The IceCube Neutrino Telescope
Abstract Construction of IceCube at the Amundsen-Scott South Pole Station was completed at the end of 2010 after eight construction seasons. The detector consists of 5,160 digital optical modules on 86 cables with 60 modules each, viewing in total a cubic kilometer of ice between 1,450 and 2,450 met...
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Online Access: | http://dx.doi.org/10.1017/s1743921312016742 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921312016742 |
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crcambridgeupr:10.1017/s1743921312016742 2024-09-15T17:39:13+00:00 The IceCube Neutrino Telescope Gaisser, Thomas K. 2012 http://dx.doi.org/10.1017/s1743921312016742 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921312016742 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Proceedings of the International Astronomical Union volume 8, issue S288, page 105-114 ISSN 1743-9213 1743-9221 journal-article 2012 crcambridgeupr https://doi.org/10.1017/s1743921312016742 2024-08-07T04:02:36Z Abstract Construction of IceCube at the Amundsen-Scott South Pole Station was completed at the end of 2010 after eight construction seasons. The detector consists of 5,160 digital optical modules on 86 cables with 60 modules each, viewing in total a cubic kilometer of ice between 1,450 and 2,450 meters below the surface. IceCube includes a sub-array called DeepCore consisting of 8 special cables, and providing a more densely instrumented region with a lower energy threshold in the deep center of the array. IceCube also includes an air shower array called IceTop directly above the deep detector. Optical modules in all three components of the detector are fully integrated into a single data acquisition system. Data taking and analysis began during construction and continues with the completed detector. This paper describes recent results from IceCube. Article in Journal/Newspaper Amundsen-Scott South pole Cambridge University Press Proceedings of the International Astronomical Union 8 S288 105 114 |
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Cambridge University Press |
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English |
description |
Abstract Construction of IceCube at the Amundsen-Scott South Pole Station was completed at the end of 2010 after eight construction seasons. The detector consists of 5,160 digital optical modules on 86 cables with 60 modules each, viewing in total a cubic kilometer of ice between 1,450 and 2,450 meters below the surface. IceCube includes a sub-array called DeepCore consisting of 8 special cables, and providing a more densely instrumented region with a lower energy threshold in the deep center of the array. IceCube also includes an air shower array called IceTop directly above the deep detector. Optical modules in all three components of the detector are fully integrated into a single data acquisition system. Data taking and analysis began during construction and continues with the completed detector. This paper describes recent results from IceCube. |
format |
Article in Journal/Newspaper |
author |
Gaisser, Thomas K. |
spellingShingle |
Gaisser, Thomas K. The IceCube Neutrino Telescope |
author_facet |
Gaisser, Thomas K. |
author_sort |
Gaisser, Thomas K. |
title |
The IceCube Neutrino Telescope |
title_short |
The IceCube Neutrino Telescope |
title_full |
The IceCube Neutrino Telescope |
title_fullStr |
The IceCube Neutrino Telescope |
title_full_unstemmed |
The IceCube Neutrino Telescope |
title_sort |
icecube neutrino telescope |
publisher |
Cambridge University Press (CUP) |
publishDate |
2012 |
url |
http://dx.doi.org/10.1017/s1743921312016742 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921312016742 |
genre |
Amundsen-Scott South pole |
genre_facet |
Amundsen-Scott South pole |
op_source |
Proceedings of the International Astronomical Union volume 8, issue S288, page 105-114 ISSN 1743-9213 1743-9221 |
op_rights |
https://www.cambridge.org/core/terms |
op_doi |
https://doi.org/10.1017/s1743921312016742 |
container_title |
Proceedings of the International Astronomical Union |
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8 |
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S288 |
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105 |
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114 |
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1810478495883591680 |