TY - JOUR
T1 - Energy-dependent expectations for the full KM3NeT/ARCA detector
T2 - International Cosmic Ray Conference
AU - Ibnsalih, W. I.
AU - Ambrosone, A.
AU - Marinelli, A.
AU - Miele, G.
AU - Migliozzi, P.
AU - Musone, M. R.
AU - KM3NeT collaboration,
AU - Filipović, M. D.
N1 - Conference code: 38th
PY - 2024/9/27
Y1 - 2024/9/27
N2 - The energy-dependent expectations for the full KM3NeT/ARCA detector, both for diffuse and point-like signals are presented. For the diffuse analysis, the 90% C.L. quasi-differential sensitivity for 10 years of the full detector operations is computed, and compared with the IceCube measured diffuse spectrum. The whole energy range observable by ARCA ∼ (1 TeV − 100 PeV) is taken into account, selecting upgoing track-like as well as all-sky cascade-like events. For the point-like analysis, the differential sensitivity for several declinations is computed, selecting upgoing tracks νμ and ν̄μ charge-current interactions. Some particular starburst galaxies (SBGs) are considered such as NGC 1068, the Small Magellanic Cloud (SMC) and Circinus Galaxy. The resulting sensitvities demonstrate the importance of KM3NeT/ARCA to link star-forming processes with high-energy neutrino production within a few years of operation.
AB - The energy-dependent expectations for the full KM3NeT/ARCA detector, both for diffuse and point-like signals are presented. For the diffuse analysis, the 90% C.L. quasi-differential sensitivity for 10 years of the full detector operations is computed, and compared with the IceCube measured diffuse spectrum. The whole energy range observable by ARCA ∼ (1 TeV − 100 PeV) is taken into account, selecting upgoing track-like as well as all-sky cascade-like events. For the point-like analysis, the differential sensitivity for several declinations is computed, selecting upgoing tracks νμ and ν̄μ charge-current interactions. Some particular starburst galaxies (SBGs) are considered such as NGC 1068, the Small Magellanic Cloud (SMC) and Circinus Galaxy. The resulting sensitvities demonstrate the importance of KM3NeT/ARCA to link star-forming processes with high-energy neutrino production within a few years of operation.
UR - http://www.scopus.com/inward/record.url?scp=85212305874&partnerID=8YFLogxK
U2 - 10.22323/1.444.1150
DO - 10.22323/1.444.1150
M3 - Article
AN - SCOPUS:85212305874
SN - 1824-8039
VL - 444
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 1150
Y2 - 26 July 2023 through 3 August 2023
ER -