The UKIRT Infrared Deep Sky Survey (UKIDSS)
Andy Lawrence,Stephen J. Warren,Omar Almaini,Alastair C. Edge,Nigel Hambly,Richard F. Jameson,Philip W. Lucas,M. Casali,Andrew J. Adamson,Simon Dye,J. P. Emerson,S. Foucaud,P. C. Hewett,Paul Hirst,Simon Hodgkin,Mike Irwin,N. Lodieu,Richard G. McMahon,Chris Simpson,Chris Simpson,Ian Smail,Daniel J. Mortlock,M. Folger +22 more
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The final version published in MNRAS August 2007 included significant revisions including significant revisions to the original version April 2006.Abstract:
Final published version including significant revisions. Twenty four pages, fourteen figures. Original version April 2006; final version published in MNRAS August 2007read more
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SPECTRAL ENERGY DISTRIBUTIONS OF QSOs AT z > 5: COMMON ACTIVE GALACTIC NUCLEUS-HEATED DUST AND OCCASIONALLY STRONG STAR-FORMATION
C. Leipski,Klaus Meisenheimer,Fabian Walter,Ulrich Klaas,Helmut Dannerbauer,G. De Rosa,X. Fan,M. Haas,Oliver Krause,H. W. Rix +9 more
TL;DR: In this article, spectral energy distributions of 69 QSOs at z > 5, covering a rest frame wavelength range of 0.1 μm to ~80 μm, were presented.
Journal ArticleDOI
The galaxy-halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS field
Jean Coupon,Stéphane Arnouts,L. van Waerbeke,T. Moutard,O. Ilbert,E. van Uitert,Thomas Erben,B. Garilli,Luigi Guzzo,Luigi Guzzo,Catherine Heymans,Hendrik Hildebrandt,Henk Hoekstra,Martin Kilbinger,Thomas D. Kitching,Yannick Mellier,Lance Miller,Marco Scodeggio,C. Bonnett,Enzo Branchini,Enzo Branchini,I. Davidzon,I. Davidzon,G. De Lucia,Alexander Fritz,Liping Fu,P. Hudelot,Michael J. Hudson,Michael J. Hudson,Konrad Kuijken,Alexie Leauthaud,O. Le Fevre,H. J. McCracken,Lauro Moscardini,Lauro Moscardini,Barnaby Rowe,Tim Schrabback,E. Semboloni,Malin Velander +38 more
TL;DR: In this paper, the authors present new constraints on the relationship between galaxies and their host dark matter haloes, measured from the location of the peak of the stellar-to-halo mass ratio (SHMR), up to the most massive galaxy clusters at redshift z ∼ 0.8 and over a volume of nearly 0.1 Gpc3.
Journal ArticleDOI
SLOAN LOW-MASS WIDE PAIRS OF KINEMATICALLY EQUIVALENT STARS (SLoWPoKES): A CATALOG OF VERY WIDE, LOW-MASS PAIRS
Saurav Dhital,Andrew A. West,Andrew A. West,Keivan G. Stassun,Keivan G. Stassun,John J. Bochanski +5 more
TL;DR: The Sloan Low-mass Wide Pairs of Kinematically equivalent Stars (SLoWPoKES) as discussed by the authors is a large collection of very wide (projected separation 500 AU) common proper motion pairs identified from the Sloan Digital Sky Survey.
Journal ArticleDOI
The sloan digital sky survey quasar lens search. v. final catalog from the seventh data release
Naohisa Inada,Naohisa Inada,Masamune Oguri,Min-Su Shin,Min-Su Shin,Issha Kayo,Issha Kayo,Michael A. Strauss,Tomoki Morokuma,Cristian E. Rusu,Masataka Fukugita,Masataka Fukugita,Christopher S. Kochanek,Gordon T. Richards,Donald P. Schneider,Donald G. York,Neta A. Bahcall,Joshua A. Frieman,Joshua A. Frieman,Patrick B. Hall,Richard L. White +20 more
TL;DR: In this article, the final statistical sample of lensed quasars from the Sloan Digital Sky Survey (SDSS) Quasar Lens Search (SQLS) was presented.
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Are Compton-thick AGNs the missing link between mergers and black hole growth?
Dale D. Kocevski,Murray Brightman,Kirpal Nandra,Anton M. Koekemoer,Mara Salvato,James Aird,Eric F. Bell,Li Ting Hsu,Jeyhan S. Kartaltepe,David C. Koo,Jennifer M. Lotz,Daniel H. McIntosh,Mark Mozena,David J. Rosario,Jonathan R. Trump +14 more
TL;DR: In this article, the authors examined the host morphologies of heavily obscured active galactic nuclei (AGNs) at z = 1 to test whether obscured super-massive black hole growth at this epoch is preferentially linked to galaxy mergers.
References
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The Two Micron All Sky Survey (2MASS)
Michael F. Skrutskie,Michael F. Skrutskie,Roc M. Cutri,R. Stiening,Martin D. Weinberg,Stephen E. Schneider,John M. Carpenter,Chas Beichman,R. Capps,T. Chester,J. Elias,John P. Huchra,James Liebert,C. Lonsdale,David G. Monet,Stephan D. Price,Patrick Seitzer,Thomas H. Jarrett,J. D. Kirkpatrick,John E. Gizis,E. Howard,T. Evans,John W. Fowler,L. Fullmer,Robert L. Hurt,R. M. Light,E. L. Kopan,K. A. Marsh,H. McCallon,R. Tam,S. D. Van Dyk,S. Wheelock +31 more
TL;DR: The Two Micron All Sky Survey (2MASS) as mentioned in this paper collected 25.4 Tbytes of raw imaging data from two dedicated 1.3 m diameter telescopes located at Mount Hopkins, Arizona and CerroTololo, Chile.
