Improving the muon track reconstruction of IceCube and IceCube-Gen2

8th Very Large Volume Neutrino Telescope Workshop, Dubna, Russia, 2 Oct 2018 - 4 Oct 2018; The European physical journal / Web of Conferences Web of Conferences : proceedings proceedings 207, 05002 - (2019). doi:10.1051/epjconf/201920705002 : IceCube is a cubic-kilometer Cherenkov telescope operatin...

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Main Authors: Bradascio, Federica, Glüsenkamp, Thorsten
Format: Text
Language:English
Published: Deutsches Elektronen-Synchrotron, DESY, Hamburg 2019
Subjects:
Online Access:https://dx.doi.org/10.3204/pubdb-2020-00372
http://bib-pubdb1.desy.de/record/434829
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author Bradascio, Federica
Glüsenkamp, Thorsten
author_facet Bradascio, Federica
Glüsenkamp, Thorsten
author_sort Bradascio, Federica
collection DataCite
description 8th Very Large Volume Neutrino Telescope Workshop, Dubna, Russia, 2 Oct 2018 - 4 Oct 2018; The European physical journal / Web of Conferences Web of Conferences : proceedings proceedings 207, 05002 - (2019). doi:10.1051/epjconf/201920705002 : IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. Its goal is to detect astrophysical neutrinos and identify their sources. High-energy muon neutrinos are identified through the secondary muons produced via charge current interactions with the ice. The present bestperforming directional reconstruction of the muon track is a maximum likelihood method which uses the arrival time distribution of Cherenkov photons registered by the experiment’s photomultipliers. Known systematic shortcomings of this method are to assume continuous energy loss along the muon track, and to neglect photomultiplier-related effects such as prepulses and afterpulses. This work discusses an improvement of about 20% to the muon angular resolution of IceCube and its planned extension, IceCube-Gen2. In the reconstruction scheme presented here, the expected arrival time distribution is now parametrized by a predetermined stochastic muon energy loss pattern. The inclusion of pre- and afterpulses modelling in the PDF has also been studied, but no noticeable improvement was found, in particular in comparison to the modification of the energy loss profile. : Published by EDP Sciences, Les Ulis
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op_doi https://doi.org/10.3204/pubdb-2020-00372
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spelling ftdatacite:10.3204/pubdb-2020-00372 2025-01-17T00:52:29+00:00 Improving the muon track reconstruction of IceCube and IceCube-Gen2 Bradascio, Federica Glüsenkamp, Thorsten 2019 https://dx.doi.org/10.3204/pubdb-2020-00372 http://bib-pubdb1.desy.de/record/434829 en eng Deutsches Elektronen-Synchrotron, DESY, Hamburg https://dx.doi.org/10.1051/epjconf/201920705002 530 muon tracks muon energy loss muon track data analysis muon secondary muon production charge current radiation Cherenkov IceCube angular resolution Cherenkov counter photomultiplier neutrino muon stochastic photon pole ice Text Journal article article-journal ScholarlyArticle 2019 ftdatacite https://doi.org/10.3204/pubdb-2020-00372 https://doi.org/10.1051/epjconf/201920705002 2021-11-05T12:55:41Z 8th Very Large Volume Neutrino Telescope Workshop, Dubna, Russia, 2 Oct 2018 - 4 Oct 2018; The European physical journal / Web of Conferences Web of Conferences : proceedings proceedings 207, 05002 - (2019). doi:10.1051/epjconf/201920705002 : IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. Its goal is to detect astrophysical neutrinos and identify their sources. High-energy muon neutrinos are identified through the secondary muons produced via charge current interactions with the ice. The present bestperforming directional reconstruction of the muon track is a maximum likelihood method which uses the arrival time distribution of Cherenkov photons registered by the experiment’s photomultipliers. Known systematic shortcomings of this method are to assume continuous energy loss along the muon track, and to neglect photomultiplier-related effects such as prepulses and afterpulses. This work discusses an improvement of about 20% to the muon angular resolution of IceCube and its planned extension, IceCube-Gen2. In the reconstruction scheme presented here, the expected arrival time distribution is now parametrized by a predetermined stochastic muon energy loss pattern. The inclusion of pre- and afterpulses modelling in the PDF has also been studied, but no noticeable improvement was found, in particular in comparison to the modification of the energy loss profile. : Published by EDP Sciences, Les Ulis Text South pole DataCite South Pole
spellingShingle 530
muon tracks
muon energy loss
muon track data analysis
muon secondary
muon production
charge current
radiation Cherenkov
IceCube
angular resolution
Cherenkov counter
photomultiplier
neutrino muon
stochastic
photon
pole
ice
Bradascio, Federica
Glüsenkamp, Thorsten
Improving the muon track reconstruction of IceCube and IceCube-Gen2
title Improving the muon track reconstruction of IceCube and IceCube-Gen2
title_full Improving the muon track reconstruction of IceCube and IceCube-Gen2
title_fullStr Improving the muon track reconstruction of IceCube and IceCube-Gen2
title_full_unstemmed Improving the muon track reconstruction of IceCube and IceCube-Gen2
title_short Improving the muon track reconstruction of IceCube and IceCube-Gen2
title_sort improving the muon track reconstruction of icecube and icecube-gen2
topic 530
muon tracks
muon energy loss
muon track data analysis
muon secondary
muon production
charge current
radiation Cherenkov
IceCube
angular resolution
Cherenkov counter
photomultiplier
neutrino muon
stochastic
photon
pole
ice
topic_facet 530
muon tracks
muon energy loss
muon track data analysis
muon secondary
muon production
charge current
radiation Cherenkov
IceCube
angular resolution
Cherenkov counter
photomultiplier
neutrino muon
stochastic
photon
pole
ice
url https://dx.doi.org/10.3204/pubdb-2020-00372
http://bib-pubdb1.desy.de/record/434829