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Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data
Journal article   Open access   Peer reviewed

Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data

Maryon Ahrens, Christian Bohm, Kunal Deoskar, Chad Finley, Klas Hultqvist, Erin O'Sullivan and Christian Walck
Astroparticle physics, v 116, p102392
2020
url
https://doi.org/10.1016/j.astropartphys.2019.102392View
Published, Version of Record (VoR)Open Access (License Unspecified) Open

Abstract

Fysik Naturvetenskap Neutrinos Point sources Veto techniques Natural Sciences Physical Sciences
Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos with a typical energy cutoff well below 100 TeV. For the IceCube Neutrino Observatory located at the South Pole, the southern sky, containing the inner part of the Galactic plane and the Galactic Center, is a particularly challenging region at these energies, because of the large background of atmospheric muons. In this paper, we present recent advancements in data selection strategies for track-like muon neutrino events with energies below 100 TeV from the southern sky. The strategies utilize the outer detector regions as veto and features of the signal pattern to reduce the background of atmospheric muons to a level which, for the first time, allows IceCube searching for point-like sources of neutrinos in the southern sky at energies between 100 GeV and several TeV in the muon neutrino charged current channel. No significant clustering of neutrinos above background expectation was observed in four years of data recorded with the completed IceCube detector. Upper limits on the neutrino flux for a number of spectral hypotheses are reported for a list of astrophysical objects in the southern hemisphere.

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Collaboration types
Domestic collaboration
International collaboration
Web of Science research areas
Astronomy & Astrophysics
Physics, Particles & Fields
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