Image Details
Caption: Figure E1.
Spectral luminosities of the low-speed ejecta at different times. The red dashed line indicates the effective temperature of the photon-emission sphere at rem. The black dotted line shows the spectral luminosity obtained from radiative-transfer postprocessing of the Guangqi RHD solution with RADMC-3D. The blue dashed line shows the best-fit blackbody.
© 2026. The Author(s). Published by the American Astronomical Society.