Compton-Thick AGN and the Synthesis of the Cosmic X-Ray Background : The Suzaku Perspective(Chapter 10. Super Massive Black Holes, The Extreme Universe in the Suzaku Era)

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概要

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• We discuss the abundance of Compton-thick AGN as estimated by the most recent population synthesis models of the cosmic X-ray background. Only a small fraction of these elusive objects have been detected so far, in line with the model expectations. The advances expected by the broad band detectors on board Suzaku are briefly reviewed.

• 2007-12-19

著者

• HASINGER Gunther

  Max-Planck-Institut fur extraterrestrische Physik

• GILLI Roberto

  INAF-Osservatorio Astronomico di Bologna

• COMASTRI Andrea

  INAF-Osservatorio Astronomico di Bologna

• VIGNALI Cristian

  Dipartimento di Astronomia, Universita degli Studi di Bologna

• Vignali Cristian

  Dipartimento Di Astronomia Universita Di Bologna

関連論文

• The X-Ray Observatory Suzaku
• Compton-Thick AGN and the Synthesis of the Cosmic X-Ray Background : The Suzaku Perspective(Chapter 10. Super Massive Black Holes, The Extreme Universe in the Suzaku Era)
• Suzaku Observation of Abell 2204 : Galaxy Cluster Gas Temperature Measurement Up to the Virial Radius(Chapter 2. Thermal Structure/Dynamics of Groups and Clusters of Galaxies, The Extreme Universe in the Suzaku Era)
• Compton Thick AGN in the Suzaku Era(Chapter 10. Super Massive Black Holes, The Extreme Universe in the Suzaku Era)
• Suzaku Observations of SN 1987A

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