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Fig. 8

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Maximum-likelihood parameters for the spherical harmonic power coefficient C11 (upper) and hotspot offset (lower) for the full sample of GCM fits and Spitzer phase curve fits in two filter bands. Blue points are the results of fits to GCMs, circles and squares correspond to inverted and non-inverted atmospheres. Red squares and black circles represent fits to the Spitzer phase curves in filters IRAC 1 and 2, respectively.

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