Infrared Faint Radio Sources in the Extended Chandra Deep Field South

Details Infrared Faint Radio Sources in the Extended Chandra Deep Field South Infrared Faint Radio Sources in the Extended Chandra Deep Field South

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21342428h&link_type=abstract

American Astronomical Society, AAS Meeting #213, #424.28; Bulletin of the American Astronomical Society, Vol. 41, p.250

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Scientific paper

Infrared-Faint Radio Sources (IFRSs) are a class of radio objects found in the Australia Telescope Large Area Survey (ATLAS) which have no observable counterpart in the Spitzer Wide-area Infrared Extragalactic Survey (SWIRE). 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 AGN (z > 2).

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