Output of the magphys SED fitting performed in one of the central pixels and in one of the outermost pixels of NGC 1566 (upper panels) and of NGC 5236 (bottom panels). The green data points are the observed fluxes in the available bands and the χ² of the fit (black line) is reported in the upper left corner of the plots. At the bottom of each subfigure, we also display the difference in dex between the observations and the best-fitting model with the associated error bars; when not visible they are smaller than the corresponding markers.