Fig. 3.
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ISP λmax–K diagram for the Type II SNe in this study. Several Type Ia SNe (black crosses; Patat et al. 2015; Zelaya et al. 2017; Cikota et al. 2018) and a large number of MW stars (gray crosses; Whittet et al. 1992) are also included. The colored points show the best-fit values of the Type II SNe, and the lines represent the 1σ confidence intervals for the fitting.
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