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.

Long-term monitoring of the ANTARES optical module efficiencies using K-40 decays in sea water / Albert, A., Andre, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J.j., Aublin, J., Avgitas, T., Baret, B., Barrios-Marti, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Boumaaza, J., Bourret, S., Bouwhuis, M.c., Branzas, H., Bruijn, R., et al.. - In: THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS. - ISSN 1434-6044. - 78:8(2018), pp. 669.--669.-. [10.1140/epjc/s10052-018-6132-2]

Long-term monitoring of the ANTARES optical module efficiencies using K-40 decays in sea water

Trovato A;
2018-01-01

Abstract

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.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11368/3002963
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