Summary of DBNets results on the collected catalogue of observations and a comparison with proposed planet masses available in the literature. The rings and squares indicate estimates obtained examining dust substructures while the stars refer to kinematical detections. The results are presented (from top to bottom) in ascending order with respect to the uncertainty of the DBNets results. The red dashed line separates results according to the uncertainty threshold of 0.25 dex. References: Dong & Fung (2017); Toci et al. (2019); Zhang et al. (2018); Pérez et al. (2019); Lodato et al. (2019); Kim et al. (2020); Marino et al. (2018); Wang et al. (2021); Clarke et al. (2018); Jin et al. (2016); Facchini et al. (2020); Bae et al. (2018); Huang et al. (2020a); Veronesi et al. (2020); Baruteau et al. (2019); Izquierdo et al. (2022); Fedele et al. (2018); Pinte et al. (2019).