Very High Energy Gamma-Ray Observations with H.E.S.S
| dc.creator | van Eldik, Christopher | |
| dc.date | 2006-06-20 | |
| dc.date.accessioned | 2026-07-07T07:12:14Z | |
| dc.date.available | 2026-07-07T07:12:14Z | |
| dc.description | The H.E.S.S. Imaging Atmospheric Cherenkov Telescope Array is currently the most sensitive instrument for Very High Energy (VHE) gamma-ray observations in the energy range of about 0.1-10 TeV. During more than two years of operation with the complete 4-telescope array, many galactic and extragalactic VHE gamma-ray sources have been discovered. With its superior sensitivity and its large field-of-view camera, H.E.S.S. is particularly suited for surveys and detailed studies of extended sources. A selection of recent H.E.S.S. results is presented in this proceeding. | |
| dc.description | 8 pages, 4 figures, to appear in the proceedings of the 41st Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 11-18 March 2006 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0606486 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0606486 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/112016 | |
| dc.subject | Astrophysics | |
| dc.title | Very High Energy Gamma-Ray Observations with H.E.S.S | |
| dc.type | text |