{"paper":{"title":"Search for relativistic magnetic monopoles with five years of the ANTARES detector data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Capone, A. Coleiro, A. Creusot, A. Deschamps, A. Domi, A. Enzenh\\\"ofer, A.J. Heijboer, A. Kouchner, A. Margiotta, A. Marinelli, A. Moussa, A. S\\'anchez-Losa, A. Trovato, A. Vizzoca, B. Baret, B. Vallage, C. Distefano, C. Donzaud, C. Hugon, C. Lachaud, C. Pellegrino, C. Perrina, C. Racca, C. Sieger, C. T\\\"onnis, C.W James, D. Dornic, D. Drouhin, D. Els\\\"asser, D. F. E. Samtleben, D. Kie{\\ss}ling, D. Lef\\`evre, D. Turpin, D. Vivolo, E. Leonora, E. Nezri, F. Sch\\\"ussler, F. Versari, G. Anton, G. De Bonis, G. E. P\\u{a}v\\u{a}la\\c{s}, G. Illuminati, G. Riccobene, H. Costantini, H. Glotin, H. van Haren, I. Di Palma, I. El Bojaddaini, I. Felis, I. Kreykenbohm, I. Salvadori, J.A.B. Coelho, J.A. Mart\\'inez-Mora, J. Barrios-Mart\\'i, J. Brunner, J. Busto, J. Carr, J.D. Zornoza, J. Hofest\\\"adt, J. H\\\"o{\\ss}l, J.-J. Aubert, J.J. Hern\\'andez-Rey, J. Wilms, J. Z\\'u\\~niga, K. Graf, K. Melis, L.A. Fusco, L. Caramete, L. Quinn, M. Andr\\'e, M. Anghinolfi, M. Ardid, M.C. Bouwhuis, M. Circella, M. de Jong, M. Jongen, M. Kadler, M. Kreter, M. Lotze, M. Marcelin, M. Organokov, M. Salda\\~na, M. Sanguineti, M. Spurio, M. Taiuti, O. Kalekin, P. Coyle, P. Gay, P. Migliozzi, P. Piattelli, P. Sapienza, R. Bormuth, R. Bruijn, R. Coniglione, R. Gracia Ruiz, R. Lahmann, R. Mele, S. Basa, S. Biagi, S. Bourret, S. Celli, S. Galat\\`a, S. Hallmann, S. Loucatos, S. Navas, T. Avgitas, T. Chiarusi, T. Eberl, T. Gr\\'egoire, Th. Stolarczyk, T. Michael, T. Pradier, U. Katz, V. Bertin, V. Giordano, V. Kulikovskiy, V. Popa, V. Van Elewyck, Y. Hello, Y. Tayalati","submitted_at":"2017-03-01T18:15:02Z","abstract_excerpt":"A search for magnetic monopoles using five years of data recorded with the ANTARES neutrino telescope from January 2008 to December 2012 with a total live time of 1121 days is presented. The analysis is carried out in the range $\\beta$ $>$ $0.6$ of magnetic monopole velocities using a strategy based on run-by-run Monte Carlo simulations. No signal above the background expectation from atmospheric muons and atmospheric neutrinos is observed, and upper limits are set on the magnetic monopole flux ranging from $5.7 \\times 10^{-16}$ to $1.5 \\times 10^{-18}$ cm$^{-2} \\cdot $ s$^{-1} \\cdot $ sr$^{-1"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.00424","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}