Fig. 2
Upper panels: RV versus time, periodogram of RV and detection limits (from left to right) for the G2V star HD 183414, covering a time span of 189 days. The detection limits have been computed using the rms-based method (black line), LPA (orange stars). Lower panels: same for the A5V star HD 39060 covering a time span of 2600 days.
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