The Fourth Data Release of the Sloan Digital Sky Survey
The Fourth Data Release of the Sloan Digital Sky Survey
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DOI：
10.1086/497917
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发表时间：
2005-07
期刊：
影响因子：
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通讯作者：
J. Adelman-McCarthy;M. Agüeros;S. Allam;K. S. Anderson;S. Anderson;J. Annis;N. Bahcall;I. Baldry;J. Barentine;A. Berlind;M. Bernardi;M. Blanton;W. Boroski;H. Brewington;J. Brinchmann;J. Brinkmann;R. Brunner;T. Budavári;L. Carey;M. Carr;F. Castander;A. Connolly;I. Csabai;P. Czarapata;J. Dalcanton;M. Doi;F. Dong;D. Eisenstein;M. Evans;Xiaohui Fan;D. Finkbeiner;S. Friedman;J. Frieman;M. Fukugita;B. Gillespie;K. Glazebrook;J. Gray;E. Grebel;J. Gunn;V. Gurbani;E. D. Haas;P. Hall;F. Harris;M. Harvanek;S. Hawley;Jeffrey Hayes;J. Hendry;G. Hennessy;R. Hindsley;C. Hirata;C. Hogan;D. Hogg;D. Holmgren;J. Holtzman;S. Ichikawa;Ž. Ivezić;S. Jester;D. Johnston;A. Jorgensen;M. Jurić;S. Kent;S. Kleinman;G. Knapp;A. Kniazev;R. Kron;J. Krzesinski;N. Kuropatkin;D. Lamb;H. Lampeitl;Brian C. Lee;R. F. Leger;Huan Lin;D. Long;J. Loveday;R. Lupton;B. Margon;David Martı́Ínez-Delgado;R. Mandelbaum;T. Matsubara;P. McGehee;T. Mckay;A. Meiksin;J. Munn;R. Nakajima;T. Nash;E. Neilsen;H. Newberg;P. Newman;R. Nichol;T. Nicinski;M. Nieto-Santisteban;A. Nitta;W. O'Mullane;S. Okamura;R. Owen;N. Padmanabhan;G. Pauls;J. Peoples;J. Pier;A. Pope;D. Pourbaix;Thomas R. Quinn;G. Richards;M. Richmond;C. Rockosi;D. Schlegel;D. Schneider;Joshua Schroeder;R. Scranton;U. Seljak;E. Sheldon;K. Shimasaku;J. A. Smith;V. Smolčić;S. Snedden;C. Stoughton;M. Strauss;M. Subbarao;A. Szalay;I. Szapudi;P. Szkody;M. Tegmark;A. Thakar;D. Tucker;A. Uomoto;D. Berk;Jan vandenBerg;M. Vogeley;W. Voges;N. Vogt;L. Walkowicz;D. Weinberg;A. West;S. White;Yongzhong Xu;B. Yanny;D. Yocum;D. York;I. Zehavi;S. Zibetti
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文献类型：
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作者：
J. Adelman-McCarthy;M. Agüeros;S. Allam;K. S. Anderson;S. Anderson;J. Annis;N. Bahcall;I. Baldry;J. Barentine;A. Berlind;M. Bernardi;M. Blanton;W. Boroski;H. Brewington;J. Brinchmann;J. Brinkmann;R. Brunner;T. Budavári;L. Carey;M. Carr;F. Castander;A. Connolly;I. Csabai;P. Czarapata;J. Dalcanton;M. Doi;F. Dong;D. Eisenstein;M. Evans;Xiaohui Fan;D. Finkbeiner;S. Friedman;J. Frieman;M. Fukugita;B. Gillespie;K. Glazebrook;J. Gray;E. Grebel;J. Gunn;V. Gurbani;E. D. Haas;P. Hall;F. Harris;M. Harvanek;S. Hawley;Jeffrey Hayes;J. Hendry;G. Hennessy;R. Hindsley;C. Hirata;C. Hogan;D. Hogg;D. Holmgren;J. Holtzman;S. Ichikawa;Ž. Ivezić;S. Jester;D. Johnston;A. Jorgensen;M. Jurić;S. Kent;S. Kleinman;G. Knapp;A. Kniazev;R. Kron;J. Krzesinski;N. Kuropatkin;D. Lamb;H. Lampeitl;Brian C. Lee;R. F. Leger;Huan Lin;D. Long;J. Loveday;R. Lupton;B. Margon;David Martı́Ínez-Delgado;R. Mandelbaum;T. Matsubara;P. McGehee;T. Mckay;A. Meiksin;J. Munn;R. Nakajima;T. Nash;E. Neilsen;H. Newberg;P. Newman;R. Nichol;T. Nicinski;M. Nieto-Santisteban;A. Nitta;W. O'Mullane;S. Okamura;R. Owen;N. Padmanabhan;G. Pauls;J. Peoples;J. Pier;A. Pope;D. Pourbaix;Thomas R. Quinn;G. Richards;M. Richmond;C. Rockosi;D. Schlegel;D. Schneider;Joshua Schroeder;R. Scranton;U. Seljak;E. Sheldon;K. Shimasaku;J. A. Smith;V. Smolčić;S. Snedden;C. Stoughton;M. Strauss;M. Subbarao;A. Szalay;I. Szapudi;P. Szkody;M. Tegmark;A. Thakar;D. Tucker;A. Uomoto;D. Berk;Jan vandenBerg;M. Vogeley;W. Voges;N. Vogt;L. Walkowicz;D. Weinberg;A. West;S. White;Yongzhong Xu;B. Yanny;D. Yocum;D. York;I. Zehavi;S. Zibetti
本文描述了斯隆数字巡天（SDSS）的第四次数据发布，包括2004年6月之前所有的巡天质量数据。数据发布包括在6670度2上选择的1.8亿个物体的五波段光度数据，以及使用标准SDSS目标选择算法从4783度2的成像数据中选择的673,280个星系、类星体和恒星光谱。这些数字比第三次公布的数据增加了大约25%。第四次数据发布还包括使用各种替代算法选择的额外131840个物体光谱，以解决从银河系厚盘中的恒星运动学到暗淡星系和类星体种群的科学问题。
This paper describes the fourth data release of the Sloan Digital Sky Survey (SDSS), including all survey-quality data taken through June 2004. The data release includes five-band photometric data for 180 million objects selected over 6670 deg 2 , and 673,280 spectra of galaxies, quasars, and stars selected from 4783 deg 2 of that imaging data using the standard SDSS target selection algorithms. These numbers represent a roughly 25% increment over those of the Third Data Release. The Fourth Data Release also includes an additional 131,840 spectra of objects selected using a variety of alternative algorithms, to address scientific issues ranging from the kinematics of stars in the Milky Way thick disk to populations of faint galaxies and quasars.