Fig. 2
Top panel: phase-folded RV measurements of TrES-4 obtained with HARPS-N (blue circles) and, superimposed, the best-fit Keplerian orbit model (black solid line). The Keck/HIRES RVs from M07 (green diamonds) and K14 (red squares) and the two best-fit orbital solutions obtained in these papers are also shown. Bottom panel: residuals from the best-fit model to the HARPS-N RVs.
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