructure Roadmap with dedication and enthusiasm. We acknowledge the help received from the ‘computergroep’ of the Leiden Observatory in setting up and hosting the web-based discussion forum. We also thank the Liverpool John Moores University Conference and Events team, Computing and Information Services department and the staff and students of the LJMU Astrophysics Research Institute who helped with the organisation and running of the Roadmap Symposium, and the astronomical community at large for their invaluable input to the whole process.
    [Show full text]
  • Chris Impey — Curriculum Vita
    Chris Impey- Curriculum Vita 1 Chris Impey — Curriculum Vita Contents 1 Personal……………………………………………………………. 2 2 Education………………………………………………………….. 2 3 Appointments……………………………………………………… 2 4 Professional Awards……………………………………………….. 3 5 Professional Societies………………………………………………. 3 6 Departmental Service………………………………………………. 3 7 University Service…………………………………………………... 4 8 Astronomy Service…………………………………………………. 7 9 University Teaching Awards and Grants……………………………. 9 10 Teaching Experience………………………………………………… 9 11 Student Advising……………………………………………………. 10 12 Observing Experience……………………………………………… 12 13 Invited Educational Presentations………………………………….. 12 14 Invited Research Presentations……………………………………… 18 15 Books Authored…………………………………………………….. 20 16 Books Edited……………………………………………………….. 21 17 Educational Publications…………………………………………… 22 18 Astronomy Refereed Publications ………..………………………… 26 19 Published Conference Proceedings…………………………………. 40 20 Educational Grants Awarded……………………………………….. 46 21 Research Grants Awarded…………………………………………... 48 Chris Impey- Curriculum Vita 2 1 Personal Born: 25 January 1956, Edinburgh, Scotland British Citizen; U.S. Permanent Resident 2 Education B.Sc., Physics, 1977, University of London (1st Class Honors) Ph.D., Astronomy, 1981, University of Edinburgh, Scotland Thesis Title: Polarization Studies of BL Lac Objects Thesis Directors: R.D. Wolstencroft and P.W.J.L. Brand Foreign Languages: Spanish (strong) and French (fair) 3 Appointments Research Assistant, Centre European pour la Recherche Nuclear (CERN), Geneva, Switzerland,
    [Show full text]