Fig. A.1.
Luminosity-weighted stellar population properties maps for NGC 5473 (first two columns) and NGC 5485 (last two columns) determined by J-PLUS/MUFFIT (first row), CALIFA/STARLIGHT (second row), and CALIFA/STECKMAP (third row). The color range is the same for the different methods. The center of the galaxy is indicated with a white cross in each panel.
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