The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III
- Autores
- Alam, Shadab; Albareti, Franco D.; Prieto, Carlos Allende; Anders, F.; Anderson, Scott F.; Anderton, Timothy; Andrews, Brett H.; Armengaud, Eric; Aubourg, Éric; Bailey, Stephen; Basu, Sarbani; Bautista, Julian E.; Beaton, Rachael L.; Beers, Timothy C.; Bender, Chad F.; Berlind, Andreas A.; Beutler, Florian; Bhardwaj, Vaishali; Bird, Jonathan C.; Bizyaev, Dmitry; Blake, Cullen H.; Blanton, Michael R.; Blomqvist, Michael; Bochanski, John J.; Bolton, Adam S.; Bovy, Jo; Shelden, Bradley, A.; Brandt, W. N.; Brauer, D. E.; Nuza, Sebastian Ernesto; Scoccola, Claudia Graciela
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The third generation of the Sloan Digital Sky Survey (SDSS-III) tookdata from 2008 to 2014 using the original SDSS wide-field imager, theoriginal and an upgraded multi-object fiber-fed optical spectrograph, anew near-infrared high-resolution spectrograph, and a novel opticalinterferometer. All of the data from SDSS-III are now made public. Inparticular, this paper describes Data Release 11 (DR11) including alldata acquired through 2013 July, and Data Release 12 (DR12) adding dataacquired through 2014 July (including all data included in previous datareleases), marking the end of SDSS-III observing. Relative to ourprevious public release (DR10), DR12 adds one million new spectra ofgalaxies and quasars from the Baryon Oscillation Spectroscopic Survey(BOSS) over an additional 3000 deg2 of sky, more than triplesthe number of H-band spectra of stars as part of the Apache PointObservatory (APO) Galactic Evolution Experiment (APOGEE), and includesrepeated accurate radial velocity measurements of 5500 stars from theMulti-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS).The APOGEE outputs now include the measured abundances of 15 differentelements for each star. In total, SDSS-III added 5200 deg2 ofugriz imaging; 155,520 spectra of 138,099 stars as part of the SloanExploration of Galactic Understanding and Evolution 2 (SEGUE-2) survey;2,497,484 BOSS spectra of 1,372,737 galaxies, 294,512 quasars, and247,216 stars over 9376 deg2; 618,080 APOGEE spectra of156,593 stars; and 197,040 MARVELS spectra of 5513 stars. Since itsfirst light in 1998, SDSS has imaged over 1/3 of the Celestial sphere infive bands and obtained over five million astronomical spectra.
Fil: Alam, Shadab. University of Carnegie Mellon; Estados Unidos
Fil: Albareti, Franco D.. Universidad Autónoma de Madrid; España
Fil: Prieto, Carlos Allende. Universidad de La Laguna; España
Fil: Anders, F.. Leibniz Institute For Astrophysics Potsdam; Alemania
Fil: Anderson, Scott F.. University of Utah; Estados Unidos
Fil: Anderton, Timothy. University of Utah; Estados Unidos
Fil: Andrews, Brett H.. Ohio State University; Estados Unidos. University of Pittsburgh; Estados Unidos
Fil: Armengaud, Eric. Service de Physique Des Particules; Francia
Fil: Aubourg, Éric. Université Paris Diderot - Paris 7; Francia
Fil: Bailey, Stephen. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Basu, Sarbani. University of Yale; Estados Unidos
Fil: Bautista, Julian E.. Université Paris Diderot - Paris 7; Francia
Fil: Beaton, Rachael L.. University of Virginia; Estados Unidos
Fil: Beers, Timothy C.. University of Notre Dame; Estados Unidos
Fil: Bender, Chad F.. Pennsylvania State University; Estados Unidos
Fil: Berlind, Andreas A.. Vanderbilt University; Estados Unidos
Fil: Beutler, Florian. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Bhardwaj, Vaishali. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Bird, Jonathan C.. Vanderbilt University; Estados Unidos
Fil: Bizyaev, Dmitry. Apache Point Observatory; Estados Unidos
Fil: Blake, Cullen H.. University of Pennsylvania; Estados Unidos
