Monte Carlo simulations for the ANTARES underwater neutrino telescope
Monte Carlo simulations are a unique tool to check the response of a detector and to monitor its performance. For a deep-sea neutrino telescope, the variability of the environmental conditions that can affect the behaviour of the data acquisition system must be considered, in addition to a reliable...
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| Veröffentlicht in: | Journal of cosmology and astroparticle physics 2021-01, Vol.2021 (1), p.64-64 |
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| creator | Albert, A. André, M. Anghinolfi, M. Anton, G. Ardid, M. Aubert, J.-J. Aublin, J. Baret, B. Basa, S. Belhorma, B. Bertin, V. Biagi, S. Bissinger, M. Boumaaza, J. Bouta, M. Bouwhuis, M.C. Brânzaş, H. Bruijn, R. Brunner, J. Busto, J. Capone, A. Caramete, L. Carr, J. Cecchini, S. Celli, S. Chabab, M. Chau, T.N. Moursli, R. Cherkaoui El Chiarusi, T. Circella, M. Coleiro, A. Colomer-Molla, M. Coniglione, R. Coyle, P. Creusot, A. Díaz, A.F. de Wasseige, G. Deschamps, A. Distefano, C. Palma, I. Di Domi, A. Donzaud, C. Dornic, D. Drouhin, D. Eberl, T. Khayati, N. El Enzenhöfer, A. Ettahiri, A. Fermani, P. Ferrara, G. Filippini, F. Fusco, L. Gay, P. Glotin, H. Gozzini, R. Graf, K. Guidi, C. Hallmann, S. Haren, H. van Heijboer, A.J. Hello, Y. Hernández-Rey, J.J. Hößl, J. Hofestädt, J. Huang, F. Illuminati, G. James, C.W. de Jong, M. de Jong, P. Jongen, M. Kadler, M. Kalekin, O. Katz, U. Khan-Chowdhury, N.R. Kouchner, A. Kreykenbohm, I. Kulikovskiy, V. Lahmann, R. Breton, R. Le Lefèvre, D. Leonora, E. Levi, G. Lincetto, M. Lopez-Coto, D. Loucatos, S. Manczak, J. Marcelin, M. Margiotta, A. Marinelli, A. Martínez-Mora, J.A. Mazzou, S. Melis, K. Migliozzi, P. Moser, M. Moussa, A. Muller, R. Nauta, L. Navas, S. Nezri, E. Nuñez-Castiñeyra, A. |
| description | Monte Carlo simulations are a unique tool to check the response of a detector and to monitor its performance. For a deep-sea neutrino telescope, the variability of the environmental conditions that can affect the behaviour of the data acquisition system must be considered, in addition to a reliable description of the active parts of the detector and of the features of physics events, in order to produce a realistic set of simulated events. In this paper, the software tools used to produce neutrino and cosmic ray signatures in the telescope and the strategy developed to represent the time evolution of the natural environment and of the detector efficiency are described. |
| doi_str_mv | 10.1088/1475-7516/2021/01/064 |
| format | Article |
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Le ; Lefèvre, D. ; Leonora, E. ; Levi, G. ; Lincetto, M. ; Lopez-Coto, D. ; Loucatos, S. ; Manczak, J. ; Marcelin, M. ; Margiotta, A. ; Marinelli, A. ; Martínez-Mora, J.A. ; Mazzou, S. ; Melis, K. ; Migliozzi, P. ; Moser, M. ; Moussa, A. ; Muller, R. ; Nauta, L. ; Navas, S. ; Nezri, E. ; Nuñez-Castiñeyra, A.</creator><creatorcontrib>Albert, A. ; André, M. ; Anghinolfi, M. ; Anton, G. ; Ardid, M. ; Aubert, J.