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Fox, B. Hoffmann, B. Ruzybayev, B. Semburg, C. Bohm, C. Colnard, C. De Clercq, C. Finley, C. Ha, Ch. Weaver, C. H. Wiebusch, C. P\\'erez de los Heros, C. Rott, C. Spiering, C. Walck, C. Wendt, C. Xu, D. Altmann, D. Berley, D. Bertrand, D. Bindig, D. Bose, D. Chirkin, D. F. Cowen, D. G\\'ora, D. Grant, D. Heinen, D. J. Boersma, D. J. Koskinen, D. L. Xu, D. Pieloth, D. R. Nygren, D. Rutledge, D. R. Williams, D. Ryckbosch, D. Seckel, D. Tosi, D. Z. Besson, E. A. Strahler, E. Bernardini, E. Blaufuss, E. Jacobi, E. Middell, E. Resconi, F. Clevermann, F. Descamps, F. Halzen, F. Kislat, F. Rothmaier, F. Yuan, G. C. Hill, G. de Vries-Uiterweerd, G. Kohnen, G. Kroll, G. M. Spiczak, G. S. Japaridze, G. T. Przybylski, G. W. Sullivan, G. Yodh, H.-G. Sander, H. Johansson, H. Kolanoski, H. Landsman, H. S. Matis, H. Taavola, H. Wissing, I. Taboada, J. A. Aguilar, J. Adams, J. A. Goodman, J. Auffenberg, J. Berdermann, J. Blumenthal, J. C. Davis, J. C. D\\'iaz-V\\'elez, J. Daughhetee, J. Dreyer, J. Eisch, J. Feintzeig, J. Gallagher, J.-H. K\\\"ohne, J. Jacobsen, J. J. Beatty, J. K. Becker, J. Kiryluk, J. L. Bazo Alba, J. L\\\"unemann, J. Madsen, J. Miller, J. P. Dumm, J. Petrovic, J.-P. H\\\"ul{\\ss}, J. Posselt, J. P. Rodrigues, J. P. Yanez, J. Vandenbroucke, J. van Santen, J. W. Nam, K. Andeen, K. Beattie, K. D. Hoffman, K. Filimonov, K. Han, K. Hanson, K.-H. Becker, K. Helbing, K.-H. Kampert, K. Hoshina, K. Hultqvist, K. Laihem, K. Mase, K. Meagher, K. Rawlins, K. S. Caballero-Mora, K. Schatto, K. Wiebe, K. Woschnagg, L. Demir\\\"ors, L. Gerhardt, L. Gladstone, L. K\\\"opke, L. Paul, M. Ackermann, M. Ahlers, M. Baker, M. Bissok, M. Carson, M. Danninger, M. Dierckxsens, M. Dunkman, M. Gurtner, M. J. Larson, M. Kowalski, M. Krasberg, M. Labare, M. L. Benabderrahmane, M. M. Allen, M. Merck, M. Olivo, M. Ribordy, M. Richman, M. Santander, M. Schunck, M. Stamatikos, M. St\\\"uer, M. V. D'Agostino, M. Vehring, M. Voge, M. Wallraff, M. Walter, M. Wolf, M. Zoll The ROTSE Collaboration: C. W. Akerlof, N. Kurahashi, N. Milke, N. van Eijndhoven, N. Whitehorn, O. Botner, O. Engdeg{\\aa}rd, O. Fadiran, O. Schulz, P. A. Evenson, P. A. Toale, P. Berghaus, P. B. Price, P. Desiati, P. Herquet, P. Kenny, P. M\\'esz\\'aros, P. O. Hulth, P. Redl, P. Zarzhitsky, Q. Swillens, R. Bay, R. Franke, R. G. Stokstad, R. Hellauer, R. Lauer, R. Maruyama, R. Morse, R. Nahnhauer, R. Porrata, R. Str\\\"om, R. W. Ellsworth, R. Wischnewski, S. Bechet, S. BenZvi, S. B\\\"oser, S. B. Pandey, S. Buitink, S. Cohen, S. Euler, S. Grullon, S. Hickford, S. H. Seo, S. Hussain, S. Kopper, S. Miarecki, S. M. Movit, S. Odrowski, S. Panknin, S. R. Klein, S. Sarkar, S. Seunarine, S. Ter-Antonyan, S. Tilav, S. Toscano, S. W. Barwick, S. Westerhoff, S. Yoshida, T. Abu-Zayyad, T. Degner, T. DeYoung, T. Feusels, T. Fischer-Wasels, T. Gl\\\"usenkamp, T. Griesel, The