Probability density functions of the frequencies of substellar companions around FGK stars based on the parametric model, computed for companions with semimajor axes in the range a = 5–300 au (plain line) or a = 10–300 au (dashed line), and using the BEX-COND-hot evolutionary tracks for the mass conversion of the detection limits. The median values and 68% confidence intervals are provided in Table 2. The same plots for BA and M stars are shown in Fig. C.1.
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