Design & Performance Goals for the IceCube Upgrade

The IceCube Upgrade is an under construction next-generation detector extension of the IceCube Neutrino Observatory. The deployment of additional strings with improved photosensors at denser spacings than the current detector will dramatically enhance many of IceCube’s analyses, including atmospheri...

Full description

Bibliographic Details
Main Author: D. Jason Koskinen
Format: Conference Object
Language:unknown
Published: Zenodo 2022
Subjects:
Online Access:https://doi.org/10.5281/zenodo.6805225
id ftzenodo:oai:zenodo.org:6805225
record_format openpolar
spelling ftzenodo:oai:zenodo.org:6805225 2024-09-15T18:36:40+00:00 Design & Performance Goals for the IceCube Upgrade D. Jason Koskinen 2022-07-07 https://doi.org/10.5281/zenodo.6805225 unknown Zenodo https://zenodo.org/communities/neutrino2022-posters https://doi.org/10.5281/zenodo.6805224 https://doi.org/10.5281/zenodo.6805225 oai:zenodo.org:6805225 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.680522510.5281/zenodo.6805224 2024-07-26T23:59:38Z The IceCube Upgrade is an under construction next-generation detector extension of the IceCube Neutrino Observatory. The deployment of additional strings with improved photosensors at denser spacings than the current detector will dramatically enhance many of IceCube’s analyses, including atmospheric neutrino oscillation analyses, indirect searches for dark matter, and 1-100 GeV neutrino astronomy. New calibration devices will improve systematic uncertainties; notably those related to photon scattering and absorption in the South Pole ice which impact angular and energy reconstruction resolutions across the highest and lowest energy ranges to which IceCube is sensitive. This poster will provide an overview of the layout, design, hardware, and performance goals of the IceCube Upgrade.The IceCube Upgrade is an under construction next-generation detector extension of the IceCube Neutrino Observatory. The deployment of additional strings with improved photosensors at denser spacings than the current detector will dramatically enhance many of IceCube’s analyses, including atmospheric neutrino oscillation analyses, indirect searches for dark matter, and 1-100 GeV neutrino astronomy. New calibration devices will improve systematic uncertainties; notably those related to photon scattering and absorption in the South Pole ice which impact angular and energy reconstruction resolutions across the highest and lowest energy ranges to which IceCube is sensitive. This poster will provide an overview of the layout, design, hardware, and performance goals of the IceCube Upgrade. Conference Object South pole Zenodo
institution Open Polar
collection Zenodo
op_collection_id ftzenodo
language unknown
description The IceCube Upgrade is an under construction next-generation detector extension of the IceCube Neutrino Observatory. The deployment of additional strings with improved photosensors at denser spacings than the current detector will dramatically enhance many of IceCube’s analyses, including atmospheric neutrino oscillation analyses, indirect searches for dark matter, and 1-100 GeV neutrino astronomy. New calibration devices will improve systematic uncertainties; notably those related to photon scattering and absorption in the South Pole ice which impact angular and energy reconstruction resolutions across the highest and lowest energy ranges to which IceCube is sensitive. This poster will provide an overview of the layout, design, hardware, and performance goals of the IceCube Upgrade.The IceCube Upgrade is an under construction next-generation detector extension of the IceCube Neutrino Observatory. The deployment of additional strings with improved photosensors at denser spacings than the current detector will dramatically enhance many of IceCube’s analyses, including atmospheric neutrino oscillation analyses, indirect searches for dark matter, and 1-100 GeV neutrino astronomy. New calibration devices will improve systematic uncertainties; notably those related to photon scattering and absorption in the South Pole ice which impact angular and energy reconstruction resolutions across the highest and lowest energy ranges to which IceCube is sensitive. This poster will provide an overview of the layout, design, hardware, and performance goals of the IceCube Upgrade.
format Conference Object
author D. Jason Koskinen
spellingShingle D. Jason Koskinen
Design & Performance Goals for the IceCube Upgrade
author_facet D. Jason Koskinen
author_sort D. Jason Koskinen
title Design & Performance Goals for the IceCube Upgrade
title_short Design & Performance Goals for the IceCube Upgrade
title_full Design & Performance Goals for the IceCube Upgrade
title_fullStr Design & Performance Goals for the IceCube Upgrade
title_full_unstemmed Design & Performance Goals for the IceCube Upgrade
title_sort design & performance goals for the icecube upgrade
publisher Zenodo
publishDate 2022
url https://doi.org/10.5281/zenodo.6805225
genre South pole
genre_facet South pole
op_relation https://zenodo.org/communities/neutrino2022-posters
https://doi.org/10.5281/zenodo.6805224
https://doi.org/10.5281/zenodo.6805225
oai:zenodo.org:6805225
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.680522510.5281/zenodo.6805224
_version_ 1810480356057415680