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Fig. 9

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Revised occurrence rates of giant planets. Top: based on the data of Mayor et al. (2011), which should be compared with Fig. 4 of Fernandes et al. (2019). We note that one planet with imprecise orbital parameters (and hence bin) was removed from the analysis. Middle: based on the data of Rosenthal et al. (2021), which should be compared with Figs. 2 and 3 of Fulton et al. (2021). Bottom: same as middle, but assuming a uniform distribution instead of a beta distribution for the eccentricities.

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