Effects of the model assumptions and statistical methods: the CMF results of Brinkman et al. (2024, 2025) that were computed from the best literature values for planet mass and radius (a), the median of the CMF posterior distribution (b), and the optimal CMF that corresponds to the case in which the likelihood function reaches its minimum value in the MCMC chain (c). For the purpose of direct comparison, the planet samples selected here are consistent with Brinkman et al. (2024, 2025).