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Fig. 23


Comparison of our observed Spitzer occultation data with synthetic emission spectra for GJ 436b from Moses et al. (2013). The green and blue curves correspond respectively to the best fit retrieved model, given S10 data, using the method of Line et al. and the 300×-solar model. The model band averages in the six bands are shown as coloured squares. Our Spitzer data are shown as orange circles.

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