Fig. 12
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ESPRESSO FWHM measurements (top), RV measurements (middle), RV residuals (next bottom) from long-term cycle (red thick dashed line) and SHO (PROT and PROT/2) GP model (grey solid line), and RV residuals (bottom) from the Keplerian model (grey shaded area), and GLS periodograms (left) of GJ 699. The uncertainties include the jitter term coming from the global model E1e in Table 3, with prior and posterior parameters given in Table 6.
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