Fig. 6.
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Top panel: Ensemble power spectra for the quasars in the BHM1, BHM2, and BHM3 samples (mean values of the BH mass in each sample are reported in the legend). Dashed, solid, and dotted lines indicate the the best-fit BPL models to the power spectra. Thinner lines of the same colour and style are noise-subtracted. Bottom panels: Best-fit residuals.
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