SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS
Daniel J. EisensteinHarvard College Observatory, Cambridge, MA 02138, USADavid H. WeinbergCenter for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210, USAEric AgolDepartment of Astronomy, University of Washington, Seattle, WA 98195, USAH. AiharaThe University of TokyoCarlos Allende PrietoDepartamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, SpainScott F. AndersonDepartment of Astronomy, University of Washington, Seattle, WA 98195, USAJames A. ArnsKaiser Optical Systems, Ann Arbor, MI 48103, USAÉ. AubourgInstitut de Recherche sur les Lois Fondamentales de l'UniversS. BaileyLawrence Berkeley National Laboratory, Berkeley, CA 94720, USAE. BalbinotInstituto de Física, UFRGS, Porto Alegre, RS 91501-970, BrazilRobert H. BarkhouserCenter for Astrophysical Sciences, Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USATimothy C. BeersMichigan State UniversityAndreas A. BerlindDepartment of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235, USASteven J. BickertonDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USADmitry BizyaevMichael R. BlantonCenter for Cosmology and Particle Physics, New York University, New York, NY 10003, USAJohn J. BochanskiDepartment of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USAA. BoltonDepartment of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USACasey T. BosmanDepartment of Astronomy, University of Florida, Bryant Space Science Center, Gainesville, FL 32611-2055, USAJo BovyCenter for Cosmology and Particle Physics, New York University, New York, NY 10003, USAW. N. BrandtDepartment of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USAB. BreslauerDepartment of Astronomy, University of Virginia, Charlottesville, VA 22904-4325, USAH. BrewingtonJ. BrinkmannPeter J. BrownDepartment of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USAJoel R. BrownsteinDepartment of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USADan BürgerDepartment of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235, USANicolás G. BuscaLaboratoire AstroParticule et CosmologieH. CampbellInstitute of Cosmology and Gravitation (ICG), University of Portsmouth, Portsmouth, PO1 3FX, UKPhillip A. CargileDepartment of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235, USAW. CarithersLawrence Berkeley National Laboratory, Berkeley, CA 94720, USAJoleen K. CarlbergDepartment of Astronomy, University of Virginia, Charlottesville, VA 22904-4325, USAMichael A. CarrDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USALiang ChangDepartment of Astronomy, University of Florida, Bryant Space Science Center, Gainesville, FL 32611-2055, USAYanmei ChenDepartment of Astronomy, University of Wisconsin–Madison, Madison, WI 53706-1582, USAC. ChiappiniLaboratório Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro, RJ 20921-400, BrazilJohan ComparatLaboratoire d'Astrophysique de Marseille, CNRS-Université de Provence, 13388 Marseille Cedex 13, FranceN. ConnollyDepartment of Physics, Hamilton College, Clinton, NY 13323, USAMarina CortêsLawrence Berkeley National Laboratory, Berkeley, CA 94720, USARupert A. C. CroftBruce and Astrid McWilliams Center for Cosmology, Carnegie Mellon University, Pittsburgh, PA 15213, USAKátia CunhaNational Optical Astronomy Observatory, Tucson, AZ 85719, USALuiz N. da CostaLaboratório Interinstitucional de e-AstronomiaJames R. A. DavenportDepartment of Astronomy, University of Washington, Seattle, WA 98195, USAKyle DawsonDepartment of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USANathan De LeeDepartment of Astronomy, University of Florida, Bryant Space Science Center, Gainesville, FL 32611-2055, USAG. F. Porto de MelloObservatório do Valongo, Universidade Federal do Rio de Janeiro, Ladeira do Pedro Antônio 43, 20080-090 Rio de Janeiro, BrazilF. de SimoniLaboratório Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro, RJ 20921-400, BrazilJanice DeanDepartment of Astronomy, University of Virginia, Charlottesville, VA 22904-4325, USASaurav DhitalDepartment of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235, USAAnne EaletInstitut National de Physique Nucléaire et de Physique des ParticulesGarrett EbelkeApache Point Observatory, Sunspot, NM 88349, USAEdward M. EdmondsonInstitute of Cosmology and Gravitation (ICG), University of Portsmouth, Portsmouth, PO1 3FX, UKJ. EitingDepartment of Physics, Ohio State University, Columbus, OH 43210, USAS. EscoffierInstitut National de Physique Nucléaire et de Physique des ParticulesM. EspositoDepartamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, SpainMichael L. EvansDepartment of Astronomy, University of Washington, Seattle, WA 