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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Format: | Text |
Language: | English |
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Deutsches Elektronen-Synchrotron, DESY, Hamburg
2019
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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 |
format | Text |
genre | South pole |
genre_facet | South pole |
geographic | South Pole |
geographic_facet | South Pole |
id | ftdatacite:10.3204/pubdb-2020-00372 |
institution | Open Polar |
language | English |
op_collection_id | ftdatacite |
op_doi | https://doi.org/10.3204/pubdb-2020-00372 https://doi.org/10.1051/epjconf/201920705002 |
op_relation | https://dx.doi.org/10.1051/epjconf/201920705002 |
publishDate | 2019 |
publisher | Deutsches Elektronen-Synchrotron, DESY, Hamburg |
record_format | openpolar |
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 |