Observation of Galactic TeV Gamma Ray Sources with H.E.S.S.

Physics

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Scientific paper

The first telescope of the H.E.S.S. stereoscopic Cherenkov telescope system started operation in summer 2002. In spring 2003 a second telescope was added, allowing stereoscopic observations. A number of known or potential TeV gamma-ray emitters in the southern sky were observed. Data on the Crab nebula taken at large zenith angles show a clear signal and serve to verify the performance and calibration of the instrument. Observations of other Galactic sources are also summarized.

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