The Compton-thick AGN in the CDF-N
arXiv:0909.0224
Abstract
We present X-ray spectral analysis of the brightest sources (f_{2-10 keV}>10^{-15}\sim2$. The number count vs. flux distribution of the candidate Compton-thick AGN as well as their distribution with redshift agree reasonably well with the predictions of the X-ray background synthesis models of Gilli et al.
13 pages, to appear in Astronomy & Astrophysics