The hard X-ray luminosity function from ASCA surveys

Y. Ueda, Masayuki Akiyama, K. Ohta, T. Miyaji

研究成果: Article査読

4 被引用数 (Scopus)

抄録

We summarize the nature of hard X-ray populations at "bright" fluxes > 10-13 erg cm-2 s-1 (2-10 keV) from optical identification of ASCA surveys, and present results of the hard X-ray luminosity function (HXLF) of Active Galactic Nuclei (AGN). Combined with HEAO1 and Chandra surveys we construct a hard-band selected sample with extremely high degree of completeness (>95%), consisting of 228 AGNs over the flux range 10-11 ∼ 3 × 10-15 erg cm-2 s-1 (2-10 keV). We find evidence that the percentage of "type-II" AGNs decreases with the intrinsic luminosity. The intrinsic HXLF of the whole AGNs (including type-II AGNs) is well described with the pure luminosity evolution (PLE) model up to redshift of 3. Our results directly constrain the evolution of AGNs that produce a major part of the hard X-ray background.

本文言語English
ページ(範囲)36-39
ページ数4
ジャーナルAstronomische Nachrichten
324
1-2
出版ステータスPublished - 2003 1 1
外部発表はい

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

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