Catalogo Articoli (Spogli Riviste)

OPAC HELP

Titolo:
Results from the AMANDA high energy neutrino detector
Autore:
Andres, E; Askebjer, P; Bai, X; Barouch, G; Barwick, SW; Bay, RC; Becker, KH; Bergstrom, L; Bertrand, D; Biron, A; Booth, J; Botner, O; Bouchta, A; Boyce, MM; Carius, S; Chirkin, D; Conrad, J; Costa, CGS; Cowen, DF; Dailing, J; Dalberg, E; DeYoung, T; Desiati, P; Dewulf, JP; Doksus, P; Edsjo, J; Ekstrom, P; Erlandsson, B; Feser, T; Gaug, M; Goldschmidt, A; Goobar, B; Haase, H; Hallgren, A; Halzen, F; Hanson, K; Hardtke, R; He, YD; Hellwig, M; Heukenkamp, H; Hill, GC; Hulth, PO; Hundertmark, S; Jacobsen, J; Karle, A; Kim, J; Koci, B; Kopke, L; Kowalski, M; Leich, H; Leuthold, M; Lindahl, P; Liubarsky, I; Loaiza, P; Lowder, DM; Ludvig, J; Madsen, J; Marciniewski, P; Matis, H; Mikolajski, T; Miller, TC; Minaeva, Y; Miocinovic, P; Mock, P; Morse, R; Neunhoffer, T; Newcomer, FM; Niessen, P; Nygren, DR; de los Heros, CP; Porrata, R; Price, PB; Rawlins, K; Reed, C; Rhode, W; Richards, A; Richter, S; Martino, JR; Romenesko, P; Ross, D; Rubinstein, H; Sander, HG; Scheider, T; Schmidt, T; Schneider, D; Schneider, E; Schwarz, R; Silvestri, A; Solarz, M; Spiczak, G; Spiering, C; Starinski, N; Steele, D; Steffen, P; Stokstad, RG; Streicher, O; Sun, Q; Taboada, I; Thollander, L; Thon, T; Tilav, S; Vander Donckt, M; Walck, C; Weinheimer, C; Wiebusch, CH; Wischnewski, R; Woschnagg, K; Wu, W; Yodh, G; Young, S;
Indirizzi:
Univ Wisconsin, Dept Phys, Madison, WI 53706 USA Univ Wisconsin Madison WI USA 53706 sin, Dept Phys, Madison, WI 53706 USA Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA Univ Delaware NewarkDE USA 19716 , Bartol Res Inst, Newark, DE 19716 USA DESY, D-15735 Zeuthen, Germany DESY Zeuthen Germany D-15735DESY, D-15735 Zeuthen, Germany Univ Kalmar, Dept Technol, S-39129 Kalmar, Sweden Univ Kalmar Kalmar Sweden S-39129 , Dept Technol, S-39129 Kalmar, Sweden Univ Stockholm, Dept Phys, S-11385 Stockholm, Sweden Univ Stockholm Stockholm Sweden S-11385 Phys, S-11385 Stockholm, Sweden Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA Univ Calif Berkeley Berkeley CA USA 94720 pt Phys, Berkeley, CA 94720 USA Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA Univ Calif Irvine Irvine CA USA 92697 Phys & Astron, Irvine, CA 92697 USA Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA Univ Penn Philadelphia PA USA 19104 & Astron, Philadelphia, PA 19104 USA Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA Univ Calif Berkeley Berkeley CA USA 94720 atl Lab, Berkeley, CA 94720 USA Free Univ Brussels, B-1050 Brussels, Belgium Free Univ Brussels BrusselsBelgium B-1050 els, B-1050 Brussels, Belgium Univ Uppsala, Dept Radiat Sci, S-75121 Uppsala, Sweden Univ Uppsala Uppsala Sweden S-75121 Radiat Sci, S-75121 Uppsala, Sweden Univ Mainz, Inst Phys, D-55099 Mainz, Germany Univ Mainz Mainz Germany D-55099 ainz, Inst Phys, D-55099 Mainz, Germany BUGH Wuppertal, Fachbereich Phys 8, D-42097 Wuppertal, Germany BUGH Wuppertal Wuppertal Germany D-42097 s 8, D-42097 Wuppertal, Germany
Titolo Testata:
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS
, volume: 91, anno: 2001,
pagine: 423 - 430
SICI:
0920-5632(200101)91:<423:RFTAHE>2.0.ZU;2-H
Fonte:
ISI
Lingua:
ENG
Soggetto:
ASTROPHYSICAL SOURCES;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
Citazioni:
29
Recensione:
Indirizzi per estratti:
Indirizzo: Andres, E Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA Univ Wisconsin 1150 Univ Ave Madison WI USA 53706 , WI 53706 USA
Citazione:
E. Andres et al., "Results from the AMANDA high energy neutrino detector", NUCL PH B-P, 91, 2001, pp. 423-430

Abstract

This paper briefly summarizes the search for astronomical sources of high-energy neutrinos using the AMANDA-B10 detector. The complete data set from 1997 was analyzed. Far E-mu > 10 TeV, the detector exceeds 10,000 m(2) in effective area between declinations of 25 and 90 degrees. Neutrinos generated in the atmosphere by cosmic ray interactions were used to verify the overall sensitivity of the detector. The absolute pointing accuracy and angularresolution has been confirmed by the analysis of coincident events betweenthe SPASE air shower array and the AMANDA detector. Preliminary flux limits from point source candidates are presented. For declinations larger than 45 degrees, our results compare favorably to existing limits for sources in the Southern sky. We also present the current status of the searches for high energy neutrino emission from diffusely distributed sources, GRBs, andWIMPs from the center of the earth.

ASDD Area Sistemi Dipartimentali e Documentali, Università di Bologna, Catalogo delle riviste ed altri periodici
Documento generato il 26/09/20 alle ore 05:37:03