Blazars: the next gamma-ray view of GLAST
| dc.creator | Ciprini, Stefano | |
| dc.date | 2003-08-21 | |
| dc.date | 2003-11-20 | |
| dc.date.accessioned | 2026-07-07T02:09:17Z | |
| dc.date.available | 2026-07-07T02:09:17Z | |
| dc.description | Blazars, the extreme family of AGN, can be strong gamma-ray emitters and constitute the largest fraction of identified point sources of EGRET. The next Gamma-ray Large Area Space Telescope (GLAST) is a high energy (30MeV-300GeV) gamma-ray astronomy mission, planned for launch at the end of 2006. GLAST performances will allow to detect few thousands of gamma-ray blazars, with a broad band coverage and temporal resolution, also in quiescent emission phases, providing probably many answers about these sources. | |
| dc.description | 4 pages, 4 figures. To be appeared in "XLVII Congresso Nazionale SAIt 2003. Memorie della SAIt - Supplementi" (web-based journal). Edited by L. Girardi & S. Zaggia. 2003. Proceedings of XLVII National Conference of SAIt, held in Trieste, Italy, April 14-17, 2003 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0308377 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0308377 | |
| dc.identifier | Mem.Soc.Ast.It. 3 (2003) 238 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6377 | |
| dc.subject | Astrophysics | |
| dc.title | Blazars: the next gamma-ray view of GLAST | |
| dc.type | text |