Results from MAGIC's first observation cycle on galactic sources

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dc.creatorRico, Javier
dc.date2006-09-06
dc.date.accessioned2026-07-07T10:40:01Z
dc.date.available2026-07-07T10:40:01Z
dc.descriptionDuring its Cycle I, the MAGIC telescope targeted about 250 hours several galactic sources sought to be, or detected previously by other experiments in the same energy domain, gamma-ray emitters. This paper reviews some results of such MAGIC observations covering, among others, supernova remnants, the Galactic Center and microquasars. We will concentrate on the recent discovery at very high energy gamma-rays of the microquasar LS I +61 303.
dc.description6 pages, 8 figures. Prepared for "The Multi-messenger Approach to High-energy Gamma-ray Sources", Barcelona (Spain) 4-7 July 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0609149
dc.identifierhttp://arxiv.org/abs/astro-ph/0609149
dc.identifierAstrophys.SpaceSci.309:285-291,2007
dc.identifierdoi:10.1007/s10509-007-9465-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181231
dc.subjectAstrophysics
dc.titleResults from MAGIC's first observation cycle on galactic sources
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