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| HAL : in2p3-00365817, version 1 |
| Fiche détaillée |  Récupérer au format |
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| 30th International Cosmic Ray Conference - ICRC'07, Merida : Mexique (2007) |
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| Observation of the SNR Cassiopeia A with the MAGIC telescope. |
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| E. De Oña Wilhelmi1V. VitaleA. RobertN. MankuzhiyilJ. Cortina |
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| (2008) |
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| The Supernova remnant Cassiopeia A was observed with the 17 meter imaging atmospheric Cherenkov telescope MAGIC for about 50 hours in winter 2006/07. The observations were performed in the so-called wobble mode, under moderated Moon illumination. Above 1 TeV, Cas A has been detected by the HEGRA Stereoscopic Cherenkov Telescope System, at the level of few percent of Crab. The detection of TeV gamma-rays proves that Cas A is a site of CR acceleration for particles - either nucleons or electrons - with multi-TeV energies. A detailed study of the Cas A spectrum and its extention to lower energies, where MAGIC achieves its best sensitivity, will be presented. |
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| 1 : | APC - AstroParticule et Cosmologie |
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| APC - AHE |
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| Thème(s) | : | Physique/Astrophysique/Astrophysique stellaire et solaire Planète et Univers/Astrophysique/Astrophysique stellaire et solaire |
| in2p3-00365817, version 1 | |
| http://hal.in2p3.fr/in2p3-00365817 | |
| oai:hal.in2p3.fr:in2p3-00365817 | |
| Contributeur : Simone Lantz | |
| Soumis le : Vendredi 6 Mars 2009, 10:34:26 | |
| Dernière modification le : Samedi 23 Juin 2012, 12:38:01 | |
