MSRs for quiescent galaxies in different redshift bins (left) where the points represent the median values in each quartile and the solid lines represent the fits to the data bin. The uncertainty on the stellar mass, computed as the MAD divided by the square root of the number of galaxies, is of the order of ∼0.01. Dependence of α and log(A) with redshift (right) for VIPERS (red triangles) and from the literature (blue circles). The fit for the intercept with redshift is shown as a red dot-dash (VIPERS) and blue dash line (all data points).