Status of the ANTARES Project

The ANTARES collaboration is constructing a neutrino telescope in the Mediterranean Sea at a depth of 2400 metres, about 40 kilometres off the French coast near Toulon. The detector will consist of 12 vertical strings anchored at the sea bottom, each supporting 25 triplets of optical modules equippe...

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Published in:The European Physical Journal C
Main Author: Katz, U F
Language:English
Published: 2003
Subjects:
Online Access:https://doi.org/10.1140/epjcd/s2004-03-1755-x
http://cds.cern.ch/record/678806
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spelling ftcern:oai:cds.cern.ch:678806 2024-09-15T18:36:45+00:00 Status of the ANTARES Project Katz, U F 2003-10-26 https://doi.org/10.1140/epjcd/s2004-03-1755-x http://cds.cern.ch/record/678806 eng eng doi:10.1140/epjcd/s2004-03-1755-x http://cds.cern.ch/record/678806 astro-ph/0310736 FAU-PI-1-2003-01 oai:cds.cern.ch:678806 Astrophysics and Astronomy 2003 ftcern https://doi.org/10.1140/epjcd/s2004-03-1755-x 2024-07-22T13:50:50Z The ANTARES collaboration is constructing a neutrino telescope in the Mediterranean Sea at a depth of 2400 metres, about 40 kilometres off the French coast near Toulon. The detector will consist of 12 vertical strings anchored at the sea bottom, each supporting 25 triplets of optical modules equipped with photomultipliers, yielding sensitivity to neutrinos with energies above some 10 GeV. The effective detector area is roughly 0.1 square kilometres for neutrino energies exceeding 10 TeV. The measurement of the Cherenkov light emitted by muons produced in muon-neutrino charged-current interactions in water and under-sea rock will permit the reconstruction of the neutrino direction with an accuracy of better than 0.3 degrees at high energies. ANTARES will complement the field of view of neutrino telescopes at the South Pole in the low-background searches for point-sources of high-energy cosmic neutrinos and will also be sensitive to neutrinos produced by WIMP annihilation in the Sun or the Galactic centre. Other/Unknown Material South pole CERN Document Server (CDS) The European Physical Journal C 33 S1 s971 s974
institution Open Polar
collection CERN Document Server (CDS)
op_collection_id ftcern
language English
topic Astrophysics and Astronomy
spellingShingle Astrophysics and Astronomy
Katz, U F
Status of the ANTARES Project
topic_facet Astrophysics and Astronomy
description The ANTARES collaboration is constructing a neutrino telescope in the Mediterranean Sea at a depth of 2400 metres, about 40 kilometres off the French coast near Toulon. The detector will consist of 12 vertical strings anchored at the sea bottom, each supporting 25 triplets of optical modules equipped with photomultipliers, yielding sensitivity to neutrinos with energies above some 10 GeV. The effective detector area is roughly 0.1 square kilometres for neutrino energies exceeding 10 TeV. The measurement of the Cherenkov light emitted by muons produced in muon-neutrino charged-current interactions in water and under-sea rock will permit the reconstruction of the neutrino direction with an accuracy of better than 0.3 degrees at high energies. ANTARES will complement the field of view of neutrino telescopes at the South Pole in the low-background searches for point-sources of high-energy cosmic neutrinos and will also be sensitive to neutrinos produced by WIMP annihilation in the Sun or the Galactic centre.
author Katz, U F
author_facet Katz, U F
author_sort Katz, U F
title Status of the ANTARES Project
title_short Status of the ANTARES Project
title_full Status of the ANTARES Project
title_fullStr Status of the ANTARES Project
title_full_unstemmed Status of the ANTARES Project
title_sort status of the antares project
publishDate 2003
url https://doi.org/10.1140/epjcd/s2004-03-1755-x
http://cds.cern.ch/record/678806
genre South pole
genre_facet South pole
op_relation doi:10.1140/epjcd/s2004-03-1755-x
http://cds.cern.ch/record/678806
astro-ph/0310736
FAU-PI-1-2003-01
oai:cds.cern.ch:678806
op_doi https://doi.org/10.1140/epjcd/s2004-03-1755-x
container_title The European Physical Journal C
container_volume 33
container_issue S1
container_start_page s971
op_container_end_page s974
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