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Anatoli Fedynitch
Researcher at Ruhr University Bochum
Publications - 175
Citations - 12811
Anatoli Fedynitch is an academic researcher from Ruhr University Bochum. The author has contributed to research in topics: Neutrino & Neutrino detector. The author has an hindex of 51, co-authored 138 publications receiving 11462 citations. Previous affiliations of Anatoli Fedynitch include University of Tokyo & Karlsruhe Institute of Technology.
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Journal ArticleDOI
Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
M. G. Aartsen,Rasha Abbasi,Y. Abdou,Markus Ackermann,Jenni Adams,Juanan Aguilar,Markus Ahlers,D. Altmann,J. Auffenberg,X. Bai,Michael J. Baker,S. W. Barwick,V. Baum,R. C. Bay,J. J. Beatty,S. Bechet,J. Becker Tjus,K.-H. Becker,M. L. Benabderrahmane,Segev BenZvi,P. Berghaus,D. Berley,Elisa Bernardini,A. Bernhard,D. Bertrand,D. Z. Besson,Gary Binder,Gary Binder,Daniel Bindig,M. Bissok,E. Blaufuss,J. Blumenthal,D. J. Boersma,S. Bohaichuk,C. Bohm,D. Bose,S. Böser,Olga Botner,L. Brayeur,H.-P. Bretz,A. M. Brown,R. Bruijn,Jürgen Brunner,M. J. Carson,J. Casey,M. Casier,Dmitry Chirkin,A. Christov,B. Christy,K. Clark,F. Clevermann,S. Coenders,Seth M. Cohen,D. F. Cowen,A. H. Cruz Silva,M. Danninger,J. Daughhetee,J. C. Davis,M. Day,C. De Clercq,S. De Ridder,Paolo Desiati,K. D. de Vries,Tyce DeYoung,Juan Carlos Diaz-Velez,Matt Dunkman,R. Eagan,B. Eberhardt,B. Eichmann,J. Eisch,R. W. Ellsworth,S. Euler,Paul Evenson,O. Fadiran,A. R. Fazely,Anatoli Fedynitch,J. Feintzeig,T. Feusels,Kirill Filimonov,Chad Finley,T. Fischer-Wasels,S. Flis,A. Franckowiak,K. Frantzen,T. Fuchs,Thomas K. Gaisser,J. C. Gallagher,L. Gerhardt,L. Gerhardt,L. Gladstone,Thorsten Glusenkamp,A. Goldschmidt,G. Golup,J. G. Gonzalez,J. A. Goodman,Dariusz Gora,Dylan T. Grandmont +96 more
TL;DR: The presence of a high-energy neutrino flux containing the most energetic neutrinos ever observed is revealed, including 28 events at energies between 30 and 1200 TeV, although the origin of this flux is unknown and the findings are consistent with expectations for a neutRino population with origins outside the solar system.
Journal ArticleDOI
Observation of high-energy astrophysical neutrinos in three years of icecube data
