Temperature–pressure proflies (solid line) of WASP-79 b atmosphere (top) assuming radiative transfer equilibrium and condensation curves (dotted lines). The atmospheric structure is computed for different interior temperatures from 35OK (light red) to 800 K (red). Gas species abundances in the WASP-79 b atmosphere (bottom) obtained with Exo-REM, assuming a l0× solar metallicity, non-equilibrium chemistry, an Eddy diffusion coefficient of 10⁸ cm² s⁻¹, and an interior temperature of 600 K.