Extended Data Fig. 4: Phase-folded plots of the RV signals for the two planets of the V1298 Tau planetary system for which we could not confirm the RV signals.
From: Rapid contraction of giant planets orbiting the 20-million-year-old star V1298 Tau
a: Phase-folded representation of the best-fitting Keplerian orbit (red line) for V1298 Tau c. b: Same for V1298 Tau d. c and d: Residuals after the fit for both cases. For a better visualisation, only HARPS and CARMENES data have been included. In all cases, 1σ error bars (internal RV uncertainties) of the measurements are shown.