M. G. Aartsen,Markus Ackermann,Jenni Adams,Juanan Aguilar,Markus Ahlers,Maryon Ahrens,D. Altmann,T. Anderson,Carlos Arguelles,T. C. Arlen,J. Auffenberg,Xinhua Bai,Steven W. Barwick,V. Baum,J. J. Beatty,J. Becker Tjus,K.-H. Becker,Segev BenZvi,P. Berghaus,D. Berley,Elisa Bernardini,A. Bernhard,D. Z. Besson,G. Binder,G. Binder,Daniel Bindig,M. Bissok,E. Blaufuss,J. Blumenthal,D. J. Boersma,Christian Bohm,D. Bose,S. Böser,Olga Botner,L. Brayeur,H.-P. Bretz,A. M. Brown,J. Casey,M. Casier,Dmitry Chirkin,A. Christov,B. Christy,K. Clark,L. Classen,F. Clevermann,S. Coenders,D. F. Cowen,A. H. Cruz Silva,M. Danninger,J. Daughhetee,J. C. Davis,M. Day,J. P. A. M. de André,C. De Clercq,S. De Ridder,Paolo Desiati,K. D. de Vries,Tyce DeYoung,J. C. Díaz-Vélez,Matt Dunkman,R. Eagan,B. Eberhardt,B. Eichmann,J. Eisch,S. Euler,Paul Evenson,O. Fadiran,A. R. Fazely,Anatoli Fedynitch,J. Feintzeig,J. Felde,T. Feusels,Kirill Filimonov,Chad Finley,T. Fischer-Wasels,S. Flis,A. Franckowiak,K. Frantzen,T. Fuchs,Thomas K. Gaisser,Jay Gallagher,L. Gerhardt,L. Gerhardt,D. Gier,L. Gladstone,Thorsten Glusenkamp,A. Goldschmidt,G. Golup,Javier Gonzalez,J. A. Goodman,Dariusz Gora,D. T. Grandmont,Darren Grant,P. Gretskov,J. C. Groh,Axel Groß,C. Ha,C. Ha,C. Haack,A. Haj Ismail,P. Hallen,Allan Hallgren,Francis Halzen,Kael Hanson,Dustin Hebecker,D. Heereman,Dirk Heinen,K. Helbing,R. Hellauer,D. Hellwig,S. Hickford,G. C. Hill,Kara Hoffman,R. Hoffmann,A. Homeier,K. Hoshina,F. Huang,W. Huelsnitz,P. O. Hulth,Klas Hultqvist,S. Hussain,Aya Ishihara,E. Jacobi,J. E. Jacobsen,K. Jagielski,George Japaridze,K. Jero,O. Jlelati,M. Jurkovic,B. Kaminsky,Alexander Kappes,Timo Karg,Albrecht Karle,M. Kauer,J. L. Kelley,Ali Kheirandish,J. Kiryluk,J. Kläs,Spencer Klein,Spencer Klein,J.-H. Köhne,G. Kohnen,Hermann Kolanoski,A. Koob,L. Köpke,C. Kopper,Sandro Kopper,D. J. Koskinen,M. Kowalski,A. Kriesten,K. Krings,G. Kroll,J. Kunnen,Naoko Kurahashi,Takao Kuwabara,M. Labare,D. T. Larsen,M. J. Larson,M. Lesiak-Bzdak,M. Leuermann,J. Leute,J. Lünemann,Oscar Macias,James Madsen,Giorgio Maggi,Reina H. Maruyama,K. Mase,H. S. Matis,Frank McNally,K. Meagher,A. Meli,Thomas Meures,S. Miarecki,S. Miarecki,E. Middell,E. Middlemas,N. Milke,J. Miller,L. Mohrmann,Teresa Montaruli,R. Morse,R. Nahnhauer,U. Naumann,Hans Niederhausen,Sarah Nowicki,Dave Nygren,A. Obertacke,S. Odrowski,A. Olivas,A. Omairat,A. O'Murchadha,T. Palczewski,Larissa Paul,Ö. Penek,Joshua Pepper,C. Pérez de los Heros,C. Pfendner,Damian Pieloth,E. Pinat,J. Posselt,P. B. Price,Gerald Przybylski,J. Pütz,M. Quinnan,L. Rädel,Mohamed Rameez,K. Rawlins,P. Redl,I. Rees,René Reimann,Elisa Resconi,Wolfgang Rhode,Mike Richman,Benedikt Riedel,Sally Robertson,J. P. Rodrigues,Martin Rongen,Carsten Rott,Tim Ruhe,B. Ruzybayev,Dirk Ryckbosch,S. M. Saba,H. G. Sander,Marcos Santander,Subir Sarkar,Subir