Aims. We investigate here the X-ray luminosity function (XLF) of absorbed (NH between 4 1021 and 1024 cm-2) and unabsorbed (NH < 4 1021 cm-2) AGN, the fraction of absorbed AGN as a function of LX (and z), the intrinsic NH distribution of the AGN population, and the XLF of Compton thick (NH > 1024 cm-2) AGN.
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