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Fig. 2
GLS Periodogram of the RV residuals of HD 20003 at each step after removing, from top-left to bottom-right, the magnetic cycle effect plus a second-order polynomial drift, then the two planets at 11 and 33 days one after the other, and finally the signal at 184 days. The GLS periodogram of the raw RVs is shown in Fig. 1.
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