Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array
The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic ra...
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Enthalten in: Physical review / D - [S.l.] : Soc., 1970, 66(2002), 1 |
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volume:66 ; year:2002 ; number:1 ; extent:20 |
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| 520 | |a The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05×109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope. | ||
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(DE-627)NLEJ249954524 (DE-601)aps:849946bd0f840ab2192cffe0f6e4bf7ca530891e DE-627 ger DE-627 rakwb Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array 2002 Online-Ressource 20 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05×109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Andrés, E. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Dalberg, E. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Edsjö, J. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Heukenkamp, H. oth Hill, G. C. oth Hulth, P. O. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Loaiza, P. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ögelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Streicher, O. oth Sudhoff, P. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Thon, T. oth Tilav, S. oth Vander Donckt, M. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Wiedeman, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 66(2002), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:66 year:2002 number:1 extent:20 https://www.tib.eu/de/suchen/id/aps%3A849946bd0f840ab2192cffe0f6e4bf7ca530891e Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 66 2002 1 20 |
| spelling |
(DE-627)NLEJ249954524 (DE-601)aps:849946bd0f840ab2192cffe0f6e4bf7ca530891e DE-627 ger DE-627 rakwb Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array 2002 Online-Ressource 20 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05×109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Andrés, E. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Dalberg, E. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Edsjö, J. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Heukenkamp, H. oth Hill, G. C. oth Hulth, P. O. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Loaiza, P. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ögelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Streicher, O. oth Sudhoff, P. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Thon, T. oth Tilav, S. oth Vander Donckt, M. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Wiedeman, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 66(2002), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:66 year:2002 number:1 extent:20 https://www.tib.eu/de/suchen/id/aps%3A849946bd0f840ab2192cffe0f6e4bf7ca530891e Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 66 2002 1 20 |
| allfields_unstemmed |
(DE-627)NLEJ249954524 (DE-601)aps:849946bd0f840ab2192cffe0f6e4bf7ca530891e DE-627 ger DE-627 rakwb Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array 2002 Online-Ressource 20 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05×109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Andrés, E. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Dalberg, E. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Edsjö, J. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Heukenkamp, H. oth Hill, G. C. oth Hulth, P. O. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Loaiza, P. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ögelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Streicher, O. oth Sudhoff, P. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Thon, T. oth Tilav, S. oth Vander Donckt, M. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Wiedeman, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 66(2002), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:66 year:2002 number:1 extent:20 https://www.tib.eu/de/suchen/id/aps%3A849946bd0f840ab2192cffe0f6e4bf7ca530891e Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 66 2002 1 20 |
