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SEARCH FOR HIGH-ENERGY MUON NEUTRINOS FROM THE "NAKED-EYE" GRB 080319B WITH THE IceCube NEUTRINO TELESCOPE
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2009 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 701Article in journal (Refereed) Published
Abstract [en]

We report on a search with the IceCube detector for high-energy muon neutrinos from GRB 080319B, one of the brightest gamma-ray bursts (GRBs) ever observed. The fireball model predicts that a mean of 0.1 events should be detected by IceCube for a bulk Lorentz boost of the jet of 300. In both the direct on-time window of 66 s and an extended window of about 300 s around the GRB, no excess was found above background. The 90% CL upper limit on the number of track-like events from the GRB is 2.7, corresponding to a muon neutrino fluence limit of 9.5 x 10(-3) erg cm(-2) in the energy range between 120 TeV and 2.2 PeV, which contains 90% of the expected events.

Place, publisher, year, edition, pages
2009. Vol. 701
Keyword [en]
gamma rays: bursts methods: data analysis neutrinos telescopes gamma-ray bursts upper limits emission amanda tev variability selection fireballs 970417a physics Astronomy & Astrophysics
Research subject
SWEDARP, IceCube
Identifiers
URN: urn:nbn:se:polar:diva-1997DOI: 10.1088/0004-637x/701/2/1721OAI: oai:DiVA.org:polar-1997DiVA: diva2:814822
Note

