We will briefly discuss the importance of sensitive X-ray observations above 10 keV for a better understanding of the physical mechanisms associated to the Supermassive Black Hole primary emission and to the cosmological evolution of the most obscured Active Galactic Nuclei.
Comastri A., Gilli R., Fiore F., Vignali C., Della Ceca R., Malaguti G. (2008). The Simbol-X view of the unresolved X-ray background. s.l : Memories of SAIt.
The Simbol-X view of the unresolved X-ray background
VIGNALI, CRISTIAN;
2008
Abstract
We will briefly discuss the importance of sensitive X-ray observations above 10 keV for a better understanding of the physical mechanisms associated to the Supermassive Black Hole primary emission and to the cosmological evolution of the most obscured Active Galactic Nuclei.File in questo prodotto:
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