  We perform a fit to the recent Xenon100 data and study its implications for
Dark Matter scenarios. We find that Inelastic Dark Matter is disfavoured as an
explana- tion to the DAMA/LIBRA annual modulation signal. Concerning the scalar
singlet DM model, we find that the Xenon100 data disfavors its constrained
limit. We study the CMSSM as well as the low scale phenomenological MSSM taking
into account latest Tevatron and LHC data (1.1/fb) about sparticles and Bs
\rightarrow {\mu}{\mu}. After the EPS 2011 conference, LHC excludes the
"Higgs-resonance" region of DM freeze-out and Xenon100 disfavors the
"well-tempered" bino/higgsino, realized in the "focus-point" region of the
CMSSM parameter space. The preferred region shifts to heavier sparticles,
higher fine-tuning, higher tan {\beta} and the quality of the fit deteriorates.