Sarkar,K. Schatto,F. Scheriau,T. O. B. Schmidt,M. Schmitz,S. Schoenen,S. Schöneberg,A. Schönwald,A. Schukraft,L. Schulte,O. Schulz,D. Seckel,Y. Sestayo,S. Seunarine,Rezo Shanidze,C. Sheremata,M. W. E. Smith,Dennis Soldin,Glenn Spiczak,Christian Spiering,Michael Stamatikos,Todor Stanev,N. A. Stanisha,A. Stasik,T. Stezelberger,R. G. Stokstad,A. Stößl,E. A. Strahler,R. Ström,N. L. Strotjohann,G. W. Sullivan,H. Taavola,Ignacio Taboada,A. Tamburro,A. Tepe,Samvel Ter-Antonyan,A. Terliuk,G. Tešić,S. Tilav,P. A. Toale,M. N. Tobin,Delia Tosi,Maria Tselengidou,E. Unger,M. Usner,Sofia Vallecorsa,N. van Eijndhoven,Justin Vandenbroucke,J. van Santen,M. Vehring,M. Voge,Matthias Vraeghe,C. Walck,M. Wallraff,Ch. Weaver,M. Wellons,Chris Wendt,S. Westerhoff,B. J. Whelan,Nathan Whitehorn,Nathan Whitehorn,C. Wichary,K. Wiebe,Christopher Wiebusch,Dawn Williams,H. Wissing,Matthias Wolf,T. R. Wood,Kurt Woschnagg,Donglian Xu,Xianwu Xu,J. P. Yanez,G. B. Yodh,S. Yoshida,P. Zarzhitsky,J. Ziemann,S. Zierke,M. Zoll +302 more
TL;DR: Results from an analysis with a third year of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV-PeV range at the level of 10(-8) GeV cm-2 s-1 sr-1 per flavor and reject a purely atmospheric explanation for the combined three-year data at 5.7σ.
Journal ArticleDOI
First observation of PeV-energy neutrinos with IceCube
M. G. Aartsen,Rasha Abbasi,Y. Abdou,Markus Ackermann,Jenni Adams,Juanan Aguilar,Markus Ahlers,D. Altmann,J. Auffenberg,Xinhua Bai,Michael J. Baker,Steven W. Barwick,V. Baum,R. C. Bay,J. J. Beatty,S. Bechet,J. Becker Tjus,K. H. Becker,Michael S. Bell,M. L. Benabderrahmane,Segev BenZvi,J. Berdermann,P. Berghaus,D. Berley,Elisa Bernardini,A. Bernhard,D. Bertrand,D. Z. Besson,Gary Binder,Gary Binder,Daniel Bindig,M. Bissok,E. Blaufuss,J. Blumenthal,D. J. Boersma,S. Bohaichuk,Christian Bohm,D. Bose,S. Böser,Olga Botner,L. Brayeur,H.-P. Bretz,A. M. Brown,R. Bruijn,Jürgen Brunner,M. J. Carson,J. Casey,M. Casier,Dmitry Chirkin,A. Christov,B. Christy,K. Clark,F. Clevermann,S. Coenders,Seth M. Cohen,D. F. Cowen,A. H. Cruz Silva,M. Danninger,J. Daughhetee,J. C. Davis,C. De Clercq,S. De Ridder,Paolo Desiati,Tyce DeYoung,J. C. Díaz-Vélez,Matt Dunkman,R. Eagan,B. Eberhardt,J. Eisch,R. W. Ellsworth,S. Euler,Paul Evenson,O. Fadiran,A. R. Fazely,Anatoli Fedynitch,J. Feintzeig,T. Feusels,Kirill Filimonov,Chad Finley,T. Fischer-Wasels,S. Flis,A. Franckowiak,R. Franke,K. Frantzen,T. Fuchs,Thomas K. Gaisser,Jay Gallagher,L. Gerhardt,L. Gerhardt,L. Gladstone,Thorsten Glusenkamp,A. Goldschmidt,G. Golup,Javier Gonzalez,J. A. Goodman,Dariusz Gora,Darren Grant,Axel