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

2005/08/11 by Trevor C. Weekes, Weekes, Trevor C.
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #Gamma-ray bursts and supernovae #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0508253

22 pages, 11 figures, Lectures given at the International Heraeus Summer School on ''Physics with Cosmic Accelerators'', Bad Honnef, Germany, July 5 - 16, 2004 (to be published by Springer-Verlag in their Lecture Notes Series)

arxiv created 2005/08/11 · arxiv updated 2009/12/01

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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