Image Details
Caption: Figure 5.
Time-lag analysis of the continuum and broad Hβ emission during the normal phase. Same as Figure 4, but for the normal phase. Both methods yield a consistent reverberation lag of ∼5 days, with the MICA lag posterior distribution having a median of ∼5.4 days, indicating a stable BLR response under presumably unobscured conditions.
© 2026. The Author(s). Published by the American Astronomical Society.