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dc.contributor.authorDíaz García, Antonio Francisco 
dc.contributor.authorAlbert, A.
dc.contributor.authorNavas Concha, Sergio 
dc.contributor.authorAntares Collaboration
dc.date.accessioned2019-11-26T11:23:32Z
dc.date.available2019-11-26T11:23:32Z
dc.date.issued2018
dc.identifier.citationAlbert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J. J., ... & Basa, S. (2018). Long-term monitoring of the ANTARES optical module efficiencies using $$^{40}\mathrm {{K}} $$ decays in sea water. The European Physical Journal C, 78(8), 669.es_ES
dc.identifier.urihttp://hdl.handle.net/10481/58076
dc.description.abstractCherenkov 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.es_ES
dc.language.isoenges_ES
dc.publisherSpringer Naturees_ES
dc.rightsAtribución 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.titleLong-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea wateres_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.1140/epjc/s10052-018-6132-2


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