Comparison of low-mass/small planet occurrence rates from various surveys (adapted from Sab21). The parameter range is 1 to 10 M_⊕ in M_pl sin i for RV surveys and 1.3 to 3.7 R_⊕ in R_pl for transit surveys. The error bars for transit surveys are Poisson errors based on the number of planet detections in the respective bins, and error bars from RV surveys are the 16% and 84% levels of the occurrence rate posterior distributions. Results using transiting planets from the Kepler mission are represented as triangles (Morton & Swift 2014; Dressing & Charbonneau 2015; Mulders et al. 2015; Gaidos et al. 2016; Hsu et al. 2020), and rates from the HARPS, HADES, and CARMENES RV surveys are represented as squares (Bonfils et al. 2013; Sabotta et al. 2021; Pinamonti et al. 2022, and this work). The grey square shows the occurrence rate from this work with the assumption of a log-uniform distribution in M_pl sin i.