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

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dc.creatorShinozaki, K.
dc.creatorMiyaji, T.
dc.creatorIshisaki, Y.
dc.creatorUeda, Y.
dc.creatorOgasaka, Y.
dc.creatorHayashida, K.
dc.creatorAwaki, H.
dc.date2004-02-16
dc.date.accessioned2026-07-07T10:47:47Z
dc.date.available2026-07-07T10:47:47Z
dc.descriptionWe 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.
dc.descriptionPTPTex v0.88, 2 pages with 4 figures, Proceedings of the "Stellar-Mass, Intermediate -Masss, and Supermassive Black Holes" in Kyoto, Japan
dc.identifierhttps://arxiv.org/abs/astro-ph/0402363
dc.identifierhttp://arxiv.org/abs/astro-ph/0402363
dc.identifierProg.Theor.Phys.Suppl.155:417-418,2004
dc.identifierdoi:10.1143/PTPS.155.417
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183654
dc.subjectAstrophysics
dc.titleSpectral Statistics and Luminosity Function of a Hard X-ray Complete Sample of Brightest AGNs
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