Abstract
We combine the results of the Spitzer IRAC Shallow Survey and the Chandra XBoötes Survey of the 8.5 deg 2 Boötes field of the NOAO Deep Wide-Field Survey to produce the largest comparison of mid-IR and X-ray sources to date. The comparison is limited to sources with X-ray fluxes >8×10 -15 ergs cm -2 s -1 in the 0.5-7.0 keV range and mid-IR sources with 3.6 μm fluxes brighter than 18.4 mag (12.3 μJy). In this most sensitive IRAC band, 85% of the 3086 X-ray sources have mid-IR counterparts at an 80% confidence level based on a Bayesian matching technique. Only 2.5% of the sample have no IRAC counterpart at all based on visual inspection. Even for a smaller but a significantly deeper Chandra survey in the same field, the IRAC Shallow Survey recovers most of the X-ray sources. A majority (65%) of the Chandra sources detected
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CITATION STYLE
Gorjian, V., Brodwin, M., Kochanek, C. S., Murray, S., Stern, D., Brand, K., … Willner, S. P. (2008). The Mid‐Infrared Properties of X‐Ray Sources. The Astrophysical Journal, 679(2), 1040–1046. https://doi.org/10.1086/587431
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