RECENT RESULTS FROM AMANDA

RECENT RESULTS FROM AMANDA

Presented by D. F. Cowen for the AMANDA Collaboration,E. Andrés,P. Askebjer,X. Bai,G. Barouch,S. W. Barwick,R. C. Bay,K.-H. Becker,L. Bergström,D. Bertrand,D. Bierenbaum,A. Biron,J. Booth,O. Botner,A. Bouchta,M. M. Boyce,S. Carius,A. Chen,D. Chirkin,J. Conrad,J. Cooley,C. G. S. Costa,D. F. Cowen,J. Dailing,E. Dalberg,Tyce DeYoung,P. Desiati,J.-P. Dewulf,P. Doksus,J. Edsjö,P. Ekström,B. Erlandsson,T. Feser,Markus Gaug,A. Goldschmidt,A. Goobar,L. Gray,H. Haase,A. Hallgren,F. Halzen,K. Hanson,R. Hardtke,Y. D. He,M. Hellwig,H. Heukenkamp,Gary Hill,P. O. Hulth,S. Hundertmark,J. Jacobsen,V. Kandhadai,A. Karle,J. Kim,B. Koci,L. Köpke,Marek Kowalski,H. Leich,M. Leuthold,P. Lindahl,I. Liubarsky,Pia Loaiza,D. M. Lowder,J. Ludvig,J. Madsen,P. Marciniewski,H. S. Matis,A. Mihalyi,T. Mikolajski,T. C. Miller,Y. Minaeva,P. Miočinović,P. C. Mock,R. Morse,T. Neunhöffer,F. M. Newcomer,P. Niessen,D. R. Nygren,H. Ogelman,Carlos Pérez De Los Heros,R. Porrata,P. B. Price,K. Rawlins,C. Reed,W. Rhode,A. Richards,S. Richter,J. Rodríguez Martino,P. Romenesko,D. Ross,H. Rubinstein,H.-G. Sander,T. Scheider,T. Schmidt,D. Schneider,R. Schwarz,A. Silvestri,M. Solarz,G. M. Spiczak,C. Spiering,N. Starinsky,D. Steele,P. Steffen,R. G. Stokstad,Ole Streicher,Q. Sun,I. Taboada,L. Thollander,T. Thon,S. Tilav,N. Usechak,M. Vander Donckt,C. Walck,C. Weinheimer,C. H. Wiebusch,R. Wischnewski,H. Wissing,K. Woschnagg,W. Wu,G. Yodh,S. Young;Presented by D. F. Cowen for the AMANDA Collaboration;E. Andrés;P. Askebjer;X. Bai;G. Barouch;S. W. Barwick;R. C. Bay;K.-H. Becker;L. Bergström;D. Bertrand;D. Bierenbaum;A. Biron;J. Booth;O. Botner;A. Bouchta;M. M. Boyce;S. Carius;A. Chen;D. Chirkin;J. Conrad;J. Cooley;C. G. S. Costa;D. F. Cowen;J. Dailing;E. Dalberg;Tyce DeYoung;P. Desiati;J.-P. Dewulf;P. Doksus;J. Edsjö;P. Ekström;B. Erlandsson;T. Feser;Markus Gaug;A. Goldschmidt;A. Goobar;L. Gray;H. Haase;A. Hallgren;F. Halzen;K. Hanson;R. Hardtke;Y. D. He;M. Hellwig;H. Heukenkamp;Gary Hill;P. O. Hulth;S. Hundertmark;J. Jacobsen;V. Kandhadai;A. Karle;J. Kim;B. Koci;L. Köpke;Marek Kowalski;H. Leich;M. Leuthold;P. Lindahl;I. Liubarsky;Pia Loaiza;D. M. Lowder;J. Ludvig;J. Madsen;P. Marciniewski;H. S. Matis;A. Mihalyi;T. Mikolajski;T. C. Miller;Y. Minaeva;P. Miočinović;P. C. Mock;R. Morse;T. Neunhöffer;F. M. Newcomer;P. Niessen;D. R. Nygren;H. Ogelman;Carlos Pérez De Los Heros;R. Porrata;P. B. Price;K. Rawlins;C. Reed;W. Rhode;A. Richards;S. Richter;J. Rodríguez Martino;P. Romenesko;D. Ross;H. Rubinstein;H.-G. Sander;T. Scheider;T. Schmidt;D. Schneider;R. Schwarz;A. Silvestri;M. Solarz;G. M. Spiczak;C. Spiering;N. Starinsky;D. Steele;P. Steffen;R. G. Stokstad;Ole Streicher;Q. Sun;I. Taboada;L. Thollander;T. Thon;S. Tilav;N. Usechak;M. Vander Donckt;C. Walck;C. Weinheimer;C. H. Wiebusch;R. Wischnewski;H. Wissing;K. Woschnagg;W. Wu;G. Yodh;S. Young;
international journal of modern physics a 2001 Vol. 16 pp. 1013-1015
134
young2001internationalrecent

Abstract

We present results based on data taken in 1997 with the 302-PMT Antarctic Muon and Neutrino Detector Array-B10 ("AMANDA-B10") array. Atmospheric neutrinos created in the northern hemisphere are observed indirectly through their charged current interactions which produce relativistic, Cherenkov-light-emitting upgoing muons in the South Pole ice cap. The reconstructed angular distribution of these events is in good agreement with expectation and demonstrates the viability of this ice-based device as a neutrino telescope.

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