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Evidence for Infrared-Faint Radio Sources as z > 1 Radio-Loud AGN

Infrared-Faint Radio Sources (IFRSs) are a class of radio objects found in the Australia Telescope Large Area Survey (ATLAS) which have no observable mid-infrared counterpart in the Spitzer Wide-area Infrared Extragalactic (SWIRE) survey. The extended Chandra Deep Field South now has even deeper Spitzer imaging (3.6 to 70 micron) from a number of Legacy surveys. We report the detections of two IFRS sources in IRAC images. The non-detection of two other IFRSs allows us to constrain the source type. Detailed modeling of the SED of these objects shows that they are consistent with high redshift (z > 1) AGN.

preprint2010arXivOpen access
M. T. HuynhR. P. NorrisB. SianaE. Middelberg
astro-ph.CO
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M. T. HuynhR. P. NorrisB. SianaE. Middelberg

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