Neutrino Astronomy with the IceCube Observatory and Implications for Astroparticle Physics
The IceCube Observatory is a km^3 neutrino telescope currently under construction at the geographic South Pole. It will comprise 4800 optical sensors deployed on 80 vertical strings between 1450 and 2450 meters under the ice surface. Currently IceCube is operational and recording data with 40 string...
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ftdatacite:10.48550/arxiv.0812.4004 2023-05-15T18:22:28+02:00 Neutrino Astronomy with the IceCube Observatory and Implications for Astroparticle Physics Desiati, Paolo 2008 https://dx.doi.org/10.48550/arxiv.0812.4004 https://arxiv.org/abs/0812.4004 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics astro-ph FOS Physical sciences Preprint Article article CreativeWork 2008 ftdatacite https://doi.org/10.48550/arxiv.0812.4004 2022-04-01T14:54:32Z The IceCube Observatory is a km^3 neutrino telescope currently under construction at the geographic South Pole. It will comprise 4800 optical sensors deployed on 80 vertical strings between 1450 and 2450 meters under the ice surface. Currently IceCube is operational and recording data with 40 strings (i.e. 2400 optical sensors). The IceCube Observatory will collect an unprecedented number of high energy neutrinos that will allow us to pursue studies of the atmospheric neutrino flux, and to search for extraterrestrial sources of neutrinos, whether point-like or unresolved. IceCube results will have an important impact on neutrino astrophysics, especially if combined with observations done with other cosmic messengers, such as gamma rays or ultra high energy cosmic rays. They may also reveal clues on the origin of cosmic rays at ultra high energies. Here we report results from AMANDA and the most recent results from the first 22 strings of IceCube. : 12 pages, 4 figures, proceeding of the Vulcano Workshop 2008, Vulcano (ME), Italy (2008) Report South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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Astrophysics astro-ph FOS Physical sciences |
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Astrophysics astro-ph FOS Physical sciences Desiati, Paolo Neutrino Astronomy with the IceCube Observatory and Implications for Astroparticle Physics |
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Astrophysics astro-ph FOS Physical sciences |
description |
The IceCube Observatory is a km^3 neutrino telescope currently under construction at the geographic South Pole. It will comprise 4800 optical sensors deployed on 80 vertical strings between 1450 and 2450 meters under the ice surface. Currently IceCube is operational and recording data with 40 strings (i.e. 2400 optical sensors). The IceCube Observatory will collect an unprecedented number of high energy neutrinos that will allow us to pursue studies of the atmospheric neutrino flux, and to search for extraterrestrial sources of neutrinos, whether point-like or unresolved. IceCube results will have an important impact on neutrino astrophysics, especially if combined with observations done with other cosmic messengers, such as gamma rays or ultra high energy cosmic rays. They may also reveal clues on the origin of cosmic rays at ultra high energies. Here we report results from AMANDA and the most recent results from the first 22 strings of IceCube. : 12 pages, 4 figures, proceeding of the Vulcano Workshop 2008, Vulcano (ME), Italy (2008) |
format |
Report |
author |
Desiati, Paolo |
author_facet |
Desiati, Paolo |
author_sort |
Desiati, Paolo |
title |
Neutrino Astronomy with the IceCube Observatory and Implications for Astroparticle Physics |
title_short |
Neutrino Astronomy with the IceCube Observatory and Implications for Astroparticle Physics |
title_full |
Neutrino Astronomy with the IceCube Observatory and Implications for Astroparticle Physics |
title_fullStr |
Neutrino Astronomy with the IceCube Observatory and Implications for Astroparticle Physics |
title_full_unstemmed |
Neutrino Astronomy with the IceCube Observatory and Implications for Astroparticle Physics |
title_sort |
neutrino astronomy with the icecube observatory and implications for astroparticle physics |
publisher |
arXiv |
publishDate |
2008 |
url |
https://dx.doi.org/10.48550/arxiv.0812.4004 https://arxiv.org/abs/0812.4004 |
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South Pole |
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South Pole |
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South pole |
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South pole |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.0812.4004 |
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1766201877648637952 |