Search Results - "Romenesko, P."

The AMANDA neutrino telescope: principle of operation and first results by Andres, E., Askebjer, P., Barwick, S.W., Bay, R., Bergström, L., Biron, A., Booth, J., Bouchta, A., Carius, S., 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.

“…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…”
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Observation of high-energy neutrinos using erenkov detectors embedded deep in Antarctic ice by Desiati, P, Karle, A, Steele, D, Ögelman, H, Hulth, P. O, Lindahl, P, Koci, B, Bertrand, D, Schwarz, R, Jacobsen, J, Mio inovi, P, Morse, R, Barouch, G, Schmidt, T, Rawlins, K, Silvestri, A, Marciniewski, P, Richter, S, Chirkin, D, Newcomer, F. M, Usechak, N, Spiering, C, Chen, A, Martino, J. Rodríguez, Wu, W, Conrad, J, Young, S, Mikolajski, T, Goldschmidt, A, Askebjer, P, Bai, X, Kim, J, Leuthold, M, Richards, A, Romenesko, P, Andrés, E, Lowder, D. M, Wiebusch, C. H, Rhode, W, Boyce, M. M, DeYoung, T, Tilav, S, Neunhöffer, T, Schneider, E, Halzen, F, Mock, P. C, Weinheimer, C, Bay, R. C, Wischnewski, R, Costa, C. G. S, Hallgren, A, Köpke, L, Leich, H, Stokstad, R. G, Walck, C, Dewulf, J.-P, Bierenbaum, D, Solarz, M, Steffen, P, Goobar, A, Wissing, H, Pérez de los Heros, C, Vander Donckt, M, Reed, C, Thollander, L, Matis, H. S, Biron, A, Streicher, O, Edsjö, J, Barwick, S. W, Dailing, J, Spiczak, G. M, Gaug, M, Hundertmark, S, Carius, S, Erlandsson, B, Sander, H.-G, He, Y. D, Kowalski, M, Yodh, G, Madsen, J, Dalberg, E, Gray, L, Sun, Q, Hardtke, R, Ross, D, Loaiza, P, Thon, T, Doksus, P, Porrata, R, Scheider, T, Nygren, D. R, Schneider, D, Hill, G. C, Niessen, P, Becker, K.-H, Bouchta, A, Minaeva, Y, Cowen, D. F, Hanson, K

“…Neutrinos are elementary particles that carry no electric charge and have little mass. As they interact only weakly with other particles, they can penetrate…”
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Observation of high-energy neutrinos using #268;erenkov detectors embedded deep in Antarctic ice by Andres, E, Askebjer, P, Bai, X, Barouch, G, Barwick, S. W, Bay, R. C, Becker, K.-H, Bergstrom, L, Bertrand, D, Bierenbaum, D, Biron, A, Booth, J, Botner, O, Bouchta, A, Boyce, M. M, Carius, S, 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, Edsjo, J, Erlandsson, B, Gaug, M, Goldschmidt, A, Hallgren, A, Halzen, F, Hanson, K, He, Y. D, Hellwig, M, Heukenkamp, H, Hill, G. C, Hulth, P. O, Hundertmark, S, Jacobsen, J, Kandhadai, V, Kim, J, Koci, B, Kopke, L, Kowalski, M, Leich, H, Leuthold, M, Lindahl, P, Loaiza, P, Lowder, D. M, Ludvig, J, Marciniewski, P, Matis, H. S, Mihalyi, A, Mikolajski, T, Miller, T. C, Minaeva, Y, Miočinović, P, Mock, P. C, Morse, R, Neunhoffer, T, Newcomer, F. M, Nygren, D. R, Ogelman, H, Perez de los Heros, C, Porrata, R, Price, P. B, Rawlins, K, Rhode, W, Richards, A, Richter, S, Martino, J. Rodriguez, Romenesko, P, Ross, D, Sander, H.-G, Scheider, T, Schmidt, T, Schneider, D, Schneider, E, Silvestri, A, Solarz, M, Spiczak, G. M, Starinsky, N, Steele, D, Streicher, O, Sun, Q, Taboada, I, Thollander, L, Thon, T, Tilav, S, Usechak, N, Vander Donckt, M, Walck, C, Weinheimer, C, Wiebusch, C. H, Wissing, H, Woschnagg, K, Wu, W, Young, S

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The AMANDA neutrino telescope by Andrés, E.C., Askebjer, P., Barwick, S.W., Bay, R.C., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, S., 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.

“…With an effective telescope area of order 10 4 m 2 for TeV neutrinos, a threshold near ∼50 GeV and a pointing accuracy of 2.5 degrees per muon track, the…”
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The AMANDA Neutrino Detector by Wischnewski, R., Andrés, E., Askebjer, P., Barwick, S., Bay, R., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, S., 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 Heros, 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.

“…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…”
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