Spectral Statistics and Luminosity Function of a Hard X-Ray Complete Sample of Brightest AGNs(Poster) :

• SHINOZAKI,Keisuke

  Experimental Astrophysics Group, Department of Physics, Tokyo Metropolitan University

• MIYAJI,Takamitsu

  Department of Physics, Carnegie Mellon University

• ISHISAKI,Yoshitaka

  Experimental Astrophysics Group, Department of Physics, Tokyo Metropolitan University

• UEDA,Yoshihiro

  ISAS

• OGASAKA,Yasushi

  JAXA

• HAYASHIDA,Kiyoshi

  Department of Astrophysics, Nagoya University

• AWAKI,Hisamitsu

  Department of Astrophysics, Osaka University

抄録

Investigating the X-ray luminosity function of AGNs in different redshifts is very important in understanding growth of super massive black holes in centers of galaxies over the cosmological time scale. As a part of this, we are investigating the statistics of the X-ray spectral properties of a complete flux-limited sample of bright AGNs. The purpose of this investigation is to provide the present-day constraint on the evolution of absorbed and unabsorbed AGNs, and to constrain the AGN population synthesis model of the total X-ray background.

収録刊行物

• Progress of theoretical physics. Supplement

  Progress of theoretical physics. Supplement 417-418, 2004-11-15

  Progress of Theoretical Physics

詳細情報

• CRID: 1540572720350893952
• NII論文ID: 110001216444
• NII書誌ID: AA00791466
• Web Site: http://dl.ndl.go.jp/info:ndljp/pid/10885733
• 本文言語コード: en
• データソース種別:
  • NDL-Digital
  • CiNii Articles