Fig. A.1.
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Flux variation gradient diagrams for all filter pairs. Black points are the observed fluxes; the OLS-bisector fit (black line) gives the AGN slope ΓAGN (values in each panel). Dashed red lines show the range of host slopes from Sakata et al. (2010) (yellow region); their intersections with ΓAGN yield the host fluxes. Blue lines indicate the corresponding AGN flux ranges.
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