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Your search keyword '"Romenesko, P."' showing total 11 results
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11 results on '"Romenesko, P."'

1. Calibration and survey of AMANDA with the SPASE detectors

Author

Ahrens, J., Bai, X., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bernardini, E., Bertrand, D., Binon, F., Biron, A., Böser, S., Botner, O., Bouchta, A., Bouhali, O., Burgess, T., Carius, Staffan, Castermans, T., Chirkin, D., Conrad, J., Cooley, J., Cowen, D. F., Davour, A., de Clercq, C., DeYoung, T., Desiati, P., Doksus, P., Ekström, P., Engel, R., Evenson, P., Feser, T., Gaisser, T. K., 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, G. C., Hinton, J. A., Hughey, B., Hulth, P. O., Hultqvist, K., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Köpke, L., Kowalski, M., Kuehn, K., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Lloyd-Evans, J., Madsen, J., Mandli, K., Marciniewski, P., Martello, D., Matis, H. S., McParland, C. P., Messarius, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ögelman, H., Olbrechts, P., Perez de los Heros, C., Pohl, A. C., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Resconi, E., Rhode, W., Ribordy, M., Richter, S., Rochester, K., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schmidt, T., Schinarakis, K., Schlenstedt, S., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Splczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Steele, D., Steffen, P., Stokstad, R. G., Sulanke, K. -H, Taboada, I., Tilav, S., Walck, C., Wagner, W., Wang, Y. -R, Watson, A. A., Weinheimer, C., Wiebusch, C. H., Wiedemann, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., Ahrens, J., Bai, X., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bernardini, E., Bertrand, D., Binon, F., Biron, A., Böser, S., Botner, O., Bouchta, A., Bouhali, O., Burgess, T., Carius, Staffan, Castermans, T., Chirkin, D., Conrad, J., Cooley, J., Cowen, D. F., Davour, A., de Clercq, C., DeYoung, T., Desiati, P., Doksus, P., Ekström, P., Engel, R., Evenson, P., Feser, T., Gaisser, T. K., 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, G. C., Hinton, J. A., Hughey, B., Hulth, P. O., Hultqvist, K., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Köpke, L., Kowalski, M., Kuehn, K., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Lloyd-Evans, J., Madsen, J., Mandli, K., Marciniewski, P., Martello, D., Matis, H. S., McParland, C. P., Messarius, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ögelman, H., Olbrechts, P., Perez de los Heros, C., Pohl, A. C., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Resconi, E., Rhode, W., Ribordy, M., Richter, S., Rochester, K., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schmidt, T., Schinarakis, K., Schlenstedt, S., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Splczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Steele, D., Steffen, P., Stokstad, R. G., Sulanke, K. -H, Taboada, I., Tilav, S., Walck, C., Wagner, W., Wang, Y. -R, Watson, A. A., Weinheimer, C., Wiebusch, C. H., Wiedemann, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.

Abstract

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. © 2003 Elsevier B.V. All rights reserved., Source: Scopus

Published
2004
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2. Limits on diffuse fluxes of high energy extraterrestrial neutrinos with the AMANDA-B10 detector

