Relation between the total stellar mass (M_∗) estimated by fitting the integrated multi-wavelength photometry of the whole galaxy and the measured luminosity from the HST H-band flux (without k-correction) for a sample of disk-dominated (B/T< 0.2, left) and bulge-dominated galaxies (B/T> 0.8, right). Individual galaxies are shown with filled colored circles. The best-fit relation is shown with a straight line, and the dispersion around this relation is shown with light solid lines on each side. The global dispersion is given in the top left corner of each plot and is computed from the median absolute deviation (MAD) using 1.48 × MAD(ΔM_∗).