We investigated the statistics of the X-ray spectral properties of a complete flux-limited sample of bright AGNs from HEAO-1 all-sky catalogs to provide the bright end constraint of the evolution of AGN hard X-ray luminosity function (HXLF) and the AGN population synthesis model of the X-ray background. Spectral studies have been made using ASCA and XMM-Newton observation data for almost all AGNs in this sample.
@article{arxiv.astro-ph/0402363,
title = {Spectral Statistics and Luminosity Function of a Hard X-ray Complete Sample of Brightest AGNs},
author = {K. Shinozaki and T. Miyaji and Y. Ishisaki and Y. Ueda and Y. Ogasaka and K. Hayashida and H. Awaki},
journal= {arXiv preprint arXiv:astro-ph/0402363},
year = {2008}
}
Comments
PTPTex v0.88, 2 pages with 4 figures, Proceedings of the "Stellar-Mass, Intermediate -Masss, and Supermassive Black Holes" in Kyoto, Japan