X-ray Stacking Of 70μM Detected Sources In The C-COSMOS Field

Details X-ray Stacking Of 70μM Detected Sources In The C-COSMOS Field X-ray Stacking Of 70μM Detected Sources In The C-COSMOS Field

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21342004k&link_type=abstract

American Astronomical Society, AAS Meeting #213, #420.04; Bulletin of the American Astronomical Society, Vol. 41, p.236

Astronomy and Astrophysics

Astronomy

Scientific paper

Sources detected at 70μm in the COSMOS field are infrared luminous galaxies predominantly in the range 00.5 sources (H-S/H+S = -0.270) than for the z<0.5 sources (H-S/H+S = -0.516). For the sources z>0.5 the hard X-ray spectral shape indicates they are dominated by more intrinsically luminous AGN compared to the softer X-ray spectral shape of the nearby sources which is characteristic of star formation. The harder composite X-ray SED for the more distant objects suggests that luminous 70μm sources are a valuable way to find high-redshift obscured AGN.

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