Calibration and survey of AMANDA with the SPASE detectors

被引:14
作者
Ahrens, J
Bai, X
Barwick, SW
Bay, RC
Becka, T
Becker, KH
Bernardini, E
Bertrand, D
Binon, F
Biron, A
Böser, S
Botner, O
Bouchta, A
Bouhali, O
Burgess, T
Carius, S
Castermans, T
Chirkin, D
Conrad, J
Cooley, J
Cowen, DF
Davour, A
De Clercq, C
DeYoung, T
Desiati, P
Dewulf, JP
Dickinson, E
Doksus, P
Ekström, P
Engel, R
Evenson, P
Feser, T
Gaisser, TK [1 ]
Ganugapati, R
Gaug, M
Geenen, H
Gerhardt, L
Goldschmidt, A
Hallgren, A
Halzen, F
Hanson, K
Hardtke, R
Hauschildt, T
Hellwig, M
Herquet, P
Hill, GC
Hinton, JA
Hughey, B
Hulth, PO
Hultqvist, K
机构
[1] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA
[2] Johannes Gutenberg Univ Mainz, Inst Phys, D-55099 Mainz, Germany
[3] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA
[4] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[5] Berg Univ Wuppertal, Fachbereich Phys 8, D-42097 Wuppertal, Germany
[6] DESY Zeuthen, D-15735 Zeuthen, Germany
[7] Free Univ Brussels, Fac Sci, B-1050 Brussels, Belgium
[8] Uppsala Univ, Div High Energy Phys, S-75121 Uppsala, Sweden
[9] Univ Stockholm, Dept Phys, S-10691 Stockholm, Sweden
[10] Kalmar Univ, Dept Technol, S-39182 Kalmar, Sweden
[11] Univ Mons, B-7000 Mons, Belgium
[12] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[13] Penn State Univ, Dept Phys, University Pk, PA 16802 USA
[14] Free Univ Brussels, Dienst ELEM, B-1050 Brussels, Belgium
[15] Univ Leeds, Leeds LS2 9JT, W Yorkshire, England
[16] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA
[17] Univ London Imperial Coll Sci Technol & Med, London SW7 2AZ, England
[18] Univ Wisconsin, Dept Phys, River Falls, WI 54022 USA
[19] Univ Simon Bolivar, Dept Fis, Caracas 1080A, Venezuela
关键词
cosmic rays; neutrino telescopes;
D O I
10.1016/j.nima.2003.12.007
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We report on the analysis of air showers observed in coincidence by the Antarctic Muon and Neutrino detector array (AMANDA-B10) and the South Pole Air Shower Experiment (SPASE-1 and SPASE-2). We discuss the use of coincident events for calibration and survey of the deep AMANDA detector as well as the response of AMANDA to muon bundles. This analysis uses data taken during 1997 when both SPASE-1 and SPASE-2 were in operation to provide a stereo view of AMANDA. (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码:347 / 359
页数:13
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