KM3NeT is a network of submarine Cherenkov neutrino telescopes under construction in two different sites in the Mediterranean Sea [1]. The detector at the Italian site, close to the Sicilian coast and named ARCA, will be devoted to the detection of high-energy astrophysical neutrinos coming from sources in the Universe, while the detector at the French site, in the Toulon bay and named ORCA, will exploit atmospheric neutrinos to determine the neutrino mass hierarchy. The telescopes are an array of flexible strings anchored to the sea floor and held close to vertical by submerged buoys. The strings are instrumented with digital optical modules hosted within pressure-resistant glass spheres, each housing 31 3” photomultipliers tubes and the readout electronics. The geometry of the detectors has been adapted to their physics goals. The first calibrations and results of ARCA and ORCA are presented.

Status and first results from the ARCA and ORCA lines of the KM3NeT experiment / Fermani, Paolo; DI PALMA, Irene. - 209:(2019). (Intervento presentato al convegno RICAP18, 7th Roma International Conference on Astroparticle Physics tenutosi a Roma; Italy) [10.1051/epjconf/201920901006].

Status and first results from the ARCA and ORCA lines of the KM3NeT experiment

PAOLO FERMANI
Primo
;
IRENE DI PALMA
2019

Abstract

KM3NeT is a network of submarine Cherenkov neutrino telescopes under construction in two different sites in the Mediterranean Sea [1]. The detector at the Italian site, close to the Sicilian coast and named ARCA, will be devoted to the detection of high-energy astrophysical neutrinos coming from sources in the Universe, while the detector at the French site, in the Toulon bay and named ORCA, will exploit atmospheric neutrinos to determine the neutrino mass hierarchy. The telescopes are an array of flexible strings anchored to the sea floor and held close to vertical by submerged buoys. The strings are instrumented with digital optical modules hosted within pressure-resistant glass spheres, each housing 31 3” photomultipliers tubes and the readout electronics. The geometry of the detectors has been adapted to their physics goals. The first calibrations and results of ARCA and ORCA are presented.
2019
RICAP18, 7th Roma International Conference on Astroparticle Physics
neutrino telescopes; astroparticle physics; calibration
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
Status and first results from the ARCA and ORCA lines of the KM3NeT experiment / Fermani, Paolo; DI PALMA, Irene. - 209:(2019). (Intervento presentato al convegno RICAP18, 7th Roma International Conference on Astroparticle Physics tenutosi a Roma; Italy) [10.1051/epjconf/201920901006].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1355230
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