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dc.contributor.authorAlbert, A.
dc.contributor.authorAndré, M.
dc.contributor.authorAnghinolfi, M.
dc.contributor.authorAnton, G.
dc.contributor.authorArdid, M.
dc.contributor.authorAubert, J.
dc.contributor.authorAublin, J.
dc.contributor.authorAvgitas, T.
dc.contributor.authorBaret, B.
dc.contributor.authorBarrios-Martí, J.
dc.contributor.authorBasa, S.
dc.contributor.authorBelhorma, B.
dc.contributor.authorBertin, V.
dc.contributor.authorBiagi, S.
dc.contributor.authorBormuth, R.
dc.contributor.authorBoumaaza, J.
dc.contributor.authorBourret, S.
dc.contributor.authorBouwhuis, M.
dc.contributor.authorBrânzas, H.
dc.contributor.authorBruijn, R.
dc.contributor.authorBrunner, J.
dc.contributor.authorBusto, J.
dc.contributor.authorCapone, A.
dc.contributor.authorCaramete, L.
dc.contributor.authorCarr, J.
dc.contributor.authorCelli, S.
dc.contributor.authorChabab, M.
dc.contributor.authorEl Moursli, R.
dc.contributor.authorChiarusi, T.
dc.contributor.authorCircella, M.
dc.contributor.authorCoelho, J.
dc.contributor.authorColeiro, A.
dc.contributor.authorColomer, M.
dc.contributor.authorConiglione, R.
dc.contributor.authorCostantini, H.
dc.contributor.authorCoyle, P.
dc.contributor.authorCreusot, A.
dc.contributor.authorDíaz, A.
dc.contributor.authorDeschamps, A.
dc.contributor.authorDistefano, C.
dc.contributor.authorPalma, I.
dc.contributor.authorDomi, A.
dc.contributor.authorDonzaud, C.
dc.contributor.authorDornic, D.
dc.contributor.authorDrouhin, D.
dc.contributor.authorEberl, T.
dc.contributor.authorEl Bojaddaini, I.
dc.contributor.authorEl Khayati, N.
dc.contributor.authorElsässer, D.
dc.contributor.authorEnzenhöfer, A.
dc.contributor.authorEttahiri, A.
dc.contributor.authorFassi, F.
dc.contributor.authorFelis, I.
dc.contributor.authorFerrara, G.
dc.contributor.authorFusco, L.
dc.contributor.authorGay, P.
dc.contributor.authorGlotin, H.
dc.contributor.authorGrégoire, T.
dc.contributor.authorRuiz, R.
dc.contributor.authorGraf, K.
dc.contributor.authorHallmann, S.
dc.contributor.authorvan Haren, H.
dc.contributor.authorHeijboer, A.
dc.contributor.authorHello, Y.
dc.contributor.authorHernández-Rey, J.
dc.contributor.authorHößl, J.
dc.contributor.authorHofestädt, J.
dc.contributor.authorIlluminati, G.
dc.contributor.authorJames, Clancy
dc.contributor.authorde Jong, M.
dc.contributor.authorJongen, M.
dc.contributor.authorKadler, M.
dc.contributor.authorKalekin, O.
dc.contributor.authorKatz, U.
dc.contributor.authorKouchner, A.
dc.contributor.authorKreter, M.
dc.contributor.authorKreykenbohm, I.
dc.contributor.authorKulikovskiy, V.
dc.contributor.authorLachaud, C.
dc.contributor.authorLahmann, R.
dc.contributor.authorLefèvre, D.
dc.contributor.authorLeonora, E.
dc.contributor.authorLevi, G.
dc.date.accessioned2018-12-13T09:11:22Z
dc.date.available2018-12-13T09:11:22Z
dc.date.created2018-12-12T02:47:00Z
dc.date.issued2018
dc.identifier.citationAlbert, A. and Andr�, M. and Anghinolfi, M. and Anton, G. and Ardid, M. and Aubert, J. and Aublin, J. et al. 2018. Long-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration. European Physical Journal C. 78 (8).
dc.identifier.urihttp://hdl.handle.net/20.500.11937/71788
dc.identifier.doi10.1140/epjc/s10052-018-6132-2
dc.description.abstract

© 2018, The Author(s). Cherenkov light induced by radioactive decay products is one of the major sources of background light for deep-sea neutrino telescopes such as ANTARES. These decays are at the same time a powerful calibration source. Using data collected by the ANTARES neutrino telescope from mid 2008 to 2017, the time evolution of the photon detection efficiency of optical modules is studied. A modest loss of only 20% in 9 years is observed. The relative time calibration between adjacent modules is derived as well.

dc.titleLong-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration
dc.typeJournal Article
dcterms.source.volume78
dcterms.source.number8
dcterms.source.issn1434-6044
dcterms.source.titleEuropean Physical Journal C
curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusFulltext not available


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