Author

Ahrens, J., Bai, X., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bernardini, E., Bertrand, D., Biron, A., Boeser, S., Botner, O., Bouchta, A., Bouhali, O., Burgess, T., Carius, Staffan, Castermans, T., Chirkin, D., Conrad, J., Cooley, J., Cowen, D. F., Davour, A., de Clercq, C., DeYoung, T., Desiati, P., Doksus, P., Ekström, P., Feser, T., Gaisser, T. K., 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, G. C., Hulth, P. O., Hughey, B., Hultqvist, K., Hundertmark, S., Jacobsen, J., Karle, A., Kuehn, K., Kim, J., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Madsen, J., Mandli, K., Marciniewski, P., Matis, H., McParland, C. P., Messarius, T., Miller, T. C., Minaeva, Y., Miocinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ögelman, H., Olbrechts, P., Pérez de los Heros, C., Pohl, A. C., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Resconi, E., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schlenstedt, S., Schinarakis, K., Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Stamatikos, M., Spiczak, G. M., Spiering, C., Steele, D., Steffen, P., Stokstad, R. G., Sulanke, K. -H, Taboada, I., Tilav, S., Wagner, W., Walck, C., Wang, Y. -R, Wiebusch, C. H., Wiedemann, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., Ahrens, J., Bai, X., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bernardini, E., Bertrand, D., Biron, A., Boeser, S., Botner, O., Bouchta, A., Bouhali, O., Burgess, T., Carius, Staffan, Castermans, T., Chirkin, D., Conrad, J., Cooley, J., Cowen, D. F., Davour, A., de Clercq, C., DeYoung, T., Desiati, P., Doksus, P., Ekström, P., Feser, T., Gaisser, T. K., 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, G. C., Hulth, P. O., Hughey, B., Hultqvist, K., Hundertmark, S., Jacobsen, J., Karle, A., Kuehn, K., Kim, J., Köpke, L., Kowalski, M., Lamoureux, J. I., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Madsen, J., Mandli, K., Marciniewski, P., Matis, H., McParland, C. P., Messarius, T., Miller, T. C., Minaeva, Y., Miocinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ögelman, H., Olbrechts, P., Pérez de los Heros, C., Pohl, A. C., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Resconi, E., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schlenstedt, S., Schinarakis, K., Schmidt, T., Schneider, D., Schwarz, R., Silvestri, A., Solarz, M., Stamatikos, M., Spiczak, G. M., Spiering, C., Steele, D., Steffen, P., Stokstad, R. G., Sulanke, K. -H, Taboada, I., Tilav, S., Wagner, W., Walck, C., Wang, Y. -R, Wiebusch, C. H., Wiedemann, C., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.

Abstract

A report on the limits, which could be placed on diffuse fluxes of high energy extraterrestrial neutrinos, was presented. The incorporation of neutrino oscillations was necessary for interpreting the limits in terms of the flux from a cosmological distributions of sources. The energetic accelerated environments were presented as the sources of high energy extraterrestrial neutrinos., Art. No.: 251101

Published
2003
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3. Limits to the muon flux from WIMP annihilation in the center of the Earth with the AMANDA detector

Author

Ahrens, J., Andrés, E., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bertrand, D., Biron, A., Botner, O., Bouchta, A., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., De Clercq, C., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaisser, T. K., Gaug, M., Gerhardt, L., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hauschildt, T., Hellwig, M., 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., Loaiza, P., Lowder, D. M., Ludvig, J., 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., Ogelman, H., Olbrechts, Ph., Pérez De Los Heros, C., Pohl, A., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Sulanke, K. H., Taboada, I., Thollander, L., Thon, T., Ahrens, J., Andrés, E., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bertrand, D., Biron, A., Botner, O., Bouchta, A., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., De Clercq, C., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaisser, T. K., Gaug, M., Gerhardt, L., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., Hauschildt, T., Hellwig, M., 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., Loaiza, P., Lowder, D. M., Ludvig, J., 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., Ogelman, H., Olbrechts, Ph., Pérez De Los Heros, C., Pohl, A., Porrata, R., Price, P. B., Przybylski, G. T., Rawlins, K., Rhode, W., Ribordy, M., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Sander, H. -G, Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sudhoff, P., Sulanke, K. H., Taboada, I., Thollander, L., and Thon, T.

Abstract

A search for nearly vertical up-going muon-neutrinos from neutralino annihilations in the center of the Earth has been performed with the AMANDA-B10 neutrino detector. The data collected in 130.1 days of live time in 1997, ∼10 9 events, have been analyzed for this search. No excess over the expected atmospheric neutrino background has been observed. An upper limit at 90% confidence level has been obtained on the annihilation rate of neutralinos in the center of the Earth, as well as the corresponding muon flux limit, both as a function of the neutralino mass in the range 100 GeV-5000 GeV. © 2002 The American Physical Society., Art. No.: 032006

Published
2002
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4. Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array

Author

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, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., de Clercq, C., de Young, 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., 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, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., de Clercq, C., de Young, 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., and Young, S.

