  In this work, we perform a comparative analysis between the density-dependent
quark model and the vector MIT bag model using Bayesian analysis. We impose
four recent observational astrophysical constraints on both models to determine
their model-dependent parameters in an optimized manner. The restrictions are
aimed at producing stars with maximum masses $2 - 2.35$ M$_\odot$ and a
mass-radii diagram compatible with the observed pulsars: PSR J0740+6620, PSR
J0952-0607, PSR J0030+0451 and the compact object XMMU J173203.3-344518. With
this analysis, the parameter dependence of the nuclear equation of state (EoS)
of both models is restricted.

Nuclear Theory