Neutrino Astronomy at the South Pole: Status of the AMANDA Experiment

AMANDA (Antarctic Muon And Neutrino Detector Array) is a neutrino telescope built under the southern polar icecap, and its scope is exploring the possibility to detect high energy cosmic neutrinos generated by powerful celestial objects where acceleration mechanisms can bring protons up to 10^20 eV....

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Bibliographic Details
Main Authors: Desiati, P, Collaboration, FTAMANDA, Bland, FK
Format: Article in Journal/Newspaper
Language:unknown
Published: 2003
Subjects:
Online Access:http://discovery.ucl.ac.uk/1375091/
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spelling ftucl:oai:eprints.ucl.ac.uk.OAI2:1375091 2023-05-15T14:02:04+02:00 Neutrino Astronomy at the South Pole: Status of the AMANDA Experiment Desiati, P Collaboration, FTAMANDA Bland, FK 2003-06-25 http://discovery.ucl.ac.uk/1375091/ unknown (2003) astro-ph Article 2003 ftucl 2015-02-12T23:20:24Z AMANDA (Antarctic Muon And Neutrino Detector Array) is a neutrino telescope built under the southern polar icecap, and its scope is exploring the possibility to detect high energy cosmic neutrinos generated by powerful celestial objects where acceleration mechanisms can bring protons up to 10^20 eV. We describe the achievements and results from the AMANDA-B10 prototype and the preliminary results from the current AMANDA-II detector showing a dramatic increase in sensitivity. An outlook on IceCube will be given. Article in Journal/Newspaper Antarc* Antarctic South pole South pole University College London: UCL Discovery Antarctic South Pole
institution Open Polar
collection University College London: UCL Discovery
op_collection_id ftucl
language unknown
topic astro-ph
spellingShingle astro-ph
Desiati, P
Collaboration, FTAMANDA
Bland, FK
Neutrino Astronomy at the South Pole: Status of the AMANDA Experiment
topic_facet astro-ph
description AMANDA (Antarctic Muon And Neutrino Detector Array) is a neutrino telescope built under the southern polar icecap, and its scope is exploring the possibility to detect high energy cosmic neutrinos generated by powerful celestial objects where acceleration mechanisms can bring protons up to 10^20 eV. We describe the achievements and results from the AMANDA-B10 prototype and the preliminary results from the current AMANDA-II detector showing a dramatic increase in sensitivity. An outlook on IceCube will be given.
format Article in Journal/Newspaper
author Desiati, P
Collaboration, FTAMANDA
Bland, FK
author_facet Desiati, P
Collaboration, FTAMANDA
Bland, FK
author_sort Desiati, P
title Neutrino Astronomy at the South Pole: Status of the AMANDA Experiment
title_short Neutrino Astronomy at the South Pole: Status of the AMANDA Experiment
title_full Neutrino Astronomy at the South Pole: Status of the AMANDA Experiment
title_fullStr Neutrino Astronomy at the South Pole: Status of the AMANDA Experiment
title_full_unstemmed Neutrino Astronomy at the South Pole: Status of the AMANDA Experiment
title_sort neutrino astronomy at the south pole: status of the amanda experiment
publishDate 2003
url http://discovery.ucl.ac.uk/1375091/
geographic Antarctic
South Pole
geographic_facet Antarctic
South Pole
genre Antarc*
Antarctic
South pole
South pole
genre_facet Antarc*
Antarctic
South pole
South pole
op_source (2003)
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