Fig. 4.
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Wavelength dependence of the ISP (normalized to the polarization at 4000 Å) toward SN 2013ej, SN 2012aw, and SN 2001dh (colored points) with their Serkowski law best fits (colored lines). For comparison, the data of three Type Ia SNe (SN 2014J, SN 2008fp, and SN 2006X; Patat et al. 2015) and a Galactic star (HD 43384; Cikota et al. 2018) are also plotted.
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