Stacked excess surface density profiles, ΔΣ, of the red and blue lenses (points in corresponding colors) in our KiDS-Bright sample in the four stellar mass bins labeled at the top. The lines indicate the best-fitting halo model, with contributions from both centrals and satellites (red and blue lines with shaded bands enclosing the 68% credible intervals). We note that the model was fit to all stellar mass bins simultaneously, but separately for the red and blue populations.