Median stellar mass difference for our sample of galaxies as a function of redshift in the case of different SED fitting codes. The stellar mass reference at z ≈ 0 is computed for each individual code using the same photometric filters. This difference can reach 0.2−0.3 dex by z ∼ 1. We find that LEPHARE (with no added emission lines) gives the best overall results for z <  1 of all used codes, but it still underestimates the stellar masses at z ≳ 0.5. The shaded region indicates the redshifts for which the SED fitting codes are not well calibrated as we are mostly probing regions in the rest-frame UV.