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

Simple item page
dc.creatorWeekes, Trevor C.
dc.date2005-08-11
dc.date.accessioned2026-07-07T02:18:26Z
dc.date.available2026-07-07T02:18:26Z
dc.descriptionThe 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.
dc.description22 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)
dc.identifierhttps://arxiv.org/abs/astro-ph/0508253
dc.identifierhttp://arxiv.org/abs/astro-ph/0508253
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9487
dc.subjectAstrophysics
dc.titleThe Atmospheric Cherenkov Imaging Technique for Very High Energy Gamma-ray Astronomy
dc.typetext

Files

Collections

arXiv