Long-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration
© 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...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Journal Article |
| Published: |
2018
|
| Online Access: | http://hdl.handle.net/20.500.11937/71788 |
| _version_ | 1848762572488048640 |
|---|---|
| author | Albert, A. André, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. Aublin, J. Avgitas, T. Baret, B. Barrios-Martí, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Boumaaza, J. Bourret, S. Bouwhuis, M. Brânzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Chabab, M. El Moursli, R. Chiarusi, T. Circella, M. Coelho, J. Coleiro, A. Colomer, M. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Díaz, A. Deschamps, A. Distefano, C. Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsässer, D. Enzenhöfer, A. Ettahiri, A. Fassi, F. Felis, I. Ferrara, G. Fusco, L. Gay, P. Glotin, H. Grégoire, T. Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. Hello, Y. Hernández-Rey, J. Hößl, J. Hofestädt, J. Illuminati, G. James, Clancy de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefèvre, D. Leonora, E. Levi, G. |
| author_facet | Albert, A. André, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. Aublin, J. Avgitas, T. Baret, B. Barrios-Martí, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Boumaaza, J. Bourret, S. Bouwhuis, M. Brânzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Chabab, M. El Moursli, R. Chiarusi, T. Circella, M. Coelho, J. Coleiro, A. Colomer, M. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Díaz, A. Deschamps, A. Distefano, C. Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsässer, D. Enzenhöfer, A. Ettahiri, A. Fassi, F. Felis, I. Ferrara, G. Fusco, L. Gay, P. Glotin, H. Grégoire, T. Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. Hello, Y. Hernández-Rey, J. Hößl, J. Hofestädt, J. Illuminati, G. James, Clancy de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefèvre, D. Leonora, E. Levi, G. |
| author_sort | Albert, A. |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | © 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. |
| first_indexed | 2025-11-14T10:49:42Z |
| format | Journal Article |
| id | curtin-20.500.11937-71788 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T10:49:42Z |
| publishDate | 2018 |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-717882023-08-02T06:39:12Z Long-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration Albert, A. André, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. Aublin, J. Avgitas, T. Baret, B. Barrios-Martí, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Boumaaza, J. Bourret, S. Bouwhuis, M. Brânzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Chabab, M. El Moursli, R. Chiarusi, T. Circella, M. Coelho, J. Coleiro, A. Colomer, M. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Díaz, A. Deschamps, A. Distefano, C. Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsässer, D. Enzenhöfer, A. Ettahiri, A. Fassi, F. Felis, I. Ferrara, G. Fusco, L. Gay, P. Glotin, H. Grégoire, T. Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. Hello, Y. Hernández-Rey, J. Hößl, J. Hofestädt, J. Illuminati, G. James, Clancy de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefèvre, D. Leonora, E. Levi, G. © 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. 2018 Journal Article http://hdl.handle.net/20.500.11937/71788 10.1140/epjc/s10052-018-6132-2 restricted |
| spellingShingle | Albert, A. André, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J. Aublin, J. Avgitas, T. Baret, B. Barrios-Martí, J. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bormuth, R. Boumaaza, J. Bourret, S. Bouwhuis, M. Brânzas, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Celli, S. Chabab, M. El Moursli, R. Chiarusi, T. Circella, M. Coelho, J. Coleiro, A. Colomer, M. Coniglione, R. Costantini, H. Coyle, P. Creusot, A. Díaz, A. Deschamps, A. Distefano, C. Palma, I. Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. El Bojaddaini, I. El Khayati, N. Elsässer, D. Enzenhöfer, A. Ettahiri, A. Fassi, F. Felis, I. Ferrara, G. Fusco, L. Gay, P. Glotin, H. Grégoire, T. Ruiz, R. Graf, K. Hallmann, S. van Haren, H. Heijboer, A. Hello, Y. Hernández-Rey, J. Hößl, J. Hofestädt, J. Illuminati, G. James, Clancy de Jong, M. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Kouchner, A. Kreter, M. Kreykenbohm, I. Kulikovskiy, V. Lachaud, C. Lahmann, R. Lefèvre, D. Leonora, E. Levi, G. Long-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration |
| title | Long-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration |
| title_full | Long-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration |
| title_fullStr | Long-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration |
| title_full_unstemmed | Long-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration |
| title_short | Long-term monitoring of the ANTARES optical module efficiencies using 40K decays in sea water: The ANTARES Collaboration |
| title_sort | long-term monitoring of the antares optical module efficiencies using 40k decays in sea water: the antares collaboration |
| url | http://hdl.handle.net/20.500.11937/71788 |