The Infrared Array Camera (IRAC) shallow survey

被引：186
作者：
Eisenhardt, PR
Stern, D
Brodwin, M
Fazio, GG
Rieke, GH
Rieke, MJ
Werner, MW
Wright, EL
Allen, LE
Arendt, RG
Ashby, MLN
Barmby, P
Forrest, WJ
Hora, JL
Huang, JS
Huchra, J
Pahre, MA
Pipher, JL
Reach, WT
Smith, HA
Stauffer, JR
Wang, Z
Willner, SP
Brown, MJI
Dey, A
Jannuzi, BT
Tiede, GP
机构：
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[3] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[4] Univ Calif Los Angeles, Los Angeles, CA 90095 USA
[5] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[6] Univ Rochester, Rochester, NY 14627 USA
[7] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA
[8] Natl Opt Astron Observ, Tucson, AZ 85726 USA
[9] Bowling Green State Univ, Bowling Green, OH 43403 USA
来源：
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2004年 / 154卷 / 01期
关键词：
infrared : galaxies; infrared : stars; surveys;
D O I：
10.1086/423180
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Infrared Array Camera (IRAC) shallow survey covers 8.5 deg(2) in the NOAO Deep Wide-Field Survey in Bootes with three or more 30 s exposures per position. An overview of the survey design, reduction, calibration, star-galaxy separation, and initial results is provided. The survey includes approximate to370,000, 280,000, 38,000, and 34,000 sources brighter than the 5 sigma limits of 6.4, 8.8, 51, and 50 muJy at 3.6, 4.5, 5.8, and 8 mum, respectively, including some with unusual spectral energy distributions.
引用
收藏
页码：48 / 53
页数：6
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