Fig. 14.

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EPM regression obtained for SN 2005cs in the two versions (the left plot shows the more conservative approach, where we adopted a flat prior for t0, and the right plot shows the fit for the t0 prior that is informed by the light curve). The x-axis shows the time elapsed since the explosion epoch t0, MJD 53548.73, for both plots. The points show the evolution of Θ/vph for this supernova as inferred from spectral fitting. The shaded region shows the uncertainty of the fit.
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