Getting there: from AMANDA to IceCube
AMANDA is a neutrino telescope consisting of 677 optical modules embedded at 1.5-2 km depth in the ice cap under the Amundsen-Scott South Pole station. In this contribution we summarize AMANDA results on measuring the atmospheric neutrino spectrum, on searches for a neutrino flux from the galactic p...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.222.2234 2023-05-15T13:24:24+02:00 Getting there: from AMANDA to IceCube Carlos P. De Los Heros The Pennsylvania State University CiteSeerX Archives 2005 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.222.2234 http://pos.sissa.it/archive/conferences/021/023/HEP2005_023.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.222.2234 http://pos.sissa.it/archive/conferences/021/023/HEP2005_023.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://pos.sissa.it/archive/conferences/021/023/HEP2005_023.pdf text 2005 ftciteseerx 2016-01-07T18:22:09Z AMANDA is a neutrino telescope consisting of 677 optical modules embedded at 1.5-2 km depth in the ice cap under the Amundsen-Scott South Pole station. In this contribution we summarize AMANDA results on measuring the atmospheric neutrino spectrum, on searches for a neutrino flux from the galactic plane, for a diffuse and point-like flux of cosmic high energy neutrinos and searches for dark matter candidates in the form of MSSM neutralinos. 90%CL limits are presented for these searches, as well as for a list of specific point source candidates. The status and physics capabilities of IceCube, the successor of AMANDA, are also summarized. Text Amundsen-Scott Ice cap South pole Unknown South Pole Amundsen-Scott ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen Scott South Pole Station ENVELOPE(0.000,0.000,-90.000,-90.000) Amundsen-Scott South Pole Station ENVELOPE(139.273,139.273,-89.998,-89.998) |
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ftciteseerx |
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English |
description |
AMANDA is a neutrino telescope consisting of 677 optical modules embedded at 1.5-2 km depth in the ice cap under the Amundsen-Scott South Pole station. In this contribution we summarize AMANDA results on measuring the atmospheric neutrino spectrum, on searches for a neutrino flux from the galactic plane, for a diffuse and point-like flux of cosmic high energy neutrinos and searches for dark matter candidates in the form of MSSM neutralinos. 90%CL limits are presented for these searches, as well as for a list of specific point source candidates. The status and physics capabilities of IceCube, the successor of AMANDA, are also summarized. |
author2 |
The Pennsylvania State University CiteSeerX Archives |
format |
Text |
author |
Carlos P. De Los Heros |
spellingShingle |
Carlos P. De Los Heros Getting there: from AMANDA to IceCube |
author_facet |
Carlos P. De Los Heros |
author_sort |
Carlos P. De Los Heros |
title |
Getting there: from AMANDA to IceCube |
title_short |
Getting there: from AMANDA to IceCube |
title_full |
Getting there: from AMANDA to IceCube |
title_fullStr |
Getting there: from AMANDA to IceCube |
title_full_unstemmed |
Getting there: from AMANDA to IceCube |
title_sort |
getting there: from amanda to icecube |
publishDate |
2005 |
url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.222.2234 http://pos.sissa.it/archive/conferences/021/023/HEP2005_023.pdf |
long_lat |
ENVELOPE(0.000,0.000,-90.000,-90.000) ENVELOPE(0.000,0.000,-90.000,-90.000) ENVELOPE(139.273,139.273,-89.998,-89.998) |
geographic |
South Pole Amundsen-Scott Amundsen Scott South Pole Station Amundsen-Scott South Pole Station |
geographic_facet |
South Pole Amundsen-Scott Amundsen Scott South Pole Station Amundsen-Scott South Pole Station |
genre |
Amundsen-Scott Ice cap South pole |
genre_facet |
Amundsen-Scott Ice cap South pole |
op_source |
http://pos.sissa.it/archive/conferences/021/023/HEP2005_023.pdf |
op_relation |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.222.2234 http://pos.sissa.it/archive/conferences/021/023/HEP2005_023.pdf |
op_rights |
Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766379532406751232 |