Toward the Standard Population Synthesis Model of the X-Ray Background:Evolution of Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations

Ueda Y., Akiyama M., Hasinger G., Miyaji, T., Watson M.G.

ApJ (2014), in press

ASCII data of predicted log N log S relations (see Figure 16) GZIPED TAR FILE