The Space Density of Compton Thick AGN

Astronomy and Astrophysics – Astrophysics

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Scientific paper

Most cosmic accretion onto super-massive black holes is obscured by gas and dust that absorbs all but the hardest X-ray photons. By performing deep observations at very high energies, E>10; keV, it is possible to obtain a complete sample of the AGN population, including the elusive Compton thick (CT) sources. Here, we present a study of the population of CT AGN and its relationship to the extragalactic X-ray background. Based on observations at rest frame energies greater than 10 keV, we found that in the local Universe CT AGN are less numerous than previously expected, and contribute only ˜10% of the extragalactic X-ray radiation. We compare the observed spatial density of local and high redshift CT sources and find an apparent lack of CT AGN in the nearby Universe. This indicates that the most obscured sources follow a different evolution than mildy-absorbed AGN. Finally, we present prospects for the detection of highly obscured AGN at the epoch of maximum supermassive black hole growth, z˜1, using planned space missions like NuSTAR and EXIST.
E.T. gratefully acknowledges the support provided by NASA through Chandra Postdoctoral Fellowship Award Number PF8-90055 issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of NASA under contract NAS8-03060. This work was made possible by support from NASA/INTEGRAL grant NNG05GM79G.

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