Abstract
The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its Second Data Release. This data release consists of 3324 deg 2 of five-band (ugriz) imaging data with photometry for over 88 million unique objects, 367,360 spectra of galaxies, quasars, stars, and calibrating blank sky patches selected over 2627 deg2 of this area, and tables of measured parameters from these data. The imaging data reach a depth of r ≈ 22.2 (95% completeness limit for point sources) and are photometrically and astrometrically calibrated to 2% rms and 100 mas rms per coordinate, respectively. The imaging data have all been processed through a new version of the SDSS imaging pipeline, in which the most important improvement since the last data release is fixing an error in the model fits to each object. The result is that model magnitudes are now a good proxy for point-spread function magnitudes for point sources, and Petrosian magnitudes for extended sources. The spectroscopy extends from 3800 to 9200 Å at a resolution of 2000. The spectroscopic software now repairs a systematic error in the radial velocities of certain types of stars and has substantially improved spectrophotometry. All data included in the SDSS Early Data Release and First Data Release are reprocessed with the improved pipelines and included in the Second Data Release. Further characteristics of the data are described, as are the data products themselves and the tools for accessing them.
Original language | English (US) |
---|---|
Pages (from-to) | 502-512 |
Number of pages | 11 |
Journal | Astronomical Journal |
Volume | 128 |
Issue number | 1 1783 |
DOIs | |
State | Published - Jul 2004 |
Keywords
- Atlases
- Catalogs
- Surveys
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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The second data release of the sloan digital sky survey. / Abazajian, Kevork; Adelman-McCarthy, Jennifer K.; Agüeros, Marcel A.; Allam, Sahar S.; Kurt, S. J.Anderson; Anderson, Scott F.; Annis, James; Bahcall, Neta A.; Baldry, Ivan K.; Bastian, Steven; Berlind, Andreas; Bernardi, Mariangela; Blanton, Michael R.; Bochanski, John J.; Boroski, William N.; Briggs, John W.; Brinkmann, J.; Brunner, Robert J.; Budavári, Tamás; Carey, Larry N.; Carliles, Samuel; Castander, Francisco J.; Connolly, A. J.; Csabai, István; Doi, Mamoru; Dong, Feng; Eisenstein, Daniel J.; Evans, Michael L.; Fan, Xiaohui; Finkbeiner, Douglas P.; Friedman, Scott D.; Frieman, Joshua A.; Fukugita, Masataka; Gal, Roy R.; Gillespie, Bruce; Glazebrook, Karl; Gray, Jim; Grebel, Eva K.; Gunn, James E.; Gurbani, Vijay K.; Hall, Patrick B.; Hamabe, Masaru; Harris, Frederick H.; Harris, Hugh C.; Harvanek, Michael; Heckman, Timothy M.; Hendry, John S.; Hennessy, Gregory S.; Hindsley, Robert B.; Hogan, Craig J.; Hogg, David W.; Holmgren, Donald J.; Ichikawa, Shin ichi; Ichikawa, Takashi; Ivezić, Željko; Jester, Sebastian; Johnston, David E.; Jorgensen, Anders M.; Kent, Stephen M.; Kleinman, S. J.; Knapp, G. R.; Kniazev, Alexei Y.; Kron, Richard G.; Krzesinski, Jurek; Kunszt, Peter Z.; Kuropatkin, Nickolai; Lamb, Donald Q.; Lampeitl, Hubert; Lee, Brian C.; Leger, R. French; Li, Nolan; Lin, Huan; Loh, Yeong Shang; Long, Daniel C.; Loveday, Jon; Lupton, Robert H.; Malik, Tanu; Margon, Bruce; Matsubara, Takahiko; McGehee, Peregrine M.; McKay, Timothy A.; Meiksin, Avery; Munn, Jeffrey A.; Nakajima, Reiko; Nash, Thomas; Neilsen, Eric H.; Newberg, Heidi J.; Newman, Peter R.; Nichol, Robert C.; Nicinski, Tom; Nieto-Santisteban, Maria; Nitta, Atsuko; Okamura, Sadanori; O'Mullane, William; Ostriker, Jeremiah P.; Owen, Russell; Padmanabhan, Nikhil; Peoples, John; Pier, Jeffrey R.; Pope, Adrian C.; Quinn, Thomas R.; Richards, Gordon T.; Richmond, Michael W.; Hans-Rix, Walter; Rockosi, Constance M.; Schlegel, David J.; Schneider, Donald P.; Scranton, Ryan; Sekiguchi, Maki; Seljak, Uros; Sergey, Gary; Sesar, Branimir; Sheldon, Erin; Shimasaku, Kazu; Siegmund, Walter A.; Silvestri, Nicole M.; Smith, J. Allyn; Smolčić, Vernesa; Snedden, Stephanie A.; Stebbins, Albert; Stoughton, Chris; Strauss, Michael A.; Subba, Mark Rao; Szalay, Alexander S.; Szapudi, István; Szkody, Paula; Szokoly, Gyula P.; Tegmark, Max; Teodoro, Luis; Thakar, Aniruddha R.; Tremonti, Christy; Tucker, Douglas L.; Uomoto, Alan; vanden Berk, Daniel E.; Vandenberg, Jan; Vogeley, Michael S.; Voges, Wolfgang; Vogt, Nicole P.; Walkowicz, Lucianne M.; Wang, Shu i.; Weinberg, David H.; West, Andrew A.; White, Simon D.M.; Wilhite, Brian C.; Xu, Yongzhong; Yanny, Brian; Yasuda, Naoki; Yip, Ching Wa; Yocum, D. R.; York, Donald G.; Zehavi, Idit; Zibetti, Stefano; Zucker, Daniel B.
