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The AMANDA neutrino telescope

Andrés, E. C. (author)
Askebjer, P. (author)
Barwick, S. W. (author)
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Bay, R. C. (author)
Bergström, L. (author)
Biron, A. (author)
Booth, J. (author)
Botner, O. (author)
Bouchta, A. (author)
Carius, Staffan (author)
Högskolan i Kalmar,Naturvetenskapliga institutionen
Carlson, M. (author)
Chinowsky, W. (author)
Chirkin, D. (author)
Conrad, J. (author)
Costa, C. G. S. (author)
Cowen, D. (author)
Dalberg, E. (author)
DeYoung, T. (author)
Edsjö, J. (author)
Ekström, P. (author)
Goobar, A. (author)
Gray, L. (author)
Hallgren, A. (author)
Halzen, F. (author)
Hardtke, R. (author)
Hart, S. (author)
He, Y. (author)
De Los Heros, C. P. (author)
Hill, G. (author)
Hulth, P. O. (author)
Hundertmark, S. (author)
Jacobsen, J. (author)
Jones, A. (author)
Kandhadai, V. (author)
Karle, A. (author)
Kim, J. (author)
Leich, H. (author)
Leuthold, M. (author)
Lindahl, P. (author)
Högskolan i Kalmar,Naturvetenskapliga institutionen
Liubarsky, I. (author)
Loaiza, P. (author)
Lowder, D. (author)
Marciniewski, P. (author)
Miller, T. C. (author)
Miocinovic, P. (author)
Mock, P. C. (author)
Morse, R. (author)
Newcomer, M. (author)
Niessen, P. (author)
Nygren, D. (author)
Porrata, R. (author)
Potter, D. (author)
Price, P. B. (author)
Przybylski, G. (author)
Rhode, W. (author)
Richter, S. (author)
Rodriguez, J. (author)
Romenesko, P. (author)
Ross, D. (author)
Rubinstein, H. (author)
Schmidt, T. (author)
Schneider, E. (author)
Schwarz, R. (author)
Schwendicke, U. (author)
Smoot, G. (author)
Solarz, M. (author)
Sorin, V. (author)
Spiering, C. (author)
Steffen, P. (author)
Stokstad, R. (author)
Streicher, O. (author)
Taboada, I. (author)
Thon, T. (author)
Tilav, S. (author)
Walck, C. (author)
Wiebusch, C. H. (author)
Wischnewski, R. (author)
Woschnagg, K. (author)
Wu, W. (author)
Yodh, G. (author)
Young, S. (author)
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 (creator_code:org_t)
1999
1999
English.
In: Nuclear physics B, Proceedings supplements. - 0920-5632 .- 1873-3832. ; 77:1-3, s. 474-485
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • With an effective telescope area of order 104 m2 for TeV neutrinos, a threshold near ∼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 telescopes, reaching a scale envisaged over 25 years ago. We describe early results on the calibration of natural deep ice as a particle detector as well as on AMANDA's performance as a neutrino telescope.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Publication and Content Type

ref (subject category)
art (subject category)

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