Fig. 2
Histogram of the planet-to-star mass ratio for the two subsamples. It can be compared to Fig. 1 of Pascucci et al. (2018). The value of qbr of Pascucci et al. (2018) of log(Mpl∕M*) = −4.55 ± 0.03 is presented as a vertical black line and can be compared with mean values we calculated: − 4.59 ± 0.03 (G planets, red dashed line) and − 4.58 ± 0.04 (K planets, blue dashed line).
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