Zobrazeno 1 - 10
of 36
pro vyhledávání: '"H. Ogelman"'
Autor:
J. Ahrens, X. Bai, S.W. Barwick, T. Becka, K.-H. Becker, E. Bernardini, D. Bertrand, F. Binon, A. Biron, S. Böser, O. Botner, O. Bouhali, T. Burgess, S. Carius, T. Castermans, D. Chirkin, J. Conrad, J. Cooley, D.F. Cowen, A. Davour, C. De Clercq, T. DeYoung, P. Desiati, J.-P. Dewulf, P. Ekström, T. Feser, T.K. Gaisser, R. Ganupati, M. Gaug, H. Geenen, L. Gerhardt, A. Goldschmidt, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt, M. Hellwig, Ph. Herquet, G.C. Hill, P.O. Hulth, K. Hultqvist, S. Hundertmark, J. Jacobsen, A. Karle, L. Köpke, K. Kuehn, M. Kowalski, J.I. Lamoureux, H. Leich, M. Leuthold, P. Lindahl, I. Liubarsky, J. Madsen, K. Mandli, P. Marciniewski, H.S. Matis, C.P. McParland, T. Messarius, Y. Minaeva, P. Miočinović, R. Morse, R. Nahnhauer, T. Neunhöffer, P. Niessen, D.R. Nygren, H. Ogelman, Ph. Olbrechts, C. Pérez de los Heros, A.C. Pohl, P.B. Price, G.T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, J. Rodríguez Martino, H.-G. Sander, T. Schmidt, D. Schneider, K. Schinarakis, R. Schwarz, A. Silvestri, M. Solarz, G.M. Spiczak, C. Spiering, D. Steele, P. Steffen, R.G. Stokstad, P. Sudoff, K.-H. Sudoff, K.-H. Sulanke, I. Taboada, L. Thollander, S. Tilav, W. Wagner, C. Walck, C. Weinheimer, C.H. Wiebusch, C. Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, G. Yodh, S. Young
Publikováno v:
Nuclear Physics A. 721:C545-C548
We present results from the AMANDA high energy neutrino telescope located at the South Pole. They include measurements of the atmospheric neutrino flux, search for UHE point sources, and diffuse sources producing electromagnetic/hadronic showers at t
Autor:
J. Ahrens, X. Bai, S.W. Barwick, T. Becka, K.-H. Becker, E. Bernaxdini, D. Bertrand, F. Binon, A. Birone, S. Böser, O. Botnerg, O. Bouhali, T. Burgess, S. Carius, T. Castermans, A. Chen, D. Chirkin, J. Conrad, J. Cooley, D.F. Cowen, A. Davour, C. De Clercq, T. DeYoung, P. Desiati, J.-P. Dewulf, P. Doksus, P. Ekström, T. Feser, T.K. Gaisser, M. Gaug, L. Gerhardt, A. Goldschmidt, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt, M. Hellwig, P. Herquet, G.C. Hill, P.O. Hulth, S. Hundertmark, J. Jacobsen, A. Karle, B. Koci, L. Köpke, K. Kuehn, M. Kowalski, J.I. Lamoureux, H. Leich, M. Leuthold, P. Lindahl, I. Liubarsky, J. Madsen, P. Marciniewski, H.S. Matis, C.P. McParland, Y. Minaeva, P. Miočinović, R. Morse, R. Nahnhauer, T. Neunhöffer, P. Niessen, D.R. Nygren, H. Ogelman, Ph. Olbrechts, C. Pérez de los Heros, A.C. Pohl, P.B. Price, G.T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, J. Rodríguez Martino, D. Ross, H.-G. Sander, T. Schmidt, D. Schneider, R. Schwarz, A. Silvestri, M. Solarz, G.M. Spiczak, C. Spiering, D. Steele, P. Steffen, R.G. Stokstad, P. Sudhoff, K.-H. Sulanke, I. Taboada, L. Thollander, S. Tilav, C. Walck, C. Weinheimer, C.H. Wiebusch, C. Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, G. Yodh, S. Young
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 118:371-379
We show new results from both the older and newer incarnations of AMANDA (AMANDA-B10 and AMANDA-II, respectively). These results demonstrate that AMANDA is a functioning, multipurpose detector with significant physics and astrophysics reach. They inc
Publikováno v:
The Astrophysical Journal. 475:224-230
We present a VLA image of the Vela X region, a nebula thought to be powered by the young pulsar B0833-45, at a resolution of approximately 13. The morphology of this synchrotron nebula is dominated by a network of fine, overlapping linear filaments.
