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Fig. 13


Emission phase curves computed for the synchronous case with an Earth-like atmosphere, for 4 spectral bands used in the GCM. Gray areas indicate the 1-sigma variability due to meteorology (mainly changing cloudiness). Dashed curves are calculated for a planet with no atmosphere with a constant surface albedo of 0.2. Contrary to Fig. 12, these plots include a dependency of the planetary radius on the inclination of R ∝ (M/sini)0.27.

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