Fig. 6
Top: HD 50499 RV curves. Blue: CORALIE-98 data; green: CORALIE-07; purple: CORALIE-14 data; red: HARPS data; and orange: HIRES data (Butler et al. 2017). The Keplerian models are represented by black curves. Middle: RV residuals of HD 50499. Bottom: periodogram of the residuals of HD 50499 after the two planetary signals were removed, indicating that there are no more significant signals remaining in the data. The three black lines represent the 10, 1 and 0.1% FAPs in ascending order.
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