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20 April 2024
 
  » arxiv » astro-ph/0411485

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Obscured AGN in Multiwavelength Surveys
Ezequiel Treister ; C.M. Urry ; Jeff Van Duyne ; the GOODS AGN Team ;
Date 17 Nov 2004
Subject astro-ph
AffiliationYale/U. de Chile), C.M. Urry (Yale), Jeff Van Duyne (Yale
AbstractUsing a simple unification model for AGN, with a fixed ratio of obscured to unobscured AGN of 3:1, we explain the X-ray, optical and infrared properties of the X-ray sources in the GOODS fields. That is, the GOODS data are consistent with the existence of a large population of obscured AGN out to high redshifts. About half of these are so obscured that they are missed even by hard X-ray observations, and are detected only in deep infrared observations. The previously reported decreasing trend of obscured to total AGN ratio with increasing X-ray luminosity can be explained entirely as a selection effect.
Source arXiv, astro-ph/0411485
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