Sensitivity results of the atmospheric thermal structure on different scenarios for a 200x solar metallicity atmosphere. The blue presents the nominal scenario of complete energy redistribution and ϕ_H=10⁻¹² gcm⁻²s⁻¹ with haze optical properties from He et al. (2024). The orange and black lines present a 5×Φ_H and 20×Φ_H scenarios with the same optical constants, while the purple line demonstrates the impact of a more absorbing compositions such as that of soots (Lavvas & Koskinen 2017). The red line corresponds to the nominal Φ_H and refractive index case, but energy deposition on the day side. The dotted lines present the condensation curves for H₂O and NH₄SH. The inset presents the impact of each scenario on the H₂O (solid lines) and NH₃ (dashed lines) mole fractions, with colours corresponding to the temperature cases of the main plots.