Muon track reconstruction and data selection techniques in AMANDA

J. Ahrens; X. Bai; R. Bay; S. W. Barwick; T. Becka; J. K. Becker; K. H. Becker; E. Bernardini; D. Bertrand; A. Biron; D. J. Boersma; S. Böser; O. Botner; A. Bouchta; O. Bouhali; T. Burgess; S. Carius; T. Castermans; D. Chirkin; B. Collin; J. Conrad; J. Cooley; D. F. Cowen; A. Davour; C. De Clercq; T. DeYoung; P. Desiati; J. P. Dewulf; P. Ekström; T. Feser; M. Gaug; T. K. Gaisser; R. Ganugapati; H. Geenen; L. Gerhardt; A. Groß; A. Goldschmidt; A. Hallgren; F. Halzen; K. Hanson; R. Hardtke; T. Harenberg; T. Hauschildt; K. Helbing; M. Hellwig; P. Herquet; G. C. Hill; D. Hubert; B. Hughey; P. O. Hulth; K. Hultqvist; S. Hundertmark; J. Jacobsen; A. Karle; M. Kestel; L. Köpke; M. Kowalski; K. Kuehn; J. I. Lamoureux; H. Leich; M. Leuthold; P. Lindahl; I. Liubarsky; J. Madsen; P. Marciniewski; H. S. Matis; C. P. McParland; T. Messarius; Y. Minaeva; P. Miočinović; P. C. Mock; R. Morse; K. S. Münich; J. Nam; R. Nahnhauer; T. Neunhöffer; P. Niessen; D. R. Nygren; 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. Rodríguez Martino; D. Ross; H. G. Sander; K. Schinarakis; S. Schlenstedt; T. Schmidt; D. Schneider; C. H. Wiebusch

doi:10.1016/j.nima.2004.01.065

Muon track reconstruction and data selection techniques in AMANDA

J. Ahrens, X. Bai, R. Bay, S. W. Barwick, T. Becka, J. K. Becker, K. H. Becker, E. Bernardini, D. Bertrand, A. Biron, D. J. Boersma, S. Böser, O. Botner, A. Bouchta, O. Bouhali, T. Burgess, S. Carius, T. Castermans, D. Chirkin, B. CollinJ. Conrad, J. Cooley, D. F. Cowen, A. Davour, C. De Clercq, T. DeYoung, P. Desiati, J. P. Dewulf, P. Ekström, T. Feser, M. Gaug, T. K. Gaisser, R. Ganugapati, H. Geenen, L. Gerhardt, A. Groß, A. Goldschmidt, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Harenberg, T. Hauschildt, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, D. Hubert, B. Hughey, P. O. Hulth, K. Hultqvist, S. Hundertmark, J. Jacobsen, A. Karle, M. Kestel, L. Köpke, M. Kowalski, K. Kuehn, J. I. Lamoureux, H. Leich, M. Leuthold, P. Lindahl, I. Liubarsky, J. Madsen, P. Marciniewski, H. S. Matis, C. P. McParland, T. Messarius, Y. Minaeva, P. Miočinović, P. C. Mock, R. Morse, K. S. Münich, J. Nam, R. Nahnhauer, T. Neunhöffer, P. Niessen, D. R. Nygren, 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. Rodríguez Martino, D. Ross, H. G. Sander, K. Schinarakis, S. Schlenstedt, T. Schmidt, D. Schneider, C. H. Wiebusch

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

241 Scopus citations

Abstract

The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice between 1500 and 2000 m. The primary goal of this detector is to discover astrophysical sources of high-energy neutrinos. A high-energy muon neutrino coming through the earth from the Northern Hemisphere can be identified by the secondary muon moving upward through the detector. The muon tracks are reconstructed with a maximum likelihood method. It models the arrival times and amplitudes of Cherenkov photons registered by the photo-multipliers. This paper describes the different methods of reconstruction, which have been successfully implemented within AMANDA. Strategies for optimizing the reconstruction performance and rejecting background are presented. For a typical analysis procedure the direction of tracks are reconstructed with about 2° accuracy.

