High Energy Neutrino Astronomy: IceCube 22 and 40 strings
In this paper, after a short introduction to the physics of neutrino telescopes, we will report on first performances of the IceCube detector and a selection of preliminary results obtained from data taken while IceCube operated in a partially completed configuration (22 strings and 40 strings). We...
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ftdatacite:10.48550/arxiv.1012.0415 2023-05-15T18:22:20+02:00 High Energy Neutrino Astronomy: IceCube 22 and 40 strings Resconi, E. 2010 https://dx.doi.org/10.48550/arxiv.1012.0415 https://arxiv.org/abs/1012.0415 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE High Energy Physics - Experiment hep-ex FOS Physical sciences Preprint Article article CreativeWork 2010 ftdatacite https://doi.org/10.48550/arxiv.1012.0415 2022-04-01T14:14:51Z In this paper, after a short introduction to the physics of neutrino telescopes, we will report on first performances of the IceCube detector and a selection of preliminary results obtained from data taken while IceCube operated in a partially completed configuration (22 strings and 40 strings). We will emphasize new analysis methods recently developed for the study of the Southern Hemisphere as well as for extended regions. Based on the long term experience of AMANDA and IceCube, the South Pole ice has proven to be an ideal site for astroparticle physics. New ideas and projects about the future beyond IceCube will conclude this presentation. : 7 pages, 3 figures, Conference proceeding to XXIV International Conference on Neutrino Physics and Astrophysics 2010 Report South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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DataCite Metadata Store (German National Library of Science and Technology) |
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High Energy Astrophysical Phenomena astro-ph.HE High Energy Physics - Experiment hep-ex FOS Physical sciences |
spellingShingle |
High Energy Astrophysical Phenomena astro-ph.HE High Energy Physics - Experiment hep-ex FOS Physical sciences Resconi, E. High Energy Neutrino Astronomy: IceCube 22 and 40 strings |
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High Energy Astrophysical Phenomena astro-ph.HE High Energy Physics - Experiment hep-ex FOS Physical sciences |
description |
In this paper, after a short introduction to the physics of neutrino telescopes, we will report on first performances of the IceCube detector and a selection of preliminary results obtained from data taken while IceCube operated in a partially completed configuration (22 strings and 40 strings). We will emphasize new analysis methods recently developed for the study of the Southern Hemisphere as well as for extended regions. Based on the long term experience of AMANDA and IceCube, the South Pole ice has proven to be an ideal site for astroparticle physics. New ideas and projects about the future beyond IceCube will conclude this presentation. : 7 pages, 3 figures, Conference proceeding to XXIV International Conference on Neutrino Physics and Astrophysics 2010 |
format |
Report |
author |
Resconi, E. |
author_facet |
Resconi, E. |
author_sort |
Resconi, E. |
title |
High Energy Neutrino Astronomy: IceCube 22 and 40 strings |
title_short |
High Energy Neutrino Astronomy: IceCube 22 and 40 strings |
title_full |
High Energy Neutrino Astronomy: IceCube 22 and 40 strings |
title_fullStr |
High Energy Neutrino Astronomy: IceCube 22 and 40 strings |
title_full_unstemmed |
High Energy Neutrino Astronomy: IceCube 22 and 40 strings |
title_sort |
high energy neutrino astronomy: icecube 22 and 40 strings |
publisher |
arXiv |
publishDate |
2010 |
url |
https://dx.doi.org/10.48550/arxiv.1012.0415 https://arxiv.org/abs/1012.0415 |
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South Pole |
geographic_facet |
South Pole |
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South pole |
genre_facet |
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.1012.0415 |
_version_ |
1766201731453026304 |