Fig. 2
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Difference between the PSF (point spread function) magnitude and the CModel magnitude in the gri bands, and the mean gri value (bottom right) vs. magnitude for the ECDFS field (analogous to Fig. 1 from Slater et al. 2020). The colormap encodes the number of stars per bin. The bimodal distribution of stars and galaxies (more precisely, unresolved and resolved sources) is evident.
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