-J. ; Aublin, J. ; Baret, B. ; Basa, S. ; Belhorma, B. ; Bertin, V. ; Biagi, S. ; Bissinger, M. ; Boumaaza, J. ; Bouta, M. ; Bouwhuis, M.C. ; Brânzaş, H. ; Bruijn, R. ; Brunner, J. ; Busto, J. ; Capone, A. ; Caramete, L. ; Carr, J. ; Cecchini, S. ; Celli, S. ; Chabab, M. ; Chau, T.N. ; Moursli, R. Cherkaoui El ; Chiarusi, T. ; Circella, M. ; Coleiro, A. ; Colomer-Molla, M. ; Coniglione, R. ; Coyle, P. ; Creusot, A. ; Díaz, A.F. ; de Wasseige, G. ; Deschamps, A. ; Distefano, C. ; Palma, I. Di ; Domi, A. ; Donzaud, C. ; Dornic, D. ; Drouhin, D. ; Eberl, T. ; Khayati, N. El ; Enzenhöfer, A. ; Ettahiri, A. ; Fermani, P. ; Ferrara, G. ; Filippini, F. ; Fusco, L. ; Gay, P. ; Glotin, H. ; Gozzini, R. ; Graf, K. ; Guidi, C. ; Hallmann, S. ; Haren, H. van ; Heijboer, A.J. ; Hello, Y. ; Hernández-Rey, J.J. ; Hößl, J. ; Hofestädt, J. ; Huang, F. ; Illuminati, G. ; James, C.W. ; de Jong, M. ; de Jong, P. ; Jongen, M. ; Kadler, M. ; Kalekin, O. ; Katz, U. ; Khan-Chowdhury, N.R. ; Kouchner, A. ; Kreykenbohm, I. ; Kulikovskiy, V. ; Lahmann, R. ; Breton, R. Le ; Lefèvre, D. ; Leonora, E. ; Levi, G. ; Lincetto, M. ; Lopez-Coto, D. ; Loucatos, S. ; Manczak, J. ; Marcelin, M. ; Margiotta, A. ; Marinelli, A. ; Martínez-Mora, J.A. ; Mazzou, S. ; Melis, K. ; Migliozzi, P. ; Moser, M. ; Moussa, A. ; Muller, R. ; Nauta, L. ; Navas, S. ; Nezri, E. ; Nuñez-Castiñeyra, A.</creatorcontrib><description>Monte Carlo simulations are a unique tool to check the response of a detector and to monitor its performance. For a deep-sea neutrino telescope, the variability of the environmental conditions that can affect the behaviour of the data acquisition system must be considered, in addition to a reliable description of the active parts of the detector and of the features of physics events, in order to produce a realistic set of simulated events. In this paper, the software tools used to produce neutrino and cosmic ray signatures in the telescope and the strategy developed to represent the time evolution of the natural environment and of the detector efficiency are described.</description><identifier>ISSN: 1475-7516</identifier><identifier>ISSN: 1475-7508</identifier><identifier>EISSN: 1475-7516</identifier><identifier>DOI: 10.1088/1475-7516/2021/01/064</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Astrophysics ; Cosmic rays ; Data acquisition ; Deep sea ; Environmental conditions ; Instrumentation and Detectors ; Neutrinos ; Physics ; Sensors ; Simulation ; Software ; Software development tools ; Telescopes ; Underwater</subject><ispartof>Journal of cosmology and astroparticle physics, 2021-01, Vol.2021 (1), p.64-64</ispartof><rights>Copyright IOP Publishing Jan 2021</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c428t-bc097c1a87a9ca3525ccf3c0979caf1dd70a76ef98fc9f0d85d83be6d0d7243e3</citedby><orcidid>0000-0002-3556-1452 ; 0000-0003-3725-4920 ; 0000-0002-7063-4418 ; 0000-0001-7642-6225 ; 0000-0001-6064-3858 ; 0000-0001-5683-0570 ; 0000-0003-1694-3807 ; 0000-0002-9719-2277 ; 0000-0003-1500-6571 ; 0000-0001-5152-9631 ; 0000-0002-2131-7299</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27922,27923</link.rule.ids><backlink>$$Uhttps://hal.science/hal-03171382$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Albert, A.</creatorcontrib><creatorcontrib>André, M.