  We examine the NMSSM at the cosmic frontier in the post Higgs discovery
world. For DM relic abundance consistent with measurement, we find the
neutralino can either be singlino or bino dominated. Wino and higgsino DM
generally yield a lower abundance, but offer opportunities of detection at
IceCube. For both cases, future SI direct detection experiments cover a
majority of the model, including nearly all of the bino and higgsino scenarios.
