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Fig. 6


Correlation plots and marginalized probability density functions for fBDB and fPPL∕LN in the parametric model around BA (left), FGK (center), and M (right) stars computed for companions with masses in the range Mp = 1–75 MJup and semimajor axes in the range a = 5–300 au, and using the BEX-COND-hot evolutionary tracks at the optimal stellar ages. Contour lines in the correlation plots correspond to regions containing 68, 95, and 99% of the posterior, respectively. For the FGK subsample, the scale of the axes is different from that of the two other subsamples.

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