Correlation plots and marginalized PDFs for f_GI and f_CA in the population model around FGK stars, computed for companions with masses in the range M_p = 1–75 M_Jup 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.