Absolute (Ṁ_acc) and relative (Ṁ_acc/M_⋆) accretion rate histories (left and right panel respectively) as a function of the look-back time for the galaxies in our sample segregated by their current stellar mass (colors). In both panels the shaded areas correspond to the uncertainties derived from the error of the average value in the ChEHs and SFHs. This is not representative of the scatter of the distribution within each bin, which is indicated in the left side of the left panel.