Emission contribution function of a strongly irradiated super-Earth orbiting a Sun-like star at 0.015 AU. The temperature profile in the left panel is from the models showcased in Fig. 3. The dashed line is the effective temperature of the planet T = 2950 K. The right panel show the emitting region of the atmosphere as a function of wavelength. Major contributing molecules are indicated in their respective regions. Lesser contributing opacities are discussed in the text. Spectra are shown at a resolution of λ/∆λ = 600.