  The detailed origin of the diffuse gamma-ray background is still unknown.
However, the contribution of unresolved sources is expected to induce
small-scale anisotropies in this emission, which may provide a way to identify
and constrain the properties of its contributors. Recent studies have predicted
the contributions to the angular power spectrum (APS) from extragalactic and
galactic dark matter (DM) annihilation or decay. The Fermi-LAT collaboration
reported detection of angular power with a significance larger than $3\sigma$
in the energy range from 1 GeV to 10 GeV on 22 months of data [Ackermann et al.
2012]. For these preliminary results the already published Fermi-LAT APS
measurements [Ackermann et al. 2012] are compared to the accurate predictions
for DM anisotropies from state-of-the-art cosmological simulations as presented
in [Fornasa et al. 2013] to derive constraints on different DM candidates.
