Analysis methods for Atmospheric Cerenkov Telescopes

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dc.creatorde Naurois, Mathieu
dc.date2006-07-12
dc.date.accessioned2026-07-07T07:15:39Z
dc.date.available2026-07-07T07:15:39Z
dc.descriptionThree 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.
dc.description12 pages, 10 figures, proceedings of the conference "Towards a Network of Atmospheric Cherenkov Detectors VII", April 2005, Palaiseau, France
dc.identifierhttps://arxiv.org/abs/astro-ph/0607247
dc.identifierhttp://arxiv.org/abs/astro-ph/0607247
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/113294
dc.subjectAstrophysics
dc.titleAnalysis methods for Atmospheric Cerenkov Telescopes
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