  We briefly review the motivations and features of focus point supersymmetry
and in particular the focus point region of the CMSSM. Applying the constraint
that the neutralino is a thermal relic, we examine current and projected
collider and dark matter constraints on the focus point region. We demonstrate
that the focus point region is currently constrained by multiple dark matter
experiments, and future sensitivy on multiple fronts will probe large portions
of the parameter space.
