Atmospheric profiles for four representative planets, while those for the other planets are presented in Fig. A.1. Left: Pressure–temperature profiles retrieved from the standard disequilibrium retrieval (blue), equilibrium retrieval (orange), and disequilibrium retrievals with the same K_zz (green) and with fixed T_int (red; only shown for planets with masses larger than half Jupiter mass). The solid lines show the median models while the shaded regions indicate the 1, 2, and 3σ confidence intervals. Right: Median abundance profiles of H₂O, CO, and CH₄ (left) and those of CO₂, NH₃, and N₂ (right) from the standard disequilibrium retrieval (thick solid lines), equilibrium retrieval (thick dashed lines), and disequilibrium retrievals with the same K_zz (thick dotted lines) and with fixed T_int (thick dash-dotted lines; only shown for planets with masses larger than half Jupiter mass). For reference, the median abundance profiles for the case where the equilibrium chemistry is imposed are shown with the corresponding thin lines.