Temporal evolution of mass, radius, and mass-loss rate of TOI-5795 b. The left, middle and right panels show the evolution of planetary mass, radius, and mass-loss rate, respectively. Colours indicate different high-energy evolutionary tracks: the blue line refers to the low state (lowest 2% percentile of the activity distribution), the red line refers to the high state (2% percentile), and the pink line refers to PMSF (based on the X-ray luminosity evolution of Penz & Micela 2008, combined with the X-ray to EUV conversion from Sanz-Forcada et al. 2025).