Fig. C.2.
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Stokes parameters of SN 2017gci and bright field stars measured at four epochs displayed on the Q – U plane. The SN (teal) and the field stars passing the selection criteria (olive) as well as derived Galactic ISPs (red) are shown. The second epoch consists only one cycle of observations, making the ISP estimate less reliable. For the other three epochs the derived values of ISP are consistent.
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