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We apply the Jeans Axisymmetric Multi-Gaussian Expansion method to thestellar kinematic maps of 40 Sa-Sd EDGE-CALIFA galaxies and derive theircircular velocity curves (CVCs). The CVCs are classified using the DynamicalClassification method developed in Kalinova et al. (2015) . We also calculatethe observational baryon efficiency, OBE, where$M_*/M_b=M_*/(M_*+M_{HI}+M_{H_2})$ of the galaxies using their stellar mass,total neutral hydrogen mass and total molecular gas from CO luminosities.Slow-rising, Flat and Round-peaked CVC types correspond to specific OBEs,stellar and dark matter (DM) halo mass values, while the Sharp-peaked CVCs spanin the whole DM halo mass range of $10^{11}-10^{14} M_{\odot}$.

Bridging Galaxy Dynamics and Baryon Efficiency of 40 EDGE-CALIFA galaxies