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Fig. 3

image

Radial velocity data from the SONG telescope (gray) with the best-fit Keplerian model (black) from the joint photometricand RV analysis. The data are plotted as a function of time (left) and phase-folded (right) to highlight that we allowed for the possibility of a linear trend in the RV. In the panel on the right side the best-fitting RV trend was removed from the data and model. The best-fit parameters are displayed in Table 4. The bottom plot shows the residuals.

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