Fig. C.1.

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Final MUSE spectra of the AGN (purple) and star (orange) systems, with target names and redshifts indicated in each panel. The spectra were extracted from circular apertures of 5 px, corrected for Galactic extinction, normalized to Gaia magnitudes, and shifted to the rest frame. Vertical dotted lines indicate the positions of the expected AGN emission lines. The gap around 6000 Å corresponds to the NGC used in AO observations.
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