  Neutrino astronomy has entered an exciting time with the completion of the
first km3-scale neutrino telescope at the South Pole (IceCube) and the
successful operation of the first under-sea neutrino telescope in the
Mediterranean (Antares). This new generation of experiments is approaching the
sensitivity levels required to explore at least part of the current landscape
of neutrino flux predictions from astrophysical sources, bringing neutrino
astronomy on the verge of its first discovery. This contribution presents the
current status and latest results of the operating neutrino telescopes, with a
particular emphasis on the link with the phenomenology of high-energy cosmic
rays.
