Image Details
Caption: Figure 5.
Similar to Figure 4, but for Eddington ratios and Eddington ratio detection thresholds. We use the J. Kormendy & L. C. Ho (2013) MBH–σ relation and the H. Netzer (2019) bolometric corrections to calculate the Eddington ratios; the qualitative trends do not depend on these choices.
© 2026. The Author(s). Published by the American Astronomical Society.