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dc.contributor.authorAlves Garre, Sergio
dc.contributor.authorAndré, Michel
dc.contributor.authorAnghinolfi, Marco
dc.contributor.authorAnton, Gisela
dc.contributor.authorArdid Ramírez, Miguel
dc.contributor.authorAublin, J.
dc.contributor.authorBelhorma, Bouchra
dc.contributor.authorBendahman, Meriem
dc.contributor.authorBertin, Vincent
dc.contributor.authorBissinger, Matthias
dc.contributor.authorBoumaaza, Jihad
dc.contributor.authorBruijn Berenguer, Frederic de
dc.contributor.otherCentre Tecnològic de Vilanova i la Geltrú
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament d'Enginyeria Química
dc.date.accessioned2023-03-21T18:54:24Z
dc.date.available2023-03-21T18:54:24Z
dc.date.issued2021
dc.identifier.citationAlves, S. [et al.]. Searches for point-like sources of cosmic neutrinos with 13 years of ANTARES data. A: International Cosmic Ray Conference. "37th International Cosmic Ray Conference: ICRC2021: 12-23 July 2021, Berlin, Germany-online". Ithaca, NY: arXiv, 2021, ISBN 18248039.
dc.identifier.isbn18248039
dc.identifier.urihttp://hdl.handle.net/2117/385268
dc.description.abstractThe main goal of the ANTARES neutrino telescope is the identification of neutrinos from astrophysical sources. Thanks to its location in the Northern hemisphere, ANTARES can rely on an advantageous view of the Southern Sky, in particular for neutrino energies below 100 TeV. This feature, combined with a very good angular resolution for high-quality selected events, makes the telescope an excellent tool to test for the presence of point-like sources, especially of Galactic origin. In ANTARES, track-like events are reconstructed with a median angular resolution of 0.4º while for shower-like events a median angular resolution of 3º is achieved. The ANTARES Collaboration published the result of the search for cosmic point-like neutrino sources using track-like and shower-like events collected during nine years of data taking [Phys. Rev. D 96 (2017) 082001]. In this contribution, the update to this analysis using a total of 13 years of data recorded between early 2007 and early 2020 (3845 days of livetime) is presented. Moreover, the results of the dedicated searches for neutrino candidates from the tidal disruption events AT2019dsg and AT2019fdr, recently indicated as the most likely counterparts of two high-energy IceCube neutrinos, IC191001A and IC200530A, are reported.
dc.language.isoeng
dc.publisherarXiv
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subjectÀrees temàtiques de la UPC::Física
dc.subject.lcshAstrophysics
dc.subject.lcshTelescopes
dc.subject.lcshNeutrinos
dc.subject.lcshNeutrino astrophysics
dc.titleSearches for point-like sources of cosmic neutrinos with 13 years of ANTARES data
dc.typeConference report
dc.subject.lemacNeutrins
dc.subject.lemacAstrofísica
dc.contributor.groupUniversitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
dc.relation.publisherversionhttps://pos.sissa.it/395/1161
dc.rights.accessOpen Access
local.identifier.drac35109049
dc.description.versionPostprint (published version)
local.citation.authorAlves, S.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aublin, J.; Belhorma, B.; Bendahman, M.; Bertin, V.; Bissinger, M.; Boumaaza, J.; De Bruijn, F.
local.citation.contributorInternational Cosmic Ray Conference
local.citation.pubplaceIthaca, NY
local.citation.publicationName37th International Cosmic Ray Conference: ICRC2021: 12-23 July 2021, Berlin, Germany-online
dc.description.authorshipArticle signat per 142 autors/es: A. Albert, S. Alves, M. André, M. Anghinolfi, G. Anton, M. Ardid, S. Ardid, J.-J. Aubert, J. Aublin, B. Baret, S. Basa,B. Belhorma, B. Belhorma, M. Bendahman, V. Bertin, S. Biagi, M. Bissinger, J. Boumaaza, M. Bouta, M.C. Bouwhuis, H. Brânzas, R. Bruijn, J. Brunner, J. Busto, B. Caiffi, A. Capone, L. Caramete, J. Carr, V. Carretero, S. Celli, M. Chabab,T. N. Chau, R. Cherkaoui El Moursli, T. Chiarusi, M. Circella, A. Coleiro, M. Colomer-Molla, R. Coniglione, P. Coyle, A. Creusot, A. F. Díaz, G. de Wasseige, A. Deschamps, C. Distefano, I. Di Palma, A. Domi, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, T. van Eeden, D. van Eijk, N. El Khayati, A. Enzenhöfer, P. Fermani, G. Ferrara, F. Filippini, L.A. Fusco, Y. Gatelet, P. Gay, H. Glotin, R. Gozzini, R. Gracia Ruiz, K. Graf, C. Guidi, S. Hallmann, H. van Haren, A.J. Heijboer, Y. Hello, J.J. Hernández-Rey, J. Hößl, J. Hofestädt, F. Huang, G. Illuminati, C.W James, B. Jisse-Jung, M. de Jong, P. de Jong, M. Kadler, O. Kalekin, U. Katz, N.R. Khan Chowdhury, A. Kouchner, I. Kreykenbohm, V. Kulikovskiy, R. Lahmann, R. Le Breton, D. Lefèvre, E. Leonora, G. Levi, M. Lincetto, D. Lopez-Coto, S. Loucatos, L. Maderer, J. Manczak, M. Marcelin, A. Margiotta, A. Marinelli, J.A. Martínez-Mora, K. Melis, P. Migliozzi, A. Moussa, R. Muller, L.Nauta, S.Navas, E.Nezri, B. O’Fearraigh, A. Paun, G.E. Pavalas, C. Pellegrino, M. Perrin-Terrin,V. Pestel, P. Piattelli, C. Pieterse, C. Poirè,V. Popa, T. Pradier,N. Randazzo, S.Reck, G. Riccobene, A. Romanov, A. Sánchez-Losa, F. Salesa Greus, D. F. E. Samtleben, M. Sanguineti, P. Sapienza, J. Schnabel, J. Schumann, F. Schüssler, M. Spurio, Th. Stolarczyk, M. Taiuti, Y. Tayalati, S.J. Tingay, B. Vallage, V. Van Elewyck, F. Versari, S. Viola, D. Vivolo, J. Wilms, S. Zavatarelli5, A. Zegarelli, J.D. Zornoza, and J. Zúñiga


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