Effect of model selection and age uncertainty on planet occurrence (𝒜 = [5,13] M_Jup × [10,100] au): results for the entire sample (red squares), the BA subsample (blue diamonds), the FGK subsample (green circles) using: the standard ATMO-NEQ-weak model (ATMO-NW); the same model with lower (ATMO-NW, L) and upper (ATMO-NW, U) ages; the ATMO model with no (ATMO-C) and strong (ATMO-NS) disequilibrium chemistry; the AMES-Cond model (AMES-COND) and the Sonora Bobcat model (SONORA). A Jeffreys prior is assumed (see Section 3.4).