Image Details
Caption: Figure 8.
Ensemble SFs for the Seyfert 1 sample. (a) SFs for RQ and RL subsamples. Dashed lines represent the best-fit models. (b)–(f) SFs for subsamples binned in the Lbol–ξEdd plane. The flattening of the slope with increasing Eddington ratio is evident across luminosity bins.
© 2026. The Author(s). Published by the American Astronomical Society.