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Fig. B.1

Fig. B.1 Refer to the following caption and surrounding text.

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RV curve based on ephemeris provided by Kokori et al. (2023) (top) and Patel & Espinoza (2022) (bottom). The two nights are visually horizontally well aligned in the top panel, while there is clear misalignment in the bottom panel. For visual purposes, only night 1 (blue) and night 3 (green) are plotted. Contact points are plotted as dashed vertical lines in black. RV are corrected for the stellar velocity induced by the planet.

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