  We investigate the prospects of indirect and direct dark matter searches
within the minimal supersymmetric standard model with nine parameters (MSSM-9).
These nine parameters include three gaugino masses, Higgs, slepton and squark
masses, all treated independently. We perform a Bayesian Monte Carlo scan of
the parameter space taking into consideration all available particle physics
constraints such as the Higgs mass of 126 GeV, upper limits on the scattering
cross-section from direct-detection experiments, and assuming that the MSSM-9
provides all the dark matter abundance through thermal freeze-out mechanism.
Within this framework we find two most probable regions for dark matter: 1-TeV
higgsino-like and 3-TeV wino-like neutralinos. We discuss prospects for future
indirect (in particular the Cherenkov Telescope Array, CTA) and direct
detection experiments. We find that for slightly contracted dark matter
profiles in our Galaxy, which can be caused by the effects of baryonic infall
in the Galactic center, CTA will be able to probe a large fraction of the
remaining allowed region in synergy with future direct detection experiments
like XENON-1T.
