Bayesian event reconstruction and background rejection in neutrino detectors

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dc.creatorHill, Gary C.
dc.date2001-06-05
dc.date.accessioned2026-07-07T01:58:48Z
dc.date.available2026-07-07T01:58:48Z
dc.descriptionSeveral large volume, high energy neutrino detectors are in operation or in the design stage. Upward going signal neutrino events must be separated from large backgrounds of downgoing cosmic ray induced atmospheric muons. To this end, a Bayesian extension of the traditional maximum likelihood reconstruction method will be described. Further, it will be shown how signals can be separated from backgrounds through integration of Bayesian posterior probability densities.
dc.description4 pages, Proceedings of the 27th International Cosmic Ray Conference, Hamburg, 2001
dc.identifierhttps://arxiv.org/abs/astro-ph/0106081
dc.identifierhttp://arxiv.org/abs/astro-ph/0106081
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2862
dc.subjectAstrophysics
dc.titleBayesian event reconstruction and background rejection in neutrino detectors
dc.typetext

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