Probability density distributions of galaxy g − r colours (left panel), probabilities of being late type (p_l, middle panel), and star formations rates (SFRs, in log M_⊙/yr, right panel) for high (h, log   M_s ≥ 10.25, solid lines) and low (l, log   M_s < 10.25, dashed lines) stellar mass galaxies in the superclusters of filament (F, red lines) and spider (S, blue lines) morphology.