Extended Data Fig. 6: Reconstructed light curves from the best-fit model parameters from all the light curve models for RV = 3.1.
From: Shock cooling of a red-supergiant supernova at redshift 3 in lensed images
a–f, Data shown are from the RSG model (a), the BSG model (b), the CSM-homologous model for a prior on the CSM mass of M < 0.1M⊙ (c), the CSM-homologous model for a prior on the CSM mass of M < 1M⊙ (d), the CSM-planar model for a prior on the CSM mass of M < 0.1M⊙ (e), and the CSM-planar model for a prior on the CSM mass of M < 1M⊙ (f). Data points and error bars correspond to the measured values and ±1σ uncertainties of the flux densities, respectively. Reconstructed light curves with all our choices of RV are available from an online repository75.
