Implementation of the trigger algorithm for the NEMO project

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dc.creatord'Angelo, G.
dc.creatorRiccio, G.
dc.creatorBrescia, M.
dc.date2007-01-22
dc.date.accessioned2026-07-07T07:42:02Z
dc.date.available2026-07-07T07:42:02Z
dc.descriptionWe describe the implementation of trigger algorithm specifically tailored on the characteristics of the neutrino telescope NEMO. Extensive testing against realistic simulations shows that, by making use of the uncorrelated nature of the noise produced mainly by the decay of K-40 beta-decay, this trigger is capable to discriminate among different types of muonic events.
dc.descriptionPublished in the Proceedings of the "I Workshop of Astronomy and Astrophysics for Students", Eds. N.R. Napolitano & M. Paolillo, Naples, 19-20 April 2006 (astro-ph/0701577)
dc.identifierhttps://arxiv.org/abs/astro-ph/0701622
dc.identifierhttp://arxiv.org/abs/astro-ph/0701622
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/122339
dc.subjectAstrophysics
dc.titleImplementation of the trigger algorithm for the NEMO project
dc.typetext

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