Fig. 8.
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Correlations between the X-ray [0.2 − 2.3 keV], broad Hα (a), and narrow [O III] (b) luminosities. The color-coding represents the velocity dispersion of the stellar component and links the kinematics to the AGN activity. The dashed lines and equations near the top of the panel denote the best-fit correlations. The uniform scaling between the X-ray and line luminosities reinforces their common AGN origin.
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