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Fig. 3.


Phase-folded RV curves of π Men b (upper panel) and c (middle panel), and transit light curve of π Men c (lower panel). The best-fitting transit and Keplerian models are overplotted with thick black lines. The zero phases of the RV curves of π Men b (upper panel) and c (lower panel) correspond to the time of inferior conjunction and transit epoch, respectively (Table A.4). The TESS data points are shown with red circles (lower panel). The AAT data and the two sets of HARPS RVs (HS1 and HS2) are shown with circles, diamonds, and squares, respectively. The vertical gray lines mark the error bars including jitter.

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