Fig. 7
Top panel: time series of the RV measurements of EPIC 249893012. Blue dots correspond to HARPS, red dots to HARPS-N, and green dots to CARMENES measurements. The best-fit model to the data is shown with a black thick line. The model includes three Keplerian curves and one sine curve mimicking the stellar signal at half the rotation period. Middle left panel: phase-folded RV measurements over the period of planet b after removing the signals from planets c and d and stellar activity. Middle right panel: phase-folded RV measurements over the period of planet c, after removing the signal from the other planets and stellar activity. Bottom left panel: phase-folded RV measurements over the period of planet d, after subtracting the signal from planets b and c and stellar activity. Bottom right panel: phase-folded RV measurements over half the rotation period of the star after removing the signals from the three planets.
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