Fig. 7
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Transmission spectra (top left), phase curves (top right), planetary spectral flux at a longitudinal viewing angle of 15° (center left) and 195° (center right), and brightness temperature at a longitudinal viewing angle of 15° (lower left) and 195° (lower right) based on the post-processing of the GCM simulations. The line styles denote post-processing with (solid) and without (dashed) cloud opacity.
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