Comparison of SED-based stellar masses and kinematic-based stellar masses. The kinematic-based stellar mass M_⋆ are obtained from GALPAK^3D disk-halo fits, while the SED-based M_⋆ are derived from the HST photometry. The error bars represent the 95% confidence intervals. The M_⋆ obtained with GALPAK^3D (one of the 14 free parameters in Sect. 3.2) and from HST photometry are completely independent, except for ID912 (open circle). The dashed line shows the 1:1 line and this figure shows the two are in excellent agreement, except for ID919 and ID943.