Recent Results of Point Source Searches with the IceCube Neutrino Telescope Erik Strahler
Abstract. IceCube is a km 3 scale neutrino detector being constructed deep in the Antarctic ice. When complete, IceCube will consist of 4800 optical modules deployed on 80 strings between 1450 and 2450 m of depth. During the 2007-2008 data taking season, 22 strings were operational. This configurati...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.250.6026 2023-05-15T13:54:53+02:00 Recent Results of Point Source Searches with the IceCube Neutrino Telescope Erik Strahler For The Icecube Collaboration The Pennsylvania State University CiteSeerX Archives 905 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.250.6026 http://arxiv.org/pdf/0905.4705v1.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.250.6026 http://arxiv.org/pdf/0905.4705v1.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://arxiv.org/pdf/0905.4705v1.pdf text ftciteseerx 2016-01-07T19:43:49Z Abstract. IceCube is a km 3 scale neutrino detector being constructed deep in the Antarctic ice. When complete, IceCube will consist of 4800 optical modules deployed on 80 strings between 1450 and 2450 m of depth. During the 2007-2008 data taking season, 22 strings were operational. This configuration is already much larger than previous neutrino telescopes and provides better sensitivity to point sources of high energy (>1 TeV) neutrino emission. Such astrophysical objects are leading candidates for the acceleration of cosmic rays. We describe the IceCube detector and present the methods and results of several recent searches for steady (e.g. AGN) and transient (GRB) point sources. 1. Text Antarc* Antarctic Unknown Antarctic The Antarctic |
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Abstract. IceCube is a km 3 scale neutrino detector being constructed deep in the Antarctic ice. When complete, IceCube will consist of 4800 optical modules deployed on 80 strings between 1450 and 2450 m of depth. During the 2007-2008 data taking season, 22 strings were operational. This configuration is already much larger than previous neutrino telescopes and provides better sensitivity to point sources of high energy (>1 TeV) neutrino emission. Such astrophysical objects are leading candidates for the acceleration of cosmic rays. We describe the IceCube detector and present the methods and results of several recent searches for steady (e.g. AGN) and transient (GRB) point sources. 1. |
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The Pennsylvania State University CiteSeerX Archives |
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For The Icecube Collaboration |
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For The Icecube Collaboration Recent Results of Point Source Searches with the IceCube Neutrino Telescope Erik Strahler |
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For The Icecube Collaboration |
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For The Icecube Collaboration |
title |
Recent Results of Point Source Searches with the IceCube Neutrino Telescope Erik Strahler |
title_short |
Recent Results of Point Source Searches with the IceCube Neutrino Telescope Erik Strahler |
title_full |
Recent Results of Point Source Searches with the IceCube Neutrino Telescope Erik Strahler |
title_fullStr |
Recent Results of Point Source Searches with the IceCube Neutrino Telescope Erik Strahler |
title_full_unstemmed |
Recent Results of Point Source Searches with the IceCube Neutrino Telescope Erik Strahler |
title_sort |
recent results of point source searches with the icecube neutrino telescope erik strahler |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.250.6026 http://arxiv.org/pdf/0905.4705v1.pdf |
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Antarctic The Antarctic |
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Antarctic The Antarctic |
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Antarc* Antarctic |
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Antarc* Antarctic |
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http://arxiv.org/pdf/0905.4705v1.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.250.6026 http://arxiv.org/pdf/0905.4705v1.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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1766261092059709440 |