Occurrence rates of theoretically calculated planets by Burn et al. (2021). The same bins as in Figs. 3, 4, and 5 are used. Values of sin i are randomly assigned to the synthetic systems following the expected distribution for randomly oriented systems (Schlecker et al. 2022). The top panel shows the synthetic occurrence for the combined discrete stellar masses of 0.3 M_⊙ and 0.5 M_⊙. The bottom panels show the deviation from observations measured in standard deviations (f_p,synthetic – f_p)/S_fp for the indicated stellar masses compared to the observational data from Figs. 5 (left) and 4 (right). Where observational upper limits are in agreement with theory, the box is left blank.