The Infrared Array Camera (IRAC) shallow survey

被引：187

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

页码：48 / 53

页数：6

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