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Fig. C.3.
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Q – U planes for the stars used to measure the ISP for SN 2018ffj, SN 2019neq and SN 2020tcw. We note that the star was saturated in the first epoch of SN 2019neq and it is excluded and that the first epoch of SN 2018ffj and the second epoch of SN 2019neq were excluded due to the high lunar illumination (see Section 2.2).
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