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dc.contributor.authorAartsen, M.
dc.contributor.authorAbbasi, R.
dc.contributor.authorAbdou, Y.
dc.contributor.authorAckermann, M.
dc.contributor.authorAdams, J.
dc.contributor.authorAguilar, J.
dc.contributor.authorAhlers, M.
dc.contributor.authorAltmann, D.
dc.contributor.authorAuffenberg, J.
dc.contributor.authorBai, X.
dc.contributor.authorBaker, M.
dc.contributor.authorBarwick, S.
dc.contributor.authorBaum, V.
dc.contributor.authorBay, R.
dc.contributor.authorBeatty, J.
dc.contributor.authorBechet, S.
dc.contributor.authorBecker Tjus, J.
dc.contributor.authorBecker, K.
dc.contributor.authorBenabderrahmane, M.
dc.contributor.authorBenZvi, S.
dc.contributor.authorBerghaus, P.
dc.contributor.authorBerley, D.
dc.contributor.authorBernardini, E.
dc.contributor.authorBernhard, A.
dc.contributor.authorBertrand, D.
dc.contributor.authorBesson, D.
dc.contributor.authorBinder, G.
dc.contributor.authorBindig, D.
dc.contributor.authorBissok, M.
dc.contributor.authorBlaufuss, E.
dc.contributor.authorBlumenthal, J.
dc.contributor.authorBoersma, D.
dc.contributor.authorBohaichuk, S.
dc.contributor.authorBohm, C.
dc.contributor.authorBose, D.
dc.contributor.authorBöser, S.
dc.contributor.authorBotner, O.
dc.contributor.authorBrayeur, L.
dc.contributor.authorBretz, H.
dc.contributor.authorBrown, A.
dc.contributor.authorBruijn, R.
dc.contributor.authorBrunner, J.
dc.contributor.authorCarson, Michael
dc.contributor.authorCasey, J.
dc.contributor.authorCasier, M.
dc.contributor.authorChirkin, D.
dc.contributor.authorChristov, A.
dc.contributor.authorChristy, B.
dc.contributor.authorClark, K.
dc.contributor.authorClevermann, F.
dc.contributor.authorCoenders, S.
dc.contributor.authorCohen, S.
dc.contributor.authorCowen, D.
dc.contributor.authorCruz Silva, A.
dc.contributor.authorDanninger, M.
dc.contributor.authorDaughhetee, J.
dc.contributor.authorDavis, J.
dc.contributor.authorDay, M.
dc.contributor.authorDe Clercq, C.
dc.contributor.authorDe Ridder, S.
dc.contributor.authorDesiati, P.
dc.contributor.authorDe Vries, K.
dc.contributor.authorDe With, M.
dc.contributor.authorDeYoung, T.
dc.contributor.authorDíaz-Vélez, J.
dc.contributor.authorDunkman, M.
dc.contributor.authorEagan, R.
dc.contributor.authorEberhardt, B.
dc.contributor.authorEichmann, B.
dc.contributor.authorEisch, J.
dc.contributor.authorEllsworth, R.
dc.contributor.authorEuler, S.
dc.contributor.authorEvenson, P.
dc.contributor.authorFadiran, O.
dc.contributor.authorFazely, A.
dc.contributor.authorFedynitch, A.
dc.contributor.authorFeintzeig, J.
dc.contributor.authorFeusels, T.
dc.contributor.authorFilimonov, K.
dc.contributor.authorFinley, C.
dc.contributor.authorFischer-Wasels, T.
dc.contributor.authorFlis, S.
dc.contributor.authorFranckowiak, A.
dc.contributor.authorFrantzen, K.
dc.contributor.authorFuchs, T.
dc.contributor.authorGaisser, T.
dc.contributor.authorGallagher, J.
dc.contributor.authorGerhardt, L.
dc.contributor.authorGladstone, L.
dc.contributor.authorGlüsenkamp, T.
dc.contributor.authorGoldschmidt, A.
dc.contributor.authorGolup, G.
dc.contributor.authorGonzalez, J.
dc.contributor.authorGoodman, J.
dc.contributor.authorGóra, D.
dc.contributor.authorGrandmont, D.
dc.date.accessioned2017-01-30T12:49:05Z
dc.date.available2017-01-30T12:49:05Z
dc.date.created2016-01-18T20:00:43Z
dc.date.issued2013
dc.identifier.citationAartsen, M. and Abbasi, R. and Abdou, Y. and Ackermann, M. and Adams, J. and Aguilar, J. and Ahlers, M. et al. 2013. Evidence for high-energy extraterrestrial neutrinos at the icecube detector. Science. 342 (6161).
dc.identifier.urihttp://hdl.handle.net/20.500.11937/25557
dc.identifier.doi10.1126/science.1242856
dc.description.abstract

We report on results of an all-sky search for high-energy neutrino events interacting within the IceCube neutrino detector conducted between May 2010 and May 2012. The search follows up on the previous detection of two PeV neutrino events, with improved sensitivity and extended energy coverage down to about 30 TeV. Twenty-six additional events were observed, substantially more than expected from atmospheric backgrounds. Combined, both searches reject a purely atmospheric origin for the 28 events at the 4σ level. These 28 events, which include the highest energy neutrinos ever observed, have flavors, directions, and energies inconsistent with those expected from the atmospheric muon and neutrino backgrounds. These properties are, however, consistent with generic predictions for an additional component of extraterrestrial origin.

dc.titleEvidence for high-energy extraterrestrial neutrinos at the icecube detector
dc.typeJournal Article
dcterms.source.volume342
dcterms.source.number6161
dcterms.source.issn0036-8075
dcterms.source.titleScience
curtin.departmentDepartment of Exploration Geophysics
curtin.accessStatusFulltext not available


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