Neutrino astronomy with IceCube and AMANDA
Since the early 1990s, the South Pole has been the site of the construction of the world's first under-ice Cherenkov neutrino telescopes - AMANDA and IceCube. The AMANDA detector was completed in 2000, and its successor IceCube, a kilometre scale neutrino detector, began construction in 2005. C...
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ftdatacite:10.48550/arxiv.astro-ph/0611773 2023-05-15T18:22:07+02:00 Neutrino astronomy with IceCube and AMANDA Hill, Gary C. 2006 https://dx.doi.org/10.48550/arxiv.astro-ph/0611773 https://arxiv.org/abs/astro-ph/0611773 unknown arXiv Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences Preprint Article article CreativeWork 2006 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0611773 2022-04-01T15:53:32Z Since the early 1990s, the South Pole has been the site of the construction of the world's first under-ice Cherenkov neutrino telescopes - AMANDA and IceCube. The AMANDA detector was completed in 2000, and its successor IceCube, a kilometre scale neutrino detector, began construction in 2005. Completion of IceCube is scheduled for 2011. This paper will give an overview of the history, construction, latest physics results and potential of these detectors. : Proceeding of the IceCube/AMANDA talk at Neutrino 2006, Santa Fe, June 2006. To appear in Journal of Physics, Conference Series 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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Astrophysics astro-ph FOS Physical sciences |
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Astrophysics astro-ph FOS Physical sciences Hill, Gary C. Neutrino astronomy with IceCube and AMANDA |
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Astrophysics astro-ph FOS Physical sciences |
description |
Since the early 1990s, the South Pole has been the site of the construction of the world's first under-ice Cherenkov neutrino telescopes - AMANDA and IceCube. The AMANDA detector was completed in 2000, and its successor IceCube, a kilometre scale neutrino detector, began construction in 2005. Completion of IceCube is scheduled for 2011. This paper will give an overview of the history, construction, latest physics results and potential of these detectors. : Proceeding of the IceCube/AMANDA talk at Neutrino 2006, Santa Fe, June 2006. To appear in Journal of Physics, Conference Series |
format |
Report |
author |
Hill, Gary C. |
author_facet |
Hill, Gary C. |
author_sort |
Hill, Gary C. |
title |
Neutrino astronomy with IceCube and AMANDA |
title_short |
Neutrino astronomy with IceCube and AMANDA |
title_full |
Neutrino astronomy with IceCube and AMANDA |
title_fullStr |
Neutrino astronomy with IceCube and AMANDA |
title_full_unstemmed |
Neutrino astronomy with IceCube and AMANDA |
title_sort |
neutrino astronomy with icecube and amanda |
publisher |
arXiv |
publishDate |
2006 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0611773 https://arxiv.org/abs/astro-ph/0611773 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_rights |
Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ |
op_doi |
https://doi.org/10.48550/arxiv.astro-ph/0611773 |
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1766201477100994560 |