Observation of Galactic Sources of Very High Energy Gamma-Rays with the MAGIC Telescope

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dc.creatorBartko, Hendrik
dc.date2006-12-04
dc.date2006-12-07
dc.date.accessioned2026-07-07T07:31:02Z
dc.date.available2026-07-07T07:31:02Z
dc.descriptionDuring its first cycle of observations, the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov) telescope has observed very high energy gamma-rays from five galactic objects: the Crab Nebula, the SNRs HESS J1813-178 and HESS J1834-087, the Galactic Center and the gamma-ray binary LS I +61 303. After a short introduction to the MAGIC telescope and the data analysis procedure, the results of these five sources are reviewed.
dc.descriptionTo appear in the proceedings of the International School of Cosmics Ray Astrophysics (ISCRA) 15th Course: Astrophysics at Ultra-High Energies, Erice, Sicily, Italy, 20-27 Jun 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0612065
dc.identifierhttp://arxiv.org/abs/astro-ph/0612065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118612
dc.subjectAstrophysics
dc.titleObservation of Galactic Sources of Very High Energy Gamma-Rays with the MAGIC Telescope
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