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The Sloan Digital Sky Survey: Technical Summary
TL;DR: The Sloan Digital Sky Survey (SDSS) as mentioned in this paper provides the data to support detailed investigations of the distribution of luminous and non-luminous matter in the Universe: a photometrically and astrometrically calibrated digital imaging survey of pi steradians above about Galactic latitude 30 degrees in five broad optical bands.
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The Sloan Digital Sky Survey: Technical summary
Donald G. York,Jennifer Adelman,John E. Anderson,Scott F. Anderson,James Annis,Neta A. Bahcall,J. A. Bakken,Robert H. Barkhouser,Steven Bastian,E. Berman,William N. Boroski,Steve Bracker,Charlie Briegel,John W. Briggs,Jon Brinkmann,Robert J. Brunner,Scott Burles,Larry N. Carey,Michael A. Carr,Francisco J. Castander,Francisco J. Castander,Bing Chen,Patrick L. Colestock,Andrew J. Connolly,James H. Crocker,István Csabai,István Csabai,Paul C. Czarapata,John Eric Davis,Mamoru Doi,Tom Dombeck,Daniel J. Eisenstein,Nancy Ellman,Brian R. Elms,Brian R. Elms,Michael L. Evans,Xiaohui Fan,Glenn R. Federwitz,Larry Fiscelli,Scott D. Friedman,Joshua A. Frieman,Joshua A. Frieman,Masataka Fukugita,Bruce Gillespie,James E. Gunn,Vijay K. Gurbani,Ernst De Haas,M. Haldeman,Frederick H. Harris,Jeffrey J. E. Hayes,Timothy M. Heckman,Gregory S. Hennessy,Robert B. Hindsley,S. Holm,Donald J. Holmgren,Chi Hao Huang,Charles L. Hull,Don Husby,Shin-Ichi Ichikawa,Takashi Ichikawa,Zěljko Ivezić,Stephen M. Kent,Rita S. J. Kim,E. Kinney,Mark A. Klaene,A. N. Kleinman,Scot Kleinman,Gillian R. Knapp,John Korienek,Richard G. Kron,Richard G. Kron,Peter Z. Kunszt,D. Q. Lamb,Brian C. Lee,R. French Leger,Siriluk Limmongkol,Carl Lindenmeyer,Dan Long,Craig Loomis,Jon Loveday,Rich Lucinio,Robert H. Lupton,Bryan Mackinnon,Bryan Mackinnon,Edward J. Mannery,Paul M. Mantsch,Bruce Margon,Peregrine M. McGehee,Timothy A. McKay,Avery Meiksin,Aronne Merelli,David G. Monet,Jeffrey A. Munn,Vijay K. Narayanan,Thomas Nash,Eric H. Neilsen,Rich Neswold,Heidi Jo Newberg,Heidi Jo Newberg,Robert C. Nichol,T. Nicinski,T. Nicinski,Mario Nonino,Norio Okada,Sadanori Okamura,Jeremiah P. Ostriker,Russell Owen,A. George Pauls,John Peoples,R. Peterson,Don Petravick,Jeffrey R. Pier,Adrian Pope,Ruth Pordes,Angela Prosapio,R. Rechenmacher,Thomas R. Quinn,Gordon T. Richards,Michael Richmond,Claudio H. Rivetta,Constance M. Rockosi,Kurt Ruthmansdorfer,Dale Sandford,David J. Schlegel,Donald P. Schneider,Maki Sekiguchi,G. Sergey,Kazuhiro Shimasaku,Walter A. Siegmund,Stephen A. Smee,J. Allyn Smith,S. A. Snedden,Robert Stone,Chris Stoughton,Michael A. Strauss,Christopher W. Stubbs,Mark SubbaRao,Alexander S. Szalay,István Szapudi,Gyula P. Szokoly,Anirudda R. Thakar,Christy Tremonti,Douglas L. Tucker,Alan Uomoto,Daniel E. Vanden Berk,Michael S. Vogeley,Patrick Waddell,Shu I. Wang,Masaru Watanabe,David H. Weinberg,Brian Yanny,Naoki Yasuda +151 more
TL;DR: The Sloan Digital Sky Survey (SDSS) as discussed by the authors provides the data to support detailed investigations of the distribution of luminous and non-luminous matter in the universe: a photometrically and astrometrically calibrated digital imaging survey of π sr above about Galactic latitude 30° in five broad optical bands to a depth of g' ~ 23 mag.
Astronomical Data Analysis Software and Systems
TL;DR: The ADS abstract service at: http://adswww.harvard.edu has been updated considerably in the last year and new capabilities in the search engine include searching for multi-word phrases and searching for various logical combinations of search terms.
Journal ArticleDOI
The optical and near-infrared properties of galaxies. I. Luminosity and stellar mass functions
TL;DR: In this article, a large sample of galaxies from the 2MASS and the Sloan Digital Sky Survey (SDSS) was used to calculate galaxy luminosity and stellar mass functions in the local Universe.
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