Groß,M. Gurtner,C. Ha,C. Ha,A. Haj Ismail,P. Hallen,Allan Hallgren,Francis Halzen,Kael Hanson,D. Heereman,Dirk Heinen,K. Helbing,R. Hellauer,S. Hickford,G. C. Hill,Kara Hoffman,R. Hoffmann,A. Homeier,K. Hoshina,W. Huelsnitz,P. O. Hulth,Klas Hultqvist,S. Hussain,Aya Ishihara,E. Jacobi,J. E. Jacobsen,K. Jagielski,George Japaridze,K. Jero,O. Jlelati,B. Kaminsky,Alexander Kappes,Timo Karg,Albrecht Karle,J. L. Kelley,J. Kiryluk,Fabian Kislat,J. Kläs,Spencer Klein,Spencer Klein,J.-H. Köhne,G. Kohnen,Hermann Kolanoski,L. Köpke,C. Kopper,Sandro Kopper,D. J. Koskinen,M. Kowalski,M. Krasberg,K. Krings,G. Kroll,J. Kunnen,Naoko Kurahashi,Takao Kuwabara,M. Labare,H. Landsman,M. J. Larson,M. Lesiak-Bzdak,M. Leuermann,J. Leute,J. Lünemann,James Madsen,Reina H. Maruyama,K. Mase,H. S. Matis,Frank McNally,K. Meagher,M. Merck,Peter Mészáros,Thomas Meures,S. Miarecki,S. Miarecki,E. Middell,N. Milke,J. Miller,L. Mohrmann,Teresa Montaruli,R. Morse,R. Nahnhauer,U. Naumann,Hans Niederhausen,Sarah Nowicki,Dave Nygren,A. Obertacke,S. Odrowski,A. Olivas,M. Olivo,A. O'Murchadha,Larissa Paul,Joshua Pepper,C. Pérez de los Heros,C. Pfendner,Damian Pieloth,E. Pinat,N. Pirk,J. Posselt,P. B. Price,Gerald Przybylski,L. Rädel,Mohamed Rameez,K. Rawlins,P. Redl,René Reimann,Elisa Resconi,Wolfgang Rhode,M. Ribordy,M. Richman,Benedikt Riedel,J. P. Rodrigues,Carsten Rott,Tim Ruhe,B. Ruzybayev,Dirk Ryckbosch,S. M. Saba,T. Salameh,H. G. Sander,Marcos Santander,Subir Sarkar,K. Schatto,M. Scheel,F. Scheriau,T. O. B. Schmidt,M. Schmitz,S. Schoenen,S. Schöneberg,A. Schönwald,A. Schukraft,L. Schulte,O. Schulz,D. Seckel,Y. Sestayo,S. Seunarine,C. Sheremata,M. W. E. Smith,M. Soiron,Dennis Soldin,Glenn Spiczak,Christian Spiering,Michael Stamatikos,Todor Stanev,A. Stasik,T. Stezelberger,R. G. Stokstad,A. Stößl,E. A. Strahler,R. Ström,G. W. Sullivan,H. Taavola,Ignacio Taboada,A. Tamburro,Samvel Ter-Antonyan,G. Tešić,S. Tilav,P. A. Toale,Simona Toscano,M. Usner,D. van der Drift,D. van der Drift,N. van Eijndhoven,A. Van Overloop,J. van Santen,M. Vehring,M. Voge,Matthias Vraeghe,C. Walck,T. Waldenmaier,M. Wallraff,R. Wasserman,Ch. Weaver,M. Wellons,Chris Wendt,S. Westerhoff,Nathan Whitehorn,K. Wiebe,Christopher Wiebusch,Dawn Williams,H. Wissing,Matthias Wolf,T. R. Wood,Kurt Woschnagg,Chun Xu,Donglian Xu,Xianwu Xu,J. P. Yanez,G. B. Yodh,S. Yoshida,P. Zarzhitsky,J. Ziemann,S. Zierke,A. Zilles,M. Zoll +287 more
TL;DR: These two neutrino-induced events could be a first indication of an astrophysical neutrinos flux; the moderate significance, however, does not permit a definitive conclusion at this time.
