The High Redshift AGN Population in the COSMOS Survey

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Scientific paper

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Scientific paper

We have identified a sample of high redshift / obscured AGN candidates in the COSMOS survey through cross-correlating the X-ray, Spitzer, radio, HST, and ground-based optical/IR observations of the field. The large area of the survey enables a wide range of AGN environments to be probed, in addition to sampling the faint end of the AGN luminosity function at high redshift. We discuss results from SED modelling and spectroscopy in the infrared that we have obtained for several AGN in this sample, which provide constraints on their redshifts and other properties.

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