Fig. 7
Cumulative normalised distributions of the mutual distances for the reference, the non-physical, and the RV populations. Only planets with a period less than 5 yr and radial velocity semi-amplitude larger than 3 m s−1, and (for the RV population) orbiting around stars of mass between 0.85 M⊙ and 1.15 M⊙ have been considered.
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