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Fig. 7

image

Probability density functions of the frequencies of substellar companions around FGK stars based on the parametric model, 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 (plain line), BEX-COND-warm (dashed line) or COND-2003 (dotted line) evolutionary tracks for the mass conversion of the detection limits. The median values and 68% confidence intervals are provided in Table 2.

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