Temporal evolution of mass, radius, and mass loss rate for three different values of planetary mass for each planet in the TOI-2076 system. The left panels show the evolution of planetary parameters for planet b, the middle panels for planet c, and the right panel for planet d. Solid lines represent models in which we describe the stellar X-ray flux evolution using the law proposed by Penz et al. (2008), and EUV radiation using the law developed by Sanz-Forcada et al. (2022). Dashed lines represent models where the XUV evolution is described using the Johnstone et al. (2021) description. The vertical dotted grey line is located at the current stellar age.