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First search for extremely high energy cosmogenic neutrinos with the IceCube neutrino observatory

dc.contributor.authorAbbasi, R.
dc.contributor.authorAbdou, Y.
dc.contributor.authorAbu-Zayyad, T.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J.
dc.contributor.authorAhlers, M.
dc.contributor.authorAndeen, K.
dc.contributor.authorAuffenberg, J.
dc.contributor.authorBai, X.
dc.contributor.authorBaker, M.
dc.contributor.authorBarwick, S.
dc.contributor.authorBay, R.
dc.contributor.authorBazo Alba, J.
dc.contributor.authorBeattie, K.
dc.contributor.authorBeatty, J.
dc.contributor.authorBechet, S.
dc.contributor.authorBecker, J.
dc.contributor.authorBecker, K.
dc.contributor.authorBenabderrahmane, M.
dc.contributor.authorBerdermann, J.
dc.contributor.authorBerghaus, P.
dc.contributor.authorBerley, D.
dc.contributor.authorBernardini, E.
dc.contributor.authorBertrand, D.
dc.contributor.authorBesson, D.
dc.contributor.authorBissok, M.
dc.contributor.authorBlaufuss, E.
dc.contributor.authorBoersma, D.
dc.contributor.authorBohm, C.
dc.contributor.authorBöser, S.
dc.contributor.authorBotner, O.
dc.contributor.authorBradley, L.
dc.contributor.authorBraun, J.
dc.contributor.authorBuitink, S.
dc.contributor.authorCarson, Michael
dc.contributor.authorChirkin, D.
dc.contributor.authorChristy, B.
dc.contributor.authorClem, J.
dc.contributor.authorClevermann, F.
dc.contributor.authorCohen, S.
dc.contributor.authorColnard, C.
dc.contributor.authorCowen, D.
dc.contributor.authorD'Agostino, M.
dc.contributor.authorDanninger, M.
dc.contributor.authorDavis, J.
dc.contributor.authorDe Clercq, C.
dc.contributor.authorDemirörs, L.
dc.contributor.authorDepaepe, O.
dc.contributor.authorDescamps, F.
dc.contributor.authorDesiati, P.
dc.contributor.authorDe Vries-Uiterweerd, G.
dc.contributor.authorDeyoung, T.
dc.contributor.authorDíaz-Vélez, J.
dc.contributor.authorDreyer, J.
dc.contributor.authorDumm, J.
dc.contributor.authorDuvoort, M.
dc.contributor.authorEhrlich, R.
dc.contributor.authorEisch, J.
dc.contributor.authorEllsworth, R.
dc.contributor.authorEngdegård, O.
dc.contributor.authorEuler, S.
dc.contributor.authorEvenson, P.
dc.contributor.authorFadiran, O.
dc.contributor.authorFazely, A.
dc.contributor.authorFeusels, T.
dc.contributor.authorFilimonov, K.
dc.contributor.authorFinley, C.
dc.contributor.authorFoerster, M.
dc.contributor.authorFox, B.
dc.contributor.authorFranckowiak, A.
dc.contributor.authorFranke, R.
dc.contributor.authorGaisser, T.
dc.contributor.authorGallagher, J.
dc.contributor.authorGanugapati, R.
dc.contributor.authorGeisler, M.
dc.contributor.authorGerhardt, L.
dc.contributor.authorGladstone, L.
dc.contributor.authorGlüsenkamp, T.
dc.contributor.authorGoldschmidt, A.
dc.contributor.authorGoodman, J.
dc.contributor.authorGrant, D.
dc.contributor.authorGriesel, T.
dc.contributor.authorGroß, A.
dc.contributor.authorGrullon, S.
dc.contributor.authorGurtner, M.
dc.contributor.authorHa, C.
dc.contributor.authorHallgren, A.
dc.contributor.authorHalzen, F.
dc.contributor.authorHan, K.
dc.contributor.authorHanson, K.
dc.contributor.authorHelbing, K.
dc.contributor.authorHerquet, P.
dc.contributor.authorHickford, S.
dc.contributor.authorHill, G.
dc.contributor.authorHoffman, K.
dc.contributor.authorHomeier, A.
dc.date.accessioned2017-01-30T13:25:18Z
dc.date.available2017-01-30T13:25:18Z
dc.date.created2016-09-12T08:37:03Z
dc.date.issued2010
dc.identifier.citationAbbasi, R. and Abdou, Y. and Abu-Zayyad, T. and Adams, J. and Aguilar, J. and Ahlers, M. and Andeen, K. et al. 2010. First search for extremely high energy cosmogenic neutrinos with the IceCube neutrino observatory. Physical Review D - Particles, Fields, Gravitation and Cosmology. 82 (7).
dc.identifier.urihttp://hdl.handle.net/20.500.11937/31433
dc.identifier.doi10.1103/PhysRevD.82.072003
dc.description.abstract

We report on the results of the search for extremely-high energy neutrinos with energies above 107GeV obtained with the partially (~30%) constructed IceCube in 2007. From the absence of signal events in the sample of 242.1 days of effective live time, we derive a 90% C.L. model independent differential upper limit based on the number of signal events per energy decade at E2?e+?µ+?t1. 4×10?-6GeVcm?-2?sec??-1sr?-1 for neutrinos in the energy range from 3×107 to 3×109GeV. © 2010 The American Physical Society.
dc.titleFirst search for extremely high energy cosmogenic neutrinos with the IceCube neutrino observatory
dc.typeJournal Article
dcterms.source.volume82
dcterms.source.number7
dcterms.source.issn1550-7998
dcterms.source.titlePhysical Review D - Particles, Fields, Gravitation and Cosmology
curtin.departmentDepartment of Exploration Geophysics
curtin.accessStatusFulltext not available


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