Fil: Blanton, Michael R.. New York University; Estados Unidos
Fil: Blomqvist, Michael. University of California at Irvine; Estados Unidos
Fil: Bochanski, John J.. University of Washington; Estados Unidos
Fil: Bolton, Adam S.. University of Utah; Estados Unidos
Fil: Bovy, Jo. Institute For Advanced Studies; Estados Unidos
Fil: Shelden, Bradley, A.. Apache Point Observatory; Estados Unidos
Fil: Brandt, W. N.. Pennsylvania State University; Estados Unidos
Fil: Brauer, D. E.. Leibniz Institute For Astrophysics Potsdam; Alemania
Fil: Nuza, Sebastian Ernesto. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Institut Max Planck Fuer Gesellschaft. Max Planck Institute For Extraterrestrial Physics; Alemania
Fil: Scoccola, Claudia Graciela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina - Materia
-
Atlases
Catalogs
Surveys - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/125299
Ver los metadatos del registro completo
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The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-IIIAlam, ShadabAlbareti, Franco D.Prieto, Carlos AllendeAnders, F.Anderson, Scott F.Anderton, TimothyAndrews, Brett H.Armengaud, EricAubourg, ÉricBailey, StephenBasu, SarbaniBautista, Julian E.Beaton, Rachael L.Beers, Timothy C.Bender, Chad F.Berlind, Andreas A.Beutler, FlorianBhardwaj, VaishaliBird, Jonathan C.Bizyaev, DmitryBlake, Cullen H.Blanton, Michael R.Blomqvist, MichaelBochanski, John J.Bolton, Adam S.Bovy, JoShelden, Bradley, A.Brandt, W. N.Brauer, D. E.Nuza, Sebastian ErnestoScoccola, Claudia GracielaAtlasesCatalogsSurveyshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The third generation of the Sloan Digital Sky Survey (SDSS-III) tookdata from 2008 to 2014 using the original SDSS wide-field imager, theoriginal and an upgraded multi-object fiber-fed optical spectrograph, anew near-infrared high-resolution spectrograph, and a novel opticalinterferometer. All of the data from SDSS-III are now made public. Inparticular, this paper describes Data Release 11 (DR11) including alldata acquired through 2013 July, and Data Release 12 (DR12) adding dataacquired through 2014 July (including all data included in previous datareleases), marking the end of SDSS-III observing. Relative to ourprevious public release (DR10), DR12 adds one million new spectra ofgalaxies and quasars from the Baryon Oscillation Spectroscopic Survey(BOSS) over an additional 3000 deg2 of sky, more than triplesthe number of H-band spectra of stars as part of the Apache PointObservatory (APO) Galactic Evolution Experiment (APOGEE), and includesrepeated accurate radial velocity measurements of 5500 stars from theMulti-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS).The APOGEE outputs now include the measured abundances of 15 differentelements for each star. In total, SDSS-III added 5200 deg2 ofugriz imaging; 155,520 spectra of 138,099 stars as part of the SloanExploration of Galactic Understanding and Evolution 2 (SEGUE-2) survey;2,497,484 BOSS spectra of 1,372,737 galaxies, 294,512 quasars, and247,216 stars over 9376 deg2; 618,080 APOGEE spectra of156,593 stars; and 197,040 MARVELS spectra of 5513 stars. Since itsfirst light in 1998, SDSS has imaged over 1/3 of the Celestial sphere infive bands and obtained over five million astronomical spectra.Fil: Alam, Shadab. University of Carnegie Mellon; Estados UnidosFil: Albareti, Franco D.. Universidad Autónoma de Madrid; EspañaFil: Prieto, Carlos Allende. Universidad de La Laguna; EspañaFil: Anders, F.. Leibniz Institute For Astrophysics Potsdam; AlemaniaFil: Anderson, Scott F.. University of Utah; Estados UnidosFil: Anderton, Timothy. University of Utah; Estados UnidosFil: Andrews, Brett H.. Ohio State University; Estados Unidos. University of Pittsburgh; Estados UnidosFil: Armengaud, Eric. Service