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Fig. B.9
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Stacked Bayesian GLS periodograms of the signals detected in the RVs. Left panel: Zoom in on the long-period planetary signal at 1218.5 d. Middle panel: Zoom in on the 2.27 d period signal. Right panel: Zoom in on the 69.94 d variable signal, which appears in the RV residuals after the 2-planet model is subtracted.
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