Fig. 5.
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Spectro-photometric SED-fitting of two galaxies (a quiescent and a star-forming one) in our sample. The lines are the best-fit SEDs from different codes and SFH choice. Photometric data are shown as white diamonds. The error bars are smaller than the size of the points. The 1D spectra in F115W, F150W, and F200W are shown in black. The right panels show a zoomed-in view of the spectra in linear scale. The 3σ errors are plotted as shaded grey areas. We report the median S/N of the 1D spectra.
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