A transition between the hot and the ultra-hot Jupiter atmospheres

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Table B.1

Measure of the gradient of temperature vs. irradiation temperatures for three different temperatures: the individual brightness temperatures ( and ) and the dayside effective temperature (T_day), calculated as a weighted mean.

	T_eff
BB	0.85 ± 0.03	0.81 ± 0.05	0.92 ± 0.05
ATLAS	0.80 ± 0.03	0.79 ± 0.04	0.84 ± 0.04
PHOENIX	0.80 ± 0.03	0.76 ± 0.05	0.84 ± 0.05

Notes. Each set of temperatures is calculated using three different stellar models: blackbodies, ATLAS models, and PHOENIX models. Figure 3 displays the individual brightness temperatures for PHOENIX models and Fig. C.1 displays the effective temperatures.

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