Performance Limits for Cherenkov Instruments

Simple item page
dc.creatorHofmann, W.
dc.date2006-03-03
dc.date2006-03-17
dc.date.accessioned2026-07-07T07:00:57Z
dc.date.available2026-07-07T07:00:57Z
dc.descriptionThe performance of Cherenkov instruments for the detection of very high energy gamma rays is ultimately limited by the fluctuations in the development of air showers. With particular emphasis on the angular resolution, the ultimate performance limits are investigated on the basis of simulations.
dc.descriptionTalk presented at the Cherenkov 2005 Workshop, Palaiseau; 7 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0603076
dc.identifierhttp://arxiv.org/abs/astro-ph/0603076
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/108138
dc.subjectAstrophysics
dc.titlePerformance Limits for Cherenkov Instruments
dc.typetext

Files

Collections

arXiv