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

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概要

• 論文の詳細を見る

• 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.

• 2004-11-15

著者

• AWAKI Hisamitsu

  Department of Physics, Ehime University

• OGASAKA Yasushi

  Department of Particle and Astrophysics, Nagoya University

• MIYAJI Takamitsu

  Department of Physics, Carnegie Mellon University

• Hayashida Kiyoshi

  Department Of Astrophysics Osaka University

• SHINOZAKI Keisuke

  Experimental Astrophysics Group, Department of Physics, Tokyo Metropolitan University

• ISHISAKI Yoshitaka

  Experimental Astrophysics Group, Department of Physics, Tokyo Metropolitan University

• Awaki H

  Department Of Physics Ehime University

• Awaki Hisamitsu

  Department Of Physics Ehime University

• Ogasaka Y

  The Institute Of Space And Astronautical Science

• Shinozaki Keisuke

  Experimental Astrophysics Group Department Of Physics Tokyo Metropolitan University

• Miyaji Takamitsu

  Department Of Physics Carnegie Mellon University

• UEDA Yoshihiro

  ISAS/JAXA

• Ogasaka Yasushi

  Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA)

• OGASAKA Yasushi

  Department of Astrophysics, Nagoya University

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