Testing the AGN models for the X-ray background

Details Testing the AGN models for the X-ray background Testing the AGN models for the X-ray background

2000-07-14

arxiv.org/abs/astro-ph/0007207v1

Astronomy and Astrophysics

Astrophysics

3 pages, 2 figures, to appear in the Proceedings of the 4th Italian Conference on AGNs, Mem SAIt

Scientific paper

We will briefly examine the following three issues related to the AGN
synthesis models for X-ray background: 1) the possibility that absorbed AGNs
evolve faster than unabsorbed ones; 2) the existence of the still debated
population of luminous absorbed AGNs, the so-called QSO2s; 3) the behavior of
the AGN density at a redshift above ~3.

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