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

被引：1733

作者：

Alam, Shadab ^{[1
]}

Albareti, Franco D. ^{[2
]}

Allende Prieto, Carlos ^{[3
,4
]}

Anders, F. ^{[5
]}

Anderson, Scott F. ^{[6
]}

Anderton, Timothy ^{[7
]}

Andrews, Brett H. ^{[8
,9
]}

Armengaud, Eric ^{[10
]}

Aubourg, Eric ^{[11
]}

Bailey, Stephen ^{[12
]}

Basu, Sarbani ^{[13
]}

Bautista, Julian E. ^{[11
]}

Beaton, Rachael L. ^{[14
,15
]}

Beers, Timothy C. ^{[16
,17
]}

Bender, Chad F. ^{[18
,19
]}

Berlind, Andreas A. ^{[20
]}

Beutler, Florian ^{[12
]}

Bhardwaj, Vaishali ^{[6
,12
]}

Bird, Jonathan C. ^{[20
]}

Bizyaev, Dmitry ^{[21
,22
,23
]}

Blake, Cullen H. ^{[24
]}

Blanton, Michael R. ^{[25
]}

Blomqvist, Michael ^{[26
]}

Bochanski, John J. ^{[6
,27
]}

Bolton, Adam S. ^{[7
]}

Bovy, Jo ^{[28
]}

Bradley, A. Shelden ^{[21
]}

Brandt, W. N. ^{[18
,29
,30
]}

Brauer, D. E. ^{[5
]}

Brinkmann, J. ^{[21
]}

Brown, Peter J. ^{[31
]}

Brownstein, Joel R. ^{[7
]}

Burden, Angela ^{[32
]}

Burtin, Etienne ^{[10
]}

Busca, Nicolas G. ^{[11
,33
,34
]}

Cai, Zheng ^{[35
]}

Capozzi, Diego ^{[32
]}

Rosell, Aurelio Carnero ^{[33
,34
]}

Carr, Michael A. ^{[36
]}

Carrera, Ricardo ^{[3
,4
]}

Chambers, K. C. ^{[37
]}

Chaplin, William James ^{[38
,39
]}

Chen, Yen-Chi ^{[40
]}

Chiappini, Cristina ^{[5
,34
]}

Chojnowski, S. Drew ^{[22
]}

Chuang, Chia-Hsun ^{[2
]}

Clerc, Nicolas ^{[41
]}

Comparat, Johan ^{[2
]}

Covey, Kevin ^{[42
,43
]}

Croft, Rupert A. C. ^{[1
]}

机构：

[1] 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

[11] Univ Paris Diderot, Sorbonne Paris Cite, Observ Paris, APC,CNRS IN2P3,CEA IRFU, F-75205 Paris, France

[12] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[13] Yale Univ, Dept Astron, New Haven, CT 06520 USA

[14] Univ Virginia, Dept Astron, Charlottesville, VA 22904 USA

[15] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA

[16] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA

[17] Univ Notre Dame, JINA Ctr Evolut Elements, Notre Dame, IN 46556 USA

[18] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA

[19] Penn State Univ, Ctr Exoplanets & Habitable Worlds, Davey Lab 525, University Pk, PA 16802 USA

[20] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA

[21] Apache Point Observ, Sunspot, NM 88349 USA

[22] New Mexico State Univ, Dept Astron, Las Cruces, NM 88003 USA

[23] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119992, Russia

[24] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[25] NYU, Dept Phys, Ctr Cosmol & Particle Phys, New York, NY 10003 USA

[26] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[27] Rider Univ, Lawrenceville, NJ 08648 USA

[28] Inst Adv Study, Princeton, NJ 08540 USA

[29] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA

[30] Penn State Univ, Dept Phys, University Pk, PA 16802 USA

[31] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, Dept Phys & Astron, College Stn, TX 77843 USA

[32] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[33] Observ Nacl, BR-20921400 Rio De Janeiro, RJ, Brazil

[34] Lab Interinstituc & Astron LIneA, BR-20921400 Rio De Janeiro, RJ, Brazil

[35] Steward Observ, Tucson, AZ 85721 USA

[36] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[37] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA

[38] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

[39] Aarhus Univ, Dept Phys & Astron, SAC, DK-8000 Aarhus C, Denmark

[40] Carnegie Mellon Univ, Dept Stat, Bruce & Astrid McWilliams Ctr Cosmol, Pittsburgh, PA 15213 USA

[41] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany

[42] Lowell Observ, Flagstaff, AZ 86001 USA

[43] Western Washington Univ, Dept Phys & Astron, Bellingham, WA 98225 USA

[44] Univ Barcelona, Inst Ciencies Cosmos, IEEC, E-08028 Barcelona, Spain

[45] Yale Univ, Yale Ctr Astron & Astrophys, New Haven, CT 06520 USA

[46] Univ Florida, Dept Astron, Bryant Space Sci Ctr, Gainesville, FL 32611 USA

[47] No Kentucky Univ, Dept Phys & Geol, Highland Hts, KY 41099 USA

[48] EPFL, Lab Astrophys, Observ Sauverny, CH-1290 Versoix, Switzerland

[49] Embry Riddle Aeronaut Univ, Dept Phys Sci, Daytona Beach, FL 32114 USA

[50] Univ Fed Rio de Janeiro, Observ Valongo, BR-20080090 Rio De Janeiro, Brazil

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2015年 / 219卷 / 01期

基金：

美国国家科学基金会;

关键词：

atlases; catalogs; surveys; OSCILLATION SPECTROSCOPIC SURVEY; BARYON ACOUSTIC-OSCILLATIONS; LOW-MASS STELLAR; SOLAR-LIKE STARS; FIXED-DELAY INTERFEROMETRY; BROWN DWARF CANDIDATE; LY-ALPHA FOREST; TARGET SELECTION; X-RAY; 1ST DATA;

D O I：

10.1088/0067-0049/219/1/12

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The 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.

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