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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.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.authorEngdegrd, O.
dc.contributor.authorEuler, S.
dc.contributor.authorEvenson, P.
dc.contributor.authorFadiran, O.
dc.contributor.authorFazely, A.
dc.contributor.authorFedynitch, 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.authorGunasingha, R.
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.date.accessioned2017-01-30T11:09:25Z
dc.date.available2017-01-30T11:09:25Z
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. The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector. Astroparticle Physics. 34 (1): pp. 48-58.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/8921
dc.identifier.doi10.1016/j.astropartphys.2010.05.001
dc.description.abstract

The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energy range 2-200 TeV. The result is compared to different atmospheric neutrino models and it is compatible with the atmospheric neutrinos from pion and kaon decays. No significant contribution from charm hadron decays or extraterrestrial neutrinos is detected. The capabilities to improve the measurement of the neutrino spectrum with the successor experiment IceCube are discussed.

dc.publisherElsevier
dc.titleThe energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector
dc.typeJournal Article
dcterms.source.volume34
dcterms.source.number1
dcterms.source.startPage48
dcterms.source.endPage58
dcterms.source.issn0927-6505
dcterms.source.titleAstroparticle Physics
curtin.departmentDepartment of Exploration Geophysics
curtin.accessStatusFulltext not available


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