Rolling down from the 30 keV peak: modelling the hard X-ray and gamma-ray backgrounds

Details Rolling down from the 30 keV peak: modelling the hard X-ray and gamma-ray backgrounds Rolling down from the 30 keV peak: modelling the hard X-ray and gamma-ray backgrounds

2006-04-25

arxiv.org/abs/astro-ph/0604523v1

Exper.Astron.20:41-47,2005

Astronomy and Astrophysics

Astrophysics

8 pages, 3 figures. Invited talk at the meeting "Gamma Wave 2005", Bonifacio, September 2005. To be published in "Experimental

Scientific paper

10.1007/s10686-006-9041-6

We will briefly discuss the importance of sensitive X-ray observations above
a few tens of keV for a better understanding of the physical mechanisms
associated to the Supermassive Black Hole primary emission in both radio quiet
and radio loud AGN and to the cosmological evolution of the most obscured
sources.

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