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Fig. C.2
Comparison of the SED-fitting results obtained using the Kron-radii photometry using Kron-radii on the x-axis versus results obtained using a 2′′ aperture (top row) or 3′′ (bottom row) on the y-axis. The panels show, from left to right, the stellar mass, the SFR, the sSFR, and stellar age.
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