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The Atmospheric Cherenkov Imaging Technique for Very High Energy Gamma-ray Astronomy

Trevor C. Weekes

astro-pharXiv:astro-ph/0508253

Abstract

The Atmospheric Cherenkov Imaging Technique has opened up the gamma-ray spectrumfrom 100 GeV to 50 TeV to astrophysical exploration. The development of the technique is described as are the basic principles underlying its use. The current generation of arrays of telescopes is briefly described and the early results are summarized.

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