dc.contributor.author | Aiello, S. | |
dc.contributor.author | Anguita López, Mancia | |
dc.contributor.author | Navas Concha, Sergio | |
dc.contributor.author | Díaz García, Antonio Francisco | |
dc.contributor.author | KM3NeT Collaboration | |
dc.date.accessioned | 2024-11-18T09:36:34Z | |
dc.date.available | 2024-11-18T09:36:34Z | |
dc.date.issued | 2024-09-02 | |
dc.identifier.citation | Aiello, 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.uri | https://hdl.handle.net/10481/96991 | |
dc.description.abstract | The 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.sponsorship | Czech Science Foundation (GAC˘R 24-12702S) | es_ES |
dc.description.sponsorship | Agence 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, France | es_ES |
dc.description.sponsorship | Shota Rustaveli National Science Foundation
of Georgia (SRNSFG, FR-22-13708), Georgia | es_ES |
dc.description.sponsorship | The General Secretariat
of Research and Innovation (GSRI), Greece | es_ES |
dc.description.sponsorship | Istituto 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), Italy | es_ES |
dc.description.sponsorship | Italian Ministero dell’Università e della Ricerca
(MUR), Progetto CIR01 00021 (Avviso n. 2595 del 24 dicembre
2019) | es_ES |
dc.description.sponsorship | Ministry of Higher Education, Scientific Research and Innovation,
Morocco, and the Arab Fund for Economic and Social Development,
Kuwait | es_ES |
dc.description.sponsorship | Nederlandse organisatie voor Wetenschappelijk Onderzoek
(NWO), the Netherlands | es_ES |
dc.description.sponsorship | The National Science Centre, Poland
(2021/41/N/ST2/01177) | es_ES |
dc.description.sponsorship | The 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-22-0413 | es_ES |
dc.description.sponsorship | Ministry of Education, Research, Development and
Youth of the Slovak Republic | es_ES |
dc.description.sponsorship | MCIN 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, Spain | es_ES |
dc.description.sponsorship | The European
Union’s Horizon 2020 Research and Innovation Programme (ChETECINFRA
- Project no. 101008324) | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | Springer Nature | es_ES |
dc.rights | Atribución 4.0 Internacional | * |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | * |
dc.title | Astronomy potential of KM3NeT/ARCA | es_ES |
dc.type | journal article | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/EC/H2020/101008324 | es_ES |
dc.rights.accessRights | open access | es_ES |
dc.identifier.doi | 10.1140/epjc/s10052-024-13137-2 | |
dc.type.hasVersion | VoR | es_ES |