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Analysis methods for Atmospheric Cerenkov Telescopes

By M. De Naurois

Abstract

12 pages, 10 figures, proceedings of the conference "Towards a Network of Atmospheric Cherenkov Detectors VII", April 2005, Palaiseau, FranceThree different analysis techniques for Atmospheric Imaging System are presented. The classical Hillas parameters based technique is shown to be robust and efficient, but more elaborate techniques can improve the sensitivity of the analysis. A comparison of the different analysis techniques shows that they use different information for gamma-hadron separation, and that it is possible to combine their qualities

Topics: [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph]
Publisher: HAL CCSD
Year: 2005
OAI identifier: oai:HAL:in2p3-00127339v1
Provided by: Hal-Diderot
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