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Water cherenkov detectors response to a Gamma Ray Burst in the large aperture GRB observatory

dc.rights.licensehttp://creativecommons.org/licenses/by-nc-sa/3.0/ve/
dc.contributor.authorAllard, D.
dc.contributor.authorAlvarez, C.
dc.contributor.authorAsorey, H.
dc.contributor.authorBarros, Humberto J. V.
dc.contributor.authorBertou, Xavier
dc.contributor.authorCastillo, M.
dc.contributor.authorChirinos, J. M.
dc.contributor.authorDe Castro, A.
dc.contributor.authorFlores, S.
dc.contributor.authorGomez Berisso, M.
dc.contributor.authorGrajales, J.
dc.contributor.authorGuada B., Carlos E.
dc.contributor.authorW.R. Guevara, Day
dc.contributor.authorIshitsuka, J.
dc.contributor.authorLópez, J. A.
dc.contributor.authorMartínez, O.
dc.contributor.authorMelfo, A.
dc.contributor.authorMezal, E.
dc.contributor.authorMiranda Loza, P.
dc.contributor.authorMoreno Barbosa, E.
dc.contributor.authorMurrugarrad, C.
dc.contributor.authorNúñez, Luis
dc.contributor.authorOtiniano Ormachea, L. J.
dc.contributor.authorPérez, G.
dc.contributor.authorPérez, Y.
dc.contributor.authorPonce, E.
dc.contributor.authorQuispe, J.
dc.contributor.authorQuintero, Carlos
dc.contributor.authorRivera, H.
dc.contributor.authorRosales R., Misael D.
dc.contributor.authorRovero, A. C.
dc.contributor.authorSaavedra, O.
dc.contributor.authorSalazare, H.
dc.contributor.authorTello, J. C.
dc.contributor.authorTicona Peralda, R.
dc.contributor.authorVarela, E.
dc.contributor.authorVelarde, A.
dc.contributor.authorVillasenor, L.
dc.contributor.authorWahl, D.
dc.contributor.authorZamalloa, M.A.
dc.date.accessioned2010-03-18T21:50:41Z
dc.date.available2010-03-18T21:50:41Z
dc.date.issued2009-06-04
dc.identifier.urihttp://www.saber.ula.ve/handle/123456789/30670
dc.description.abstractIn order to characterise the behaviour of Water Cherenkov Detectors (WCD) under a sudden increase of 1 GeV - 1 TeV background photons from a Gamma Ray Burst (GRB), simulations were conducted and compared to data acquired by the WCD of the Large Aperture GRB Observatory (LAGO). The LAGO operates arrays of WCD at high altitude to detect GRBs using the single particle technique. The LAGO sensitivity to GRBs is derived from the reported simulations of the gamma initiated particle showers in the atmosphere and the WCD response to secondaries.es_VE
dc.language.isoenes_VE
dc.publisherhttp://arxiv.org/es_VE
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleWater cherenkov detectors response to a Gamma Ray Burst in the large aperture GRB observatoryes_VE
dc.typeinfo:eu-repo/semantics/article
dc.description.colacion1-5es_VE
dc.description.emailjgonzale@ula.vees_VE
dc.description.emailnunez@ula.vees_VE
dc.publisher.paisPoloniaes_VE
dc.subject.keywordsGRBes_VE
dc.subject.keywordsWCDes_VE
dc.subject.keywordsLagoes_VE
dc.subject.tipoArtículoses_VE
dc.type.mediaTextoes_VE


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