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Fig. 4


Phase-folded RV measurements of HD 20003 with the best Keplerian solution represented as a black curve for each of the signals in the data. From top left to bottom right panels: planet b, planet c and the signal at 184 days. The residuals around the solution are displayed in the lower right panel. Contrarily to Fig. 1 error bars include now the instrumental + stellar jitter from the MCMC modeling. Corresponding planetary orbital elements are listed in Table 5.

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