Fig. 8

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Fitted eclipse depths from the 9 CHEOPS occultation observations (in blue) and 5 CHEOPS occultations extracted from the phase curves (in red). The eclipse depth derived from the joint CHEOPS phase curve fit is shown in green (367 ± 17 ppm, with 1σ shaded) and the mean value of these 14 occultations (320 ± 11 ppm) is shown in orange (with 1σ shaded). These two mean eclipse depths are consistent with each other by just over 2σ. The right-hand y-axis shows how the eclipse depths convert to dayside brightness temperatures, assuming the dayside hemisphere is a blackbody and radiates at a uniform temperature.
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