Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory
The evaluation of mass composition of cosmic rays in the knee region ($\sim 3$ PeV) is critical to understanding the transition in the origin of cosmic rays from galactic to extragalactic sources. The IceCube Neutrino Observatory at the South Pole is a multi-component detector consisting of the surf...
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ftdatacite:10.48550/arxiv.1908.06433 2023-05-15T18:22:20+02:00 Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory Plum, Matthias 2019 https://dx.doi.org/10.48550/arxiv.1908.06433 https://arxiv.org/abs/1908.06433 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.1908.06433 2022-03-10T16:27:39Z The evaluation of mass composition of cosmic rays in the knee region ($\sim 3$ PeV) is critical to understanding the transition in the origin of cosmic rays from galactic to extragalactic sources. The IceCube Neutrino Observatory at the South Pole is a multi-component detector consisting of the surface IceTop array and the deep in-ice IceCube detector. By applying modern machine-learning techniques to cosmic-ray air showers reconstructed coincidentally in both detector components of IceCube observatory, the energy and the mass of primary cosmic rays in this transition region can be measured. In this contribution, we will discuss the reconstruction performance and composition sensitivity of IceCube observables presently under development. : 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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DataCite Metadata Store (German National Library of Science and Technology) |
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ftdatacite |
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unknown |
topic |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
spellingShingle |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Plum, Matthias Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory |
topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
description |
The evaluation of mass composition of cosmic rays in the knee region ($\sim 3$ PeV) is critical to understanding the transition in the origin of cosmic rays from galactic to extragalactic sources. The IceCube Neutrino Observatory at the South Pole is a multi-component detector consisting of the surface IceTop array and the deep in-ice IceCube detector. By applying modern machine-learning techniques to cosmic-ray air showers reconstructed coincidentally in both detector components of IceCube observatory, the energy and the mass of primary cosmic rays in this transition region can be measured. In this contribution, we will discuss the reconstruction performance and composition sensitivity of IceCube observables presently under development. : Presented at the 36th International Cosmic Ray Conference (ICRC 2019). See arXiv:1907.11699 for all IceCube contributions |
format |
Article in Journal/Newspaper |
author |
Plum, Matthias |
author_facet |
Plum, Matthias |
author_sort |
Plum, Matthias |
title |
Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory |
title_short |
Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory |
title_full |
Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory |
title_fullStr |
Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory |
title_full_unstemmed |
Cosmic ray composition study using machine learning at the IceCube Neutrino Observatory |
title_sort |
cosmic ray composition study using machine learning at the icecube neutrino observatory |
publisher |
arXiv |
publishDate |
2019 |
url |
https://dx.doi.org/10.48550/arxiv.1908.06433 https://arxiv.org/abs/1908.06433 |
geographic |
South Pole |
geographic_facet |
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.1908.06433 |
_version_ |
1766201737721413632 |