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Fig. 12.
g − r, g − i, B − r, and B − i color evolution for our SNe Ic-BL. The g − r color is fit with the expression used by Burns et al. (2014) and Stritzinger et al. (2018), and the best fit with its 3σ uncertainties is shown by red lines. All of the colors are MW and host-galaxy extinction corrected.
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