Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory
The IceCube Neutrino Observatory at the South Pole is a multi-component detector capable of measuring the cosmic ray energy spectrum and composition from PeV to EeV, the energy region typically thought to cover the transition from galactic to extragalactic sources of cosmic rays. The IceTop array at...
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ftdatacite:10.48550/arxiv.1908.08139 2023-05-15T18:22:34+02:00 Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory Andeen, Karen Plum, Matthias 2019 https://dx.doi.org/10.48550/arxiv.1908.08139 https://arxiv.org/abs/1908.08139 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Article CreativeWork article Preprint 2019 ftdatacite https://doi.org/10.48550/arxiv.1908.08139 2022-03-10T16:27:27Z The IceCube Neutrino Observatory at the South Pole is a multi-component detector capable of measuring the cosmic ray energy spectrum and composition from PeV to EeV, the energy region typically thought to cover the transition from galactic to extragalactic sources of cosmic rays. The IceTop array at the surface is sensitive to the electromagnetic part of the air shower while the deep in-ice array detects the high-energy (TeV) muonic component of air showers. IceTop's reconstructed shower size parameter, S$_{125}$, is unfolded into a high statistics all-particle energy spectrum. Furthermore, for air showers that pass through both arrays, the in-ice reconstructed muon energy loss information is combined with S$_{125}$ in a machine learning algorithm to simultaneously extract both the all-particle energy spectrum and individual spectra for elemental groups. The all-particle spectra as well as spectra for individual elemental groups are presented. : Presented at the 36th International Cosmic Ray Conference (ICRC 2019). See arXiv:1907.11699 for all IceCube contributions Article in Journal/Newspaper South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
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High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Andeen, Karen Plum, Matthias Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory |
topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
description |
The IceCube Neutrino Observatory at the South Pole is a multi-component detector capable of measuring the cosmic ray energy spectrum and composition from PeV to EeV, the energy region typically thought to cover the transition from galactic to extragalactic sources of cosmic rays. The IceTop array at the surface is sensitive to the electromagnetic part of the air shower while the deep in-ice array detects the high-energy (TeV) muonic component of air showers. IceTop's reconstructed shower size parameter, S$_{125}$, is unfolded into a high statistics all-particle energy spectrum. Furthermore, for air showers that pass through both arrays, the in-ice reconstructed muon energy loss information is combined with S$_{125}$ in a machine learning algorithm to simultaneously extract both the all-particle energy spectrum and individual spectra for elemental groups. The all-particle spectra as well as spectra for individual elemental groups are presented. : Presented at the 36th International Cosmic Ray Conference (ICRC 2019). See arXiv:1907.11699 for all IceCube contributions |
format |
Article in Journal/Newspaper |
author |
Andeen, Karen Plum, Matthias |
author_facet |
Andeen, Karen Plum, Matthias |
author_sort |
Andeen, Karen |
title |
Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory |
title_short |
Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory |
title_full |
Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory |
title_fullStr |
Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory |
title_full_unstemmed |
Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory |
title_sort |
cosmic ray spectrum and composition from pev to eev from the icecube neutrino observatory |
publisher |
arXiv |
publishDate |
2019 |
url |
https://dx.doi.org/10.48550/arxiv.1908.08139 https://arxiv.org/abs/1908.08139 |
geographic |
South Pole |
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South Pole |
genre |
South pole |
genre_facet |
South pole |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1908.08139 |
_version_ |
1766201972350779392 |