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The Simbol-X view of the unresolved X-ray background

A. Comastri, R. Gilli, F. Fiore, C. Vignali, R. Della Ceca, G. Malaguti

arXiv, 2007

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.

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