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dc.contributor.authorAiello, S.
dc.contributor.authorAnguita López, Mancia 
dc.contributor.authorNavas Concha, Sergio 
dc.contributor.authorDíaz García, Antonio Francisco 
dc.contributor.authorKM3NeT Collaboration
dc.date.accessioned2024-11-18T09:36:34Z
dc.date.available2024-11-18T09:36:34Z
dc.date.issued2024-09-02
dc.identifier.citationAiello, S. & Anguita López, M. KM3NeT Collaboration. et. al. Eur. Phys. J. C (2024) 84:885. [https://doi.org/10.1140/epjc/s10052-024-13137-2]es_ES
dc.identifier.urihttps://hdl.handle.net/10481/96991
dc.description.abstractThe KM3NeT/ARCA neutrino detector is currently under construction at 3500 m depth offshore Capo Passero, Sicily, in the Mediterranean Sea. The main science objectives are the detection of high-energy cosmic neutrinos and the discovery of their sources. Simulations were conducted for the full KM3NeT/ARCA detector, instrumenting a volume of 1 km3, to estimate the sensitivity and discovery potential to point-like neutrino sources. This paper covers the reconstruction of track- and shower-like signatures, as well as the criteria employed for neutrino event selection. With an angular resolution below 0.1◦ for tracks and under 2◦ for showers, the sensitivity to point-like neutrino sources surpasses existing observed limits across the entire sky.es_ES
dc.description.sponsorshipCzech Science Foundation (GAC˘R 24-12702S)es_ES
dc.description.sponsorshipAgence Nationale de la Recherche (contract ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Européenne (FEDER fund and Marie Curie Program), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Îlede- France Region, Francees_ES
dc.description.sponsorshipShota Rustaveli National Science Foundation of Georgia (SRNSFG, FR-22-13708), Georgiaes_ES
dc.description.sponsorshipThe General Secretariat of Research and Innovation (GSRI), Greecees_ES
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN) and Ministero dell’Università e della Ricerca (MUR), through PRIN 2022 program (Grant PANTHEON 2022E2J4RK, Next Generation EU) and PON R&I program (Avviso n. 424 del 28 febbraio 2018, Progetto PACK-PIR01 00021), Italyes_ES
dc.description.sponsorshipItalian Ministero dell’Università e della Ricerca (MUR), Progetto CIR01 00021 (Avviso n. 2595 del 24 dicembre 2019)es_ES
dc.description.sponsorshipMinistry of Higher Education, Scientific Research and Innovation, Morocco, and the Arab Fund for Economic and Social Development, Kuwaites_ES
dc.description.sponsorshipNederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlandses_ES
dc.description.sponsorshipThe National Science Centre, Poland (2021/41/N/ST2/01177)es_ES
dc.description.sponsorshipThe grant “AstroCeNT: Particle Astrophysics Science and Technology Centre”, carried out within the International Research Agendas programme of the Foundation for Polish Science financed by the European Union under the European RegionalDevelopment Fund; National Authority for Scientific Research (ANCS), Romania; Slovak Research and Development Agency under Contract No. APVV-22-0413es_ES
dc.description.sponsorshipMinistry of Education, Research, Development and Youth of the Slovak Republices_ES
dc.description.sponsorshipMCIN for PID2021-124591NB-C41, -C42, -C43, funded by MCIN/AEI/10.13039/501100011033 and by “ERDFAway ofmaking Europe”, forASFAE/2022/014, ASFAE/2022 /023, with funding from the EU NextGenerationEU (PRTR-C17.I01), GeneralitatValenciana, and for CSIC-INFRA23013, GeneralitatValenciana for PROMETEO /2020/019, for Grant AST22_6.2 with funding from Consejería de Universidad, Investigación e Innovación and Gobierno de España and European Union - NextGenerationEU, for CIDEGENT/ 2018/034, /2019/043, /2020/049, /2021/23 and for GRISOLIAP/ 2021/192 and EU for MSC/101025085, Spaines_ES
dc.description.sponsorshipThe European Union’s Horizon 2020 Research and Innovation Programme (ChETECINFRA - Project no. 101008324)es_ES
dc.language.isoenges_ES
dc.publisherSpringer Naturees_ES
dc.rightsAtribución 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.titleAstronomy potential of KM3NeT/ARCAes_ES
dc.typejournal articlees_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/101008324es_ES
dc.rights.accessRightsopen accesses_ES
dc.identifier.doi10.1140/epjc/s10052-024-13137-2
dc.type.hasVersionVoRes_ES


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