Over- and underestimation of the observed morphological fractions in CANDELS as a function of redshift. Dotted, dashed and solid lines represent the low-stellar mass sample (M_* < 10¹⁰ M_⊙), high-stellar mass sample (M_* ≥ 10¹⁰ M_⊙) and the entire sample, respectively. The y-axis represents the difference between the observed and corrected fractions. So all the values within the light-gray region correspond to underestimations of the morphological fractions, while the white area indicates the overestimation. Notably, the differences between the observed and corrected fractions increase with redshift, with the exception of the spheroid class.