IceCube — the next generation neutrino telescope at the South Pole

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Title: IceCube — the next generation neutrino telescope at the South Pole
Authors: Karle, A.1, Ahrens, J.2, Bahcall, J.N.3, Bai, X.2, Becka, T.2, Becker, K.-H.4, Besson, D.Z.5, Berley, D.6, Bernardini, E.7, Bertrand, D.8, Binon, F.8, Biron, A.7, Böser, S.7, Bohm, C., Botner, O.9, Bouhali, O.8, Burgess, Th.10, Castermans, T.11, Chirkin, D.12, Conrad, J.9
Source: Nuclear Physics B Proceedings Supplement. Apr2003, Vol. 118 Issue 1-3, p388. 8p.
Subjects: Neutrinos, Telescopes, Detectors, Galaxies, Astrophysics
Abstract: IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice Sheet near theSouth Pole. We present the conceptual design and the sensitivity of the IceCube detector to predicted fluxes of neutrinos, both atmospheric and extra-terrestrial. A complete simulation of the detector design has been used to study the detector''s capability to search for neutrinos from sources such as active galaxies, and gamma-ray bursts. [Copyright &y& Elsevier]
Copyright of Nuclear Physics B Proceedings Supplement is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: IceCube — the next generation neutrino telescope at the South Pole
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  Data: <searchLink fieldCode="AR" term="%22Karle%2C+A%2E%22">Karle, A.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Ahrens%2C+J%2E%22">Ahrens, J.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Bahcall%2C+J%2EN%2E%22">Bahcall, J.N.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Bai%2C+X%2E%22">Bai, X.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Becka%2C+T%2E%22">Becka, T.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Becker%2C+K%2E-H%2E%22">Becker, K.-H.</searchLink><relatesTo>4</relatesTo><br /><searchLink fieldCode="AR" term="%22Besson%2C+D%2EZ%2E%22">Besson, D.Z.</searchLink><relatesTo>5</relatesTo><br /><searchLink fieldCode="AR" term="%22Berley%2C+D%2E%22">Berley, D.</searchLink><relatesTo>6</relatesTo><br /><searchLink fieldCode="AR" term="%22Bernardini%2C+E%2E%22">Bernardini, E.</searchLink><relatesTo>7</relatesTo><br /><searchLink fieldCode="AR" term="%22Bertrand%2C+D%2E%22">Bertrand, D.</searchLink><relatesTo>8</relatesTo><br /><searchLink fieldCode="AR" term="%22Binon%2C+F%2E%22">Binon, F.</searchLink><relatesTo>8</relatesTo><br /><searchLink fieldCode="AR" term="%22Biron%2C+A%2E%22">Biron, A.</searchLink><relatesTo>7</relatesTo><br /><searchLink fieldCode="AR" term="%22Böser%2C+S%2E%22">Böser, S.</searchLink><relatesTo>7</relatesTo><br /><searchLink fieldCode="AR" term="%22Bohm%2C+C%2E%22">Bohm, C.</searchLink><br /><searchLink fieldCode="AR" term="%22Botner%2C+O%2E%22">Botner, O.</searchLink><relatesTo>9</relatesTo><br /><searchLink fieldCode="AR" term="%22Bouhali%2C+O%2E%22">Bouhali, O.</searchLink><relatesTo>8</relatesTo><br /><searchLink fieldCode="AR" term="%22Burgess%2C+Th%2E%22">Burgess, Th.</searchLink><relatesTo>10</relatesTo><br /><searchLink fieldCode="AR" term="%22Castermans%2C+T%2E%22">Castermans, T.</searchLink><relatesTo>11</relatesTo><br /><searchLink fieldCode="AR" term="%22Chirkin%2C+D%2E%22">Chirkin, D.</searchLink><relatesTo>12</relatesTo><br /><searchLink fieldCode="AR" term="%22Conrad%2C+J%2E%22">Conrad, J.</searchLink><relatesTo>9</relatesTo>
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  Data: <searchLink fieldCode="JN" term="%22Nuclear+Physics+B++Proceedings+Supplement%22">Nuclear Physics B Proceedings Supplement</searchLink>. Apr2003, Vol. 118 Issue 1-3, p388. 8p.
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  Data: IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice Sheet near theSouth Pole. We present the conceptual design and the sensitivity of the IceCube detector to predicted fluxes of neutrinos, both atmospheric and extra-terrestrial. A complete simulation of the detector design has been used to study the detector''s capability to search for neutrinos from sources such as active galaxies, and gamma-ray bursts. [Copyright &y& Elsevier]
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  Data: <i>Copyright of Nuclear Physics B Proceedings Supplement is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
PLink https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=egs&AN=11091368
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