{"paper":{"title":"An algorithm for the reconstruction of neutrino-induced showers in the ANTARES neutrino telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"A. Albert, A. Capone, A. Coleiro, A. Creusot, A. Deschamps, A. Domi, A. Enzenh\\\"ofer, A. Ettahiri, A. F. D\\'iaz, A.J. Heijboer, A. Kouchner, A. Margiotta, A. Marinelli, A. Moussa, A. S\\'anchez-Losa, A. Trovato, A. Vizzoca, B. Baret, B. Belhorma, 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. Fassi, 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. Br\\^anza\\c{s}, 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, N. El Khayati, O. Kalekin, P. Coyle, P. Gay, P. Migliozzi, P. Piattelli, P. Sapienza, R. Bormuth, R. Bruijn, R. Cherkaoui El Moursli, R. Coniglione, R. Gracia Ruiz, R. Lahmann, R. Mele, S. Basa, S. Biagi, S. Bourret, S. Celli, 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":"2017-08-11T18:12:54Z","abstract_excerpt":"Muons created by $\\nu_\\mu$ charged current (CC) interactions in the water surrounding the ANTARES neutrino telescope have been almost exclusively used so far in searches for cosmic neutrino sources. Due to their long range, highly energetic muons inducing Cherenkov radiation in the water are reconstructed with dedicated algorithms that allow the determination of the parent neutrino direction with a median angular resolution of about \\unit{0.4}{\\degree} for an $E^{-2}$ neutrino spectrum. In this paper, an algorithm optimised for accurate reconstruction of energy and direction of shower events i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.03649","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"}