IR-excess radio-quiet AGN: deviations from the radio-FIR correlation

Details IR-excess radio-quiet AGN: deviations from the radio-FIR correlation IR-excess radio-quiet AGN: deviations from the radio-FIR correlation

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atnf.prop.2403n&link_type=abstract

ATNF proposal C1966, Semester: July, 2009

Other

Extragalactic, Atca

Scientific paper

By stacking radio data at the position of 24 micron sources, Boyle et al. (2007) showed that the radio-FIR correlation extended down to 1 microJy, but caused some controversy by claiming a different quotient of the radio-FIR correlation from other authors. We now recognise that this is caused by a hitherto unrecognised population of infrared-excess objects which are picked up by the Boyle et al stacking technique, but are omitted from conventional radio-selected studies of the radio-FIR correlation. We suggest that these objects are radio-quiet AGN in which the IR excess is caused by dust heated by the AGN, and here we propose sensitive high-resolution observations using CABB at 6 and 3 cm to test this hypothesis.

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