In this paper, I present a summary of the status of γ-ray astronomy in the very high energy band (E > 50GeV), as of early 2007. It covers a selection of results obtained from observations made by ground-based detectors using the atmospheric Cherenkov or air shower techniques, together with short descriptions of some of the present and future experiments.
KeywordsSupernova Remnant Crab Nebula Extragalactic Source Cherenkov Light Very High Energy
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