  We apply the Jeans Axisymmetric Multi-Gaussian Expansion method to the
stellar kinematic maps of 40 Sa-Sd EDGE-CALIFA galaxies and derive their
circular velocity curves (CVCs). The CVCs are classified using the Dynamical
Classification method developed in Kalinova et al. (2015) . We also calculate
the 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 span
in the whole DM halo mass range of $10^{11}-10^{14} M_{\odot}$.
