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Measurement of the atmospheric muon flux between 2.2 and 3.4 km depth undersea with KM3NeT

Authors: Samtleben, Dorothea; Melis, Karel; Kulikovskiy, Vladimir; Lincetto, Massimiliano; Hofestädt, Jannik; Biagi, Simone; Coniglione, Rosa;

Measurement of the atmospheric muon flux between 2.2 and 3.4 km depth undersea with KM3NeT

Abstract

The KM3NeT Collaboration is currently building the next-generation large volume Cherenkov neutrino observatories in the Mediterranean Sea. The KM3NeT/ARCA detector aims at studying TeV-PeV astrophysical neutrino sources. KM3NeT/ORCA will study atmospheric neutrino oscillations at few GeV energies to determine the neutrino mass ordering. The first KM3NeT detection units were deployed between 2015 and 2017. The measurement of the atmospheric muon flux at large depths in the Mediterranean Sea obtained using data collected with the first detection units of both KM3NeT/ARCA and ORCA is presented in this contribution.

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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