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THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III

文献类型:期刊论文

AuthorAlam, Shadab1; Albareti, Franco D.2; Allende Prieto, Carlos3,4; Anders, F.5; Anderson, Scott F.6; Anderton, Timothy7; Andrews, Brett H.8,9; Armengaud, Eric10; Aubourg, Eric11; Bailey, Stephen12
SourceASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Issued Date2015-07-01
Volume219Issue:1
Keywordatlases catalogs surveys
English AbstractThe third generation of the Sloan Digital Sky Survey (SDSS-III) took data from 2008 to 2014 using the original SDSS wide-field imager, the original and an upgraded multi-object fiber-fed optical spectrograph, a new near-infrared high-resolution spectrograph, and a novel optical interferometer. All of the data from SDSS-III are now made public. In particular, this paper describes Data Release 11 (DR11) including all data acquired through 2013 July, and Data Release 12 (DR12) adding data acquired through 2014 July (including all data included in previous data releases), marking the end of SDSS-III observing. Relative to our previous public release (DR10), DR12 adds one million new spectra of galaxies and quasars from the Baryon Oscillation Spectroscopic Survey (BOSS) over an additional 3000 deg(2) of sky, more than triples the number of H-band spectra of stars as part of the Apache Point Observatory (APO) Galactic Evolution Experiment (APOGEE), and includes repeated accurate radial velocity measurements of 5500 stars from the Multi-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS). The APOGEE outputs now include the measured abundances of 15 different elements for each star. In total, SDSS-III added 5200 deg(2) of ugriz imaging; 155,520 spectra of 138,099 stars as part of the Sloan Exploration of Galactic Understanding and Evolution 2 (SEGUE-2) survey; 2,497,484 BOSS spectra of 1,372,737 galaxies, 294,512 quasars, and 247,216 stars over 9376 deg(2); 618,080 APOGEE spectra of 156,593 stars; and 197,040 MARVELS spectra of 5513 stars. Since its first light in 1998, SDSS has imaged over 1/3 of the Celestial sphere in five bands and obtained over five million astronomical spectra.
Indexed TypeSCI
Language英语
WOS IDWOS:000358858900012
源URL[http://ir.bao.ac.cn/handle/114a11/5640]  
Collection国家天文台_星系宇宙学研究部
Affiliation1.Carnegie Mellon Univ, Dept Phys, McWilliams Ctr Cosmol, Pittsburgh, PA 15213 USA
2.Univ Autonoma Madrid, Inst Fis Teor, UAM CSIC, E-28049 Madrid, Spain
3.IAC, E-38200 Tenerife, Spain
4.Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
5.Leibniz Inst Astrophys Potsdam AIP, D-14482 Potsdam, Germany
6.Univ Washington, Dept Astron, Seattle, WA 98195 USA
7.Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA
8.Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
9.Univ Pittsburgh, Dept Phys & Astron, PITT PACC, Pittsburgh, PA 15260 USA
10.CEA, Ctr Saclay, Irfu SPP, F-91191 Gif Sur Yvette, France
Recommended Citation
GB/T 7714
Alam, Shadab,Albareti, Franco D.,Allende Prieto, Carlos,et al. THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2015,219(1).
APA Alam, Shadab.,Albareti, Franco D..,Allende Prieto, Carlos.,Anders, F..,Anderson, Scott F..,...&Zhu, Guangtun.(2015).THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,219(1).
MLA Alam, Shadab,et al."THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 219.1(2015).

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