  The minimal supersymmetric setup offers a comprehensive framework to
interpret the Fermi LAT Galactic center excess. Taking into account
experimental, theoretical, and astrophysical uncertainties we can identify
valid parameter regions linked to different annihilation channels. They extend
to dark matter masses above 250 GeV. There exists a very mild tension between
the observed relic density and the annihilation rate in the center of our
galaxy for specific channels. The strongest additional constraints come from
the new generation of direct detection experiments, ruling out much of the
light and intermediate dark matter mass regime and giving preference to heavier
dark matter annihilating into a pair of top quarks.