Abstract

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., Art. No.: 012005

Published
2002
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5. Recent results from AMANDA

Author

Andrés, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Bierenbaum, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., De Young, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Gray, L., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y. D., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Mihalyi, A., Mikolajski, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Newcomer, F. M., Niessen, P., Nygren, D. R., Ogelman, H., Pérez De Los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Usechak, N., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., Andrés, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Bierenbaum, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., De Young, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Gray, L., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y. D., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Mihalyi, A., Mikolajski, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Newcomer, F. M., Niessen, P., Nygren, D. R., Ogelman, H., Pérez De Los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Rodríguez Martino, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Usechak, N., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.

Abstract

We present results based on data taken in 1997 with the 302-PMT Antarctic Muon and Neutrino Detector Array-B10 ("AMANDA-B10") array. Atmospheric neutrinos created in the northern hemisphere are observed indirectly through their charged current interactions which produce relativistic, Cherenkov-light-emitting upgoing muons in the South Pole ice cap. The reconstructed angular distribution of these events is in good agreement with expectation and demonstrates the viability of this ice-based device as a neutrino telescope., Source: Scopus

Published
2001
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6. Observation of high-energy neutrinos using Čerenkov detectors embedded deep in Antarctic ice

Author

Andrés, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Bierenbaum, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Gray, L., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y. D., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Mihalyi, A., Mikolajski, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Newcomer, F. M., Niessen, P., Nygren, D. R., Ögelman, H., Pérez De Los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Martino, J. R., Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Usechak, N., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., Andrés, E., Askebjer, P., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becker, K. -H, Bergström, L., Bertrand, D., Bierenbaum, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dailing, J., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Erlandsson, B., Feser, T., Gaug, M., Goldschmidt, A., Goobar, A., Gray, L., Haase, H., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., He, Y. D., Hellwig, M., Heukenkamp, H., Hill, G. C., Hulth, P. O., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Koci, B., Köpke, L., Kowalski, M., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D. M., Ludvig, J., Madsen, J., Marciniewski, P., Matis, H. S., Mihalyi, A., Mikolajski, T., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Newcomer, F. M., Niessen, P., Nygren, D. R., Ögelman, H., Pérez De Los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., Richards, A., Richter, S., Martino, J. R., Romenesko, P., Ross, D., Rubinstein, H., Sander, H. -G, Scheider, T., Schmidt, T., Schneider, D., Schneider, E., Schwarz, R., Silvestri, A., Solarz, M., Spiczak, G. M., Spiering, C., Starinsky, N., Steele, D., Steffen, P., Stokstad, R. G., Streicher, O., Sun, Q., Taboada, I., Thollander, L., Thon, T., Tilav, S., Usechak, N., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.

Abstract

Neutrinos are elementary particles that carry no electric charge and have little mass. As they interact only weakly with other particles, they can penetrate enormous amounts of matter, and therefore have the potential to directly convey astrophysical information from the edge of the Universe and from deep inside the most cataclysmic high-energy regions. The neutrino's great penetrating power, however, also makes this particle difficult to detect. Underground detectors have observed low-energy neutrinos from the Sun and a nearby supernova2, as well as neutrinos generated in the Earth's atmosphere. But the very low fluxes of high-energy neutrinos from cosmic sources can be observed only by much larger, expandable detectors in, for example, deep water3,4 or ice5. Here we report the detection of upwardly propagating atmospheric neutrinos by the ice-based Antarctic muon and neutrino detector array (AMANDA). These results establish a technology with which to build a kilometre-scale neutrino observatory necessary for astrophysical observations1., Source: Scopus

Published
2001
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7. Search for supernova neutrino bursts with the AMANDA detector

Author

Ahrens, J., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bertrand, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaug, M., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., 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., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Pérez de los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., 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., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., Young, S., Ahrens, J., Bai, X., Barouch, G., Barwick, S. W., Bay, R. C., Becka, T., Becker, K. -H, Bertrand, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Boyce, M. M., Carius, Staffan, Chen, A., Chirkin, D., Conrad, J., Cooley, J., Costa, C. G. S., Cowen, D. F., Dalberg, E., DeYoung, T., Desiati, P., Dewulf, J. -P, Doksus, P., Edsjö, J., Ekström, P., Feser, T., Gaug, M., Goldschmidt, A., Hallgren, A., Halzen, F., Hanson, K., Hardtke, R., 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., Miller, T. C., Minaeva, Y., Miočinović, P., Mock, P. C., Morse, R., Neunhöffer, T., Niessen, P., Nygren, D. R., Ogelman, H., Pérez de los Heros, C., Porrata, R., Price, P. B., Rawlins, K., Reed, C., Rhode, W., 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., Taboada, I., Thollander, L., Thon, T., Tilav, S., Vander Donckt, M., Walck, C., Weinheimer, C., Wiebusch, C. H., Wischnewski, R., Wissing, H., Woschnagg, K., Wu, W., Yodh, G., and Young, S.

