Density of points (blue hexagonal bins) representing the absolute difference between observed aperture magnitudes and SDSS DR12 magnitudes in the g optical bandfor all field galaxies detected in the low-deblending configuration. Although the dispersion is relatively high, the overall agreement between the two photometries is good (see text). When split into magnitude bins for host galaxies (pink and purple bins for high- and low-deblending modes, respectively), the two configurations are similar, except for the first bin, where the low-deblending case shows less consistency with SDSS.