Distribution of the number of galaxies in stellar mass bins of width 0.5 dex in our final Fornax cluster (purple), satellite (yellow, right hatched), and nearly isolated (blue, dotted and left hatched) samples. The field sample combining the satellites and isolated galaxies are plotted in dashed black lines. C22* in this figure indicates that we have included the Chamba et al. (2022) LTG and ETG sample here only to show the lack of cluster galaxies beyond M_⋆ > 10^9.5 M_⊙ (grey region).