  We present the recent progress of the hybrid quark-meson-nucleon model for
multi-messenger astronomy that unifies the thermodynamics of quark and hadronic
degrees of freedom. The obtained equation of state is in accordance with
nuclear matter properties at saturation density and with the flow constraint
from heavy ion collision experiments. The mass-radius relations and tidal
deformabilities for compact stars are calculated and compared with the latest
astrophysical observations. The phase diagram of the isospin-symmetirc matter
is studied as well in terms of the higher-order cumulants of the net-baryon
number.
