Cosmic rays primary energy estimation using Machine Learning and combined reconstruction
The IceCube Neutrino Observatory at the South Pole is capable of measuring two components of the cosmic rays air shower. The electromagnetic component using a km2 surface array IceTop, and the high-energy muonic component using km3 in-ice array IceCube between 1.5 and 2.5 km below the surface. The c...
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ftzenodo:oai:zenodo.org:6525169 2024-09-15T18:36:41+00:00 Cosmic rays primary energy estimation using Machine Learning and combined reconstruction Silverio, Diana Leon Bai, Xinhua Plum, Matthias for the IceCube Collaboration 2022-02-01 https://doi.org/10.5281/zenodo.6525169 eng eng Zenodo https://zenodo.org/communities/ml-airshowers-bartol2022 https://doi.org/10.5281/zenodo.6525168 https://doi.org/10.5281/zenodo.6525169 oai:zenodo.org:6525169 info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode Workshop on Machine learning for Cosmic-Ray Air Showers, Newark, Delaware, USA + Zoom (hybrid workshop), 31 Jan - 03 Feb 2022 info:eu-repo/semantics/lecture 2022 ftzenodo https://doi.org/10.5281/zenodo.652516910.5281/zenodo.6525168 2024-07-26T13:16:10Z The IceCube Neutrino Observatory at the South Pole is capable of measuring two components of the cosmic rays air shower. The electromagnetic component using a km2 surface array IceTop, and the high-energy muonic component using km3 in-ice array IceCube between 1.5 and 2.5 km below the surface. The combination of both arrays in conjunction with a new flexible curvature and new timing fluctuation function provides an opportunity for possible improvements of cosmic rays reconstruction. This work presents a preliminary investigation of possible improvements of cosmic rays primary energy estimation (proton, iron, helium, and oxygen) by using Machine Learning techniques and combined reconstruction. Lecture South pole Zenodo |
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English |
description |
The IceCube Neutrino Observatory at the South Pole is capable of measuring two components of the cosmic rays air shower. The electromagnetic component using a km2 surface array IceTop, and the high-energy muonic component using km3 in-ice array IceCube between 1.5 and 2.5 km below the surface. The combination of both arrays in conjunction with a new flexible curvature and new timing fluctuation function provides an opportunity for possible improvements of cosmic rays reconstruction. This work presents a preliminary investigation of possible improvements of cosmic rays primary energy estimation (proton, iron, helium, and oxygen) by using Machine Learning techniques and combined reconstruction. |
format |
Lecture |
author |
Silverio, Diana Leon Bai, Xinhua Plum, Matthias for the IceCube Collaboration |
spellingShingle |
Silverio, Diana Leon Bai, Xinhua Plum, Matthias for the IceCube Collaboration Cosmic rays primary energy estimation using Machine Learning and combined reconstruction |
author_facet |
Silverio, Diana Leon Bai, Xinhua Plum, Matthias for the IceCube Collaboration |
author_sort |
Silverio, Diana Leon |
title |
Cosmic rays primary energy estimation using Machine Learning and combined reconstruction |
title_short |
Cosmic rays primary energy estimation using Machine Learning and combined reconstruction |
title_full |
Cosmic rays primary energy estimation using Machine Learning and combined reconstruction |
title_fullStr |
Cosmic rays primary energy estimation using Machine Learning and combined reconstruction |
title_full_unstemmed |
Cosmic rays primary energy estimation using Machine Learning and combined reconstruction |
title_sort |
cosmic rays primary energy estimation using machine learning and combined reconstruction |
publisher |
Zenodo |
publishDate |
2022 |
url |
https://doi.org/10.5281/zenodo.6525169 |
genre |
South pole |
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South pole |
op_source |
Workshop on Machine learning for Cosmic-Ray Air Showers, Newark, Delaware, USA + Zoom (hybrid workshop), 31 Jan - 03 Feb 2022 |
op_relation |
https://zenodo.org/communities/ml-airshowers-bartol2022 https://doi.org/10.5281/zenodo.6525168 https://doi.org/10.5281/zenodo.6525169 oai:zenodo.org:6525169 |
op_rights |
info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode |
op_doi |
https://doi.org/10.5281/zenodo.652516910.5281/zenodo.6525168 |
_version_ |
1810480387295543296 |