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Fig. 1


TOI-148 light curves (top) and RVs (bottom) phased to the companion’s orbital period. The red lines in the upper plot show the best-fit transit model to each photometry data set from our EXOFASTv2 analysis described in Sect. 3.4.1. In the lower plot the red line shows the best-fit Keplerian model to the RVs from our EXOFASTv2 analysis.

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