de Physique Des Particules; FranciaFil: Aubourg, Éric. Université Paris Diderot - Paris 7; FranciaFil: Bailey, Stephen. Lawrence Berkeley National Laboratory; Estados UnidosFil: Basu, Sarbani. University of Yale; Estados UnidosFil: Bautista, Julian E.. Université Paris Diderot - Paris 7; FranciaFil: Beaton, Rachael L.. University of Virginia; Estados UnidosFil: Beers, Timothy C.. University of Notre Dame; Estados UnidosFil: Bender, Chad F.. Pennsylvania State University; Estados UnidosFil: Berlind, Andreas A.. Vanderbilt University; Estados UnidosFil: Beutler, Florian. Lawrence Berkeley National Laboratory; Estados UnidosFil: Bhardwaj, Vaishali. Lawrence Berkeley National Laboratory; Estados UnidosFil: Bird, Jonathan C.. Vanderbilt University; Estados UnidosFil: Bizyaev, Dmitry. Apache Point Observatory; Estados UnidosFil: Blake, Cullen H.. University of Pennsylvania; Estados UnidosFil: Blanton, Michael R.. New York University; Estados UnidosFil: Blomqvist, Michael. University of California at Irvine; Estados UnidosFil: Bochanski, John J.. University of Washington; Estados UnidosFil: Bolton, Adam S.. University of Utah; Estados UnidosFil: Bovy, Jo. Institute For Advanced Studies; Estados UnidosFil: Shelden, Bradley, A.. Apache Point Observatory; Estados UnidosFil: Brandt, W. N.. Pennsylvania State University; Estados UnidosFil: Brauer, D. E.. Leibniz Institute For Astrophysics Potsdam; AlemaniaFil: Nuza, Sebastian Ernesto. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Institut Max Planck Fuer Gesellschaft. Max Planck Institute For Extraterrestrial Physics; AlemaniaFil: Scoccola, Claudia Graciela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaIOP Publishing2015-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/125299Alam, Shadab; Albareti, Franco D.; Prieto, Carlos Allende; Anders, F.; Anderson, Scott F.; et al.; The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III; IOP Publishing; Astrophysical Journal Supplement Series; 219; 12; 7-2015; 1-270067-0049CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/0067-0049/219/1/12info:eu-repo/semantics/altIdentifier/doi/10.1088/0067-0049/219/1/12info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T12:02:42Zoai:ri.conicet.gov.ar:11336/125299instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 12:02:43.201CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III |
| title |
The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III |
| spellingShingle |
The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III Alam, Shadab Atlases Catalogs Surveys |
| title_short |
The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III |
| title_full |
The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III |
| title_fullStr |
The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III |
| title_full_unstemmed |
The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III |
| title_sort |
The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III |
| dc.creator.none.fl_str_mv |
Alam, Shadab Albareti, Franco D. Prieto, Carlos Allende Anders, F. Anderson, Scott F. Anderton, Timothy Andrews, Brett H. Armengaud, Eric Aubourg, Éric Bailey, Stephen Basu, Sarbani Bautista, Julian E. Beaton, Rachael L. Beers, Timothy C. Bender, Chad F. Berlind, Andreas A. Beutler, Florian Bhardwaj, Vaishali Bird, Jonathan C. Bizyaev, Dmitry Blake, Cullen H. Blanton, Michael R. Blomqvist, Michael Bochanski, John J. Bolton, Adam S. Bovy, Jo Shelden, Bradley, A. Brandt, W. N. Brauer, D. E. Nuza, Sebastian Ernesto Scoccola, Claudia Graciela |
| author |
Alam, Shadab |
| author_facet |
