TOWARD THE STANDARD POPULATION SYNTHESIS MODEL OF THE X-RAY BACKGROUND: EVOLUTION OF X-RAY LUMINOSITY AND ABSORPTION FUNCTIONS OF ACTIVE GALACTIC NUCLEI INCLUDING COMPTON-THICK POPULATIONS
Yoshihiro Ueda(Kyoto University), M. G. Watson(University of Leicester), G. Hasinger(Max Planck Institute for Astrophysics), T. Miyaji(Universidad Autónoma de Baja California), Masayuki Akiyama(Tohoku University)
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