pith. sign in

arxiv: 0704.1376 · v1 · submitted 2007-04-11 · 🌌 astro-ph

Compton-thick AGN and the Synthesis of the Cosmic X-ray Background: the Suzaku Perspective

classification 🌌 astro-ph
keywords backgroundcompton-thickcosmicsuzakusynthesisx-rayabundanceadvances
0
0 comments X p. Extension
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.