Fig. 3.
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Parameters for the sibling SNe Ia in this study. The panels show the redshift (top left), SALT2 x1 (top right), c (bottom left), and host galaxy stellar mass (bottom right) distributions. We did not make any selection cuts on the values of z, x1, and c, unlike for the complete DR2 sample (Rigault et al. 2025). The equivalent distribution for the entire DR2 sample is overplotted as dashed lines Smith et al. in prep.
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