Fig. A.2
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Pure CO2 case. Upper panels: Observables (right: phase curve at 15 µm, left: eclipse depth). The dotted lines represent non-stable atmospheres; these are snapshots of the atmosphere during its collapse. Lower panels: Physical quantities. Temperature profiles and temperature map for the 10 Pa case (compatible with the observations, but not stable). In the lower right panel, the red contour shows the CO2 ice caps. The red dot is the substellar point. In the lower left panel, the red line corresponds to the CO2 condensation curve.
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