Comparison between the physical parameters derived using BAGPIPES based on photometry derived using a Kron aperture and a 0.2″-radius aperture. From top left to bottom left: redshift, stellar mass, SFR and A(V). Black dots show galaxies for which the redshift is well recovered, while red dots show redshift outliers, i.e. δz = |z_kron − z_0.2″|/(1 + z_kron) > 0.15. On the top left of each panel we shown the absolute difference between the physical properties derived with Kron and 0.2″ aperture, for galaxies with a good redshift and, in brackets, for the entire sample.