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Atmospheric neutrinos with the first detection units of KM3NeT/ARCA

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Nov 2021Embargo end date: 01 Jan 2021 Netherlands Publisher:IOP PublishingJournal:Journal of Instrumentation, volume 16, page C11015 (eissn: 1748-0221,

Authors: Sinopoulou, A.; Coniglione, R.; Muller, R.S.; Tzamariudaki, E.;

doi: 10.1088/1748-0221/16/11/c11015 , 10.48550/arxiv.2107.12721

arXiv: http://arxiv.org/abs/2107.12721

handle: 11245.1/4b3cec6f-a8ee-4960-90c7-8e60bb79cb8f

Atmospheric neutrinos with the first detection units of KM3NeT/ARCA

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Abstract

Abstract The KM3NeT collaboration is constructing two deep-sea Cherenkov detectors in the Mediterranean Sea. The ARCA detector aims at TeV-PeV neutrino astronomy, while the ORCA detector is optimised for atmospheric neutrino oscillation studies at energies of a few GeV. In this contribution, an analysis of the data collected with the first deployed detection units of the ARCA detector is presented. A high-purity sample of atmospheric neutrinos is selected demonstrating the capability of the ARCA detector.

Country

Netherlands

Related Organizations

University of Amsterdam
Netherlands
Italian National Institute of Nuclear Physics
Italy
National Institute for Nuclear Physics
Italy
Laboratori Nazionali del Sud
Italy
National Technical University of Athens
Greece

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Keywords

High Energy Astrophysical Phenomena (astro-ph.HE), High Energy Physics - Experiment (hep-ex), 500, FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena, 530, High Energy Physics - Experiment

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	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average