Very High Energy Gamma-Ray Observations with H.E.S.S

Details Very High Energy Gamma-Ray Observations with H.E.S.S Very High Energy Gamma-Ray Observations with H.E.S.S

2006-06-20

arxiv.org/abs/astro-ph/0606486v1

Astronomy and Astrophysics

Astrophysics

8 pages, 4 figures, to appear in the proceedings of the 41st Rencontres de Moriond on Electroweak Interactions and Unified The

Scientific paper

The H.E.S.S. Imaging Atmospheric Cherenkov Telescope Array is currently the most sensitive instrument for Very High Energy (VHE) gamma-ray observations in the energy range of about 0.1-10 TeV. During more than two years of operation with the complete 4-telescope array, many galactic and extragalactic VHE gamma-ray sources have been discovered. With its superior sensitivity and its large field-of-view camera, H.E.S.S. is particularly suited for surveys and detailed studies of extended sources. A selection of recent H.E.S.S. results is presented in this proceeding.

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