X-ray and optical followup of gamma-ray (up to TeV) sources
| dc.creator | Masetti, N. | |
| dc.date | 2007-10-24 | |
| dc.date.accessioned | 2026-07-07T08:38:23Z | |
| dc.date.available | 2026-07-07T08:38:23Z | |
| dc.description | The imaging capabilities of the INTEGRAL and HESS observatories allow the study of hard X-ray and TeV sources with unprecedented positional accuracy. Here I review the multiwavelength followup studies which are currently being performed on the unidentified sources detected by these facilities in order to unveil their actual nature. | |
| dc.description | 11 pages, 6 figures, ChJAA in press; proceedings of the Frascati Workshop 2007 "Multifrequency behaviour of high energy cosmic sources" (F. Giovannelli & L. Sabau-Graziati eds.). The quality of Fig. 1 was degraded to fit the arXiv uploads size limits | |
| dc.identifier | https://arxiv.org/abs/0710.4447 | |
| dc.identifier | http://arxiv.org/abs/0710.4447 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/140712 | |
| dc.subject | Astrophysics | |
| dc.title | X-ray and optical followup of gamma-ray (up to TeV) sources | |
| dc.type | text |