Evolution of the planets in the logg–T_eff space, together with the coverage by the atmosphere grids given as rectangles. The colour code for the masses is given in the middle panel. Thick lines indicate cooling curves that are in the atmosphere grid and thin lines those that are outside of the grid. Top panel: evolution in the AMES-Cond grid. Middle panel: evolution in the petitCODE grid for the cloudy (f_sed = 0.5) and solar metallicity atmosphere is shown. This is representative also for other types of petitCODE atmospheres. Bottom panel: evolution in the HELIOS grid for a cloud-free atmosphere with a [M/H] = 0.6 and is representative also for the solar -metallicity evolution paths.