Fig. B.1
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Similar to Fig. 7, but comparing the the results from fitting eclipse spectra extracted from the first (blue) and second (orange) eclipses. The retrieval set-up is for our nominal case of assuming chemical equilibrium retrieval and fitting for the geometric albedo. Results are compared to the main retrieval results from fitting the full phase curve (green). Residuals are compared to the joint eclipse fit (Fig. 4). With the exception of the hot-spot area factor, similar atmospheric parameters are inferred for each eclipse separately.
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