Journal ArticleDOI
A combined maximum-likelihood analysis of the high-energy astrophysical neutrino flux measured with icecube
M. G. Aartsen,K. Abraham,Markus Ackermann,Jenni Adams,Juanan Aguilar,Markus Ahlers,Maryon Ahrens,D. Altmann,T. Anderson,M. Archinger,Carlos Arguelles,T. C. Arlen,J. Auffenberg,Xinhua Bai,Steven W. Barwick,V. Baum,R. C. Bay,J. J. Beatty,J. Becker Tjus,K.-H. Becker,E. Beiser,Segev BenZvi,P. Berghaus,D. Berley,Elisa Bernardini,A. Bernhard,D. Z. Besson,G. Binder,G. Binder,D. Bindig,M. Bissok,E. Blaufuss,J. Blumenthal,D. J. Boersma,Christian Bohm,M. Börner,F. Bos,D. Bose,S. Böser,Olga Botner,J. Braun,L. Brayeur,H.-P. Bretz,A. M. Brown,N. Buzinsky,J. Casey,M. Casier,E. Cheung,Dmitry Chirkin,A. Christov,B. Christy,K. Clark,L. Classen,S. Coenders,D. F. Cowen,A. H. Cruz Silva,J. Daughhetee,J. C. Davis,M. Day,J. P. A. M. de André,C. De Clercq,H. Dembinski,S. De Ridder,Paolo Desiati,K. D. de Vries,G. de Wasseige,Tyce DeYoung,J. C. Díaz-Vélez,J. P. Dumm,M. Dunkman,R. Eagan,B. Eberhardt,T. Ehrhardt,B. Eichmann,S. Euler,Paul Evenson,O. Fadiran,S. Fahey,A. R. Fazely,Anatoli Fedynitch,J. Feintzeig,J. Felde,Kirill Filimonov,C. Finley,T. Fischer-Wasels,S. Flis,T. Fuchs,Thomas K. Gaisser,R. Gaior,Jay Gallagher,L. Gerhardt,L. Gerhardt,Karim Ghorbani,D. Gier,L. Gladstone,M. Glagla,T. Glüsenkamp,A. Goldschmidt,G. Golup,Javier Gonzalez,J. A. Goodman,Dariusz Gora,Darren Grant,P. Gretskov,J. C. Groh,A. Gross,C. Ha,C. Ha,C. Haack,A. Haj Ismail,Allan Hallgren,Francis Halzen,B. Hansmann,Kael Hanson,D. Hebecker,D. Heereman,K. Helbing,R. Hellauer,D. Hellwig,S. Hickford,Joshua Hignight,G. C. Hill,Kara Hoffman,R. Hoffmann,K. Holzapfel,A. Homeier,K. Hoshina,K. Hoshina,F. Huang,M. E. Huber,W. Huelsnitz,P. O. Hulth,Klas Hultqvist,S. In,Aya Ishihara,E. Jacobi,George Japaridze,K. Jero,M. Jurkovic,B. Kaminsky,Alexander Kappes,T. Karg,Albrecht Karle,M. Kauer,M. Kauer,Azadeh Keivani,J. L. Kelley,J. Kemp,Ali Kheirandish,J. Kiryluk,J. Kläs,Spencer Klein,Spencer Klein,G. Kohnen,Hermann Kolanoski,R. Konietz,A. Koob,Lutz Kopke,C. Kopper,S. Kopper,D. J. Koskinen,M. Kowalski,K. Krings,G. Kroll,M. Kroll,J. Kunnen,N. Kurahashi,T. Kuwabara,M. Labare,J. L. Lanfranchi,M. J. Larson,M. Lesiak-Bzdak,M. Leuermann,J. Leuner,J. Lünemann,James Madsen,G. Maggi,Kendall Mahn,Reina H. Maruyama,K. Mase,H. S. Matis,R. Maunu,F. McNally,K. Meagher,M. Medici,A. Meli,T. Menne,G. Merino,Thomas Meures,S. Miarecki,S. Miarecki,E. Middell,E. Middlemas,J. Miller,L. Mohrmann,Teresa Montaruli,R. Morse,R. Nahnhauer,U. Naumann,H. Niederhausen,S. C. Nowicki,Dave Nygren,A. Obertacke,A. Olivas,A. Omairat,Aongus O'Murchadha,T. Palczewski,Larissa Paul,Joshua Pepper,C. Pérez de los Heros,C. Pfendner,Damian Pieloth,E. Pinat,J. Posselt,P. B. Price,Gerald