TOWARD THE STANDARD POPULATION SYNTHESIS MODEL OF THE X-RAY BACKGROUND: EVOLUTION OF X-RAY LUMINOSITY AND ABSORPTION FUNCTIONS OF ACTIVE GALACTIC NUCLEI INCLUDING COMPTON-THICK POPULATIONS

Ueda, Yoshihiro; Akiyama, Masayuki; Hasinger, G.; Miyaji, T.; G. Watson, M.

doi:10.1088/0004-637x/786/2/104

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TOWARD THE STANDARD POPULATION SYNTHESIS MODEL OF THE X-RAY BACKGROUND: EVOLUTION OF X-RAY LUMINOSITY AND ABSORPTION FUNCTIONS OF ACTIVE GALACTIC NUCLEI INCLUDING COMPTON-THICK POPULATIONS

Shared by NobleBlocks on Apr 22, 2014 • 12:00 AM UTC

Authors:

Yoshihiro Ueda

Masayuki Akiyama

G. Hasinger

Abstract

We present the most up to date X-ray luminosity function (XLF) and absorption function of active galactic nuclei (AGNs) over the redshift range from 0 to 5, utilizing the largest, highly complete sample ever available obtained from surveys performed with Swift/BAT, MAXI, ASCA, XMM-Newton, Chandra, a...

Subject

Physics

Astrophysics

ROSAT

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