Observation of Galactic Sources of Very High Energy γ-RAYS with the Magic Telescope

Details Observation of Galactic Sources of Very High Energy γ-RAYS with the Magic Telescope Observation of Galactic Sources of Very High Energy γ-RAYS with the Magic Telescope

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007auhe.conf..171b&link_type=abstract

ASTROPHYSICS AT ULTRA-HIGH ENERGIES. Proceedings of the 15th Course of the International School of Cosmic Ray Astrophysics . Hel

Astronomy and Astrophysics

Astronomy

Γ-Ray Astronomy, Galactic Objects, Galactic Center

Scientific paper

During its first cycle of observations, the MAGIC (Major Atmospheric Gamma-ray Imaging Cherenkov) telescope has observed very high energy γ-rays from five galactic objects: the Crab Nebula, the SNRs HESS J1813-178 and HESS J1834-087, the Galactic Center and the γ-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.

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