The Seyfert galaxies in the local Universe: from BeppoSAX to Simbol-X
| dc.creator | Dadina, Mauro | |
| dc.date | 2008-01-28 | |
| dc.date.accessioned | 2026-07-07T08:56:52Z | |
| dc.date.available | 2026-07-07T08:56:52Z | |
| dc.description | The operational conditions found by $BeppoSAX$ in observing nearby (z$\leq$0.1) Seyferts were reproduced for $Simbol$-$X$ in order to simulate a realistic final database of the mission. The results indicate that, even in the worst conditions, the $Simbol$-$X$ archive of pointings will allow to fully characterize the high-energy spectrum of nearby Seyferts and, most importantly, to obtain solid results on R and Ec (fundamental to model the cosmic X-Ray background, CXB). The measurement of the inclination angle of the accretion disk will be possible for $\sim$15 objects allowing to directly test the unified models for AGN. Finally, the time-dependent characteristics of the reflected component will be studied in at least $\sim$25 objects. | |
| dc.description | 4 pages, 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/0801.4340 | |
| dc.identifier | http://arxiv.org/abs/0801.4340 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/146765 | |
| dc.subject | Astrophysics | |
| dc.title | The Seyfert galaxies in the local Universe: from BeppoSAX to Simbol-X | |
| dc.type | text |