RATIONALE OF HIGH ENERGY NEUTRINO ASTRONOMY
Abstract. IceCube is a cubic-kilometer neutrino telescope under construction at the geographic South Pole. Once completed it will comprise 4800 optical sensors deployed on 80 vertical strings at depths in the ice between 1450 and 2450 meters. Part of the array is already operational and data was rec...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.243.5680 2023-05-15T18:22:05+02:00 RATIONALE OF HIGH ENERGY NEUTRINO ASTRONOMY Elisa Bernardini The Pennsylvania State University CiteSeerX Archives 901 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.243.5680 http://arxiv.org/pdf/0901.1049v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.243.5680 http://arxiv.org/pdf/0901.1049v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/0901.1049v1.pdf Cosmic neutrinos high-energy gamma-rays text ftciteseerx 2016-01-07T19:20:04Z Abstract. IceCube is a cubic-kilometer neutrino telescope under construction at the geographic South Pole. Once completed it will comprise 4800 optical sensors deployed on 80 vertical strings at depths in the ice between 1450 and 2450 meters. Part of the array is already operational and data was recorded in the configurations with 9 (year 2006/2007), 22 (year 2007/2008) and 40-strings (year 2008/2009) respectively. Here we report preliminary results on the search for point-like neutrino sources using data collected with the first 22 strings (IC-22). Text South pole Unknown South Pole |
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Cosmic neutrinos high-energy gamma-rays |
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Cosmic neutrinos high-energy gamma-rays Elisa Bernardini RATIONALE OF HIGH ENERGY NEUTRINO ASTRONOMY |
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Cosmic neutrinos high-energy gamma-rays |
description |
Abstract. IceCube is a cubic-kilometer neutrino telescope under construction at the geographic South Pole. Once completed it will comprise 4800 optical sensors deployed on 80 vertical strings at depths in the ice between 1450 and 2450 meters. Part of the array is already operational and data was recorded in the configurations with 9 (year 2006/2007), 22 (year 2007/2008) and 40-strings (year 2008/2009) respectively. Here we report preliminary results on the search for point-like neutrino sources using data collected with the first 22 strings (IC-22). |
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The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Elisa Bernardini |
author_facet |
Elisa Bernardini |
author_sort |
Elisa Bernardini |
title |
RATIONALE OF HIGH ENERGY NEUTRINO ASTRONOMY |
title_short |
RATIONALE OF HIGH ENERGY NEUTRINO ASTRONOMY |
title_full |
RATIONALE OF HIGH ENERGY NEUTRINO ASTRONOMY |
title_fullStr |
RATIONALE OF HIGH ENERGY NEUTRINO ASTRONOMY |
title_full_unstemmed |
RATIONALE OF HIGH ENERGY NEUTRINO ASTRONOMY |
title_sort |
rationale of high energy neutrino astronomy |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.243.5680 http://arxiv.org/pdf/0901.1049v1.pdf |
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South Pole |
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South Pole |
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South pole |
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South pole |
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http://arxiv.org/pdf/0901.1049v1.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.243.5680 http://arxiv.org/pdf/0901.1049v1.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766201425927340032 |