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Fig. 2

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Simulation of CARMENES data from a K7 star with a 5 M planet, with an 62.85-day orbital period using a strategy of 23 data points per semester over four semesters (middle panel in Fig. 4). Upper panel: simulated radial velocity time series. Bottom left: periodogram and the significance levels. The vertical dashed line shows the simulated period. Bottom right: phase-folded radial velocity.

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