High-Energy Neutrino Astronomy with the Super-Kamiokande Detector
  The Super-Kamiokande experiment has collected a large sample of high-energy neutrino events. These are primarily atmospheric neutrinos, but a bright enough astrophysical source could also be visible. The data have been examined for possible point and bursting neutrino sources, as well as possible WIMP annihilation signatures. No significant evidence for such sources have been found, and the resulting flux limits have been calculated. 
A. Habig (for the Super-Kamiokande Collaboration)