X-Ray Sources and a Radio Source in a Faint Mid-Infrared Sample

Details X-Ray Sources and a Radio Source in a Faint Mid-Infrared Sample X-Ray Sources and a Radio Source in a Faint Mid-Infrared Sample

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mas..conf..313s&link_type=abstract

MULTIWAVELENGTH AGN SURVEYS. Proceedings of the Guillermo Haro Conference 2003. Held 8-12 December 2003 in Cozumel, Mexico. Edit

Astronomy and Astrophysics

Astronomy

Scientific paper

The Infrared Space Observatory (ISO) have detected their 6.7 μm counterparts to all four Chandra sources and one VLA/FIRST source in the SSA13 field. The five X-ray and radio sources indicate up to 15% AGN contribution to the faint mid-infrared sky down to 12 μJy at 6.7 μm. Their long-baseline spectral energy distributions and non-stellar profiles at the optical and near-infrared suggest large contributions from their host galaxies. Their red optical colors, high spectroscopic or photometric redshifts (z > 1) and large stellar masses imply that they would be matured galaxies with vigorous star formation at very high redshifts.

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