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

Thumbnail Image

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

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

Keywords

Astrophysics

Citation

URI

http://salesiana.dossiersoluciones.com/handle/123456789/183654

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0402363
 http://arxiv.org/abs/astro-ph/0402363
 Prog.Theor.Phys.Suppl.155:417-418,2004
 doi:10.1143/PTPS.155.417

Collections

arXiv