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In this work, we perform a comparative analysis between the density-dependentquark model and the vector MIT bag model using Bayesian analysis. We imposefour recent observational astrophysical constraints on both models to determinetheir model-dependent parameters in an optimized manner. The restrictions areaimed at producing stars with maximum masses $2 - 2.35$ M$_\odot$ and amass-radii diagram compatible with the observed pulsars: PSR J0740+6620, PSRJ0952-0607, PSR J0030+0451 and the compact object XMMU J173203.3-344518. Withthis analysis, the parameter dependence of the nuclear equation of state (EoS)of both models is restricted.

A Bayesian study of quark models in view of recent astrophysical constraints