  We present a systematic search for potential dark matter subhalos in our
Galaxy among the 630 unassociated sources included in the First Fermi-LAT
Source Catalog. Assuming a hypothetical dark matter particle that could
generate observable gamma-ray photons beyond the Fermi energy range through
self-annihilation, we look for reasonable targets for ground-based Imaging
Atmospheric Cherenkov Telescopes at energies E > 100 GeV. In order to narrow
the origin of these enigmatic sources, we look for their possible counterparts
in other wavelengths including X-ray, radio, and optical spectroscopy. We find
that the synergy between Fermi and Cherenkov telescopes, along with
multiwavelength observations, could play a key role in indirect searches for
dark matter.
