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Wallace, B. Eberhardt, B. Eichmann, B. Hansmann, B. J. P. Jones, B. J. Whelan, B. Riedel, C. Arg\\\"uelles, C. Arguelles, C. Bohm, C.-C. F\\\"osig, C. De Clercq, C. Finley, C. Haack, Ch. Weaver, C. H. Wiebusch, C. Kopper, C. Kr\\\"uger, C. P\\'erez de los Heros, C. Pfendner, C. Raab, C. Rott, C. Spiering, C. Walck, C. Wendt, D. Altmann, D. Berley, D. Bindig, D. Bose, D. Chirkin, D. F. Cowen, D. G\\'ora, D. Grant, D. Hebecker, D. Heereman, D. J. Boersma, D. J. Koskinen, D. Lennarz, D. L. Xu, D. Pieloth, D. R. Nygren, D. R. Williams, D. Ryckbosch, D. Rysewyk, D. Seckel, D. Soldin, D. Tosi, D. V. Pankova, D. Z. Besson, E. Bernardini, E. Blaufuss, E. Cheung, E. del Pino Rosendo, E. Hansen, E. Jacobi, E. Middell, E. Pinat, E. Resconi, E. Unger, E. Woolsey, F. Bos, F. Halzen, F. Huang, F. McNally, G. Anton, G. Binder, G. C. Hill, G. de Wasseige, G. Golup, G. H. Collin, G. Kohnen, G. Kr\\\"uckl, G. Maggi, G. Merino, G. M. Spiczak, G. Neer, G. S. Japaridze, G. Te\\v{s}i\\'c, G. T. Przybylski, G. W. Sullivan, G. Yodh, H. Dembinski, H. Dujmovic, H. Kolanoski, H. Niederhausen, H. Pandya, H.-P. Bretz, H. Taavola, H. Wissing, I. Ansseau, IceCube Collaboration: M. G. Aartsen, I. Taboada, J. A. Aguilar, J. Adams, J. A. Pepper, J. Auffenberg, J. Becker Tjus, J. Braun, J. Casey, J. C. Davis, J. C. D\\'iaz-V\\'elez, J. Daughhetee, J. Feintzeig, J. Felde, J. Gallagher, J. G. Gonzalez, J. Hignight, J. J. Beatty, J. Kemp, J. Kiryluk, J. Kunnen, J. Leuner, J. L. Kelley, J. L. Lanfranchi, J. L\\\"unemann, J. Madsen, J. M. Conrad, J. P. A. M. de Andr\\'e, J. P. Dumm, J. Posselt, J. P. Yanez, J. Sandroos, J. Tatar, J. Vandenbroucke, J. van Santen, J. Veenkamp, K. Abraham, K. Andeen, K. B. M. Mahn, K. Clark, K. D. de Vries, K. D. Hoffman, K. Filimonov, K. Ghorbani, K. Hanson, K.-H. Becker, K. Helbing, K. Holzapfel, K. Hoshina, K. Hultqvist, K. Jero, K. Krings, K. Mase, K. Meagher, K. Rawlins, K. Satalecka, K. Wiebe, K. Woschnagg, L. Brayeur, L. Classen, L. Gerhardt, L. Gladstone, L. K\\\"opke, L. Lu, L. Mohrmann, L. R\\\"adel, L. Sabbatini, L. Schumacher, L. Wille, L. Wills, M. Ackermann, M. Ahlers, M. Ahrens, M. Archinger, M. Bissok, M. B\\\"orner, M. Casier, M. Day, M. de With, M. Dunkman, M. Glagla, M. Huber, M. Jeong, M. J. Larson, M. Jurkovic, M. Kauer, M. Kim, M. Kowalski, M. Kroll, M. Labare, M. Lesiak-Bzdak, M. Leuermann, M. Mandelartz, M. Medici, M. Meier, M. Moulai, M. N. Tobin, M. Quinnan, M. Rameez, M. Relich, M. Richman, M. Rongen, M. Schimp, M. Song, M. Stahlberg, M. Stamatikos, M. Sutherland, M. Tselengidou, M. Usner, M. van Rossem, M. Vehring, M. Voge, M. Vraeghe, M. Wallraff, M. Wolf, M. Zoll, N. Kurahashi, N. L. Strotjohann, N. van Eijndhoven, N. Wandkowsky, O. Botner, \\\"O. Penek, P. A. Evenson, P. A. Toale, P. Berghaus, P. B. Price, P. Desiati, P. Schlunder, R. Bay, R. Gaior, R. G. Stokstad, R. Hellauer, R. Hoffmann, R. Koirala, R. Konietz, R. Maruyama, R. Maunu, R. Nahnhauer, R. Reimann, R. Str\\\"om, S. Axani, S. BenZvi, S. Blot, S. B\\\"oser, S. C. Nowicki, S. Coenders, S. De Ridder, S. E. Sanchez Herrera, S. Euler, S. Fahey, S. Flis, S. Hickford, S. In, S. Kopper, S. Kunwar, S. Mancina, S. Miarecki, S. R. Klein, S. Robertson, S. Sarkar, S. Schoenen, S. Sch\\\"oneberg, S. Seunarine, S. Ter-Antonyan, S. Tilav, S. Toscano, S. Vallecorsa, S. Vanheule, S. W. Barwick, S. Westerhoff, S. Wickmann, S. Yoshida, T. Anderson, T. C. Arlen, T. DeYoung, T. Ehrhardt, T. Fuchs, T. Gl\\\"usenkamp, T. Hansmann, T. Karg, T. K. Gaisser, T. Kintscher, T. Kittler, T. Kuwabara, T. Menne, T. Meures, T. Montaruli, T. Palczewski, T. Ruhe, T. R. Wood, T. Schmidt, T. Stanev, T. Stezelberger, U. Katz, U. Naumann, V. Baum, V. di Lorenzo, W. Giang, W. Huelsnitz, W. Rhode, X. Bai, X. W. Xu, Y. Xu, Z. Griffith","submitted_at":"2016-11-11T21:02:23Z","abstract_excerpt":"The recent discovery of a diffuse cosmic neutrino flux extending up to PeV energies raises the question of which astrophysical sources generate this signal. 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