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SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS
Eisenstein, DJ; Weinberg, DH; Agol, E; Aihara, H; Prieto, CA; Anderson, SF; Arns, JA; Aubourg, E; Bailey, S; Balbinot, E; Barkhouser, R; Beers, TC; Berlind, AA; Bickerton, SJ; Bizyaev, D; Blanton, MR; Bochanski, JJ; Bolton, AS; Bosman, CT; Bovy, J; Brandt, WN; Breslauer, B; Brewington, HJ; Brinkmann, J; Brown, PJ; Brownstein, JR; Burger, D; Busca, NG; Campbell, H; Cargile, PA; Carithers, WC; Carlberg, JK; Carr, MA; Chang L(常亮); Chen, YM; Chiappini, C; Comparat, J; Connolly, N; Cortes, M; Croft, RAC; Cunha, K; da Costa, LN; Davenport, JRA; Dawson, K; De Lee, N; de Mello, GFP; de Simoni, F; Dean, J; Dhital, S; Ealet, A; Ebelke, GL; Edmondson, EM; Eiting, JM; Escoffier, S; Esposito, M; Evans, ML; Fan, XH; Castella, BF; Ferreira, LD; Fitzgerald, G; Fleming, SW; Font-Ribera, A; Ford, EB; Frinchaboy, PM; Perez, AEG; Gaudi, BS; Ge, J; Ghezzi, L; Gillespie, BA; Gilmore, G; Girardi, L; Gott, JR; Gould, A; Grebel, EK; Gunn, JE; Hamilton, JC; Harding, P; Harris, DW; Hawley, SL; Hearty, FR; Hennawi, JF; Hernandez, JIG; Ho, S; Hogg, DW; Holtzman, JA; Honscheid, K; Inada, N; Ivans, II; Jiang, LH; Jiang, P; Johnson, JA; Jordan, C; Jordan, WP; Kauffmann, G; Kazin, E; Kirkby, D; Klaene, MA; Knapp, GR; Kneib, JP; Kochanek, CS; Koesterke, L; Kollmeier, JA; Kron, RG; Lampeitl, H; Lang, D; Lawler, JE; Le Goff, JM; Lee, BL; Lee, YS; Leisenring, JM; Lin, YT; Liu, J; Long, DC; Loomis, CP; Lucatello, S; Lundgren, B; Lupton, RH; Ma, B; Ma, ZB; MacDonald, N; Mack, C; Mahadevan, S; Maia, MAG; Majewski, SR; Makler, M; Malanushenko, E; Malanushenko, V; Mandelbaum, R; Maraston, C; Margala, D; Maseman, P; Masters, KL; McBride, CK; McDonald, P; McGreer, ID; McMahon, RG; Requejo, OM; Menard, B; Miralda-Escude, J; Morrison, HL; Mullally, F; Muna, D; Murayama, H; Myers, AD; Naugle, T; Neto, AF; Nguyen, DC; Nichol, RC; Nidever, DL; O'Connell, RW; Ogando, RLC; Olmstead, MD; Oravetz, DJ; Padmanabhan, N; Paegert, M; Palanque-Delabrouille, N; Pan, KK; Pandey, P; Parejko, JK; Paris, I; Pellegrini, P; Pepper, J; Percival, WJ; Petitjean, P; Pfaffenberger, R; Pforr, J; Phleps, S; Pichon, C; Pieri, MM; Prada, F; Price-Whelan, AM; Raddick, MJ; Ramos, BHF; Reid, IN; Reyle, C; Rich, J; Richards, GT; Rieke, GH; Rieke, MJ; Rix, HW; Robin, AC; Rocha-Pinto, HJ; Rockosi, CM; Roe, NA; Rollinde, E; Ross, AJ; Ross, NP; Rossetto, B; Sanchez, AG; Santiago, B; Sayres, C; Schiavon, R; Schlegel, DJ; Schlesinger, KJ; Schmidt, SJ; Schneider, DP; Sellgren, K; Shelden, A; Sheldon, E; Shetrone, M; Shu, YP; Silverman, JD; Simmerer, J; Simmons, AE; Sivarani, T; Skrutskie, MF; Slosar, A; Smee, S; Smith, VV; Snedden, SA; Stassun, KG; Steele, O; Steinmetz, M; Stockett, MH; Stollberg, T; Strauss, MA; Szalay, AS; Tanaka, M; Thakar, AR; Thomas, D; Tinker, JL; Tofflemire, BM; Tojeiro, R; Tremonti, CA; Magana, MV; Verde, L; Vogt, NP; Wake, DA; Wan, XK; Wang, J; Weaver, BA; White, M; White, SDM; Wilson, JC; Wisniewski, JP; Wood-Vasey, WM; Yanny, B; Yasuda, N; Yeche, C; York, DG; Young, E; Zasowski, G; Zehavi, I; Zhao, B; Eisenstein, DJ (reprint author), Univ Arizona, Steward Observ, Tucson, AZ 85721 USA.
