Neutrino Astronomy at the South Pole: latest Results from AMANDA-II
AMANDA-II is the largest neutrino telescope collecting data at the moment, and its main goal is to search for sources of high energy extra-terrestrial neutrinos. The detection of such sources could give non-controversial evidence for the acceleration of charged hadrons in cosmic objects like Superno...
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ftcern:oai:cds.cern.ch:924474 2023-05-15T18:22:15+02:00 Neutrino Astronomy at the South Pole: latest Results from AMANDA-II Desiati, P 2006-01-25 http://cds.cern.ch/record/924474 eng eng http://cds.cern.ch/record/924474 astro-ph/0601571 oai:cds.cern.ch:924474 Astrophysics and Astronomy 2006 ftcern 2018-07-28T08:04:02Z AMANDA-II is the largest neutrino telescope collecting data at the moment, and its main goal is to search for sources of high energy extra-terrestrial neutrinos. The detection of such sources could give non-controversial evidence for the acceleration of charged hadrons in cosmic objects like Supernova Remnants, Micro-quasars, Active Galactic Nuclei or Gamma Ray Bursts. No significant excess has been found in searching for neutrinos from both point-like and non-localized sources. However AMANDA-II has significantly improved analysis techniques for better signal-to-noise optimization. The km$^3$-scale IceCube telescope will enlarge the observable energy range and improve the sensitivities of high energy neutrino searches due to its 30 times larger effective area. Other/Unknown Material South pole CERN Document Server (CDS) South Pole |
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CERN Document Server (CDS) |
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ftcern |
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English |
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Astrophysics and Astronomy |
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Astrophysics and Astronomy Desiati, P Neutrino Astronomy at the South Pole: latest Results from AMANDA-II |
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Astrophysics and Astronomy |
description |
AMANDA-II is the largest neutrino telescope collecting data at the moment, and its main goal is to search for sources of high energy extra-terrestrial neutrinos. The detection of such sources could give non-controversial evidence for the acceleration of charged hadrons in cosmic objects like Supernova Remnants, Micro-quasars, Active Galactic Nuclei or Gamma Ray Bursts. No significant excess has been found in searching for neutrinos from both point-like and non-localized sources. However AMANDA-II has significantly improved analysis techniques for better signal-to-noise optimization. The km$^3$-scale IceCube telescope will enlarge the observable energy range and improve the sensitivities of high energy neutrino searches due to its 30 times larger effective area. |
author |
Desiati, P |
author_facet |
Desiati, P |
author_sort |
Desiati, P |
title |
Neutrino Astronomy at the South Pole: latest Results from AMANDA-II |
title_short |
Neutrino Astronomy at the South Pole: latest Results from AMANDA-II |
title_full |
Neutrino Astronomy at the South Pole: latest Results from AMANDA-II |
title_fullStr |
Neutrino Astronomy at the South Pole: latest Results from AMANDA-II |
title_full_unstemmed |
Neutrino Astronomy at the South Pole: latest Results from AMANDA-II |
title_sort |
neutrino astronomy at the south pole: latest results from amanda-ii |
publishDate |
2006 |
url |
http://cds.cern.ch/record/924474 |
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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://cds.cern.ch/record/924474 astro-ph/0601571 oai:cds.cern.ch:924474 |
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1766201629432872960 |