Fig. 2.
Curves of the probability density functions from which the various parameters used for the Monte Carlo analysis were drawn. Clockwise, starting at the top-left, these are: the peak magnitude of the supernova in B-band, MB, peak; the rest-frame rise time of the supernova, trise; the Type Ia SN stretch parameter x1; and the host galaxy reddening parameter E(B − V)host.
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