Image Details
Caption: Figure 8.
Change in g-band magnitude versus time for photometric transitions to occur for known CL-AGN (colored circles) and Type 1 Seyferts (green squares). We perform linear regressions including only known CL-AGN (purple dashed–dotted line) and including both CL-AGN and Seyfert 1s (green dashed line). We do not detect a correlation between transition magnitude and duration at the 3σ level for either fit.
© 2026. The Author(s). Published by the American Astronomical Society.