Left: Comparison between the number of planets per radius bin at 4.57 Gyr, obtained by simulating the atmospheric mass loss due to the X-ray luminosity computed with the original prescription of Jackson et al. (2012) (blue bars) and the revisited one (this work, red bars) and EUV irradiation as in Sanz-Forcada et al. (2011), for a 1 M_⊙ parent star at solar metallicity. In the bottom panel, the numerical difference (in modulus) of planets per bin for the two considered prescriptions is shown. Right: Meaning of the plot is the same as for the left panel, but for the recalibrated prescription of Johnstone et al. (2021) as in Pezzotti et al. (2021) (blue bars) and the revisited one (this work, red bars).