Comparison of the circular velocity V₂₂ = V(R₂₂) using MOCKING between MULTINEST and MPFIT for galaxies from the MS sample. The rotation curve used was a flat model, and we removed galaxies whose circular velocity could not be reliably constrained (R₂₂ falls outside the range where there is sufficient S/N in the MUSE data cube to derive the kinematics). Red points correspond to galaxies visually classified as having no apparent velocity field in their kinematics maps, and dashed red lines correspond to a 50% difference between the two methods. The typical uncertainty is shown in the bottom-right part of the plot. Overall, values are consistent within their error bars.