  Based on a recently developed relativistic density functional approach to
color-superconducting quark matter and a novel quark-hadron transition
construction which phenomenologically accounts for the effects of inhomogeneous
pasta phases and quark-hadron continuity, we construct a class of hybrid
equations of state applicable at the regimes typical for compact star
astrophysics and heavy ion collisions. We outline that early quark
deconfinement is a notable consequence of strong diquark pairing providing a
good agreement with the observational data and driving the trajectories of the
matter evolution during the supernovae explosions toward the regimes typical
for the compact star mergers and heavy-ion collisions.