Alam, Shadab Albareti, Franco D. Prieto, Carlos Allende Anders, F. Anderson, Scott F. Anderton, Timothy Andrews, Brett H. Armengaud, Eric Aubourg, Éric Bailey, Stephen Basu, Sarbani Bautista, Julian E. Beaton, Rachael L. Beers, Timothy C. Bender, Chad F. Berlind, Andreas A. Beutler, Florian Bhardwaj, Vaishali Bird, Jonathan C. Bizyaev, Dmitry Blake, Cullen H. Blanton, Michael R. Blomqvist, Michael Bochanski, John J. Bolton, Adam S. Bovy, Jo Shelden, Bradley, A. Brandt, W. N. Brauer, D. E. Nuza, Sebastian Ernesto Scoccola, Claudia Graciela |
| author_role |
author |
| author2 |
Albareti, Franco D. Prieto, Carlos Allende Anders, F. Anderson, Scott F. Anderton, Timothy Andrews, Brett H. Armengaud, Eric Aubourg, Éric Bailey, Stephen Basu, Sarbani Bautista, Julian E. Beaton, Rachael L. Beers, Timothy C. Bender, Chad F. Berlind, Andreas A. Beutler, Florian Bhardwaj, Vaishali Bird, Jonathan C. Bizyaev, Dmitry Blake, Cullen H. Blanton, Michael R. Blomqvist, Michael Bochanski, John J. Bolton, Adam S. Bovy, Jo Shelden, Bradley, A. Brandt, W. N. Brauer, D. E. Nuza, Sebastian Ernesto Scoccola, Claudia Graciela |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
Atlases Catalogs Surveys |
| topic |
Atlases Catalogs Surveys |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
The third generation of the Sloan Digital Sky Survey (SDSS-III) tookdata from 2008 to 2014 using the original SDSS wide-field imager, theoriginal and an upgraded multi-object fiber-fed optical spectrograph, anew near-infrared high-resolution spectrograph, and a novel opticalinterferometer. All of the data from SDSS-III are now made public. Inparticular, this paper describes Data Release 11 (DR11) including alldata acquired through 2013 July, and Data Release 12 (DR12) adding dataacquired through 2014 July (including all data included in previous datareleases), marking the end of SDSS-III observing. Relative to ourprevious public release (DR10), DR12 adds one million new spectra ofgalaxies and quasars from the Baryon Oscillation Spectroscopic Survey(BOSS) over an additional 3000 deg2 of sky, more than triplesthe number of H-band spectra of stars as part of the Apache PointObservatory (APO) Galactic Evolution Experiment (APOGEE), and includesrepeated accurate radial velocity measurements of 5500 stars from theMulti-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS).The APOGEE outputs now include the measured abundances of 15 differentelements for each star. In total, SDSS-III added 5200 deg2 ofugriz imaging; 155,520 spectra of 138,099 stars as part of the SloanExploration of Galactic Understanding and Evolution 2 (SEGUE-2) survey;2,497,484 BOSS spectra of 1,372,737 galaxies, 294,512 quasars, and247,216 stars over 9376 deg2; 618,080 APOGEE spectra of156,593 stars; and 197,040 MARVELS spectra of 5513 stars. Since itsfirst light in 1998, SDSS has imaged over 1/3 of the Celestial sphere infive bands and obtained over five million astronomical spectra. Fil: Alam, Shadab. University of Carnegie Mellon; Estados Unidos Fil: Albareti, Franco D.. Universidad Autónoma de Madrid; España Fil: Prieto, Carlos Allende. Universidad de La Laguna; España Fil: Anders, F.. Leibniz Institute For Astrophysics Potsdam; Alemania Fil: Anderson, Scott F.. University of Utah; Estados Unidos Fil: Anderton, Timothy. University of Utah; Estados Unidos Fil: Andrews, Brett H.. Ohio State University; Estados Unidos. University of Pittsburgh; Estados Unidos Fil: Armengaud, Eric. Service de Physique Des Particules; Francia Fil: Aubourg, Éric. Université Paris Diderot - Paris 7; Francia Fil: Bailey, Stephen. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Basu, Sarbani. University of Yale; Estados Unidos Fil: Bautista, Julian E.. Université Paris Diderot - Paris 7; Francia Fil: Beaton, Rachael L.. University of Virginia; Estados Unidos Fil: Beers, Timothy C.. University of Notre Dame; Estados Unidos Fil: Bender, Chad F.. Pennsylvania State University; Estados Unidos Fil: Berlind, Andreas A.. Vanderbilt University; Estados Unidos Fil: Beutler, Florian. