The u′g′r′i′z′ standard-star system

被引:1396
作者
Smith, JA
Tucker, DL
Kent, S
Richmond, MW
Fukugita, M
Ichikawa, T
Ichikawa, S
Jorgensen, AM
Uomoto, A
Gunn, JE
Hamabe, M
Watanabe, M
Tolea, A
Henden, A
Annis, J
Pier, JR
McKay, TA
Brinkmann, J
Chen, B
Holtzman, J
Shimasaku, K
York, DG
机构
[1] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[2] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA
[3] Rochester Inst Technol, Dept Phys, Rochester, NY 14623 USA
[4] Univ Tokyo, Inst Cosm Ray Res, Tokyo 1888502, Japan
[5] Inst Adv Study, Princeton, NJ 08540 USA
[6] Tohoku Univ, Inst Astron, Sendai, Miyagi 9808578, Japan
[7] Natl Astron Observ, Tokyo 1818588, Japan
[8] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[9] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[10] Princeton Univ Observ, Princeton, NJ 08544 USA
[11] Japan Womens Univ, Dept Math & Phys Sci, Tokyo 1128681, Japan
[12] Inst Space & Astronaut Sci, Kanagawa 2298510, Japan
[13] USN Observ, Flagstaff Stn, Flagstaff, AZ 86002 USA
[14] Apache Point Observ, Sunspot, NM 88349 USA
[15] New Mexico State Univ, Dept Astron, Las Cruces, NM 88003 USA
[16] Univ Tokyo, Dept Astron, Tokyo 1130033, Japan
[17] Univ Tokyo, Res Ctr Early Universe, Tokyo 1130033, Japan
[18] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[19] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
关键词
catalogs; standards; stars : fundamental parameters;
D O I
10.1086/339311
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the 158 standard stars that de ne the u' g' r' i' z' photometric system. These stars form the basis for the photometric calibration of the Sloan Digital Sky Survey. The de ning instrument system and filters, the observing process, the reduction techniques, and the software used to create the stellar network are all described. We briefly discuss the history of the star selection process, the derivation of a set of transformation equations for the UBVRCIC system, and plans for future work.
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页码:2121 / 2144
页数:24
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