</creatorcontrib><creatorcontrib>Anghinolfi, M.</creatorcontrib><creatorcontrib>Anton, G.</creatorcontrib><creatorcontrib>Ardid, M.</creatorcontrib><creatorcontrib>Aubert, J.-J.</creatorcontrib><creatorcontrib>Aublin, J.</creatorcontrib><creatorcontrib>Baret, B.</creatorcontrib><creatorcontrib>Basa, S.</creatorcontrib><creatorcontrib>Belhorma, B.</creatorcontrib><creatorcontrib>Bertin, V.</creatorcontrib><creatorcontrib>Biagi, S.</creatorcontrib><creatorcontrib>Bissinger, M.</creatorcontrib><creatorcontrib>Boumaaza, J.</creatorcontrib><creatorcontrib>Bouta, M.</creatorcontrib><creatorcontrib>Bouwhuis, M.C.</creatorcontrib><creatorcontrib>Brânzaş, H.</creatorcontrib><creatorcontrib>Bruijn, R.</creatorcontrib><creatorcontrib>Brunner, J.</creatorcontrib><creatorcontrib>Busto, J.</creatorcontrib><creatorcontrib>Capone, A.</creatorcontrib><creatorcontrib>Caramete, L.</creatorcontrib><creatorcontrib>Carr, J.</creatorcontrib><creatorcontrib>Cecchini, S.</creatorcontrib><creatorcontrib>Celli, S.</creatorcontrib><creatorcontrib>Chabab, M.</creatorcontrib><creatorcontrib>Chau, T.N.</creatorcontrib><creatorcontrib>Moursli, R. 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El</creatorcontrib><creatorcontrib>Enzenhöfer, A.</creatorcontrib><creatorcontrib>Ettahiri, A.</creatorcontrib><creatorcontrib>Fermani, P.</creatorcontrib><creatorcontrib>Ferrara, G.</creatorcontrib><creatorcontrib>Filippini, F.</creatorcontrib><creatorcontrib>Fusco, L.</creatorcontrib><creatorcontrib>Gay, P.</creatorcontrib><creatorcontrib>Glotin, H.</creatorcontrib><creatorcontrib>Gozzini, R.</creatorcontrib><creatorcontrib>Graf, K.</creatorcontrib><creatorcontrib>Guidi, C.</creatorcontrib><creatorcontrib>Hallmann, S.</creatorcontrib><creatorcontrib>Haren, H. van</creatorcontrib><creatorcontrib>Heijboer, A.J.</creatorcontrib><creatorcontrib>Hello, Y.</creatorcontrib><creatorcontrib>Hernández-Rey, J.J.</creatorcontrib><creatorcontrib>Hößl, J.</creatorcontrib><creatorcontrib>Hofestädt, J.</creatorcontrib><creatorcontrib>Huang, F.</creatorcontrib><creatorcontrib>Illuminati, G.</creatorcontrib><creatorcontrib>James, C.W.</creatorcontrib><creatorcontrib>de Jong, M.</creatorcontrib><creatorcontrib>de Jong, P.</creatorcontrib><creatorcontrib>Jongen, M.</creatorcontrib><creatorcontrib>Kadler, M.</creatorcontrib><creatorcontrib>Kalekin, O.</creatorcontrib><creatorcontrib>Katz, U.</creatorcontrib><creatorcontrib>Khan-Chowdhury, N.R.</creatorcontrib><creatorcontrib>Kouchner, A.</creatorcontrib><creatorcontrib>Kreykenbohm, I.</creatorcontrib><creatorcontrib>Kulikovskiy, V.</creatorcontrib><creatorcontrib>Lahmann, R.</creatorcontrib><creatorcontrib>Breton, R. Le</creatorcontrib><creatorcontrib>Lefèvre, D.</creatorcontrib><creatorcontrib>Leonora, E.</creatorcontrib><creatorcontrib>Levi, G.</creatorcontrib><creatorcontrib>Lincetto, M.</creatorcontrib><creatorcontrib>Lopez-Coto, D.</creatorcontrib><creatorcontrib>Loucatos, S.</creatorcontrib><creatorcontrib>Manczak, J.</creatorcontrib><creatorcontrib>Marcelin, M.</creatorcontrib><creatorcontrib>Margiotta, A.</creatorcontrib><creatorcontrib>Marinelli, A.</creatorcontrib><creatorcontrib>Martínez-Mora, J.A.