98195, USAXiaohui FanBruno Femenía CastelláInstituto de Astrofísica de Canarias, E38205 La Laguna, Tenerife, SpainLetícia D. FerreiraLaboratório Interinstitucional de e-AstronomiaGreg FitzgeraldScott W. FlemingDepartment of Astronomy, University of Florida, Bryant Space Science Center, Gainesville, FL 32611-2055, USAAndreu Font-RiberaInstitut de Ciéncies de l’Espai (CSIC-IEEC), 08193 Bellaterra, Barcelona, SpainEric B. FordDepartment of Astronomy, University of Florida, Bryant Space Science Center, Gainesville, FL 32611-2055, USAPeter M. FrinchaboyDepartment of Physics & Astronomy, Texas Christian University, Fort Worth, TX 76129, USAA. E. García PérezDepartment of Astronomy, University of Virginia, Charlottesville, VA 22904-4325, USAB. Scott GaudiDepartment of Astronomy, Ohio State University, Columbus, OH 43210, USAJian GeDepartment of Astronomy, University of Florida, Bryant Space Science Center, Gainesville, FL 32611-2055, USALuan GhezziLaboratório Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro, RJ 20921-400, BrazilBruce GillespieG. GilmoreInstitute of Astronomy, University of Cambridge, Cambridge, CB3 0HA, UKL. GirardiLaboratório Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro, RJ 20921-400, BrazilJ. Richard GottDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USAAndrew GouldDepartment of Astronomy, Ohio State University, Columbus, OH 43210, USAE. K. GrebelAstronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, 69120 Heidelberg, GermanyJames E. GunnDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USAJ.–Ch. HamiltonAstroparticule et Cosmologie (APC), Université Paris-Diderot, 75205 Paris Cedex 13, FrancePaul HardingDepartment of Astronomy, Case Western Reserve University, Cleveland, OH 44106, USAD. E. HarrisDepartment of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USASuzanne L. HawleyDepartment of Astronomy, University of Washington, Seattle, WA 98195, USAFrederick R. HeartyDepartment of Astronomy, University of Virginia, Charlottesville, VA 22904-4325, USAJoseph F. HennawiMax-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, GermanyJ. I. Gónzalez HernándezInstituto de Astrofísica de Canarias, E38205 La Laguna, Tenerife, SpainShirley HoLawrence Berkeley National Laboratory, Berkeley, CA 94720, USADavid W. HoggCenter for Cosmology and Particle Physics, New York University, New York, NY 10003, USAJon A. HoltzmanDepartment of Astronomy, MSC 4500, New Mexico State University, Las Cruces, NM 88003, USAKlaus HonscheidCenter for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210, USANaohisa InadaResearch Center for the Early Universe, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, JapanInese I. IvansDepartment of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USALinhua JiangPeng JiangKey Laboratory for Research in Galaxies and Cosmology, The University of Science and Technology of China, Chinese Academy of Sciences, Hefei, Anhui 230026, ChinaJennifer A. JohnsonCenter for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210, USAC. JordanWendell P. JordanApache Point Observatory, Sunspot, NM 88349, USAGuinevere KauffmannMax-Planck-Institut für Astrophysik, D-85748 Garching, GermanyEyal KazinCenter for Cosmology and Particle Physics, New York University, New York, NY 10003, USAD. KirkbyDepartment of Physics and Astronomy, University of California, Irvine, CA 92697, USAMark A. KlaeneG. R. KnappDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USAJean‐Paul KneibLaboratoire d’Astrophysique de Marseille, CNRS-Université de Provence, 13388 Marseille Cedex 13, FranceC. S. KochanekCenter for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210, USA
2011en
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Annotatsiya
Building 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 DR8 (which occurred in Jan 2011). This paper presents an overview of the four SDSS-III surveys. BOSS will measure redshifts of 1.5 million massive galaxies and Lya forest spectra of 150,000 quasars, using the BAO 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~2.5. SEGUE-2, which is now completed, measured medium-resolution (R=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 will obtain high-resolution (R~30,000), high signal-to-noise (S/N>100 per resolution element), H-band (1.51-1.70 micron) spectra of 10^5 evolved, late-type stars, measuring separate abundances for ~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. MARVELS will monitor radial velocities of more than 8000 FGK stars with the sensitivity and cadence (10-40 m/s, ~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. (Abridged)
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