Przybylski,J. Pütz,M. Quinnan,L. Rädel,M. Rameez,K. Rawlins,P. Redl,R. Reimann,M. Relich,Elisa Resconi,Wolfgang Rhode,Mike Richman,S. Richter,B. Riedel,Sally Robertson,M. Rongen,Carsten Rott,T. Ruhe,B. Ruzybayev,D. Ryckbosch,S. M. Saba,L. Sabbatini,H. G. Sander,A. Sandrock,J. Sandroos,Subir Sarkar,Subir Sarkar,K. Schatto,F. Scheriau,M. Schimp,T. Schmidt,M. Schmitz,S. Schoenen,S. Schöneberg,A. Schönwald,A. Schukraft,L. Schulte,D. Seckel,S. Seunarine,Rezo Shanidze,M. W. E. Smith,D. Soldin,Glenn Spiczak,Christian Spiering,M. Stahlberg,Michael Stamatikos,Michael Stamatikos,Todor Stanev,N. A. Stanisha,A. Stasik,T. Stezelberger,R. G. Stokstad,A. Stössl,E. A. Strahler,R. Ström,N. L. Strotjohann,G. W. Sullivan,Michael Sutherland,H. Taavola,Ignacio Taboada,Samvel Ter-Antonyan,A. Terliuk,G. Tešić,S. Tilav,P. A. Toale,M. N. Tobin,D. Tosi,M. Tselengidou,E. Unger,M. Usner,Sofia Vallecorsa,Justin Vandenbroucke,N. van Eijndhoven,Stijn Vanheule,J. van Santen,J. Veenkamp,M. Vehring,M. Voge,M. Vraeghe,C. Walck,A. Wallace,M. Wallraff,N. Wandkowsky,Ch. Weaver,Chris Wendt,S. Westerhoff,B. J. Whelan,Nathan Whitehorn,C. Wichary,K. Wiebe,Christopher Wiebusch,L. Wille,Dawn Williams,H. Wissing,M. Wolf,T. R. Wood,Kurt Woschnagg,Donglian Xu,Xianwu Xu,Y. Xu,J. P. Yanez,G. B. Yodh,S. Yoshida,P. Zarzhitsky,M. Zoll +319 more
TL;DR: In this article, the results from six different IceCube searches for astrophysical neutrinos in a maximum-likelihood analysis are combined, and the combined event sample features high-statistics samples of shower-like and track-like events.
Journal ArticleDOI
An absence of neutrinos associated with cosmic-ray acceleration in γ-ray bursts
Rasha Abbasi,Y. Abdou,T. Abu-Zayyad,Markus Ackermann,Jenni Adams,Juanan Aguilar,Markus Ahlers,D. Altmann,Karen Andeen,J. Auffenberg,Xinhua Bai,Xinhua Bai,Michael J. Baker,Steven W. Barwick,R. C. Bay,J. L. Bazo Alba,K. Beattie,J. J. Beatty,S. Bechet,J. K. Becker,K. H. Becker,Michael S. Bell,M. L. Benabderrahmane,Segev BenZvi,J. Berdermann,P. Berghaus,D. Berley,Elisa Bernardini,D. Bertrand,D. Z. Besson,Daniel Bindig,M. Bissok,E. Blaufuss,J. Blumenthal,D. J. Boersma,Christian Bohm,D. Bose,S. Boeser,Olga Botner,L. Brayeur,A. M. Brown,Stijn Buitink,Karen S. Caballero-Mora,M. J. Carson,M. Casier,Dmitry Chirkin,B. Christy,F. Clevermann,Seth M. Cohen,C. Colnard,D. F. Cowen,A. H. Cruz Silva,M. V. D'Agostino,M. Danninger,J. Daughhetee,J. C. Davis,C. DeClercq,T. Degner,F. Descamps,Paolo Desiati,G. de Vries-Uiterweerd,Tyce DeYoung,J. C. Díaz-Vélez,M. Dierckxsens,J. Dreyer,Jon Dumm,Matt Dunkman,J. Eisch,R. W. Ellsworth,O. Engdegård,S. Euler,Paul Evenson,O. Fadiran,A. R. Fazely,Anatoli Fedynitch,J. Feintzeig,T. Feusels,Kirill Filimonov,Chad