</creatorcontrib><creatorcontrib>Mazzou, S.</creatorcontrib><creatorcontrib>Melis, K.</creatorcontrib><creatorcontrib>Migliozzi, P.</creatorcontrib><creatorcontrib>Moser, M.</creatorcontrib><creatorcontrib>Moussa, A.</creatorcontrib><creatorcontrib>Muller, R.</creatorcontrib><creatorcontrib>Nauta, L.</creatorcontrib><creatorcontrib>Navas, S.</creatorcontrib><creatorcontrib>Nezri, E.</creatorcontrib><creatorcontrib>Nuñez-Castiñeyra, A.</creatorcontrib><title>Monte Carlo simulations for the ANTARES underwater neutrino telescope</title><title>Journal of cosmology and astroparticle physics</title><description>Monte Carlo simulations are a unique tool to check the response of a detector and to monitor its performance. For a deep-sea neutrino telescope, the variability of the environmental conditions that can affect the behaviour of the data acquisition system must be considered, in addition to a reliable description of the active parts of the detector and of the features of physics events, in order to produce a realistic set of simulated events. In this paper, the software tools used to produce neutrino and cosmic ray signatures in the telescope and the strategy developed to represent the time evolution of the natural environment and of the detector efficiency are described.</description><subject>Astrophysics</subject><subject>Cosmic rays</subject><subject>Data acquisition</subject><subject>Deep sea</subject><subject>Environmental conditions</subject><subject>Instrumentation and Detectors</subject><subject>Neutrinos</subject><subject>Physics</subject><subject>Sensors</subject><subject>Simulation</subject><subject>Software</subject><subject>Software development tools</subject><subject>Telescopes</subject><subject>Underwater</subject><issn>1475-7516</issn><issn>1475-7508</issn><issn>1475-7516</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNpNkN1LwzAUxYMoqNM_QQj45ENdPpomfSxjOmEq6HwOWT5YR9fMJFX8702ZDOHAvffw43A5ANxgdI-REFNcclZwhqspQQRPUVZVnoCLo3_6bz8HlzFuESIVpeICzJ99nyycqdB5GNvd0KnU-j5C5wNMGwubl1XzNn-HQ29s-FbJBtjbIYW29zDZzkbt9_YKnDnVRXv9Nyfg42G-mi2K5evj06xZFrokIhVrjWqusRJc1VpRRpjWjo5mPh02hiPFK-tq4XTtkBHMCLq2lUGGk5JaOgF3h9yN6uQ-tDsVfqRXrVw0Szl6iGKOqSBfOLO3B3Yf_OdgY5JbP4Q-vydJKRjOKEWZYgdKBx9jsO4Yi5Ec25Vjc3JsTo7tSpRVlfQXkf5sRA</recordid><startdate>20210101</startdate><enddate>20210101</enddate><creator>Albert, A.</creator><creator>André, M.</creator><creator>Anghinolfi, M.</creator><creator>Anton, G.</creator><creator>Ardid, M.</creator><creator>Aubert, J.-J.</creator><creator>Aublin, J.</creator><creator>Baret, B.</creator><creator>Basa, S.</creator><creator>Belhorma, B.</creator><creator>Bertin, V.</creator><creator>Biagi, S.</creator><creator>Bissinger, M.</creator><creator>Boumaaza, J.</creator><creator>Bouta, M.</creator><creator>Bouwhuis, M.C.</creator><creator>Brânzaş, H.</creator><creator>Bruijn, R.</creator><creator>Brunner, J.</creator><creator>Busto, J.</creator><creator>Capone, A.</creator><creator>Caramete, L.</creator><creator>Carr, J.</creator><creator>Cecchini, S.</creator><creator>Celli, S.</creator><creator>Chabab, M.</creator><creator>Chau, T.N.</creator><creator>Moursli, R. 