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Results from the AMANDA neutrino telescope

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Title: Results from the AMANDA neutrino telescope
Authors: de los Heros, C.1, Ackermann, M.2, Ahrens, J.3, Albrecht, H.2, Bai, X.4, Bay, R.5, Bartelt, M.6, Barwick, S.W.7, Becka, T.3, Becker, K.-H., Becker, J.-K., Bernardini, E.2, Bertrand, D.8, Boersma, D.J.2, Böser, S.2, Botner, O.1, Bouchta, A.1, Bouhali, O.8, Braun, J.9, Burgess, C.10
Source: Nuclear Physics B Proceedings Supplement. Nov2004, Vol. 136 Issue 1-3, p85-92. 8p.
Subjects: Neutrinos, Telescopes, Leptons (Nuclear physics), Astronomical instruments
Abstract: We review recent results from AMANDA on the search for cosmic point sources of neutrinos, both in the diffuse and point-like channels. Assuming a E−2 spectral shape of the neutrino energy at the source, we derive limits on the diffuse ν μ flux as well as in the all-flavour diffuse flux from the cascade search. We report limits on selected point sources as well as on GRB searches. We present results on primary cosmic CR composition in the range ∼100 TeV-PeV obtained with the help of the SPASE air shower array run in coincidence with AMANDA. [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.)
Database: Engineering Source
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DbLabel: Engineering Source
An: 17114970
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PubType: Periodical
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  Data: Results from the AMANDA neutrino telescope
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  Data: <searchLink fieldCode="AR" term="%22de+los+Heros%2C+C%2E%22">de los Heros, C.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Ackermann%2C+M%2E%22">Ackermann, M.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Ahrens%2C+J%2E%22">Ahrens, J.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Albrecht%2C+H%2E%22">Albrecht, H.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Bai%2C+X%2E%22">Bai, X.</searchLink><relatesTo>4</relatesTo><br /><searchLink fieldCode="AR" term="%22Bay%2C+R%2E%22">Bay, R.</searchLink><relatesTo>5</relatesTo><br /><searchLink fieldCode="AR" term="%22Bartelt%2C+M%2E%22">Bartelt, M.</searchLink><relatesTo>6</relatesTo><br /><searchLink fieldCode="AR" term="%22Barwick%2C+S%2EW%2E%22">Barwick, S.W.</searchLink><relatesTo>7</relatesTo><br /><searchLink fieldCode="AR" term="%22Becka%2C+T%2E%22">Becka, T.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Becker%2C+K%2E-H%2E%22">Becker, K.-H.</searchLink><br /><searchLink fieldCode="AR" term="%22Becker%2C+J%2E-K%2E%22">Becker, J.-K.</searchLink><br /><searchLink fieldCode="AR" term="%22Bernardini%2C+E%2E%22">Bernardini, E.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Bertrand%2C+D%2E%22">Bertrand, D.</searchLink><relatesTo>8</relatesTo><br /><searchLink fieldCode="AR" term="%22Boersma%2C+D%2EJ%2E%22">Boersma, D.J.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Böser%2C+S%2E%22">Böser, S.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Botner%2C+O%2E%22">Botner, O.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Bouchta%2C+A%2E%22">Bouchta, A.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Bouhali%2C+O%2E%22">Bouhali, O.</searchLink><relatesTo>8</relatesTo><br /><searchLink fieldCode="AR" term="%22Braun%2C+J%2E%22">Braun, J.</searchLink><relatesTo>9</relatesTo><br /><searchLink fieldCode="AR" term="%22Burgess%2C+C%2E%22">Burgess, C.</searchLink><relatesTo>10</relatesTo>
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  Data: <searchLink fieldCode="JN" term="%22Nuclear+Physics+B++Proceedings+Supplement%22">Nuclear Physics B Proceedings Supplement</searchLink>. Nov2004, Vol. 136 Issue 1-3, p85-92. 8p.
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  Data: <searchLink fieldCode="DE" term="%22Neutrinos%22">Neutrinos</searchLink><br /><searchLink fieldCode="DE" term="%22Telescopes%22">Telescopes</searchLink><br /><searchLink fieldCode="DE" term="%22Leptons+%28Nuclear+physics%29%22">Leptons (Nuclear physics)</searchLink><br /><searchLink fieldCode="DE" term="%22Astronomical+instruments%22">Astronomical instruments</searchLink>
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  Data: We review recent results from AMANDA on the search for cosmic point sources of neutrinos, both in the diffuse and point-like channels. Assuming a E−2 spectral shape of the neutrino energy at the source, we derive limits on the diffuse ν μ flux as well as in the all-flavour diffuse flux from the cascade search. We report limits on selected point sources as well as on GRB searches. We present results on primary cosmic CR composition in the range ∼100 TeV-PeV obtained with the help of the SPASE air shower array run in coincidence with AMANDA. [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=17114970
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