Abstract

The core collapse of a massive star in the Milky Way will produce a neutrino burst, intense enough to be detected by existing underground detectors. The AMANDA neutrino telescope located deep in the South Pole ice can detect MeV neutrinos by a collective rate increase in all photo-multipliers on top of dark noise. The main source of light comes from positrons produced in the CC reaction of anti-electron neutrinos on free protons ve + p → e+ + n. This paper describes the first supernova search performed on the full sets of data taken during 1997 and 1998 (215 days of live time) with 302 of the detector's optical modules. No candidate events resulted from this search. The performance of the detector is calculated, yielding a 70% coverage of the galaxy with one background fake per year with 90% efficiency for the detector configuration under study. An upper limit at the 90% c.l. on the rate of stellar collapses in the Milky Way is derived, yielding 4.3 events per year. A trigger algorithm is presented and its performance estimated. Possible improvements of the detector hardware are reviewed., Source: Scopus

Published
2001
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8. The AMANDA neutrino detector : Status report

Author

Wischnewski, R., Andrés, E., Bai, X., Barouch, G., Barwick, S., Bay, R., Becker, K., Bergström, L., Bertrand, D., Besson, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Cowen, D. F., Costa, C., Dalberg, E., Desiati, P., Dewulf, J., Deyoung, T., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Frichter, G., Gaisser, T., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hardtke, R., Hellwig, M., Hill, G., Hulth, P., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koepke, L., Kowalski, M., Kravchenko, I., Lamoureux, J., Leich, H., Leuthold, M., Lindahl, P., Liss, T., Loaiza, P., Lowder, D., Ludvig, J., Marciniewski, P., Matis, H., Miller, T., Miocinovic, P., Mock, P., Morse, R., Neunhoeffer, T., Newcomer, M., Niessen, P., Nygren, D., de los Heros, C. P., Porrata, R., Price, P., Przybylski, G., Rawlins, K., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H., Schäfer, U., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Silvestri, A., Smoot, G., Solarz, M., Spiczak, G., Spiering, C., Starinski, N., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thollander, L., Thon, T., Tilav, S., vander Donckt, M., Walck, C., Wiebusch, C., Woschnagg, K., Wu, W., Yodh, G., Young, S., Wischnewski, R., Andrés, E., Bai, X., Barouch, G., Barwick, S., Bay, R., Becker, K., Bergström, L., Bertrand, D., Besson, D., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Cowen, D. F., Costa, C., Dalberg, E., Desiati, P., Dewulf, J., Deyoung, T., Doksus, P., Edsjö, J., Ekström, P., Feser, T., Frichter, G., Gaisser, T., Goldschmidt, A., Goobar, A., Hallgren, A., Halzen, F., Hardtke, R., Hellwig, M., Hill, G., Hulth, P., Hundertmark, S., Jacobsen, J., Karle, A., Kim, J., Koepke, L., Kowalski, M., Kravchenko, I., Lamoureux, J., Leich, H., Leuthold, M., Lindahl, P., Liss, T., Loaiza, P., Lowder, D., Ludvig, J., Marciniewski, P., Matis, H., Miller, T., Miocinovic, P., Mock, P., Morse, R., Neunhoeffer, T., Newcomer, M., Niessen, P., Nygren, D., de los Heros, C. P., Porrata, R., Price, P., Przybylski, G., Rawlins, K., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Sander, H., Schäfer, U., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Silvestri, A., Smoot, G., Solarz, M., Spiczak, G., Spiering, C., Starinski, N., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thollander, L., Thon, T., Tilav, S., vander Donckt, M., Walck, C., Wiebusch, C., Woschnagg, K., Wu, W., Yodh, G., and Young, S.

