Final MUSE spectra of the dual AGN systems, with target names and redshifts indicated in each panel. The spectra were extracted from the circular apertures shown in Fig. 2 (same color-coding), corrected for Galactic extinction, normalized to Gaia magnitudes, and shifted to the rest frame. For clarity, the spectra of the primary AGN (component A) have been re-normalized to facilitate comparison with those of component B; the applied renormalization factor is indicated in each panel. Vertical dotted purple lines mark the expected positions of prominent emission lines at the redshift of AGN A. The gap around λ_obs = 6000 Å (observed frame) corresponds to the New Generation Controllers (NGC) used in AO observations.