Mass-period diagram from planets up to low-mass M dwarfs (~150 M_J). The truemasses derived with GASTON for non-transiting planets and systems without RV drift are represented as black circles. In comparison, the true mass and period of companions in the exoplanet.eu database are plotted as orange squares, supplementary BD and low-mass M dwarfs published in Wilson et al. (2016) are plotted in green triangles, and Kiefer et al. 2019 companions are shown as purple diamonds. Only systems within 60 pc from the Sun and surrounding FGK host stars (0.52 < M_⋆ < 1.7M_⊙) are represented.