Mass-sma diagram of known exoplanets and planet candidates presented in the current work. The green lines show the degenerate mass and sma compatible with the GDR3 α_UEVA. The data for exoplanets are taken from the NEA, including those with a known mass (black dots) and those with only a minimum mass m sin i (red dots). The black dashed lines bound the BD desert region extending up to orbital periods of 80 days (∼0.36 au for a 1 M_⊙ host star; Kiefer et al. 2019, 2021). The magenta dotted line represents the commonly accepted 13.5 M_J upper-mass limit on the planetary domain.