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Le</creator><creator>Lefèvre, D.</creator><creator>Leonora, E.</creator><creator>Levi, G.</creator><creator>Lincetto, M.</creator><creator>Lopez-Coto, D.</creator><creator>Loucatos, S.</creator><creator>Manczak, J.</creator><creator>Marcelin, M.</creator><creator>Margiotta, A.</creator><creator>Marinelli, A.</creator><creator>Martínez-Mora, J.A.</creator><creator>Mazzou, S.</creator><creator>Melis, K.</creator><creator>Migliozzi, P.</creator><creator>Moser, M.</creator><creator>Moussa, A.</creator><creator>Muller, R.</creator><creator>Nauta, L.</creator><creator>Navas, S.</creator><creator>Nezri, E.</creator><creator>Nuñez-Castiñeyra, A.</creator><general>IOP Publishing</general><general>Institute of Physics (IOP)</general><scope>AAYXX</scope><scope>CITATION</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-3556-1452</orcidid><orcidid>https://orcid.org/0000-0003-3725-4920</orcidid><orcidid>https://orcid.org/0000-0002-7063-4418</orcidid><orcidid>https://orcid.org/0000-0001-7642-6225</orcidid><orcidid>https://orcid.org/0000-0001-6064-3858</orcidid><orcidid>https://orcid.org/0000-0001-5683-0570</orcidid><orcidid>https://orcid.org/0000-0003-1694-3807</orcidid><orcidid>https://orcid.org/0000-0002-9719-2277</orcidid><orcidid>https://orcid.org/0000-0003-1500-6571</orcidid><orcidid>https://orcid.org/0000-0001-5152-9631</orcidid><orcidid>https://orcid.org/0000-0002-2131-7299</orcidid></search><sort><creationdate>20210101</creationdate><title>Monte Carlo simulations for the ANTARES underwater neutrino telescope</title><author>Albert, A. ; André, M. ; Anghinolfi, M. ; Anton, G. ; Ardid, M. ; Aubert, J.-J. ; Aublin, J. ; Baret, B. ; Basa, S. ; Belhorma, B. ; Bertin, V. ; Biagi, S. ; Bissinger, M. ; Boumaaza, J. ; Bouta, M. ; Bouwhuis, M.C. ; Brânzaş, H. ; Bruijn, R. ; Brunner, J. ; Busto, J. ; Capone, A. ; Caramete, L. ; Carr, J. ; Cecchini, S. ; Celli, S. ; Chabab, M. ; Chau, T.N. ; Moursli, R. Cherkaoui El ; Chiarusi, T. ; Circella, M. ; Coleiro, A. ; Colomer-Molla, M. ; Coniglione, R. ; Coyle, P. ; Creusot, A. ; Díaz, A.F. ; de Wasseige, G. ; Deschamps, A. ; Distefano, C. ; Palma, I. Di ; Domi, A. ; Donzaud, C. ; Dornic, D. ; Drouhin, D. ; Eberl, T. ; Khayati, N. El ; Enzenhöfer, A. ; Ettahiri, A. ; Fermani, P. ; Ferrara, G. ; Filippini, F. ; Fusco, L. ; Gay, P. ; Glotin, H. ; Gozzini, R. ; Graf, K. ; Guidi, C. ; Hallmann, S. ; Haren, H. van ; Heijboer, A.J. ; Hello, Y. ; Hernández-Rey, J.J. ; Hößl, J. ; Hofestädt, J. ; Huang, F. ; Illuminati, G. ; James, C.W. ; de Jong, M. ; de Jong, P. ; Jongen, M. ; Kadler, M. ; Kalekin, O. ; Katz, U. ; Khan-Chowdhury, N.R. ; Kouchner, A. ; Kreykenbohm, I. ; Kulikovskiy, V. ; Lahmann, R. ; Breton, R. Le ; Lefèvre, D. ; Leonora, E. ; Levi, G. ; Lincetto, M. ; Lopez-Coto, D. ; Loucatos, S. ; Manczak, J. ; Marcelin, M. ; Margiotta, A. ; Marinelli, A. ; Martínez-Mora, J.A. ; Mazzou, S. ; Melis, K. ; Migliozzi, P. ; Moser, M. ; Moussa, A. ; Muller, R. ; Nauta, L. ; Navas, S. ; Nezri, E. ; Nuñez-Castiñeyra, A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c428t-bc097c1a87a9ca3525ccf3c0979caf1dd70a76ef98fc9f0d85d83be6d0d7243e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Astrophysics</topic><topic>Cosmic rays</topic><topic>Data acquisition</topic><topic>Deep sea</topic><topic>Environmental conditions</topic><topic>Instrumentation and Detectors</topic><topic>Neutrinos</topic><topic>Physics</topic><topic>Sensors</topic><topic>Simulation</topic><topic>Software</topic><topic>Software development tools</topic><topic>Telescopes</topic><topic>Underwater</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Albert, A.