Results from the AMANDA detector

M. Ackermann; J. Ahrens; H. Albrecht; X. Bai; R. Bay; M. Bartelt; S. W. Barwick; T. Becka; K. H. Becker; J. K. Becker; E. Bernardini; D. Bertrand; D. J. Boersma; S. Böser; O. Botner; A. Bouchta; O. Bouhali; J. Braun; C. Burgess; T. Burgess; T. Castermans; D. Chirkin; B. Collin; J. Conrad; J. Cooley; D. F. Cowen; A. Davour; C. De Clercq; T. DeYoung; P. Desiati; P. Ekström; T. Feser; T. K. Gaisser; R. Ganugapati; H. Geenen; L. Gerhardt; A. Goldschmidt; A. Gross; A. Halloren; F. Halzen; K. Hanson; R. Hardtke; T. Harenberg; T. Hauschildt; K. Helbing; M. Hellwig; P. Herquet; G. C. Hill; J. Hodges; D. Hubert; B. Hughey; P. O. Hulth; K. Hultqvist; S. Hundertmark; J. Jacobsen; K. H. Kampert; A. Karle; J. Kelley; M. Kestel; L. Köpke; M. Kowalski; M. Krasberg; K. Kuehn; H. Leich; M. Leuthold; I. Liubarsky; J. Madsen; K. Mandli; P. Marciniewski; H. S. Matis; C. P. McParland; T. Messarius; Y. Minaeva; P. Miocinović; R. Morse; K. Münich; R. Nahnhauer; J. W. Nam; T. Neunhöffer; P. Niessen; D. R. Nyoren; H. Ögelman; Ph Olbrechts; C. Pérez De Los Heros; A. C. Pohl; R. Porrata; P. B. Price; G. T. Przybylski; K. Rawlins; E. Resconi; W. Rhode; M. Ribordy; S. Richter; J. Rodríquez Martino; H. G. Sander; K. Schinarakis; S. Schlenstedt; D. Schneider; R. Schwarz

Results from the AMANDA detector

M. Ackermann^*
, J. Ahrens
, H. Albrecht
, X. Bai
, R. Bay
, M. Bartelt
, S. W. Barwick
, T. Becka
, K. H. Becker
, J. K. Becker
, E. Bernardini
, D. Bertrand
, D. J. Boersma
, S. Böser
, O. Botner
, A. Bouchta
, O. Bouhali
, J. Braun
, C. Burgess
, T. Burgess

T. Castermans, D. Chirkin, B. Collin, J. Conrad, J. Cooley, D. F. Cowen, A. Davour, C. De Clercq, T. DeYoung, P. Desiati, P. Ekström, T. Feser, T. K. Gaisser, R. Ganugapati, H. Geenen, L. Gerhardt, A. Goldschmidt, A. Gross, A. Halloren, F. Halzen, K. Hanson, R. Hardtke, T. Harenberg, T. Hauschildt, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, J. Hodges, D. Hubert, B. Hughey, P. O. Hulth, K. Hultqvist, S. Hundertmark, J. Jacobsen, K. H. Kampert, A. Karle, J. Kelley, M. Kestel, L. Köpke, M. Kowalski, M. Krasberg, K. Kuehn, H. Leich, M. Leuthold, I. Liubarsky, J. Madsen, K. Mandli, P. Marciniewski, H. S. Matis, C. P. McParland, T. Messarius, Y. Minaeva, P. Miocinović, R. Morse, K. Münich, R. Nahnhauer, J. W. Nam, T. Neunhöffer, P. Niessen, D. R. Nyoren, H. Ögelman, Ph Olbrechts, C. Pérez De Los Heros, A. C. Pohl, R. Porrata, P. B. Price, G. T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, J. Rodríquez Martino, H. G. Sander, K. Schinarakis, S. Schlenstedt, D. Schneider, R. Schwarz

^*Corresponding author for this work

German Electron Synchrotron
Johannes Gutenberg University Mainz
University of Delaware
University of California at Berkeley
University of Wuppertal
University of California at Irvine
Université libre de Bruxelles
Uppsala University
University of Wisconsin-Madison
Stockholm University
Universite de Mons
Pennsylvania State University
University of Maryland, College Park
Lawrence Berkeley National Laboratory
Vrije Universiteit Brussel
Imperial College London
University of Wisconsin-River Falls
Linnaeus University

Research output: Contribution to journal › Article › peer-review

Abstract

The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope based at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice, which is used as interaction and detection medium. The primary goal of this detector is the observation of astronomical sources of high-energy neutrinos. This paper shows the latest results of the search for a diffuse flux of extraterrestrial ν_μs with energies between 10¹¹ eV and 10 ¹⁸ eV, ν_μs emitted from point sources and ν_μs from dark matter annihilation in the Earth and the Sun.