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(DE-627)NLEJ249954524 (DE-601)aps:849946bd0f840ab2192cffe0f6e4bf7ca530891e DE-627 ger DE-627 rakwb Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array 2002 Online-Ressource 20 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05×109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Andrés, E. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Dalberg, E. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Edsjö, J. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Heukenkamp, H. oth Hill, G. C. oth Hulth, P. O. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Loaiza, P. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ögelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Streicher, O. oth Sudhoff, P. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Thon, T. oth Tilav, S. oth Vander Donckt, M. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Wiedeman, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 66(2002), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:66 year:2002 number:1 extent:20 https://www.tib.eu/de/suchen/id/aps%3A849946bd0f840ab2192cffe0f6e4bf7ca530891e Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 66 2002 1 20 |
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(DE-627)NLEJ249954524 (DE-601)aps:849946bd0f840ab2192cffe0f6e4bf7ca530891e DE-627 ger DE-627 rakwb Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array 2002 Online-Ressource 20 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05×109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Andrés, E. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Dalberg, E. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Edsjö, J. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Heukenkamp, H. oth Hill, G. C. oth Hulth, P. O. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Loaiza, P. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ögelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Streicher, O. oth Sudhoff, P. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Thon, T. oth Tilav, S. oth Vander Donckt, M. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Wiedeman, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 66(2002), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:66 year:2002 number:1 extent:20 https://www.tib.eu/de/suchen/id/aps%3A849946bd0f840ab2192cffe0f6e4bf7ca530891e Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 66 2002 1 20 |
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Ahrens, J. @@oth@@ Andrés, E. @@oth@@ Bai, X. @@oth@@ Barouch, G. @@oth@@ Barwick, S. W. @@oth@@ Bay, R. C. @@oth@@ Becka, T. @@oth@@ Becker, K.-H. @@oth@@ Bertrand, D. @@oth@@ Binon, F. @@oth@@ Biron, A. @@oth@@ Booth, J. @@oth@@ Botner, O. @@oth@@ Bouchta, A. @@oth@@ Bouhali, O. @@oth@@ Boyce, M. M. @@oth@@ Carius, S. @@oth@@ Chen, A. @@oth@@ Chirkin, D. @@oth@@ Conrad, J. @@oth@@ Cooley, J. @@oth@@ Costa, C. G. @@oth@@ Cowen, D. F. @@oth@@ Dalberg, E. @@oth@@ De Clercq, C. @@oth@@ DeYoung, T. @@oth@@ Desiati, P. @@oth@@ Dewulf, J.-P. @@oth@@ Doksus, P. @@oth@@ Edsjö, J. @@oth@@ Ekström, P. @@oth@@ Feser, T. @@oth@@ Frère, J.-M. @@oth@@ Gaisser, T. K. @@oth@@ Gaug, M. @@oth@@ Goldschmidt, A. @@oth@@ Hallgren, A. @@oth@@ Halzen, F. @@oth@@ Hanson, K. @@oth@@ Hardtke, R. @@oth@@ Hauschildt, T. @@oth@@ Hellwig, M. @@oth@@ Heukenkamp, H. @@oth@@ Hill, G. C. @@oth@@ Hulth, P. O. @@oth@@ Hundertmark, S. @@oth@@ Jacobsen, J. @@oth@@ Karle, A. @@oth@@ Kim, J. @@oth@@ Koci, B. @@oth@@ Köpke, L. @@oth@@ Kowalski, M. @@oth@@ Lamoureux, J. I. @@oth@@ Leich, H. @@oth@@ Leuthold, M. @@oth@@ Lindahl, P. @@oth@@ Liubarsky, I. @@oth@@ Loaiza, P. @@oth@@ Lowder, D. M. @@oth@@ Madsen, J. @@oth@@ Marciniewski, P. @@oth@@ Matis, H. S. @@oth@@ McParland, C. P. @@oth@@ Miller, T. C. @@oth@@ Minaeva, Y. @@oth@@ Miočinović, P. @@oth@@ Mock, P. C. @@oth@@ Morse, R. @@oth@@ Neunhöffer, T. @@oth@@ Niessen, P. @@oth@@ Nygren, D. R. @@oth@@ Ögelman, H. @@oth@@ Olbrechts, Ph. @@oth@@ Pérez de los Heros, C. @@oth@@ Pohl, A. C. @@oth@@ Porrata, R. @@oth@@ Price, P. B. @@oth@@ Przybylski, G. T. @@oth@@ Rawlins, K. @@oth@@ Reed, C. @@oth@@ Rhode, W. @@oth@@ Ribordy, M. @@oth@@ Richter, S. @@oth@@ Rodríguez Martino, J. @@oth@@ Romenesko, P. @@oth@@ Ross, D. @@oth@@ Sander, H.-G. @@oth@@ Schmidt, T. @@oth@@ Schneider, D. @@oth@@ Schwarz, R. @@oth@@ Silvestri, A. @@oth@@ Solarz, M. @@oth@@ Spiczak, G. M. @@oth@@ Spiering, C. @@oth@@ Starinsky, N. @@oth@@ Steele, D. @@oth@@ Steffen, P. @@oth@@ Stokstad, R. G. @@oth@@ Streicher, O. @@oth@@ Sudhoff, P. @@oth@@ Sulanke, K.-H. @@oth@@ Taboada, I. @@oth@@ Thollander, L. @@oth@@ Thon, T. @@oth@@ Tilav, S. @@oth@@ Vander Donckt, M. @@oth@@ Walck, C. @@oth@@ Weinheimer, C. @@oth@@ Wiebusch, C. H. @@oth@@ Wiedeman, C. @@oth@@ Wischnewski, R. @@oth@@ Wissing, H. @@oth@@ Woschnagg, K. @@oth@@ Wu, W. @@oth@@ Yodh, G. @@oth@@ Young, S. @@oth@@ |
