The Infrared Array Camera (IRAC) Shallow Survey
The Astrophysical Journal Supplement Series2004Vol. 154(1), pp. 48–53
Citations Over TimeTop 10% of 2004 papers
Peter Eisenhardt, Daniel Stern, M. Brodwin, G. G. Fazio, G. H. Rieke, Marcia Rieke, M. W. Werner, E. L. Wright, Shadab Alam, Richard G. Arendt, M. L. N. Ashby, P. Barmby, W. J. Forrest, Joseph L. Hora, Jiasheng Huang, J. P. 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, Arjun Dey, Buell T. Jannuzi, G. P. Tiede
Abstract
The Infrared Array Camera (IRAC) shallow survey covers 8.5 deg2 in the NOAO Deep Wide-Field Survey in Boötes 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 ≈370,000, 280,000, 38,000, and 34,000 sources brighter than the 5 σ limits of 6.4, 8.8, 51, and 50 μJy at 3.6, 4.5, 5.8, and 8 μm, respectively, including some with unusual spectral energy distributions.
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