NEUTRINO ASTRONOMY WITH ICECUBE
IceCube is a kilometer-scale high energy neutrino telescope under construction at the South Pole, a second-generation instrument expanding the capabilities of the AMANDA telescope. The scientific portfolio of IceCube includes the detection of neutrinos from astrophysical objects such as the sources...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.249.1973 2023-05-15T18:22:16+02:00 NEUTRINO ASTRONOMY WITH ICECUBE Tyce Deyoung The Pennsylvania State University CiteSeerX Archives 906 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.249.1973 http://arxiv.org/pdf/0906.4530v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.249.1973 http://arxiv.org/pdf/0906.4530v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/0906.4530v1.pdf 1. Cosmic Rays Gamma Rays and Neutrinos text ftciteseerx 2016-01-07T19:36:56Z IceCube is a kilometer-scale high energy neutrino telescope under construction at the South Pole, a second-generation instrument expanding the capabilities of the AMANDA telescope. The scientific portfolio of IceCube includes the detection of neutrinos from astrophysical objects such as the sources of the cosmic rays, the search for dark matter, and fundamental physics using a very large data set of atmospheric neutrinos. The design and status of IceCube are briefly reviewed, followed by a summary of results to date from AMANDA and initial IceCube results from the 2007 run, with 22 of a planned 86 strings operational. The new infill array known as Deep Core, which will extend IceCube’s capabilities to energies as low as 10 GeV, is also described. Text South pole Unknown South Pole |
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1. Cosmic Rays Gamma Rays and Neutrinos |
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1. Cosmic Rays Gamma Rays and Neutrinos Tyce Deyoung NEUTRINO ASTRONOMY WITH ICECUBE |
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1. Cosmic Rays Gamma Rays and Neutrinos |
description |
IceCube is a kilometer-scale high energy neutrino telescope under construction at the South Pole, a second-generation instrument expanding the capabilities of the AMANDA telescope. The scientific portfolio of IceCube includes the detection of neutrinos from astrophysical objects such as the sources of the cosmic rays, the search for dark matter, and fundamental physics using a very large data set of atmospheric neutrinos. The design and status of IceCube are briefly reviewed, followed by a summary of results to date from AMANDA and initial IceCube results from the 2007 run, with 22 of a planned 86 strings operational. The new infill array known as Deep Core, which will extend IceCube’s capabilities to energies as low as 10 GeV, is also described. |
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The Pennsylvania State University CiteSeerX Archives |
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Text |
author |
Tyce Deyoung |
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Tyce Deyoung |
author_sort |
Tyce Deyoung |
title |
NEUTRINO ASTRONOMY WITH ICECUBE |
title_short |
NEUTRINO ASTRONOMY WITH ICECUBE |
title_full |
NEUTRINO ASTRONOMY WITH ICECUBE |
title_fullStr |
NEUTRINO ASTRONOMY WITH ICECUBE |
title_full_unstemmed |
NEUTRINO ASTRONOMY WITH ICECUBE |
title_sort |
neutrino astronomy with icecube |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.249.1973 http://arxiv.org/pdf/0906.4530v1.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/0906.4530v1.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.249.1973 http://arxiv.org/pdf/0906.4530v1.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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1766201650987401216 |