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Fig. 22


Model planet-to-star flux ratios compared to the observed Spitzer occultation data. Both models assume a hot day side, with absorbed energy redistributed only over the dayside. The blue model uses solar metallicity, while the red model uses 50×-solar. The Spitzer data are orange circle while the model band averages in the six bands are shown as coloured squares. The location of prominent absorption features that differ between the models (where CO and CO2 absorb strongly) are labelled. The planet-to-star flux ratios of 500, 700, and 900 K blackbodies are shown in dashed black.

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