MAGIC is a single‐dish Cherenkov telescope located on La Palma (Spain), hence with an optimal view on the Northern sky. Sensitive in the 30 GeV—30 TeV energy band, it is nowadays the only ground‐based instrument being able to measure high‐energy γ‐rays below 100 GeV. We review the most recent experimental results on Galactic sources obtained using MAGIC. These include pulsars, binary systems, supernova remnants and unidentified sources.

Results of MAGIC galactic sources

PASCOLI, DONATELLA;
2008

Abstract

MAGIC is a single‐dish Cherenkov telescope located on La Palma (Spain), hence with an optimal view on the Northern sky. Sensitive in the 30 GeV—30 TeV energy band, it is nowadays the only ground‐based instrument being able to measure high‐energy γ‐rays below 100 GeV. We review the most recent experimental results on Galactic sources obtained using MAGIC. These include pulsars, binary systems, supernova remnants and unidentified sources.
2008
AIP conference Proceedings.High Energy Gamma-Ray Astronomy:4th International Symposium on High Energy Gamma-Ray Astronomy.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/183110
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