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

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dc.creatorComastri, Andrea
dc.creatorGilli, Roberto
dc.creatorHasinger, Guenther
dc.date2006-04-25
dc.date.accessioned2026-07-07T10:23:03Z
dc.date.available2026-07-07T10:23:03Z
dc.descriptionWe 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.
dc.description8 pages, 3 figures. Invited talk at the meeting "Gamma Wave 2005", Bonifacio, September 2005. To be published in "Experimental Astronomy"
dc.identifierhttps://arxiv.org/abs/astro-ph/0604523
dc.identifierhttp://arxiv.org/abs/astro-ph/0604523
dc.identifierExper.Astron.20:41-47,2005
dc.identifierdoi:10.1007/s10686-006-9041-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175688
dc.subjectAstrophysics
dc.titleRolling down from the 30 keV peak: modelling the hard X-ray and gamma-ray backgrounds
dc.typetext

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