Autor:
K. Hanson, J. Ahrens, X. Bai, S.W. Barwick, T. Becka, K.-H. Becker, E. Bernardini, D. Bertrand, F. Binon, A. Biron, S. Böser, O. Botner, O. Bouhali, T. Burgess, S. Carius, T. Castermans, A. Chen, D. Chirkin, J. Conrad, J. Cooley, D.F. Cowen, A. Davour, C. De Clercq, T. De Young, P. Desiati, J.-P. Dewulf, P. Doksus, P. Ekström, T. Feser, T.K. Gaisser, M. Gaug, L. Gerhardt, A. Goldschmidt, A. Hallgren, F. Halzen, R. Hardtke, T. Hauschildt, M. Hellwig, P. Herque, G.C. Hill, P.O. Hulth, S. Hundertmark, J. Jacobsen, A. Karle, B. Koci, L. Köpke, K. Kuehn, M. Kowalski, J.I. Lamoureux, H. Leich, M. Leuthold, P. Lindahl, I. Liubarsky, J. Madsen, P. Marciniewski, H.S. Matis, C.P. McParland, Y. Minaeva, P. Miočinović, R. Morse, R. Nahnhauer, T. Neunhöffer, P. Niessen, D.R. Nygren, H. Ogelman, Ph. Olbrechts, C. Pérez de los Heros, A.C. Pohl, P.B. Price, G.T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, J. Rodríguez Martino, D. Ross, H.-G. Sander, T. Schmidt, D. Schneider, R. Schwarz, A. Silvestri, M. Solarz, G.M. Spiczak, C. Spiering, D. Steele, P. Steffen, R.G. Stokstad, P. Sudhoff, K.-H. Sulanke, I. Taboada, L. Thollander, S. Tilav, C. Walck, C. Weinheimer, C.H. Wiebusch, C. Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, G. Yodh, S. Young
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 117:126-128
We present new data taken with the AMANDA-II neutrino telescope array. The AMANDA-II upgrade was completed at the beginning of 2000. It significantly extends the sensitivity of the 10-string AMANDA-B10 detector to high- and ultrahigh-energy neutrino
Autor:
H. Ogelman, E. Tepedelenlioglu
PSR B0628-28 is a radio pulsar which was first detected in the X-ray band by ROSAT and then later observed with Chandra and XMM-Newton. The Chandra observation yielded an X-ray luminosity two orders of magnitude higher than what is expected for spin-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f2ee683c7d95a2c1c5b8a98c32344af5
Autor:
A. Karle, J. Ahrens, J.N. Bahcall, X. Bai, T. Becka, K.-H. Becker, D.Z. Besson, D. Berley, E. Bernardini, D. Bertrand, F. Binon, A. Biron, S. Böser, C. Bohm, O. Botner, O. Bouhali, Th. Burgess, T. Castermans, D. Chirkin, J. Conrad, J. Cooley, D.F. Cowen, A. Davour, C. De Clercq, T. DeYoung, P. Desiati, J.-P. Dewulf, B. Dingus, R. Ellsworth, P.A. Evenson, A.R. Fazely, T. Feser, T.K. Gaisser, J. Gallagher, R. Ganugapati, A. Goldschmidt, J. Goodman, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt, M. Hellwig, P. Herquet, G.C. Hill, P.O. Hulth, K. Hultgvist, S. Hundertmark, J. Jacobsen, G.S. Japaridze, L. Köpke, M. Kowalski, J.I. Lamoureux, H. Leich, M. Leuthold, P. Lindahl, I. Liubarsky, J. Madson, P. Marciniewski, H.S. Matis, C.P. McParland, Y. Minaeva, P. Miočinović, R. Morse, R. Nahnhauer, T. Neunhöffer, P. Niessen, D.R. Nygren, H. Ogelman, Ph. Olbrechts, C. Pérez de los Heros, A.C. Pohl, P.B. Price, G.T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, H.-G. Sander, T. Schmidt, D. Schneider, D. Seckel, M. Solarz, L. Sparke, G.M. Spiczak, C. Spiering, T. Stanev, D. Steele, P. Steffen, R.G. Stokstad, P. Sudhoff, K.-H. Sulanke, G.W. Sullivan, T. Sumners, I. Taboada, L. Thollander, S. Tilav, C. Walck, C. Weinheimer, C.H. Wiebusch, Ch. Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, Sh. Yoshida
IceCube is a large neutrino telescope of the next generation to be constructed in the Antarctic Ice Sheet near the South Pole. We present the conceptual design and the sensitivity of the IceCube detector to predicted fluxes of neutrinos, both atmosph
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fc129bb7b8384d43800b695db7beee78
http://arxiv.org/abs/astro-ph/0209556
http://arxiv.org/abs/astro-ph/0209556
Publikováno v:
X-Ray Astronomy in the Exosat Era ISBN: 9789401089067
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c6c3eb3a05d22f3054f4925e832568de
https://doi.org/10.1007/978-94-009-5448-9_20
https://doi.org/10.1007/978-94-009-5448-9_20
Conference
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Conference
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Akademický článek
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