Fig. 7.
Left panels: HARPS RV data of HD 69830. The plotted period, the order of the different DRS, and the colour of the two different data sets (before and after the change of the fibres) is the same as in Fig. 5. Right panels: respective LSP of the residuals to the fitted Keplerian model with the two known planets at 8.67 and 31.64 day periods.
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