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Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array |
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observation of high energy atmospheric neutrinos with the antarctic muon and neutrino detector array |
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Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array |
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The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05×109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope. |
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The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05×109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope. |
| abstract_unstemmed |
The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about 106 times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of 1.05×109 cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope. |
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Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array |
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Ahrens, J. Andrés, E. Bai, X. Barouch, G. Barwick, S. W. Bay, R. C. Becka, T. Becker, K.-H. Bertrand, D. Binon, F. Biron, A. Booth, J. Botner, O. Bouchta, A. Bouhali, O. Boyce, M. M. Carius, S. Chen, A. Chirkin, D. Conrad, J. Cooley, J. Costa, C. G. Cowen, D. F. Dalberg, E. De Clercq, C. DeYoung, T. Desiati, P. Dewulf, J.-P. Doksus, P. Edsjö, J. Ekström, P. Feser, T. Frère, J.-M. Gaisser, T. K. Gaug, M. Goldschmidt, A. Hallgren, A. Halzen, F. Hanson, K. Hardtke, R. Hauschildt, T. Hellwig, M. Heukenkamp, H. Hill, G. C. Hulth, P. O. Hundertmark, S. Jacobsen, J. Karle, A. Kim, J. Koci, B. Köpke, L. Kowalski, M. Lamoureux, J. I. Leich, H. Leuthold, M. Lindahl, P. Liubarsky, I. Loaiza, P. Lowder, D. M. Madsen, J. Marciniewski, P. Matis, H. S. McParland, C. P. Miller, T. C. Minaeva, Y. Miočinović, P. Mock, P. C. Morse, R. Neunhöffer, T. Niessen, P. Nygren, D. R. Ögelman, H. Olbrechts, Ph Pérez de los Heros, C. Pohl, A. C. Porrata, R. Price, P. B. Przybylski, G. T. Rawlins, K. Reed, C. Rhode, W. Ribordy, M. Richter, S. Rodríguez Martino, J. Romenesko, P. Ross, D. Sander, H.-G. Schmidt, T. Schneider, D. Schwarz, R. Silvestri, A. Solarz, M. Spiczak, G. M. Spiering, C. Starinsky, N. Steele, D. Steffen, P. Stokstad, R. G. Streicher, O. Sudhoff, P. Sulanke, K.-H. Taboada, I. Thollander, L. Thon, T. Tilav, S. Vander Donckt, M. Walck, C. Weinheimer, C. Wiebusch, C. H. Wiedeman, C. Wischnewski, R. Wissing, H. Woschnagg, K. Wu, W. Yodh, G. Young, S. |
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Ahrens, J. Andrés, E. Bai, X. Barouch, G. Barwick, S. W. Bay, R. C. Becka, T. Becker, K.-H. Bertrand, D. Binon, F. Biron, A. Booth, J. Botner, O. Bouchta, A. Bouhali, O. Boyce, M. M. Carius, S. Chen, A. Chirkin, D. Conrad, J. Cooley, J. Costa, C. G. Cowen, D. F. Dalberg, E. De Clercq, C. DeYoung, T. Desiati, P. Dewulf, J.-P. Doksus, P. Edsjö, J. Ekström, P. Feser, T. Frère, J.-M. Gaisser, T. K. Gaug, M. Goldschmidt, A. Hallgren, A. Halzen, F. Hanson, K. Hardtke, R. Hauschildt, T. Hellwig, M. Heukenkamp, H. Hill, G. C. Hulth, P. O. Hundertmark, S. Jacobsen, J. Karle, A. Kim, J. Koci, B. Köpke, L. Kowalski, M. Lamoureux, J. I. Leich, H. Leuthold, M. Lindahl, P. Liubarsky, I. Loaiza, P. Lowder, D. M. Madsen, J. Marciniewski, P. Matis, H. S. McParland, C. P. Miller, T. C. Minaeva, Y. Miočinović, P. Mock, P. C. Morse, R. Neunhöffer, T. Niessen, P. Nygren, D. R. Ögelman, H. Olbrechts, Ph Pérez de los Heros, C. Pohl, A. C. Porrata, R. Price, P. B. Przybylski, G. T. Rawlins, K. Reed, C. Rhode, W. Ribordy, M. Richter, S. Rodríguez Martino, J. Romenesko, P. Ross, D. Sander, H.-G. Schmidt, T. Schneider, D. Schwarz, R. Silvestri, A. Solarz, M. Spiczak, G. M. Spiering, C. Starinsky, N. Steele, D. Steffen, P. Stokstad, R. G. Streicher, O. Sudhoff, P. Sulanke, K.-H. Taboada, I. Thollander, L. Thon, T. Tilav, S. Vander Donckt, M. Walck, C. Weinheimer, C. Wiebusch, C. H. Wiedeman, C. Wischnewski, R. Wissing, H. Woschnagg, K. Wu, W. Yodh, G. Young, S. |
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