Fig. 12.
LBOL, AGN/M* vs. distance from the mass-size relation of LTGs (distLTG) for our SBs sample. The Eddington limit is shown with a blue horizontal line, while the shaded area takes into account the spread of M* among our sample and the uncertainty of the relation between stellar mass and BH mass by Reines & Volonteri (2015). The Eddington ratio is shown on the right y-axis.
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