Fig. 3
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Top: RV time series of HD 87816 obtained between 2007 and 2024. The dots are color-coded by instrument (CORALIE98 in purple, CORALIE07 in red, and CORALIE14 in olive). Our two-planet model is overplotted in black, with one very eccentric planet orbiting with a period of 484 days and a longer-period planet at 7600 days. Bottom: residuals after subtracting the two-planet model.
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