Abstract

The first stage of the AMANDA High Energy Neutrino Detector at the South Pole, the 302 PMT array AMANDA-B10, is taking data since 1997. We describe results on atmospheric neutrinos, limits on indirect WIMP detection, seasonal muon flux variation, relativistic monopole flux limits, a search for gravitational collapse neutrinos, and a depth scan of the optical ice properties. The next stage 19-string detector AMANDA-II with ∼650 PMTs will be completed in spring 2000., Source: Scopus

Published
2000
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9. The AMANDA neutrino telescope : Principle of operation and first results

Author

Andres, E., Askebjer, P., Barwick, S. W., Bay, R., Bergström, L., Biron, A., Booth, J., Bouchta, A., Carius, Staffan, Carlson, M., Cowen, D., Dalberg, E., Deyoung, T., Ekström, P., Erlandson, B., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., Hart, S., He, Y., Heukenkamp, H., Hill, G., Hulth, P. O., Hundertmark, S., Jacobsen, J., Jones, A., Kandhadai, V., Karle, A., Koci, B., Lindahl, P., Liubarsky, I., Leuthold, M., Lowder, D. M., Marciniewski, P., Mikolajski, T., Miller, T., Miocinovic, P., Mock, P., Morse, R., Niessen, P., Pérez De Los Heros, C., Porrata, R., Potter, D., Price, P. B., Przybylski, G., Richards, A., Richter, S., Romenesko, P., Rubinstein, H., Schneider, E., Schmidt, T., Schwarz, R., Solarz, M., Spiczak, G. M., Spiering, C., Streicher, O., Sun, Q., Thollander, L., Thon, T., Tilav, S., Walck, C., Wiebusch, C., Wischnewski, R., Woschnagg, K., Yodh, G., Andres, E., Askebjer, P., Barwick, S. W., Bay, R., Bergström, L., Biron, A., Booth, J., Bouchta, A., Carius, Staffan, Carlson, M., Cowen, D., Dalberg, E., Deyoung, T., Ekström, P., Erlandson, B., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., Hart, S., He, Y., Heukenkamp, H., Hill, G., Hulth, P. O., Hundertmark, S., Jacobsen, J., Jones, A., Kandhadai, V., Karle, A., Koci, B., Lindahl, P., Liubarsky, I., Leuthold, M., Lowder, D. M., Marciniewski, P., Mikolajski, T., Miller, T., Miocinovic, P., Mock, P., Morse, R., Niessen, P., Pérez De Los Heros, C., Porrata, R., Potter, D., Price, P. B., Przybylski, G., Richards, A., Richter, S., Romenesko, P., Rubinstein, H., Schneider, E., Schmidt, T., Schwarz, R., Solarz, M., Spiczak, G. M., Spiering, C., Streicher, O., Sun, Q., Thollander, L., Thon, T., Tilav, S., Walck, C., Wiebusch, C., Wischnewski, R., Woschnagg, K., and Yodh, G.

Abstract

AMANDA is a high-energy neutrino telescope presently under construction at the geographical South Pole. In the Antarctic summer 1995/96, an array of 80 optical modules (OMs) arranged on 4 strings (AMANDA-B4) was deployed at depths between 1.5 and 2 km. In this paper we describe the design and performance of the AMANDA-B4 prototype, based on data collected between February and November 1996. Monte Carlo simulations of the detector response to down-going atmospheric muon tracks show that the global behavior of the detector is understood. We describe the data analysis method and present first results on atmospheric muon reconstruction and separation of neutrino candidates. The AMANDA array was upgraded with 216 OMs on 6 new strings in 1996/97 (AMANDA-B10), and 122 additional OMs on 3 strings in 1997/98., Source: Scopus

Published
2000
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10. The AMANDA neutrino telescope

