WFRF:(Dalberg E.)
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The AMANDA neutrino telescope
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- Andres, EC (author)
- Uppsala universitet,Institutionen för kärn- och partikelfysik
- Askebjer, P (author)
- Barwick, SW (author)
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- Bay, RC (author)
- Bergstrom, L (author)
- Biron, A (author)
- Booth, J (author)
- Botner, O (author)
- Bouchta, A (author)
- Carius, S (author)
- Carlson, M (author)
- Chinowsky, W (author)
- Chirkin, D (author)
- Conrad, J (author)
- Costa, CGS (author)
- Cowen, D (author)
- Dalberg, E (author)
- DeYoung, T (author)
- Edsjo, J (author)
- Ekstrom, P (author)
- Goobar, A (author)
- Gray, L (author)
- Hallgren, A (author)
- Halzen, F (author)
- Har, (author)
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- (creator_code:org_t)
- ELSEVIER SCIENCE BV, 1999
- 1999
- English.
- In: NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS. - : ELSEVIER SCIENCE BV. - 0920-5632. ; 77, s. 474-485
- Journal article (other academic/artistic)
Abstract
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- With an effective telescope area of order 10(4) m(2) for TeV neutrinos, a threshold near similar to 50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescop
Publication and Content Type
- vet (subject category)
- art (subject category)
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- NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS (Search for host publication in LIBRIS)
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- Andres, EC
- Askebjer, P
- Barwick, SW
- Bay, RC
- Bergstrom, L
- Biron, A
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- Booth, J
- Botner, O
- Bouchta, A
- Carius, S
- Carlson, M
- Chinowsky, W
- Chirkin, D
- Conrad, J
- Costa, CGS
- Cowen, D
- Dalberg, E
- DeYoung, T
- Edsjo, J
- Ekstrom, P
- Goobar, A
- Gray, L
- Hallgren, A
- Halzen, F
- Har,
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- Uppsala University
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