Results from MAGIC's first observation cycle on galactic sources
arXiv:astro-ph/0609149 · doi:10.1007/s10509-007-9465-0
Abstract
During 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.
6 pages, 8 figures. Prepared for "The Multi-messenger Approach to High-energy Gamma-ray Sources", Barcelona (Spain) 4-7 July 2006
References in corpus (17)
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- Sources of Relativistic Jets in the Galaxy
- Limits and Confidence Intervals in the Presence of Nuisance Parameters
- Variable Very High Energy Gamma-ray Emission from the Microquasar LS I +61 303
- Discovery of the Binary Pulsar PSR B1259-63 in Very-High-Energy Gamma Rays around Periastron with H.E.S.S
- Observation of Gamma Rays from the Galactic Center with the MAGIC Telescope
- Orbital Parameters of the Microquasar LSI +61 303
- New Catalogs of Compact Radio Sources in the Galactic Plane
- A broadband leptonic model for gamma-ray emitting microquasars
- Cosmic Rays from Microquasars: a Narrow Component to the CR Spectrum?
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- Propagation of very high energy gamma-rays inside massive binaries LS 5039 and LSI +61 303
- Observation of VHE Gamma Radiation from HESS J1834-087/W41 with the MAGIC Telescope
- Very Energetic Gamma-Rays from Microquasars and Binary Pulsars
- MAGIC observations of very high energy gamma-rays from HESS J1813-178
- High-energy gamma-ray emission from the inner jet of LS I+61 303: the hadronic contribution revisited
- Observations of Extragalactic Sources with the MAGIC Telescope