Original language	English
Pages (from-to)	169-194
Number of pages	26
Journal	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume	524
Issue number	1-3
DOIs	https://doi.org/10.1016/j.nima.2004.01.065
State	Published - 21 May 2004
Externally published	Yes

Keywords

AMANDA
Neutrino astrophysics
Neutrino telescope
Track reconstruction

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10.1016/j.nima.2004.01.065

Cite this

Ahrens, J., Bai, X., Bay, R., Barwick, S. W., Becka, T., Becker, J. K., Becker, K. H., Bernardini, E., Bertrand, D., Biron, A., Boersma, D. J., Böser, S., Botner, O., Bouchta, A., Bouhali, O., Burgess, T., Carius, S., Castermans, T., Chirkin, D., ... Wiebusch, C. H. (2004). Muon track reconstruction and data selection techniques in AMANDA. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 524(1-3), 169-194. https://doi.org/10.1016/j.nima.2004.01.065

@article{a947e0c96fb04e8fa9798688f3c240cf,

title = "Muon track reconstruction and data selection techniques in AMANDA",

abstract = "The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice between 1500 and 2000 m. The primary goal of this detector is to discover astrophysical sources of high-energy neutrinos. A high-energy muon neutrino coming through the earth from the Northern Hemisphere can be identified by the secondary muon moving upward through the detector. The muon tracks are reconstructed with a maximum likelihood method. It models the arrival times and amplitudes of Cherenkov photons registered by the photo-multipliers. This paper describes the different methods of reconstruction, which have been successfully implemented within AMANDA. Strategies for optimizing the reconstruction performance and rejecting background are presented. For a typical analysis procedure the direction of tracks are reconstructed with about 2° accuracy.",

keywords = "AMANDA, Neutrino astrophysics, Neutrino telescope, Track reconstruction",

author = "J. Ahrens and X. Bai and R. Bay and Barwick, {S. W.} and T. Becka and Becker, {J. K.} and Becker, {K. H.} and E. Bernardini and D. Bertrand and A. Biron and Boersma, {D. J.} and S. B{\"o}ser and O. Botner and A. Bouchta and O. Bouhali and T. Burgess and S. Carius 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 Dewulf, {J. P.} and P. Ekstr{\"o}m and T. Feser and M. Gaug and Gaisser, {T. K.} and R. Ganugapati and H. Geenen and L. Gerhardt and A. Gro{\ss} and A. Goldschmidt and A. Hallgren 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 D. Hubert and B. Hughey and Hulth, {P. O.} and K. Hultqvist and S. Hundertmark and J. Jacobsen and A. Karle and M. Kestel and L. K{\"o}pke and M. Kowalski and K. Kuehn and Lamoureux, {J. I.} and H. Leich and M. Leuthold and P. Lindahl and I. Liubarsky and J. Madsen and P. Marciniewski and Matis, {H. S.} and McParland, {C. P.} and T. Messarius and Y. Minaeva and P. Mio{\v c}inovi{\'c} and Mock, {P. C.} and R. Morse and M{\"u}nich, {K. S.} and J. Nam and R. Nahnhauer and T. Neunh{\"o}ffer and P. Niessen and Nygren, {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}guez} and D. Ross and Sander, {H. G.} and K. Schinarakis and S. Schlenstedt and T. Schmidt and D. Schneider and Wiebusch, {C. H.}",

year = "2004",

month = may,

day = "21",

doi = "10.1016/j.nima.2004.01.065",

language = "English",

volume = "524",

pages = "169--194",

journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

issn = "0168-9002",

publisher = "Elsevier B.V.",

number = "1-3",

}

Ahrens, J, Bai, X, Bay, R, Barwick, SW, Becka, T, Becker, JK, Becker, KH, Bernardini, E, Bertrand, D, Biron, A, Boersma, DJ, Böser, S, Botner, O, Bouchta, A, Bouhali, O, Burgess, T, Carius, S, Castermans, T, Chirkin, D, Collin, B, Conrad, J, Cooley, J, Cowen, DF, Davour, A, De Clercq, C, DeYoung, T, Desiati, P, Dewulf, JP, Ekström, P, Feser, T, Gaug, M, Gaisser, TK, Ganugapati, R, Geenen, H, Gerhardt, L, Groß, A, Goldschmidt, A, Hallgren, A, Halzen, F, Hanson, K, Hardtke, R, Harenberg, T, Hauschildt, T, Helbing, K, Hellwig, M, Herquet, P, Hill, GC, Hubert, D, Hughey, B, Hulth, PO, Hultqvist, K, Hundertmark, S, Jacobsen, J, Karle, A, Kestel, M, Köpke, L, Kowalski, M, Kuehn, K, Lamoureux, JI, Leich, H, Leuthold, M, Lindahl, P, Liubarsky, I, Madsen, J, Marciniewski, P, Matis, HS, McParland, CP, Messarius, T, Minaeva, Y, Miočinović, P, Mock, PC, Morse, R, Münich, KS, Nam, J, Nahnhauer, R, Neunhöffer, T, Niessen, P, Nygren, 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, Ross, D, Sander, HG, Schinarakis, K, Schlenstedt, S, Schmidt, T, Schneider, D & Wiebusch, CH 2004, 'Muon track reconstruction and data selection techniques in AMANDA', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 524, no. 1-3, pp. 169-194. https://doi.org/10.1016/j.nima.2004.01.065

TY - JOUR

T1 - Muon track reconstruction and data selection techniques in AMANDA

AU - Ahrens, J.

