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I will review the main theoretical and observational results associated with indirect dark matter searches.
I will notably discuss the recent PAMELA buzz,
in light of the thorough study we performed in Torino to predict the standard astrophysical contributions to the cosmic-ray electron and positron budget.
Finally,
I will show how astrophysics,
provided some theoretical/experimental improvements,
can provide powerful means to further survey the annihilating dark matter phase-space complementary to direct detection and collider physics,
emphasizing multimessenger,
multiwavelength and multiscale strategies.
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