Comparison of the upper uncertainties of the main global properties of our primary galaxy sample from three different SED fitting runs. The properties presented here are the same as in Fig. 7. The top row shows the comparison of the uncertainties of our fiducial run with those from the spectroscopy-only run, and the bottom row shows the comparison with the photometry-only run. Contours enclose 20%, 50% and 80% of the total data. The dashed orange line shows the one-to-one relation.