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

K. Shinozaki·T. Miyaji·Y. Ishisaki·Y. Ueda·Y. Ogasaka·K. Hayashida·H. Awaki
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Abstract

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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K. Shinozaki, T. Miyaji, Y. Ishisaki, Y. Ueda, Y. Ogasaka, K. Hayashida, H. Awaki. 2004-02-16. Spectral Statistics and Luminosity Function of a Hard X-ray Complete Sample of Brightest AGNs. https://doi.org/10.1143/ptps.155.417

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