Image Details
Caption: Figure 7.
Analysis of the RWB fraction in the ξEdd–Lbol plane. Left: distribution of individual RQ Seyfert 1s. The grid represents bins of 0.5 × 0.5 dex containing ≥70 sources. Right: the RWB fraction (fRWB) within each bin. The color scale indicates the fraction value. At a fixed luminosity, the RWB fraction decreases as the Eddington ratio increases.
© 2026. The Author(s). Published by the American Astronomical Society.