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Bhardwaj, Vaishali. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Bird, Jonathan C.. Vanderbilt University; Estados Unidos Fil: Bizyaev, Dmitry. Apache Point Observatory; Estados Unidos Fil: Blake, Cullen H.. University of Pennsylvania; Estados Unidos Fil: Blanton, Michael R.. New York University; Estados Unidos Fil: Blomqvist, Michael. University of California at Irvine; Estados Unidos Fil: Bochanski, John J.. University of Washington; Estados Unidos Fil: Bolton, Adam S.. University of Utah; Estados Unidos Fil: Bovy, Jo. Institute For Advanced Studies; Estados Unidos Fil: Shelden, Bradley, A.. Apache Point Observatory; Estados Unidos Fil: Brandt, W. N.. Pennsylvania State University; Estados Unidos Fil: Brauer, D. E.. Leibniz Institute For Astrophysics Potsdam; Alemania Fil: Nuza, Sebastian Ernesto. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina. Institut Max Planck Fuer Gesellschaft. Max Planck Institute For Extraterrestrial Physics; Alemania Fil: Scoccola, Claudia Graciela. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina |
| description |
The third generation of the Sloan Digital Sky Survey (SDSS-III) tookdata from 2008 to 2014 using the original SDSS wide-field imager, theoriginal and an upgraded multi-object fiber-fed optical spectrograph, anew near-infrared high-resolution spectrograph, and a novel opticalinterferometer. All of the data from SDSS-III are now made public. Inparticular, this paper describes Data Release 11 (DR11) including alldata acquired through 2013 July, and Data Release 12 (DR12) adding dataacquired through 2014 July (including all data included in previous datareleases), marking the end of SDSS-III observing. Relative to ourprevious public release (DR10), DR12 adds one million new spectra ofgalaxies and quasars from the Baryon Oscillation Spectroscopic Survey(BOSS) over an additional 3000 deg2 of sky, more than triplesthe number of H-band spectra of stars as part of the Apache PointObservatory (APO) Galactic Evolution Experiment (APOGEE), and includesrepeated accurate radial velocity measurements of 5500 stars from theMulti-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS).The APOGEE outputs now include the measured abundances of 15 differentelements for each star. In total, SDSS-III added 5200 deg2 ofugriz imaging; 155,520 spectra of 138,099 stars as part of the SloanExploration of Galactic Understanding and Evolution 2 (SEGUE-2) survey;2,497,484 BOSS spectra of 1,372,737 galaxies, 294,512 quasars, and247,216 stars over 9376 deg2; 618,080 APOGEE spectra of156,593 stars; and 197,040 MARVELS spectra of 5513 stars. Since itsfirst light in 1998, SDSS has imaged over 1/3 of the Celestial sphere infive bands and obtained over five million astronomical spectra. |
| publishDate |
2015 |
| dc.date.none.fl_str_mv |
2015-07 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/125299 Alam, Shadab; Albareti, Franco D.; Prieto, Carlos Allende; Anders, F.; Anderson, Scott F.; et al.; The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III; IOP Publishing; Astrophysical Journal Supplement Series; 219; 12; 7-2015; 1-27 0067-0049 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/125299 |
| identifier_str_mv |
Alam, Shadab; Albareti, Franco D.; Prieto, Carlos Allende; Anders, F.; Anderson, Scott F.; et al.; The Eleventh and Twelfth data releases of the Sloan Digital Sky Survey: Final data from SDSS-III; IOP Publishing; Astrophysical Journal Supplement Series; 219; 12; 7-2015; 1-27 0067-0049 CONICET Digital CONICET |
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eng |
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eng |
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