In: Astronomical Journal, Vol. 128, No. 1 1783, 07.2004, p. 502-512.Research output: Contribution to journal › Review article › peer-review
}
TY - JOUR
T1 - The second data release of the sloan digital sky survey
AU - Abazajian, Kevork
AU - Adelman-McCarthy, Jennifer K.
AU - Agüeros, Marcel A.
AU - Allam, Sahar S.
AU - Kurt, S. J.Anderson
AU - Anderson, Scott F.
AU - Annis, James
AU - Bahcall, Neta A.
AU - Baldry, Ivan K.
AU - Bastian, Steven
AU - Berlind, Andreas
AU - Bernardi, Mariangela
AU - Blanton, Michael R.
AU - Bochanski, John J.
AU - Boroski, William N.
AU - Briggs, John W.
AU - Brinkmann, J.
AU - Brunner, Robert J.
AU - Budavári, Tamás
AU - Carey, Larry N.
AU - Carliles, Samuel
AU - Castander, Francisco J.
AU - Connolly, A. J.
AU - Csabai, István
AU - Doi, Mamoru
AU - Dong, Feng
AU - Eisenstein, Daniel J.
AU - Evans, Michael L.
AU - Fan, Xiaohui
AU - Finkbeiner, Douglas P.
AU - Friedman, Scott D.
AU - Frieman, Joshua A.
AU - Fukugita, Masataka
AU - Gal, Roy R.
AU - Gillespie, Bruce
AU - Glazebrook, Karl
AU - Gray, Jim
AU - Grebel, Eva K.
AU - Gunn, James E.
AU - Gurbani, Vijay K.
AU - Hall, Patrick B.
AU - Hamabe, Masaru
AU - Harris, Frederick H.
AU - Harris, Hugh C.
AU - Harvanek, Michael
AU - Heckman, Timothy M.
AU - Hendry, John S.
AU - Hennessy, Gregory S.
AU - Hindsley, Robert B.
AU - Hogan, Craig J.
AU - Hogg, David W.
AU - Holmgren, Donald J.
AU - Ichikawa, Shin ichi
AU - Ichikawa, Takashi
AU - Ivezić, Željko
AU - Jester, Sebastian
AU - Johnston, David E.
AU - Jorgensen, Anders M.
AU - Kent, Stephen M.
AU - Kleinman, S. J.
AU - Knapp, G. R.
AU - Kniazev, Alexei Y.
AU - Kron, Richard G.
AU - Krzesinski, Jurek
AU - Kunszt, Peter Z.
AU - Kuropatkin, Nickolai
AU - Lamb, Donald Q.
AU - Lampeitl, Hubert
AU - Lee, Brian C.
AU - Leger, R. French
AU - Li, Nolan
AU - Lin, Huan
AU - Loh, Yeong Shang
AU - Long, Daniel C.
AU - Loveday, Jon
AU - Lupton, Robert H.
AU - Malik, Tanu
AU - Margon, Bruce
AU - Matsubara, Takahiko
AU - McGehee, Peregrine M.
AU - McKay, Timothy A.
AU - Meiksin, Avery
AU - Munn, Jeffrey A.
AU - Nakajima, Reiko
AU - Nash, Thomas
AU - Neilsen, Eric H.
AU - Newberg, Heidi J.
AU - Newman, Peter R.
AU - Nichol, Robert C.
AU - Nicinski, Tom
AU - Nieto-Santisteban, Maria
AU - Nitta, Atsuko
AU - Okamura, Sadanori
AU - O'Mullane, William
AU - Ostriker, Jeremiah P.
AU - Owen, Russell
AU - Padmanabhan, Nikhil
AU - Peoples, John
AU - Pier, Jeffrey R.