ISI Document Delivery No.: 480UE Times Cited: 22 Cited Reference Count: 52 Abbasi, R. Abdou, Y. Abu-Zayyad, T. Adams, J. Aguilar, J. A. Ahlers, M. Andeen, K. Auffenberg, J. Bai, X. Baker, M. Barwick, S. W. Bay, R. Alba, J. L. Bazo Beattie, K. Beatty, J. J. Bechet, S. Becker, J. K. Becker, K. -H. Benabderrahmane, M. L. Berdermann, J. Berghaus, P. Berley, D. Bernardini, E. Bertrand, D. Besson, D. Z. Bissok, M. Blaufuss, E. Boersma, D. J. Bohm, C. Bolmont, J. Botner, O. Bradley, L. Braun, J. Breder, D. Castermans, T. Chirkin, D. Christy, B. Clem, J. Cohen, S. Cowen, D. F. D'Agostino, M. V. Danninger, M. Day, C. T. De Clercq, C. Demiroers, L. Depaepe, O. Descamps, F. Desiati, P. de Vries-Uiterweerd, G. DeYoung, T. Diaz-Velez, J. C. Dreyer, J. Dumm, J. P. Duvoort, M. R. Edwards, W. R. Ehrlich, R. Eisch, J. Ellsworth, R. W. Engdegard, O. Euler, S. Evenson, P. A. Fadiran, O. Fazely, A. R. Feusels, T. Filimonov, K. Finley, C. Foerster, M. M. Fox, B. D. Franckowiak, A. Franke, R. Gaisser, T. K. Gallagher, J. Ganugapati, R. Gerhardt, L. Gladstone, L. Goldschmidt, A. Goodman, J. A. Gozzini, R. Grant, D. Griesel, T. Gross, A. Grullon, S. Gunasingha, R. M. Gurtner, M. Ha, C. Hallgren, A. Halzen, F. Han, K. Hanson, K. Hasegawa, Y. Heise, J. Helbing, K. Herquet, P. Hickford, S. Hill, G. C. Hoffman, K. D. Hoshina, K. Hubert, D. Huelsnitz, W. Huelss, J.-P. Hulth, P. O. Hultqvist, K. Hussain, S. Imlay, R. L. Inaba, M. Ishihara, A. Jacobsen, J. Japaridze, G. S. Johansson, H. Joseph, J. M. Kampert, K. -H. Kappes, A. Karg, T. Karle, A. Kelley, J. L. Kenny, P. Kiryluk, J. Kislat, F. Klein, S. R. Knops, S. Kohnen, G. Kolanoski, H. Koepke, L. Kowalski, M. Kowarik, T. Krasberg, M. Kuehn, K. Kuwabara, T. Labare, M. Lafebre, S. Laihem, K. Landsman, H. Lauer, R. Lennarz, D. Lucke, A. Lundberg, J. Luenemann, J. Madsen, J. Majumdar, P. Maruyama, R. Mase, K. Matis, H. S. McParland, C. P. Meagher, K. Merck, M. Meszaros, P. Middell, E. Milke, N. Miyamoto, H. Mohr, A. Montaruli, T. Morse, R. Movit, S. M. Muenich, K. Nahnhauer, R. Nam, J. W. Niessen, P. Nygren, D. R. Odrowski, S. Olivas, A. Olivo, M. Ono, M. Panknin, S. Patton, S. de los Heros, C. Perez Petrovic, J. Piegsa, A. Pieloth, D. Pohl, A. C. Porrata, R. Potthoff, N. Price, P. B. Prikockis, M. Przybylski, G. T. Rawlins, K. Redl, P. Resconi, E. Rhode, W. Ribordy, M. Rizzo, A. Rodrigues, J. P. Roth, P. Rothmaier, F. Rott, C. Roucelle, C. Rutledge, D. Ryckbosch, D. Sander, H. -G. Sarkar, S. Schlenstedt, S. Schmidt, T. Schneider, D. Schukraft, A. Schulz, O. Schunck, M. Seckel, D. Semburg, B. Seo, S. H. Sestayo, Y. Seunarine, S. Silvestri, A. Slipak, A. Spiczak, G. M. Spiering, C. Stamatikos, M. Stanev, T. Stephens, G. Stezelberger, T. Stokstad, R. G. Stoufer, M. C. Stoyanov, S. Strahler, E. A. Straszheim, T. Sulanke, K. -H. Sullivan, G. W. Swillens, Q. Taboada, I. Tamburro, A. Tarasova, O. Tepe, A. Ter-Antonyan, S. Terranova, C. Tilav, S. Toale, P. A. Tosi, D. Turcan, D. van Eijndhoven, N. Vandenbroucke, J. Van Overloop, A. Voigt, B. Walck, C. Waldenmaier, T. Walter, M. Wendt, C. Westerhoff, S. Whitehorn, N. Wiebusch, C. H. Wiedemann, A. Wikstrom, G. Williams, D. R. Wischnewski, R. Wissing, H. Woschnagg, K. Xu, X. W. Yodh, G. Yoshida, S. Beatty, James/D-9310-2011; Wiebusch, Christopher/G-6490-2012; Kowalski, Marek/G-5546-2012; Tamburro, Alessio/A-5703-2013; Botner, Olga/A-9110-2013; Hallgren, Allan/A-8963-2013; Sarkar, Subir/G-5978-2011; Tjus, Julia/G-8145-2012; Auffenberg, Jan/D-3954-2014 Sarkar, Subir/0000-0002-3542-858X; Auffenberg, Jan/0000-0002-1185-9094 U.S. National Science Foundation-Office; U.S. National Science Foundation-Physics Division; University of Wisconsin Alumni Research Foundation; U.S. Department of Energy; National Energy Research Scientific Computing Center; Louisiana Optical Network Initiative (LONI); Swedish Research Council; Swedish Polar Research Secretariat; Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research (BMBF); Deutsche Forschungsgemeinschaft (DFG), Germany; Fund for Scientific Research (FNRS-FWO); Flanders Institute to encourage scientific and technological research in industry (IWT); Belgian Federal Science Policy Office (Belspo); Netherlands Organisation for Scientific Research(NWO); Marsden Fund, New Zealand; SNF (Switzerland); EU Marie Curie OIF Program; Capes Foundation, Ministry of Education of Brazil We acknowledge the support from the following agencies: U.S. National Science Foundation-Office of Polar Program, U.S. National Science Foundation-Physics Division, University of Wisconsin Alumni Research Foundation, U.S. Department of Energy, and National Energy Research Scientific Computing Center, the Louisiana Optical Network Initiative (LONI) grid computing resources; Swedish Research Council, Swedish Polar Research Secretariat, and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research (BMBF), Deutsche Forschungsgemeinschaft (DFG), Germany; Fund for Scientific Research (FNRS-FWO), Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); the Netherlands Organisation for Scientific Research(NWO); Marsden Fund, New Zealand; M. R. acknowledges the support of the SNF (Switzerland); A. K. and A. G. acknowledge support by the EU Marie Curie OIF Program; J. P. R. acknowledge support by the Capes Foundation, Ministry of Education of Brazil. 22 Iop publishing ltd Bristol Astronomy & Astrophysics

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Citation style
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