Image Details
Caption: Figure 9.
Comparison of bolometric luminosities from UV continuum luminosities and those from LMIR values. Panels (a) and (b) compare the LMIR-based Lbol values to those from L3000 and L1450, respectively. Filled red circles and filled blue squares represent dust-obscured and unobscured AGNs, respectively, and the one-to-one relations are shown as the dashed black lines.
© 2026. The Author(s). Published by the American Astronomical Society.