Extended Data Table 1 Results of photometry, gravitational-lensing modelling and the Bayesian test of light curve models

From: Shock cooling of a red-supergiant supernova at redshift 3 in lensed images

  1. a, Photometry of G1, G2 and G3 in units of AB magnitude. b, Positions (α, δ), flux density (f), magnification (μ) and time delay (Δt) of the multiple SN images. Flux density and time delay are in units of nanojanskys (nJy) and days, respectively, where the time delay is defined as the relative delay with respect to S3. Photometry has been corrected for foreground Milky Way extinction. A negative magnification indicates an opposite parity. Numbers in the parentheses are the standard deviations. c, Ranges of the prior density of physical parameters R, M, v, t0 and E(B − V) for the light curve models and logarithm Bayes factors (logBi0) of the ith light curve model against the constant flux model (the null hypothesis) for RV = 3.1.
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