Dark Matter could be detected indirectly through the observation of neutrinos produced in self-annihilations or decays. Searches for such neutrino signals have resulted in stringent constraints on the dark matter self-annihilation cross section, lifetime, and the scattering cross section with matter. The talk will review recent progress in the search for dark matter at neutrino telescopes. A particular focus will be set on the opportunity to probe light dark matter models, through the interaction of astrophysical neutrinos with Galactic and extra-galactic dark matter. Limits on the dark matter neutrino scattering using the reported evidence for the first identified source of the high energy astrophysical neutrinos (Blazar TXS0506+056) will be reported.