Original language	English
Pages (from-to)	1919-1931
Number of pages	13
Journal	Acta Physica Polonica B
Volume	35
Issue number	6-7
Publication status	Published - Jun 2004
Externally published	Yes

Cite this

@article{fbac09936bda4c61a3809a5be35277c3,

title = "Results from the AMANDA detector",

abstract = "The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope based at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice, which is used as interaction and detection medium. The primary goal of this detector is the observation of astronomical sources of high-energy neutrinos. This paper shows the latest results of the search for a diffuse flux of extraterrestrial νμs with energies between 1011 eV and 10 18 eV, νμs emitted from point sources and νμs from dark matter annihilation in the Earth and the Sun.",

author = "M. Ackermann and J. Ahrens and H. Albrecht and X. Bai and R. Bay and M. Bartelt and Barwick, \{S. W.\} and T. Becka and Becker, \{K. H.\} and Becker, \{J. K.\} and E. Bernardini and D. Bertrand and Boersma, \{D. J.\} and S. B{\"o}ser and O. Botner and A. Bouchta and O. Bouhali and J. Braun and C. Burgess and T. Burgess and T. Castermans and D. Chirkin and B. Collin and J. Conrad and J. Cooley and Cowen, \{D. F.\} and A. Davour and \{De Clercq\}, C. and T. DeYoung and P. Desiati and P. Ekstr{\"o}m and T. Feser and Gaisser, \{T. K.\} and R. Ganugapati and H. Geenen and L. Gerhardt and A. Goldschmidt and A. Gross and A. Halloren and F. Halzen and K. Hanson and R. Hardtke and T. Harenberg and T. Hauschildt and K. Helbing and M. Hellwig and P. Herquet and Hill, \{G. C.\} and J. Hodges and D. Hubert and B. Hughey and Hulth, \{P. O.\} and K. Hultqvist and S. Hundertmark and J. Jacobsen and Kampert, \{K. H.\} and A. Karle and J. Kelley and M. Kestel and L. K{\"o}pke and M. Kowalski and M. Krasberg and K. Kuehn and H. Leich and M. Leuthold and I. Liubarsky and J. Madsen and K. Mandli and P. Marciniewski and Matis, \{H. S.\} and McParland, \{C. P.\} and T. Messarius and Y. Minaeva and P. Miocinovi{\'c} and R. Morse and K. M{\"u}nich and R. Nahnhauer and Nam, \{J. W.\} and T. Neunh{\"o}ffer and P. Niessen and Nyoren, \{D. R.\} and H. {\"O}gelman and Ph Olbrechts and \{P{\'e}rez De Los Heros\}, C. and Pohl, \{A. C.\} and R. Porrata and Price, \{P. B.\} and Przybylski, \{G. T.\} and K. Rawlins and E. Resconi and W. Rhode and M. Ribordy and S. Richter and Martino, \{J. Rodr{\'i}quez\} and Sander, \{H. G.\} and K. Schinarakis and S. Schlenstedt and D. Schneider and R. Schwarz",

year = "2004",

month = jun,

language = "English",

volume = "35",

pages = "1919--1931",

journal = "Acta Physica Polonica B",

issn = "0587-4254",

publisher = "Jagiellonian University",

number = "6-7",

}

Ackermann, M, Ahrens, J, Albrecht, H, Bai, X, Bay, R, Bartelt, M, Barwick, SW, Becka, T, Becker, KH, Becker, JK, Bernardini, E, Bertrand, D, Boersma, DJ, Böser, S, Botner, O, Bouchta, A, Bouhali, O, Braun, J, Burgess, C, Burgess, T, Castermans, T, Chirkin, D, Collin, B, Conrad, J, Cooley, J, Cowen, DF, Davour, A, De Clercq, C, DeYoung, T, Desiati, P, Ekström, P, Feser, T, Gaisser, TK, Ganugapati, R, Geenen, H, Gerhardt, L, Goldschmidt, A, Gross, A, Halloren, A, Halzen, F, Hanson, K, Hardtke, R, Harenberg, T, Hauschildt, T, Helbing, K, Hellwig, M, Herquet, P, Hill, GC, Hodges, J, Hubert, D, Hughey, B, Hulth, PO, Hultqvist, K, Hundertmark, S, Jacobsen, J, Kampert, KH, Karle, A, Kelley, J, Kestel, M, Köpke, L, Kowalski, M, Krasberg, M, Kuehn, K, Leich, H, Leuthold, M, Liubarsky, I, Madsen, J, Mandli, K, Marciniewski, P, Matis, HS, McParland, CP, Messarius, T, Minaeva, Y, Miocinović, P, Morse, R, Münich, K, Nahnhauer, R, Nam, JW, Neunhöffer, T, Niessen, P, Nyoren, DR, Ögelman, H, Olbrechts, P, Pérez De Los Heros, C, Pohl, AC, Porrata, R, Price, PB, Przybylski, GT, Rawlins, K, Resconi, E, Rhode, W, Ribordy, M, Richter, S, Martino, JR, Sander, HG, Schinarakis, K, Schlenstedt, S, Schneider, D & Schwarz, R 2004, 'Results from the AMANDA detector', Acta Physica Polonica B, vol. 35, no. 6-7, pp. 1919-1931.

