Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021) 2021
DOI: 10.22323/1.395.1162
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KM3NeT/ARCA sensitivity to transient neutrino sources

Abstract: The KM3NeT Collaboration is constructing a km 3 -volume neutrino telescope in the Mediterranean sea, called ARCA (Astroparticle Research with Cosmics in the Abyss), that will achieve an unprecedented sensitivity to high-energy cosmic neutrinos. This telescope will be able to reconstruct the arrival direction of the neutrinos with a precision of 0.1 • . The configuration of ARCA makes it sensitive to neutrinos in a wide energy range, from sub-TeV up to tens of PeV. Moreover, this detector has a large field of v… Show more

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“…These contributions include, among others: the characterization of PMTs [10]; the design and construction of time and positioning calibration devices [11][12][13][14][15][16][17], acoustic instruments for R&D studies [18][19][20] and several contributions to electronics (the design and construction of electronic boards [21][22][23][24][25], the development of software and firmware and studies of electronics reliability [26,27]). On the physics side, the teams have participated in searches for neutrino point sources [28][29][30][31][32][33][34][35][36], diffuse fluxes [37,38], transient sources [39][40][41], multi-messenger astronomy [42][43][44][45], search for dark matter in the Sun [46][47][48][49] and in the Galactic Centre [50][51][52][53][54][55]<...>…”
Section: Introductionmentioning
confidence: 99%
“…These contributions include, among others: the characterization of PMTs [10]; the design and construction of time and positioning calibration devices [11][12][13][14][15][16][17], acoustic instruments for R&D studies [18][19][20] and several contributions to electronics (the design and construction of electronic boards [21][22][23][24][25], the development of software and firmware and studies of electronics reliability [26,27]). On the physics side, the teams have participated in searches for neutrino point sources [28][29][30][31][32][33][34][35][36], diffuse fluxes [37,38], transient sources [39][40][41], multi-messenger astronomy [42][43][44][45], search for dark matter in the Sun [46][47][48][49] and in the Galactic Centre [50][51][52][53][54][55]<...>…”
Section: Introductionmentioning
confidence: 99%