AU - Pope, Adrian C.
AU - Quinn, Thomas R.
AU - Richards, Gordon T.
AU - Richmond, Michael W.
AU - Hans-Rix, Walter
AU - Rockosi, Constance M.
AU - Schlegel, David J.
AU - Schneider, Donald P.
AU - Scranton, Ryan
AU - Sekiguchi, Maki
AU - Seljak, Uros
AU - Sergey, Gary
AU - Sesar, Branimir
AU - Sheldon, Erin
AU - Shimasaku, Kazu
AU - Siegmund, Walter A.
AU - Silvestri, Nicole M.
AU - Smith, J. Allyn
AU - Smolčić, Vernesa
AU - Snedden, Stephanie A.
AU - Stebbins, Albert
AU - Stoughton, Chris
AU - Strauss, Michael A.
AU - Subba, Mark Rao
AU - Szalay, Alexander S.
AU - Szapudi, István
AU - Szkody, Paula
AU - Szokoly, Gyula P.
AU - Tegmark, Max
AU - Teodoro, Luis
AU - Thakar, Aniruddha R.
AU - Tremonti, Christy
AU - Tucker, Douglas L.
AU - Uomoto, Alan
AU - vanden Berk, Daniel E.
AU - Vandenberg, Jan
AU - Vogeley, Michael S.
AU - Voges, Wolfgang
AU - Vogt, Nicole P.
AU - Walkowicz, Lucianne M.
AU - Wang, Shu i.
AU - Weinberg, David H.
AU - West, Andrew A.
AU - White, Simon D.M.
AU - Wilhite, Brian C.
AU - Xu, Yongzhong
AU - Yanny, Brian
AU - Yasuda, Naoki
AU - Yip, Ching Wa
AU - Yocum, D. R.
AU - York, Donald G.
AU - Zehavi, Idit
AU - Zibetti, Stefano
AU - Zucker, Daniel B.
PY - 2004/7
Y1 - 2004/7
N2 - The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its Second Data Release. This data release consists of 3324 deg 2 of five-band (ugriz) imaging data with photometry for over 88 million unique objects, 367,360 spectra of galaxies, quasars, stars, and calibrating blank sky patches selected over 2627 deg2 of this area, and tables of measured parameters from these data. The imaging data reach a depth of r ≈ 22.2 (95% completeness limit for point sources) and are photometrically and astrometrically calibrated to 2% rms and 100 mas rms per coordinate, respectively. The imaging data have all been processed through a new version of the SDSS imaging pipeline, in which the most important improvement since the last data release is fixing an error in the model fits to each object. The result is that model magnitudes are now a good proxy for point-spread function magnitudes for point sources, and Petrosian magnitudes for extended sources. The spectroscopy extends from 3800 to 9200 Å at a resolution of 2000. The spectroscopic software now repairs a systematic error in the radial velocities of certain types of stars and has substantially improved spectrophotometry. All data included in the SDSS Early Data Release and First Data Release are reprocessed with the improved pipelines and included in the Second Data Release. Further characteristics of the data are described, as are the data products themselves and the tools for accessing them.
AB - The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its Second Data Release. This data release consists of 3324 deg 2 of five-band (ugriz) imaging data with photometry for over 88 million unique objects, 367,360 spectra of galaxies, quasars, stars, and calibrating blank sky patches selected over 2627 deg2 of this area, and tables of measured parameters from these data. The imaging data reach a depth of r ≈ 22.2 (95% completeness limit for point sources) and are photometrically and astrometrically calibrated to 2% rms and 100 mas rms per coordinate, respectively. The imaging data have all been processed through a new version of the SDSS imaging pipeline, in which the most important improvement since the last data release is fixing an error in the model fits to each object. The result is that model magnitudes are now a good proxy for point-spread function magnitudes for point sources, and Petrosian magnitudes for extended sources. The spectroscopy extends from 3800 to 9200 Å at a resolution of 2000. The spectroscopic software now repairs a systematic error in the radial velocities of certain types of stars and has substantially improved spectrophotometry. All data included in the SDSS Early Data Release and First Data Release are reprocessed with the improved pipelines and included in the Second Data Release. Further characteristics of the data are described, as are the data products themselves and the tools for accessing them.
KW - Atlases
KW - Catalogs
KW - Surveys
UR - http://www.scopus.com/inward/record.url?scp=4544347521&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=4544347521&partnerID=8YFLogxK
U2 - 10.1086/421365
DO - 10.1086/421365
M3 - Review article
AN - SCOPUS:4544347521
VL - 128
SP - 502
EP - 512
JO - Astronomical Journal
JF - Astronomical Journal
SN - 0004-6256
IS - 1 1783
ER -