</creatorcontrib><creatorcontrib>André, M.</creatorcontrib><creatorcontrib>Anghinolfi, M.</creatorcontrib><creatorcontrib>Anton, G.</creatorcontrib><creatorcontrib>Ardid, M.</creatorcontrib><creatorcontrib>Aubert, J.-J.</creatorcontrib><creatorcontrib>Aublin, J.</creatorcontrib><creatorcontrib>Baret, B.</creatorcontrib><creatorcontrib>Basa, S.</creatorcontrib><creatorcontrib>Belhorma, B.</creatorcontrib><creatorcontrib>Bertin, V.</creatorcontrib><creatorcontrib>Biagi, S.</creatorcontrib><creatorcontrib>Bissinger, M.</creatorcontrib><creatorcontrib>Boumaaza, J.</creatorcontrib><creatorcontrib>Bouta, M.</creatorcontrib><creatorcontrib>Bouwhuis, M.C.</creatorcontrib><creatorcontrib>Brânzaş, H.</creatorcontrib><creatorcontrib>Bruijn, R.</creatorcontrib><creatorcontrib>Brunner, J.</creatorcontrib><creatorcontrib>Busto, J.</creatorcontrib><creatorcontrib>Capone, A.</creatorcontrib><creatorcontrib>Caramete, L.</creatorcontrib><creatorcontrib>Carr, J.</creatorcontrib><creatorcontrib>Cecchini, S.</creatorcontrib><creatorcontrib>Celli, S.</creatorcontrib><creatorcontrib>Chabab, M.</creatorcontrib><creatorcontrib>Chau, T.N.</creatorcontrib><creatorcontrib>Moursli, R. Cherkaoui El</creatorcontrib><creatorcontrib>Chiarusi, T.</creatorcontrib><creatorcontrib>Circella, M.</creatorcontrib><creatorcontrib>Coleiro, A.</creatorcontrib><creatorcontrib>Colomer-Molla, M.</creatorcontrib><creatorcontrib>Coniglione, R.</creatorcontrib><creatorcontrib>Coyle, P.</creatorcontrib><creatorcontrib>Creusot, A.</creatorcontrib><creatorcontrib>Díaz, A.F.</creatorcontrib><creatorcontrib>de Wasseige, G.</creatorcontrib><creatorcontrib>Deschamps, A.</creatorcontrib><creatorcontrib>Distefano, C.</creatorcontrib><creatorcontrib>Palma, I. Di</creatorcontrib><creatorcontrib>Domi, A.</creatorcontrib><creatorcontrib>Donzaud, C.</creatorcontrib><creatorcontrib>Dornic, D.</creatorcontrib><creatorcontrib>Drouhin, D.</creatorcontrib><creatorcontrib>Eberl, T.</creatorcontrib><creatorcontrib>Khayati, N. El</creatorcontrib><creatorcontrib>Enzenhöfer, A.</creatorcontrib><creatorcontrib>Ettahiri, A.</creatorcontrib><creatorcontrib>Fermani, P.</creatorcontrib><creatorcontrib>Ferrara, G.</creatorcontrib><creatorcontrib>Filippini, F.</creatorcontrib><creatorcontrib>Fusco, L.</creatorcontrib><creatorcontrib>Gay, P.</creatorcontrib><creatorcontrib>Glotin, H.</creatorcontrib><creatorcontrib>Gozzini, R.</creatorcontrib><creatorcontrib>Graf, K.</creatorcontrib><creatorcontrib>Guidi, C.</creatorcontrib><creatorcontrib>Hallmann, S.</creatorcontrib><creatorcontrib>Haren, H. van</creatorcontrib><creatorcontrib>Heijboer, A.J.</creatorcontrib><creatorcontrib>Hello, Y.</creatorcontrib><creatorcontrib>Hernández-Rey, J.J.</creatorcontrib><creatorcontrib>Hößl, J.