The IRAC Shallow Survey

P. R. Eisenhardt; D. Stern; M. Brodwin; G. G. Fazio; G. H. Rieke; M. J. Rieke; M. W. Werner; E. L. Wright; L. E. Allen; R. G. Arendt; M. L. N. Ashby; P. Barmby; W. J. Forrest; J. L. Hora; J. -S. Huang; J. Huchra; M. A. Pahre; J. L. Pipher; W. T. Reach; H. A. Smith; J. R. Stauffer; Z. Wang; S. P. Willner; M. J. I. Brown; A. Dey; B. T. Jannuzi; G. P. Tiede

doi:10.1086/423180

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arXiv · astro-ph/0406251

The IRAC Shallow Survey

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Abstract

The IRAC shallow survey covers 8.5 square degrees in the NOAO Deep Wide-Field Survey in Bootes with 3 or more 30 second exposures per position. An overview of the survey design, reduction, calibration, star-galaxy separation, and initial results is provided. The survey includes approximately 370,000, 280,000, 38,000, and 34,000 sources brighter than the 5 sigma limits of 6.4, 8.8, 51, and 50 microJy at 3.6, 4.5, 5.8, and 8 microns respectively, including some with unusual spectral energy distributions.

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P. R. Eisenhardt, D. Stern, M. Brodwin, G. G. Fazio, G. H. Rieke, M. J. Rieke, M. W. Werner, E. L. Wright, L. E. Allen, R. G. Arendt, M. L. N. Ashby, P. Barmby, W. J. Forrest, J. L. Hora, J. -S. Huang, J. Huchra, M. A. Pahre, J. L. Pipher, W. T. Reach, H. A. Smith, J. R. Stauffer, Z. Wang, S. P. Willner, M. J. I. Brown, A. Dey, B. T. Jannuzi, G. P. Tiede. 2004-06-09. The IRAC Shallow Survey. https://doi.org/10.1086/423180

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