The Simbol-X view of the unresolved X-ray background
| dc.creator | Comastri, A. | |
| dc.creator | Gilli, R. | |
| dc.creator | Fiore, F. | |
| dc.creator | Vignali, C. | |
| dc.creator | Della Ceca, R. | |
| dc.creator | Malaguti, G. | |
| dc.date | 2007-11-08 | |
| dc.date.accessioned | 2026-07-07T08:41:48Z | |
| dc.date.available | 2026-07-07T08:41:48Z | |
| dc.description | 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. | |
| dc.description | 6 pages, 5 figures, to appear in proceedings of "Simbol-X: the hard X-ray Universe in focus", held in Bologna (Italy), May 14-16, 2007 | |
| dc.identifier | https://arxiv.org/abs/0711.1356 | |
| dc.identifier | http://arxiv.org/abs/0711.1356 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/141791 | |
| dc.subject | Astrophysics | |
| dc.title | The Simbol-X view of the unresolved X-ray background | |
| dc.type | text |