</creatorcontrib><creatorcontrib>Hofestädt, J.</creatorcontrib><creatorcontrib>Huang, F.</creatorcontrib><creatorcontrib>Illuminati, G.</creatorcontrib><creatorcontrib>James, C.W.</creatorcontrib><creatorcontrib>de Jong, M.</creatorcontrib><creatorcontrib>de Jong, P.</creatorcontrib><creatorcontrib>Jongen, M.</creatorcontrib><creatorcontrib>Kadler, M.</creatorcontrib><creatorcontrib>Kalekin, O.</creatorcontrib><creatorcontrib>Katz, U.</creatorcontrib><creatorcontrib>Khan-Chowdhury, N.R.</creatorcontrib><creatorcontrib>Kouchner, A.</creatorcontrib><creatorcontrib>Kreykenbohm, I.</creatorcontrib><creatorcontrib>Kulikovskiy, V.</creatorcontrib><creatorcontrib>Lahmann, R.</creatorcontrib><creatorcontrib>Breton, R. Le</creatorcontrib><creatorcontrib>Lefèvre, D.</creatorcontrib><creatorcontrib>Leonora, E.</creatorcontrib><creatorcontrib>Levi, G.</creatorcontrib><creatorcontrib>Lincetto, M.</creatorcontrib><creatorcontrib>Lopez-Coto, D.</creatorcontrib><creatorcontrib>Loucatos, S.</creatorcontrib><creatorcontrib>Manczak, J.</creatorcontrib><creatorcontrib>Marcelin, M.</creatorcontrib><creatorcontrib>Margiotta, A.</creatorcontrib><creatorcontrib>Marinelli, A.</creatorcontrib><creatorcontrib>Martínez-Mora, J.A.</creatorcontrib><creatorcontrib>Mazzou, S.</creatorcontrib><creatorcontrib>Melis, K.</creatorcontrib><creatorcontrib>Migliozzi, P.</creatorcontrib><creatorcontrib>Moser, M.</creatorcontrib><creatorcontrib>Moussa, A.</creatorcontrib><creatorcontrib>Muller, R.</creatorcontrib><creatorcontrib>Nauta, L.</creatorcontrib><creatorcontrib>Navas, S.</creatorcontrib><creatorcontrib>Nezri, E.</creatorcontrib><creatorcontrib>Nuñez-Castiñeyra, A.</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Journal of cosmology and astroparticle physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Albert, A.</au><au>André, M.</au><au>Anghinolfi, M.</au><au>Anton, G.</au><au>Ardid, M.</au><au>Aubert, J.-J.</au><au>Aublin, J.</au><au>Baret, B.</au><au>Basa, S.</au><au>Belhorma, B.</au><au>Bertin, V.</au><au>Biagi, S.</au><au>Bissinger, M.</au><au>Boumaaza, J.</au><au>Bouta, M.</au><au>Bouwhuis, M.C.</au><au>Brânzaş, H.</au><au>Bruijn, R.</au><au>Brunner, J.</au><au>Busto, J.</au><au>Capone, A.</au><au>Caramete, L.</au><au>Carr, J.</au><au>Cecchini, S.</au><au>Celli, S.</au><au>Chabab, M.</au><au>Chau, T.N.</au><au>Moursli, R. Cherkaoui El</au><au>Chiarusi, T.</au><au>Circella, M.</au><au>Coleiro, A.</au><au>Colomer-Molla, M.</au><au>Coniglione, R.</au><au>Coyle, P.</au><au>Creusot, A.</au><au>Díaz, A.F.</au><au>de Wasseige, G.</au><au>Deschamps, A.</au><au>Distefano, C.</au><au>Palma, I. Di</au><au>Domi, A.</au><au>Donzaud, C.</au><au>Dornic, D.</au><au>Drouhin, D.</au><au>Eberl, T.</au><au>Khayati, N. El</au><au>Enzenhöfer, A.</au><au>Ettahiri, A.</au><au>Fermani, P.</au><au>Ferrara, G.</au><au>Filippini, F.</au><au>Fusco, L.</au><au>Gay, P.</au><au>Glotin, H.</au><au>Gozzini, R.</au><au>Graf, K.</au><au>Guidi, C.</au><au>Hallmann, S.</au><au>Haren, H. van</au><au>Heijboer, A.J.</au><au>Hello, Y.</au><au>Hernández-Rey, J.J.</au><au>Hößl, J.</au><au>Hofestädt, J.</au><au>Huang, F.</au><au>Illuminati, G.</au><au>James, C.W.