IceCube Collaboration: R. Abbasi, T. Karg, T. K. Gaisser, T. Kowarik, T. Kuwabara, T. Meures, T. Montaruli, T. Ruhe, T. R. Wood, T. Schmidt, T. Stanev, T. Stezelberger, T. Waldenmaier, U. Naumann, W. Huelsnitz, W. Rhode, W. Zheng, X. Bai, X. W. Xu, Y. Abdou, Y. Sestayo","submitted_at":"2011-11-30T02:02:51Z","abstract_excerpt":"Context. Transient neutrino sources such as Gamma-Ray Bursts (GRBs) and Supernovae (SNe) are hypothesized to emit bursts of high-energy neutrinos on a time-scale of \\lesssim 100 s. While GRB neutrinos would be produced in high relativistic jets, core-collapse SNe might host soft-relativistic jets, which become stalled in the outer layers of the progenitor star leading to an efficient production of high-energy neutrinos. Aims. 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Carson, M. Danninger, M. Dierckxsens, M. Dunkman, M. Gurtner, M. J. Larson, M. Kowalski, M. Krasberg, M. Labare, M. L. Benabderrahmane, M. M. Allen, M. Merck, M. Olivo, M. Ribordy, M. Richman, M. Santander, M. Schunck, M. Stamatikos, M. St\\\"uer, M. V. D'Agostino, M. Vehring, M. Voge, M. Wallraff, M. Walter, M. Wolf, M. Zoll The ROTSE Collaboration: C. W. Akerlof, N. Kurahashi, N. Milke, N. van Eijndhoven, N. Whitehorn, O. Botner, O. Engdeg{\\aa}rd, O. Fadiran, O. Schulz, P. A. Evenson, P. A. Toale, P. Berghaus, P. B. Price, P. Desiati, P. Herquet, P. Kenny, P. M\\'esz\\'aros, P. O. Hulth, P. Redl, P. Zarzhitsky, Q. Swillens, R. Bay, R. Franke, R. G. Stokstad, R. Hellauer, R. Lauer, R. Maruyama, R. Morse, R. Nahnhauer, R. Porrata, R. Str\\\"om, R. W. Ellsworth, R. Wischnewski, S. Bechet, S. BenZvi, S. B\\\"oser, S. B. Pandey, S. Buitink, S. Cohen, S. Euler, S. Grullon, S. Hickford, S. H. Seo, S. Hussain, S. Kopper, S. Miarecki, S. M. Movit, S. Odrowski, S. Panknin, S. R. Klein, S. Sarkar, S. Seunarine, S. Ter-Antonyan, S. Tilav, S. Toscano, S. W. Barwick, S. Westerhoff, S. Yoshida, T. Abu-Zayyad, T. Degner, T. DeYoung, T. Feusels, T. Fischer-Wasels, T. Gl\\\"usenkamp, T. Griesel, The IceCube Collaboration: R. Abbasi, T. Karg, T. K. Gaisser, T. Kowarik, T. Kuwabara, T. Meures, T. Montaruli, T. Ruhe, T. R. Wood, T. Schmidt, T. Stanev, T. Stezelberger, T. Waldenmaier, U. Naumann, W. Huelsnitz, W. Rhode, W. Zheng, X. Bai, X. W. Xu, Y. Abdou, Y. Sestayo","submitted_at":"2011-11-30T02:02:51Z","abstract_excerpt":"Context. Transient neutrino sources such as Gamma-Ray Bursts (GRBs) and Supernovae (SNe) are hypothesized to emit bursts of high-energy neutrinos on a time-scale of \\lesssim 100 s. While GRB neutrinos would be produced in high relativistic jets, core-collapse SNe might host soft-relativistic jets, which become stalled in the outer layers of the progenitor star leading to an efficient production of high-energy neutrinos. Aims. 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