Author

Andrés, E. C., Askebjer, P., Barwick, S. W., Bay, R. C., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Costa, C. G. S., Cowen, D., Dalberg, E., DeYoung, T., Edsjö, J., Ekström, P., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., Hart, S., He, Y., De Los Heros, C. P., Hill, G., Hulth, P. O., Hundertmark, S., Jacobsen, J., Jones, A., Kandhadai, V., Karle, A., Kim, J., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D., Marciniewski, P., Miller, T. C., Miocinovic, P., Mock, P. C., Morse, R., Newcomer, M., Niessen, P., Nygren, D., Porrata, R., Potter, D., Price, P. B., Przybylski, G., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Smoot, G., Solarz, M., Sorin, V., Spiering, C., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thon, T., Tilav, S., Walck, C., Wiebusch, C. H., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., Young, S., Andrés, E. C., Askebjer, P., Barwick, S. W., Bay, R. C., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Costa, C. G. S., Cowen, D., Dalberg, E., DeYoung, T., Edsjö, J., Ekström, P., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., Hart, S., He, Y., De Los Heros, C. P., Hill, G., Hulth, P. O., Hundertmark, S., Jacobsen, J., Jones, A., Kandhadai, V., Karle, A., Kim, J., Leich, H., Leuthold, M., Lindahl, P., Liubarsky, I., Loaiza, P., Lowder, D., Marciniewski, P., Miller, T. C., Miocinovic, P., Mock, P. C., Morse, R., Newcomer, M., Niessen, P., Nygren, D., Porrata, R., Potter, D., Price, P. B., Przybylski, G., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Smoot, G., Solarz, M., Sorin, V., Spiering, C., Steffen, P., Stokstad, R., Streicher, O., Taboada, I., Thon, T., Tilav, S., Walck, C., Wiebusch, C. H., Wischnewski, R., Woschnagg, K., Wu, W., Yodh, G., and Young, S.

Abstract

With an effective telescope area of order 104 m2 for TeV neutrinos, a threshold near ∼50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe early results on the calibration of natural deep ice as a particle detector as well as on AMANDA's performance as a neutrino telescope., Source: Scopus

Published
1999
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11. The AMANDA neutrino detector

Author

Wischnewski, R., Andrés, E., Askebjer, P., Barwick, S., Bay, R., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Cowen, D., Costa, C., Dalberg, E., Deyoung, T., Edsjo, J., Ekström, P., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., He, Y., Hill, G., Hulth, P., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Leich, H., Leuthold, M., Lindahl, P., Liss, T., Liubarsky, I., Loaiza, P., Lowder, D., Marciniewski, P., Miller, T., Miocinovic, P., Mock, P., Morse, R., Newcomer, M., Niessen, P., Nygren, D., Pérez de los Hcros, C., Porrata, R., Price, P., Przybylski, G., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Smoot, G., Solarz, M., Sorin, V., Spiering, C., Steffen, P., Stokstad, R., Streicher, O., Thollander, L., Thon, T., Tilav, S., Walck, C., Wiebusch, C., Woschnagg, K., Wu, W., Yodh, G., Young, S., Wischnewski, R., Andrés, E., Askebjer, P., Barwick, S., Bay, R., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, Staffan, Carlson, M., Chinowsky, W., Chirkin, D., Cowen, D., Costa, C., Dalberg, E., Deyoung, T., Edsjo, J., Ekström, P., Goobar, A., Gray, L., Hallgren, A., Halzen, F., Hardtke, R., He, Y., Hill, G., Hulth, P., Hundertmark, S., Jacobsen, J., Kandhadai, V., Karle, A., Kim, J., Leich, H., Leuthold, M., Lindahl, P., Liss, T., Liubarsky, I., Loaiza, P., Lowder, D., Marciniewski, P., Miller, T., Miocinovic, P., Mock, P., Morse, R., Newcomer, M., Niessen, P., Nygren, D., Pérez de los Hcros, C., Porrata, R., Price, P., Przybylski, G., Rhode, W., Richter, S., Rodriguez, J., Romenesko, P., Ross, D., Rubinstein, H., Schmidt, T., Schneider, E., Schwarz, R., Schwendicke, U., Smoot, G., Solarz, M., Sorin, V., Spiering, C., Steffen, P., Stokstad, R., Streicher, O., Thollander, L., Thon, T., Tilav, S., Walck, C., Wiebusch, C., Woschnagg, K., Wu, W., Yodh, G., and Young, S.

Abstract

The first stage of the AMANDA High Energy Neutrino Detector at the South Pole, the 302 PMT array AMANDA-B with an expected effective area for TeV neutrinos of ∼ 104 m2, has been taking data since 1997. Progress with calibration, investigation of ice properties, as well as muon and neutrino data analysis are described. The next stage 20-string detector AMANDA-II with ∼800 PMTs will be completed in spring 2000., Source: Scopus

Published
1999
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