Fig. 2.

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Polarization degree P (top panel) and angle θ (bottom panel) selected for the determination of the ISP in SN 2017gmr. The red lines and the blue-shaded areas are the same as in Fig. 1. In each wavelength bin, the ISP values are the average over all five epochs, after removal of outliers as described in Sect. 4.1. The red lines show the best-fit ISP from Sect. 4.1 and Table 4.
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