Radius-period diagram for well-studied exoplanets from the TEPCat catalogue (Southworth 2011). TOI-333bis shown as a yellow star within the green triangular region defined by Mazeh et al. (2016), which outlines the ND. The blue and black points represent planets inside and outside this region, respectively, and LTT9779b and TOI-824b are highlighted for comparison. The dashed blue line at P ~ 2 days marks the orbital period below which RLO is thought to significantly affect atmospheric evolution in the desert.