Fig. A.1
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Effect of the radial-velocity bias on the detection of terrestrial planets. Left-bottom axes: Percent of terrestrial exoplanets detected, NR, as a function of the detection limit of RV signals, Kth, for different values of the orbital period P of the 100 terrestrial exoplanets in the model catalog. Right-top axes: Probability Density Function (PDF) of the RV signals of the observed terrestrial exoplanets in Dataset S1.
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