Image Details
Caption: Figure 5.
Best-fitting parameters from X-ray spectral modeling as a function of time from the UV/optical peak. From top to bottom: peak temperature (T p ) and radius (R p ) from tdediscspec; fraction of Comptonized photons (f sc) and power-law photon index (Γsc) of simPL.
© 2024. The Author(s). Published by the American Astronomical Society.