Left: the reconstructed SFR functions of the three morphological types of galaxies within 11 Mpc. The observed counts are histogrammed in bins of 0.5 dex. The dashed lines represent the best-fit model of the observed counts, while the solid lines show the true number counts expected with no sensitivity limit. Right: the reconstructed fractions of the three morphological types of galaxies according to the LV classification in bins of 10 Mpc. The fractions averaged between 100–350 Mpc are indicated as solid lines.