Dayside pressure-temperature profiles calculated for the gas giant exoplanets WASP-33b, HD 209458b, HD 189733b, GJ 436b, and GJ 1214b. The solid lines correspond to the temperature profiles calculated self-consistently with the disequilibrium composition at a time at which a steady state is reached in the atmosphere composition and temperature, while the dotted lines correspond to temperature profiles calculated at the initial time, where the composition is assumed to be given by chemical equilibrium.