Finley,T. Fischer-Wasels,S. Flis,A. Franckowiak,R. Franke,Thomas K. Gaisser,Jay Gallagher,L. Gerhardt,L. Gerhardt,L. Gladstone,T. Gluesenkamp,A. Goldschmidt,J. A. Goodman,Dariusz Gora,Darren Grant,T. Griesel,A. Gross,S. Grullon,M. Gurtner,C. Ha,C. Ha,A. Haj Ismail,Allan Hallgren,Francis Halzen,K. Han,Kael Hanson,D. Heereman,Dirk Heinen,K. Helbing,R. Hellauer,S. Hickford,G. C. Hill,Kara Hoffman,B. Hoffmann,A. Homeier,K. Hoshina,W. Huelsnitz,W. Huelsnitz,J. P. Huelss,P. O. Hulth,Klas Hultqvist,S. Hussain,Aya Ishihara,E. Jacobi,J. E. Jacobsen,S. Japaridze,H. A. B. Johansson,Alexander Kappes,Timo Karg,Albrecht Karle,J. Kiryluk,Fabian Kislat,Spencer Klein,Spencer Klein,J. H. Koehne,G. Kohnen,Hermann Kolanoski,L. Koepke,Sandro Kopper,D. J. Koskinen,M. Kowalski,T. Kowarik,M. Krasberg,G. Kroll,J. Kunnen,Naoko Kurahashi,Takao Kuwabara,M. Labare,K. Laihem,H. Landsman,M. J. Larson,R. J. Lauer,J. Luenemann,James Madsen,A. Marotta,Reina H. Maruyama,K. Mase,H. S. Matis,K. Meagher,M. Merck,P. Meszaros,Thomas Meures,S. Miarecki,S. Miarecki,E. Middell,N. Milke,J. Miller,Teresa Montaruli,R. Morse,S. M. Movit,R. Nahnhauer,J. W. Nam,U. Naumann,Sarah Nowicki,Dave Nygren,S. Odrowski,A. Olivas,M. Olivo,Aongus O'Murchadha,S. Panknin,Larissa Paul,C. Pérez de los Heros,A. Piegsa,Damian Pieloth,J. Posselt,P. B. Price,Gerald Przybylski,K. Rawlins,P. Redl,Elisa Resconi,Wolfgang Rhode,M. Ribordy,M. Richman,Benedikt Riedel,A. Rizzo,J. P. Rodrigues,F. Rothmaier,Carsten Rott,Tim Ruhe,D. Rutledge,B. Ruzybayev,Dirk Ryckbosch,H. G. Sander,Marcos Santander,Subir Sarkar,K. Schatto,T. O. B. Schmidt,S. Schoeneberg,A. Schoenwald,A. Schukraft,L. Schulte,A. Schultes,O. Schulz,O. Schulz,M. Schunck,D. Seckel,B. Semburg,S. H. Seo,Y. Sestayo,S. Seunarine,A. Silvestri,M. W. E. Smith,Glenn Spiczak,Christian Spiering,M. Stamatikos,M. Stamatikos,Todor Stanev,T. Stezelberger,R. G. Stokstad,A. Stoessl,E. A. Strahler,R. Stroem,M. Stueer,G. W. Sullivan,H. Taavola,Ignacio Taboada,A. Tamburro,Samvel Ter-Antonyan,S. Tilav,P. A. Toale,Simona Toscano,D. Tosi,N. van Eijndhoven,A. Van Overloop,J. van Santen,M. Vehring,M. Voge,C. Walck,T. Waldenmaier,M. Wallraff,M. Walter,R. Wasserman,Ch. Weaver,Chris Wendt,S. Westerhoff,Nathan Whitehorn,K. Wiebe,Christopher Wiebusch,Dawn Williams,R. Wischnewski,H. Wissing,Matthias Wolf,T. R. Wood,Kurt Woschnagg,Chun Xu,Donglian Xu,Xianwu Xu,J. P. Yanez,G. B. Yodh,S. Yoshida,P. Zarzhitsky,M. Zoll +269 more
TL;DR: An upper limit on the flux of energetic neutrinos associated with GRBs that is at least a factor of 3.7 below the predictions is reported, implying either that GRBs are not the only sources of cosmic rays with energies exceeding 1018 electronvolts or that the efficiency of neutrino production is much lower than has been predicted.