Non-minimal quintessence and phantom with nearly flat potentials
  We investigate quintessence and phantom dark energy scenarios, in which the
scalar fields evolve in nearly flat potentials and are non-minimally coupled to
gravity. We show that all such models converge to a common behavior and we
provide the corresponding approximate analytical expressions for
$w(\Omega_\phi)$ and $w(a)$. We find that non-minimal coupling leads to richer
cosmological behavior comparing to its minimal counterpart. In addition,
comparison with Baryon Acoustic Oscillation and latest Supernovae data reveals
that agreement can be established more easily and with less strict constraints
on the model parameters.
