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Atmospheric Cherenkov Gamma-ray Telescopes

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 نشر من قبل Jamie Holder
 تاريخ النشر 2015
  مجال البحث فيزياء
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 تأليف Jamie Holder




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The stereoscopic imaging atmospheric Cherenkov technique, developed in the 1980s and 1990s, is now used by a number of existing and planned gamma-ray observatories around the world. It provides the most sensitive view of the very high energy gamma-ray sky (above 30 GeV), coupled with relatively good angular and spectral resolution over a wide field-of-view. This Chapter summarizes the details of the technique, including descriptions of the telescope optical systems and cameras, as well as the most common approaches to data analysis and gamma-ray reconstruction.



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