Photometric mass estimates fixed at the MUSE-Wide spectroscopic redshifts compared to the Skelton et al. (2014) photometric mass estimates based on photometric redshift estimates. The solid line represents the 1:1 mass equivalency, while the dashed lines show ±1 dex differences between the two stellar mass estimates. Marked with blue triangles are catastrophic redshift outliers, which will be the main cause of discrepancies. At low redshift there is good agreement between the stellar masses, while at high redshift the scatter between the masses is larger due to the large photometric errors associated with these faint galaxies.