@misc{10481/96991,
year = {2024},
month = {9},
url = {https://hdl.handle.net/10481/96991},
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.},
organization = {Czech Science Foundation (GAC˘R 24-12702S)},
organization = {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},
organization = {Shota Rustaveli National Science Foundation
of Georgia (SRNSFG, FR-22-13708), Georgia},
organization = {The General Secretariat
of Research and Innovation (GSRI), Greece},
organization = {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},
organization = {Italian Ministero dell’Università e della Ricerca
(MUR), Progetto CIR01 00021 (Avviso n. 2595 del 24 dicembre
2019)},
organization = {Ministry of Higher Education, Scientific Research and Innovation,
Morocco, and the Arab Fund for Economic and Social Development,
Kuwait},
organization = {Nederlandse organisatie voor Wetenschappelijk Onderzoek
(NWO), the Netherlands},
organization = {The National Science Centre, Poland
(2021/41/N/ST2/01177)},
organization = {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},
organization = {Ministry of Education, Research, Development and
Youth of the Slovak Republic},
organization = {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},
organization = {The European
Union’s Horizon 2020 Research and Innovation Programme (ChETECINFRA
- Project no. 101008324)},
publisher = {Springer Nature},
title = {Astronomy potential of KM3NeT/ARCA},
doi = {10.1140/epjc/s10052-024-13137-2},
author = {Aiello, S. and Anguita López, Mancia and Navas Concha, Sergio and Díaz García, Antonio Francisco and KM3NeT Collaboration},
}