KM3NeT/ORCA Calibration Procedures and Capabilities

The cubic-kilometre neutrino telescope (KM3NeT) is a piece of deep-sea infrastructure composed of two neutrino telescopes consisting of large-scale 3D arrays of photomultiplier tubes (PMTs). KM3NeT is currently under construction on the Mediterranean seabed. The two telescopes are ARCA, near Sicily,...

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Published in:NuFACT 2022
Main Author: Antonio De Benedittis
Format: Text
Language:English
Published: Multidisciplinary Digital Publishing Institute 2023
Subjects:
PMT
Online Access:https://doi.org/10.3390/psf2023008044
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spelling ftmdpi:oai:mdpi.com:/2673-9984/8/1/44/ 2023-09-26T15:21:45+02:00 KM3NeT/ORCA Calibration Procedures and Capabilities Antonio De Benedittis 2023-08-23 application/pdf https://doi.org/10.3390/psf2023008044 EN eng Multidisciplinary Digital Publishing Institute https://dx.doi.org/10.3390/psf2023008044 https://creativecommons.org/licenses/by/4.0/ Physical Sciences Forum; Volume 8; Issue 1; Pages: 44 KM3NeT ORCA calibration neutrino astronomy high energy PMT Text 2023 ftmdpi https://doi.org/10.3390/psf2023008044 2023-08-27T23:53:01Z The cubic-kilometre neutrino telescope (KM3NeT) is a piece of deep-sea infrastructure composed of two neutrino telescopes consisting of large-scale 3D arrays of photomultiplier tubes (PMTs). KM3NeT is currently under construction on the Mediterranean seabed. The two telescopes are ARCA, near Sicily, which is designed for neutrino astronomy, and ORCA, near Toulon, France, designed for measurement of neutrino oscillations. The ORCA telescope, having a neutrino energy threshold in the GeV range, has as its main research goal the measurement of the neutrino mass ordering and atmospheric neutrino oscillation parameters. In this paper, we discuss the calibration procedures which are necessary to achieve these purposes. Text Orca MDPI Open Access Publishing NuFACT 2022 44
institution Open Polar
collection MDPI Open Access Publishing
op_collection_id ftmdpi
language English
topic KM3NeT
ORCA
calibration
neutrino
astronomy
high energy
PMT
spellingShingle KM3NeT
ORCA
calibration
neutrino
astronomy
high energy
PMT
Antonio De Benedittis
KM3NeT/ORCA Calibration Procedures and Capabilities
topic_facet KM3NeT
ORCA
calibration
neutrino
astronomy
high energy
PMT
description The cubic-kilometre neutrino telescope (KM3NeT) is a piece of deep-sea infrastructure composed of two neutrino telescopes consisting of large-scale 3D arrays of photomultiplier tubes (PMTs). KM3NeT is currently under construction on the Mediterranean seabed. The two telescopes are ARCA, near Sicily, which is designed for neutrino astronomy, and ORCA, near Toulon, France, designed for measurement of neutrino oscillations. The ORCA telescope, having a neutrino energy threshold in the GeV range, has as its main research goal the measurement of the neutrino mass ordering and atmospheric neutrino oscillation parameters. In this paper, we discuss the calibration procedures which are necessary to achieve these purposes.
format Text
author Antonio De Benedittis
author_facet Antonio De Benedittis
author_sort Antonio De Benedittis
title KM3NeT/ORCA Calibration Procedures and Capabilities
title_short KM3NeT/ORCA Calibration Procedures and Capabilities
title_full KM3NeT/ORCA Calibration Procedures and Capabilities
title_fullStr KM3NeT/ORCA Calibration Procedures and Capabilities
title_full_unstemmed KM3NeT/ORCA Calibration Procedures and Capabilities
title_sort km3net/orca calibration procedures and capabilities
publisher Multidisciplinary Digital Publishing Institute
publishDate 2023
url https://doi.org/10.3390/psf2023008044
genre Orca
genre_facet Orca
op_source Physical Sciences Forum; Volume 8; Issue 1; Pages: 44
op_relation https://dx.doi.org/10.3390/psf2023008044
op_rights https://creativecommons.org/licenses/by/4.0/
op_doi https://doi.org/10.3390/psf2023008044
container_title NuFACT 2022
container_start_page 44
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