X-ray and Optical Number Counts of AGN in the GOODS Fields

Details X-ray and Optical Number Counts of AGN in the GOODS Fields X-ray and Optical Number Counts of AGN in the GOODS Fields

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mas..conf...69u&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

We combine X-ray luminosity functions with appropiate spectral energy distributions (SED) to model the X-ray and optical flux distributions of the X-ray sources in the GOODS fields. A simple model based on the unified paradigm for AGN successfully reproduces the X-ray and optical number counts and is consistent with the observed spectroscopic and photometric redshift distributions. A significant population of obscured AGN are missing in the X-ray samples, but should be visible in deep far infrared observations.

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