Fig. A.1.
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Observed Hβ line in velocity space, indicated in black (uncertainties are shown in gray), while the predictions for a binary SMBH are overplotted in red (Savić et al. 2019). Top panel: Relative (scaled) total flux between the observation and the simulation. Middle panel: Host-corrected polarization degree of NGC 1566 and the simulation. Bottom panel: Variations of the polarization angle around 0° between the model and the observational data.
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