Results from Seven Years of AMANDA-II

AMANDA is a first-generation high energy neutrino telescope, which has taken data at the South Pole in its final configuration since 2000. Results from seven years of operation are presented here, including observation of the atmopheric neutrino flux and searches for astrophysical neutrinos from cos...

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Bibliographic Details
Main Author: DeYoung, Tyce
Format: Text
Language:unknown
Published: arXiv 2008
Subjects:
Astrophysics astro-ph
FOS Physical sciences
New Zealand
South Pole
Christchurch
South pole
Online Access:https://dx.doi.org/10.48550/arxiv.0810.4513
https://arxiv.org/abs/0810.4513
id ftdatacite:10.48550/arxiv.0810.4513
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spelling ftdatacite:10.48550/arxiv.0810.4513 2023-05-15T18:22:09+02:00 Results from Seven Years of AMANDA-II DeYoung, Tyce 2008 https://dx.doi.org/10.48550/arxiv.0810.4513 https://arxiv.org/abs/0810.4513 unknown arXiv https://dx.doi.org/10.1088/1742-6596/136/2/022046 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2008 ftdatacite https://doi.org/10.48550/arxiv.0810.4513 https://doi.org/10.1088/1742-6596/136/2/022046 2022-04-01T15:16:22Z AMANDA is a first-generation high energy neutrino telescope, which has taken data at the South Pole in its final configuration since 2000. Results from seven years of operation are presented here, including observation of the atmopheric neutrino flux and searches for astrophysical neutrinos from cosmic ray accelerators, gamma ray bursts, and dark matter annihilations. In 2007, AMANDA was incorporated into the IceCube neutrino telescope, where its higher density of instrumentation improves the low energy response. In the near future, AMANDA will be replaced by the IceCube Deep Core, a purpose-built low energy extension of IceCube. : Presented at Neutrino 2008, Christchurch, New Zealand Text South pole DataCite Metadata Store (German National Library of Science and Technology) New Zealand South Pole Christchurch ENVELOPE(164.167,164.167,-82.467,-82.467)
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
DeYoung, Tyce
Results from Seven Years of AMANDA-II
topic_facet Astrophysics astro-ph
FOS Physical sciences
description AMANDA is a first-generation high energy neutrino telescope, which has taken data at the South Pole in its final configuration since 2000. Results from seven years of operation are presented here, including observation of the atmopheric neutrino flux and searches for astrophysical neutrinos from cosmic ray accelerators, gamma ray bursts, and dark matter annihilations. In 2007, AMANDA was incorporated into the IceCube neutrino telescope, where its higher density of instrumentation improves the low energy response. In the near future, AMANDA will be replaced by the IceCube Deep Core, a purpose-built low energy extension of IceCube. : Presented at Neutrino 2008, Christchurch, New Zealand
format Text
author DeYoung, Tyce
author_facet DeYoung, Tyce
author_sort DeYoung, Tyce
title Results from Seven Years of AMANDA-II
title_short Results from Seven Years of AMANDA-II
title_full Results from Seven Years of AMANDA-II
title_fullStr Results from Seven Years of AMANDA-II
title_full_unstemmed Results from Seven Years of AMANDA-II
title_sort results from seven years of amanda-ii
publisher arXiv
publishDate 2008
url https://dx.doi.org/10.48550/arxiv.0810.4513
https://arxiv.org/abs/0810.4513
long_lat ENVELOPE(164.167,164.167,-82.467,-82.467)
geographic New Zealand
South Pole
Christchurch
geographic_facet New Zealand
South Pole
Christchurch
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1088/1742-6596/136/2/022046
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.0810.4513
https://doi.org/10.1088/1742-6596/136/2/022046
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