Source PublicationASTRONOMICAL JOURNAL
2011-09
Volume142Issue:3
DOI10.1088/0004-6256/142/3/72
Contribution Rank第27完成单位
Indexed BySCI
KeywordCosmology: Observations Galaxy: Evolution Planets And Satellites: Detection Surveys
AbstractBuilding on the legacy of the Sloan Digital Sky Survey (SDSS-I and II), SDSS-III is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars. In keeping with SDSS tradition, SDSS-III will provide regular public releases of all its data, beginning with SDSS Data Release 8 (DR8), which was made public in 2011 January and includes SDSS-I and SDSS-II images and spectra reprocessed with the latest pipelines and calibrations produced for the SDSS-III investigations. This paper presents an overview of the four surveys that comprise SDSS-III. The Baryon Oscillation Spectroscopic Survey will measure redshifts of 1.5 million massive galaxies and Ly alpha forest spectra of 150,000 quasars, using the baryon acoustic oscillation feature of large-scale structure to obtain percent-level determinations of the distance scale and Hubble expansion rate at z < 0.7 and at z approximate to 2.5. SEGUE-2, an already completed SDSS-III survey that is the continuation of the SDSS-II Sloan Extension for Galactic Understanding and Exploration (SEGUE), measured medium-resolution (R = lambda/lambda Delta approximate to 1800) optical spectra of 118,000 stars in a variety of target categories, probing chemical evolution, stellar kinematics and substructure, and the mass profile of the dark matter halo from the solar neighborhood to distances of 100 kpc. APOGEE, the Apache Point Observatory Galactic Evolution Experiment, will obtain high-resolution (R approximate to 30,000), high signal-to-noise ratio (S/N >= 100 per resolution element), H-band (1.51 mu m < lambda < 1.70 mu m) spectra of 105 evolved, late-type stars, measuring separate abundances for similar to 15 elements per star and creating the first high-precision spectroscopic survey of all Galactic stellar populations (bulge, bar, disks, halo) with a uniform set of stellar tracers and spectral diagnostics. The Multi-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS) will monitor radial velocities of more than 8000 FGK stars with the sensitivity and cadence (10-40 ms(-1), similar to 24 visits per star) needed to detect giant planets with periods up to two years, providing an unprecedented data set for understanding the formation and dynamical evolution of giant planet systems. As of 2011 January, SDSS-III has obtained spectra of more than 240,000 galaxies, 29,000 z >= 2.2 quasars, and 140,000 stars, including 74,000 velocity measurements of 2580 stars for MARVELS.
Funding OrganizationAlfred P. Sloan Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; University of Arizona ; Brazilian Participation Group ; Brookhaven National Laboratory ; University of Cambridge ; Carnegie Mellon University ; University of Florida ; French Participation Group ; German Participation Group ; Harvard University ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; New Mexico State University ; New York University ; Ohio State University ; Pennsylvania State University ; University of Portsmouth ; Princeton University ; Spanish Participation Group ; University of Tokyo ; University of Utah ; Vanderbilt University ; University of Virginia ; University of Washington ; Yale University
Language英语
Subject AreaAstronomy & Astrophysics
SubtypeArticle
ISSN0004-6256
URL查看原文
WOS IDWOS:000294669700006
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordDIGITAL SKY SURVEY ; BARYON ACOUSTIC-OSCILLATIONS ; SURVEY COMMISSIONING DATA ; LUMINOUS RED GALAXIES ; LENS ACS SURVEY ; STELLAR ATMOSPHERIC PARAMETERS ; SAGITTARIUS DWARF GALAXY ; VELOCITY EXPERIMENT RAVE ; ULTRACOOL WHITE-DWARFS ; INFRARED CAII TRIPLET
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Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/5403
Collection丽江天文观测站(南方基地)
Corresponding AuthorEisenstein, DJ (reprint author), Univ Arizona, Steward Observ, Tucson, AZ 85721 USA.
Recommended Citation
GB/T 7714
Eisenstein, DJ,Weinberg, DH,Agol, E,et al. SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS[J]. ASTRONOMICAL JOURNAL,2011,142(3).
APA Eisenstein, DJ.,Weinberg, DH.,Agol, E.,Aihara, H.,Prieto, CA.,...&Eisenstein, DJ .(2011).SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS.ASTRONOMICAL JOURNAL,142(3).
MLA Eisenstein, DJ,et al."SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS".ASTRONOMICAL JOURNAL 142.3(2011).
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