The H. E. S. S. Project

Details The H. E. S. S. Project The H. E. S. S. Project

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sngh.conf...53m&link_type=abstract

SCIENCE WITH THE NEW GENERATION OF HIGH ENERGY GAMMA-RAY EXPERIMENTS The Variable Gamma-Ray Sources: Their Identifications and C

Physics

Gamma Rays, Observations

Scientific paper

The H.E.S.S. Imaging Atmospheric Cherenkov Telescope Array is currently the most sensitive instrument for Very High Energy (VHE) γ-ray observations in the energy range of about 0.1-10 TeV. While the detector is well suited for studies of extended galactic sources, an extensive program of observations of variable point-sources has also been carried out in the past three years of operation. Many galactic and extragalactic VHE γ-ray sources have been discovered, and a selection of recent H.E.S.S. results is presented in this proceeding.

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