Synthetic populations of 7.9×10⁵ exoplanets generated sampling different initial circumstellar disc configurations (disc mass: 1, 5, 10% of the stellar mass; R₀: 40 and 90 au; pebble size: cm, mm, and sub-mm). Planet TOI-5795 b and its 3 σ uncertainty range are shown in black. The grey box indicates the range inwards of 0.2 au and the 3σ mass uncertainty range of the planet. The inset plot is a zoom-in of this window and shows, as a colour bar, the initial semi-major axis of the seeds.