Difference between SFR and M_star from the original GSWLC catalogue (Salim et al. 2018), and those obtained in this work. The difference ΔM_star was calculated as log(M_{star this work}/M_star); and ΔSFR was obtained in an analogous way. Panels a and b show the difference in the stellar masses and SFRs, correspondingly, as a function of redshift, with shaded areas represent standard deviation of the scatter; panels c and d present the relation between the fiducial values and the estimates obtained in this work, with contours showing the distribution of the data. Runs based on GSWLC set of parameters, FULL–run, are shown in blue-coloured lines, while those obtained from LIGHT–run – in an orange-coloured set of lines. Black solid lines visible in panels c and d represent 1:1 relations.