Comparison of the occurrence rates (left panel: 𝒜 = [2,13] M_Jup × [3,100] au; right panel: 𝒜 = [5,13] M_Jup × [10,100] au) of giant planets with previous analyses by Bowler (2016), Nielsen et al. (2019) and Vigan et al. (2021). The left and the right half of each panel are relative to BA and FGK stars, respectively. Estimates indicated by arrows are to be read as 95% upper limits, while error bars on point estimates are defined as to encompass the 68% C.I.. Question marks indicate missing data points.