Emission spectra models for MIRI only. The shown data is the Eureka! reduction from Hu et al. (2024). Each panel represent a case for the denoted heat redistribution value f . The black spectrum is the total model, where the coloured spectra indicate individual contribution of opacities. Shown in grey are the best fitting blackbody spectra corresponding to a χ² = 9.4. The two dark red data points are affected by the shadowing effect.