  Indirect detection of dark matter particles, i.e. the detection of
annihilation or decay products of Weakly Interacting Massive Particles, has
entered a pivotal phase as experiments reach sensitivities that probe the most
interesting parameter space. This period is naturally accompanied by claims of
detection. In this contribution I discuss and compare different probes
(gamma-rays, neutrinos and charged cosmic rays) and review the status and
prospects of constraints and recent detection claims.
