Stellar and gas mass fraction of our sample as a function of stellar mass and circular velocity (left and right panel, respectively) within the outer radius (R_out; i.e., visible region). The color code in both panels is the same and given as follows: the brown filled circles represent the molecular gas mass fraction (f_H2 = M_H2(<R_out)/M_bar(<R_out)), the orange filled circles indicate the star mass fraction (f_star = M_*(<R_out)/M_bar(<R_out)), and the blue filled circles represent the atomic gas mass fraction (f_HI = M_HI(< R_out)/M_bar(< R_out)). A comparison study of local late-type galaxies from Calette et al. (2018) is drawn by solid lines; the color coding is same as the high-z objects.