The IceCube Collaboration

@inproceedings{Achterberg2005TheIC,
  title={The IceCube Collaboration},
  author={Abraham Achterberg and Markus Ackermann and James P Ahrens and Xinhua Bai and B. Baret and Michael Bartelt and Ryan Bay and K. Beattie and T. Becka and Patrick Berghaus and David Berley and Elisa Bernardini and Daniel Bertrand and Erik Blaufuss and Olga Botner and Adam Bouchta and J. Braun and Thomas Burgess and Thierry Castermans and Dmitry Chirkin and John Mason Clem and J. Conrad and Anna Davour and Catherine De Clercq and Paolo Desiati and Tyce DeYoung and Jens Dreyer and Robert Ehrlich and Thomas Feser and Kirill Filimonov and Thomas K. Gaisser and R. Ganugapati and Heiko Geenen and Lisa Marie Gerhardt and Azriel Goldschmidt and Jordan A. Goodman and Allan Hallgren and Francis Halzen and David Hardtke and R. Hardtke and T. Harenberg and T. Hauschildt and D. Hays and John Heise and Klaus Helbing and Martin F. Hellwig and Ph. Herquet and Daan Hubert and Brennan Hughey and Klas Hultqvist and Stephan Hundertmark and Aya Ishihara and Janet S. Jacobsen and Abbie N Jones and Albrecht Karle and Hisashi Kawai and John Lawrence Kelley and S. Klepser and Georges Kohnen and Hermann Kolanoski and Mark Krasberg and Kyler W. Kuehn and Edward Kujawski and Hagar Landsman and Rodrigo Guedes Lang and Henri Leich and Igor Liubarsky and Johan Lundberg and J. Madsen and Pawel Marciniewski and Keiichi Mase and T. McCauley and Athina Meli and T. Messarius and Predrag Mio and Hiroko Miyamoto and Akbar Mokhtarani and Teresa Montaruli and A. Morey and R. Morse and Rolf Nahnhauer and Peter Niessen},
  year={2005}
}
The AMANDA-II data collected during the period 2000–2003 have been analysed in a search for a diffuse flux of high-energy extra-terrestrial muon neutrinos from the sum of all sources in the Universe. With no excess events seen, an upper limit of Eν × dNν/dEν< 7.4×10−8 GeV cm−2 s−1 sr−1was obtained. The sensitivity of the diffuse analysis of IceCube 9 string for 137 days of data is calculated to be Eν × dNν/dEν< 1.3× 10−7 GeV cm−2 s−1 sr−1. No excess events are observed, which confirms the… Expand
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