TY - JOUR

T1 - Results from the AMANDA detector

AU - Ackermann, M.

AU - Ahrens, J.

AU - Albrecht, H.

AU - Bai, X.

AU - Bay, R.

AU - Bartelt, M.

AU - Barwick, S. W.

AU - Becka, T.

AU - Becker, K. H.

AU - Becker, J. K.

AU - Bernardini, E.

AU - Bertrand, D.

AU - Boersma, D. J.

AU - Böser, S.

AU - Botner, O.

AU - Bouchta, A.

AU - Bouhali, O.

AU - Braun, J.

AU - Burgess, C.

AU - Burgess, T.

AU - Castermans, T.

AU - Chirkin, D.

AU - Collin, B.

AU - Conrad, J.

AU - Cooley, J.

AU - Cowen, D. F.

AU - Davour, A.

AU - De Clercq, C.

AU - DeYoung, T.

AU - Desiati, P.

AU - Ekström, P.

AU - Feser, T.

AU - Gaisser, T. K.

AU - Ganugapati, R.

AU - Geenen, H.

AU - Gerhardt, L.

AU - Goldschmidt, A.

AU - Gross, A.

AU - Halloren, A.

AU - Halzen, F.

AU - Hanson, K.

AU - Hardtke, R.

AU - Harenberg, T.

AU - Hauschildt, T.

AU - Helbing, K.

AU - Hellwig, M.

AU - Herquet, P.

AU - Hill, G. C.

AU - Hodges, J.

AU - Hubert, D.

AU - Hughey, B.

AU - Hulth, P. O.

AU - Hultqvist, K.

AU - Hundertmark, S.

AU - Jacobsen, J.

AU - Kampert, K. H.

AU - Karle, A.

AU - Kelley, J.

AU - Kestel, M.

AU - Köpke, L.

AU - Kowalski, M.

AU - Krasberg, M.

AU - Kuehn, K.

AU - Leich, H.

AU - Leuthold, M.

AU - Liubarsky, I.

AU - Madsen, J.

AU - Mandli, K.

AU - Marciniewski, P.

AU - Matis, H. S.

AU - McParland, C. P.

AU - Messarius, T.

AU - Minaeva, Y.

AU - Miocinović, P.

AU - Morse, R.

AU - Münich, K.

AU - Nahnhauer, R.

AU - Nam, J. W.

AU - Neunhöffer, T.

AU - Niessen, P.

AU - Nyoren, D. R.

AU - Ögelman, H.

AU - Olbrechts, Ph

AU - Pérez De Los Heros, C.

AU - Pohl, A. C.

AU - Porrata, R.

AU - Price, P. B.

AU - Przybylski, G. T.

AU - Rawlins, K.

AU - Resconi, E.

AU - Rhode, W.

AU - Ribordy, M.

AU - Richter, S.

AU - Martino, J. Rodríquez

AU - Sander, H. G.

AU - Schinarakis, K.

AU - Schlenstedt, S.

AU - Schneider, D.

AU - Schwarz, R.

PY - 2004/6

Y1 - 2004/6

N2 - The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope based at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice, which is used as interaction and detection medium. The primary goal of this detector is the observation of astronomical sources of high-energy neutrinos. This paper shows the latest results of the search for a diffuse flux of extraterrestrial νμs with energies between 1011 eV and 10 18 eV, νμs emitted from point sources and νμs from dark matter annihilation in the Earth and the Sun.

AB - The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope based at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice, which is used as interaction and detection medium. The primary goal of this detector is the observation of astronomical sources of high-energy neutrinos. This paper shows the latest results of the search for a diffuse flux of extraterrestrial νμs with energies between 1011 eV and 10 18 eV, νμs emitted from point sources and νμs from dark matter annihilation in the Earth and the Sun.

UR - https://www.scopus.com/pages/publications/3042821993

M3 - Article

AN - SCOPUS:3042821993

SN - 0587-4254

VL - 35

SP - 1919

EP - 1931

JO - Acta Physica Polonica B

JF - Acta Physica Polonica B

IS - 6-7

ER -

Results from the AMANDA detector

Abstract

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