</au><au>de Jong, M.</au><au>de Jong, P.</au><au>Jongen, M.</au><au>Kadler, M.</au><au>Kalekin, O.</au><au>Katz, U.</au><au>Khan-Chowdhury, N.R.</au><au>Kouchner, A.</au><au>Kreykenbohm, I.</au><au>Kulikovskiy, V.</au><au>Lahmann, R.</au><au>Breton, R. Le</au><au>Lefèvre, D.</au><au>Leonora, E.</au><au>Levi, G.</au><au>Lincetto, M.</au><au>Lopez-Coto, D.</au><au>Loucatos, S.</au><au>Manczak, J.</au><au>Marcelin, M.</au><au>Margiotta, A.</au><au>Marinelli, A.</au><au>Martínez-Mora, J.A.</au><au>Mazzou, S.</au><au>Melis, K.</au><au>Migliozzi, P.</au><au>Moser, M.</au><au>Moussa, A.</au><au>Muller, R.</au><au>Nauta, L.</au><au>Navas, S.</au><au>Nezri, E.</au><au>Nuñez-Castiñeyra, A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Monte Carlo simulations for the ANTARES underwater neutrino telescope</atitle><jtitle>Journal of cosmology and astroparticle physics</jtitle><date>2021-01-01</date><risdate>2021</risdate><volume>2021</volume><issue>1</issue><spage>64</spage><epage>64</epage><pages>64-64</pages><issn>1475-7516</issn><issn>1475-7508</issn><eissn>1475-7516</eissn><abstract>Monte Carlo simulations are a unique tool to check the response of a detector and to monitor its performance. For a deep-sea neutrino telescope, the variability of the environmental conditions that can affect the behaviour of the data acquisition system must be considered, in addition to a reliable description of the active parts of the detector and of the features of physics events, in order to produce a realistic set of simulated events. In this paper, the software tools used to produce neutrino and cosmic ray signatures in the telescope and the strategy developed to represent the time evolution of the natural environment and of the detector efficiency are described.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1475-7516/2021/01/064</doi><tpages>1</tpages><orcidid>https://orcid.org/0000-0002-3556-1452</orcidid><orcidid>https://orcid.org/0000-0003-3725-4920</orcidid><orcidid>https://orcid.org/0000-0002-7063-4418</orcidid><orcidid>https://orcid.org/0000-0001-7642-6225</orcidid><orcidid>https://orcid.org/0000-0001-6064-3858</orcidid><orcidid>https://orcid.org/0000-0001-5683-0570</orcidid><orcidid>https://orcid.org/0000-0003-1694-3807</orcidid><orcidid>https://orcid.org/0000-0002-9719-2277</orcidid><orcidid>https://orcid.org/0000-0003-1500-6571</orcidid><orcidid>https://orcid.org/0000-0001-5152-9631</orcidid><orcidid>https://orcid.org/0000-0002-2131-7299</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1475-7516 |
| ispartof | Journal of cosmology and astroparticle physics, 2021-01, Vol.2021 (1), p.64-64 |
| issn | 1475-7516 1475-7508 1475-7516 |
| language | eng |
| recordid | cdi_hal_primary_oai_HAL_hal_03171382v1 |
| source | IOP Publishing Journals; Institute of Physics (IOP) Journals - HEAL-Link |
| subjects | Astrophysics Cosmic rays Data acquisition Deep sea Environmental conditions Instrumentation and Detectors Neutrinos Physics Sensors Simulation Software Software development tools Telescopes Underwater |
| title | Monte Carlo simulations for the ANTARES underwater neutrino telescope |
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