Fig. A.1.
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Observed fν spectra (blue) and posterior spectra from Bagpipes (orange) for four of the dormant galaxies selected in this work. The filled circles are the photometry values, which are used to calibrate the spectra. We observe strong Balmer breaks and weak emission lines. Inset are the RGB cutouts of the galaxies, with the slits used for these observations overplotted in pink.
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