Fig. A.5
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Generalized Lomb-Scargle periodograms of FEROS RVs of stars in our sample. From top to bottom: (a) TIC 9344899 RVs, (b) TIC 9344899 RVs minus transiting planet signal, (c) TIC 52059926 RVs, (d) TIC 52059926 RVs minus planet signal, (e) TIC 13344668 RVs, (f) TIC 13344668 RVs minus planet signal. The vertical red lines highlight the orbital period of the companions. Horizontal dashed lines show the theoretical FAP levels of 10%, 1%, and 0.1% for each panel.
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