Spectral Statistics and Luminosity Function of a Hard X-ray Complete Sample of Brightest AGNs

Details Spectral Statistics and Luminosity Function of a Hard X-ray Complete Sample of Brightest AGNs Spectral Statistics and Luminosity Function of a Hard X-ray Complete Sample of Brightest AGNs

2004-02-16

arxiv.org/abs/astro-ph/0402363v1

Prog.Theor.Phys.Suppl.155:417-418,2004

Astronomy and Astrophysics

Astrophysics

PTPTex v0.88, 2 pages with 4 figures, Proceedings of the "Stellar-Mass, Intermediate -Masss, and Supermassive Black Holes" in

Scientific paper

10.1143/PTPS.155.417

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.

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