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

1); A. Comastri (1); Bologna); C. Vignali (3; F. Fiore (2); G. Malaguti (5) ((1) INAF - Osservatorio Astronomico di Bologna; (2) INAF - Osservatorio Astronomico di Roma; (3) Dipartimento di Astronomia; Milano; (5) INAF-IASF; R. Della Ceca (4); R. Gilli (1); Universita` di Bologna; (4) INAF - Osservatorio Astronomico di Brera

arxiv: 0711.1356 · v1 · submitted 2007-11-08 · 🌌 astro-ph

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

A. Comastri (1) , R. Gilli (1) , F. Fiore (2) , C. Vignali (3 , 1) , R. Della Ceca (4) , G. Malaguti (5) ((1) INAF - Osservatorio Astronomico di Bologna; (2) INAF - Osservatorio Astronomico di Roma; (3) Dipartimento di Astronomia , Universita` di Bologna; (4) INAF - Osservatorio Astronomico di Brera

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Milano; (5) INAF-IASF Bologna)

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keywords x-rayaboveactiveassociatedbackgroundbetterblackbriefly

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

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