Fig. C.1

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Emission spectra for different atmospheric scenarios. The curves show the planetary flux to stellar flux ratio in ppm as a function of wavelength in μm. Each panel corresponds to the atmospheric composition labelled on the top of the panel. In each panel, the top curve represents the model for no heat redistribution (f=2/3), while the bottom curve is for full redistribution (f=1/4). The shaded area covers the scenarios in between the boundary cases.
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