Distribution of planet radii and orbital periods for all confirmed small planets hosted by low-mass stars (M_* ≲ 0.65 M_⊙). The solid line represents the predicted location of the radius valley based on the gas-depleted formation model (Cloutier & Menou 2020). The dashed line shows the predicted location of the valley for the thermally-driven photoevaporation and gas-poor formation models (Van Eylen et al. 2018). The red and blue dots represents the planets TOI-6002b and TOI-5713b, respectively. The 1D radius distribution, with the location of the two planets, is shown on the right panel.