Fig. A.2.
Comparison between the flux density of 3184 SFGs in the sample (resolved and unresolved) derived from PyBDSF (corrected) and those reported by Smolčić et al. (2017a). The solid and dashed red lines show the 50th percentile, and 14th and 84th percentiles of the distribution as a function of the flux density reported in this study.
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