Comparison of components obtained for each sample: the two-halo term (top) and satellite hosts (bottom). Differently colored shaded areas represent different samples, identified here by the logarithm of their minimum stellar mass, in solar masses following the color scheme of Fig. 1. The evolution of the two-halo term (satellite) is linked to the evolution of the large-scale halo bias (mean halo mass hosting satellite galaxies), as shown in Table 3, column “b” (${\overline{M}}_{\mathrm{sat}}$).