AU - Bai, X.

AU - Bay, R.

AU - Barwick, S. W.

AU - Becka, T.

AU - Becker, J. K.

AU - Becker, K. H.

AU - Bernardini, E.

AU - Bertrand, D.

AU - Biron, A.

AU - Boersma, D. J.

AU - Böser, S.

AU - Botner, O.

AU - Bouchta, A.

AU - Bouhali, O.

AU - Burgess, T.

AU - Carius, S.

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 - Dewulf, J. P.

AU - Ekström, P.

AU - Feser, T.

AU - Gaug, M.

AU - Gaisser, T. K.

AU - Ganugapati, R.

AU - Geenen, H.

AU - Gerhardt, L.

AU - Groß, A.

AU - Goldschmidt, A.

AU - Hallgren, 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 - Hubert, D.

AU - Hughey, B.

AU - Hulth, P. O.

AU - Hultqvist, K.

AU - Hundertmark, S.

AU - Jacobsen, J.

AU - Karle, A.

AU - Kestel, M.

AU - Köpke, L.

AU - Kowalski, M.

AU - Kuehn, K.

AU - Lamoureux, J. I.

AU - Leich, H.

AU - Leuthold, M.

AU - Lindahl, P.

AU - Liubarsky, I.

AU - Madsen, J.

AU - Marciniewski, P.

AU - Matis, H. S.

AU - McParland, C. P.

AU - Messarius, T.

AU - Minaeva, Y.

AU - Miočinović, P.

AU - Mock, P. C.

AU - Morse, R.

AU - Münich, K. S.

AU - Nam, J.

AU - Nahnhauer, R.

AU - Neunhöffer, T.

AU - Niessen, P.

AU - Nygren, 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. Rodríguez

AU - Ross, D.

AU - Sander, H. G.

AU - Schinarakis, K.

AU - Schlenstedt, S.

AU - Schmidt, T.

AU - Schneider, D.

AU - Wiebusch, C. H.

PY - 2004/5/21

Y1 - 2004/5/21

N2 - The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice between 1500 and 2000 m. The primary goal of this detector is to discover astrophysical sources of high-energy neutrinos. A high-energy muon neutrino coming through the earth from the Northern Hemisphere can be identified by the secondary muon moving upward through the detector. The muon tracks are reconstructed with a maximum likelihood method. It models the arrival times and amplitudes of Cherenkov photons registered by the photo-multipliers. This paper describes the different methods of reconstruction, which have been successfully implemented within AMANDA. Strategies for optimizing the reconstruction performance and rejecting background are presented. For a typical analysis procedure the direction of tracks are reconstructed with about 2° accuracy.

AB - The Antarctic Muon And Neutrino Detector Array (AMANDA) is a high-energy neutrino telescope operating at the geographic South Pole. It is a lattice of photo-multiplier tubes buried deep in the polar ice between 1500 and 2000 m. The primary goal of this detector is to discover astrophysical sources of high-energy neutrinos. A high-energy muon neutrino coming through the earth from the Northern Hemisphere can be identified by the secondary muon moving upward through the detector. The muon tracks are reconstructed with a maximum likelihood method. It models the arrival times and amplitudes of Cherenkov photons registered by the photo-multipliers. This paper describes the different methods of reconstruction, which have been successfully implemented within AMANDA. Strategies for optimizing the reconstruction performance and rejecting background are presented. For a typical analysis procedure the direction of tracks are reconstructed with about 2° accuracy.

KW - AMANDA

KW - Neutrino astrophysics

KW - Neutrino telescope

KW - Track reconstruction

UR - http://www.scopus.com/inward/record.url?scp=2342660756&partnerID=8YFLogxK

U2 - 10.1016/j.nima.2004.01.065

DO - 10.1016/j.nima.2004.01.065

M3 - Article

AN - SCOPUS:2342660756

SN - 0168-9002

VL - 524

SP - 169

EP - 194

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

IS - 1-3

ER -

Muon track reconstruction and data selection techniques in AMANDA

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Keywords

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