Novel Background Rejection Techniques in a Search for Ultra-high Energy Neutrinos Using an ARIANNA Detector Station at the South Pole
The ARIANNA detector array is a radio-based neutrino detector array consisting of autonomous, solar-powered stations separated by 1km. It is designed to detect neutrinos with energies above 1017eV that interact with the cold, transparent polar ice. An ARIANNA detector station located near the South...
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ftzenodo:oai:zenodo.org:6785194 2024-09-15T18:36:38+00:00 Novel Background Rejection Techniques in a Search for Ultra-high Energy Neutrinos Using an ARIANNA Detector Station at the South Pole Leshan Zhao 2022-07-01 https://doi.org/10.5281/zenodo.6785194 unknown Zenodo https://zenodo.org/communities/neutrino2022-posters https://doi.org/10.5281/zenodo.6785193 https://doi.org/10.5281/zenodo.6785194 oai:zenodo.org:6785194 info:eu-repo/semantics/openAccess Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode info:eu-repo/semantics/conferencePoster 2022 ftzenodo https://doi.org/10.5281/zenodo.678519410.5281/zenodo.6785193 2024-07-26T09:45:07Z The ARIANNA detector array is a radio-based neutrino detector array consisting of autonomous, solar-powered stations separated by 1km. It is designed to detect neutrinos with energies above 1017eV that interact with the cold, transparent polar ice. An ARIANNA detector station located near the South Pole has been equipped with 4 downward-facing LPDAs, 2 upward-facing LPDAs, and 2 dipole antennas, and has been taking data from December 2018 to January 2021. We provide a preliminary report on the improvement in background rejection due to novel analysis techniques utilizing the newly added upward-facing LPDAs and dipole antennas. Conference Object South pole Zenodo |
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description |
The ARIANNA detector array is a radio-based neutrino detector array consisting of autonomous, solar-powered stations separated by 1km. It is designed to detect neutrinos with energies above 1017eV that interact with the cold, transparent polar ice. An ARIANNA detector station located near the South Pole has been equipped with 4 downward-facing LPDAs, 2 upward-facing LPDAs, and 2 dipole antennas, and has been taking data from December 2018 to January 2021. We provide a preliminary report on the improvement in background rejection due to novel analysis techniques utilizing the newly added upward-facing LPDAs and dipole antennas. |
format |
Conference Object |
author |
Leshan Zhao |
spellingShingle |
Leshan Zhao Novel Background Rejection Techniques in a Search for Ultra-high Energy Neutrinos Using an ARIANNA Detector Station at the South Pole |
author_facet |
Leshan Zhao |
author_sort |
Leshan Zhao |
title |
Novel Background Rejection Techniques in a Search for Ultra-high Energy Neutrinos Using an ARIANNA Detector Station at the South Pole |
title_short |
Novel Background Rejection Techniques in a Search for Ultra-high Energy Neutrinos Using an ARIANNA Detector Station at the South Pole |
title_full |
Novel Background Rejection Techniques in a Search for Ultra-high Energy Neutrinos Using an ARIANNA Detector Station at the South Pole |
title_fullStr |
Novel Background Rejection Techniques in a Search for Ultra-high Energy Neutrinos Using an ARIANNA Detector Station at the South Pole |
title_full_unstemmed |
Novel Background Rejection Techniques in a Search for Ultra-high Energy Neutrinos Using an ARIANNA Detector Station at the South Pole |
title_sort |
novel background rejection techniques in a search for ultra-high energy neutrinos using an arianna detector station at the south pole |
publisher |
Zenodo |
publishDate |
2022 |
url |
https://doi.org/10.5281/zenodo.6785194 |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://zenodo.org/communities/neutrino2022-posters https://doi.org/10.5281/zenodo.6785193 https://doi.org/10.5281/zenodo.6785194 oai:zenodo.org:6785194 |
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.678519410.5281/zenodo.6785193 |
_version_ |
1810480312725012480 |