Evidence for disequilibrium chemistry from vertical mixing in hot Jupiter atmospheres - A comprehensive survey of transiting close-in gas giant exoplanets with warm-Spitzer/IRAC

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Table 5

Correlations between parameters and the transit depth ratio.

Parameter	r	p	Res Var
T_eq (a = 0)	−0.35	0.01	7.23
T_eff	−0.34	0.02	7.14
Stellar log (g)	0.13	0.36	6.98
[Fe/H]	−0.21	0.15	4.48
R_p	−0.26	0.07	8.11
Inclination	0.20	0.18	7.03
a (AU)	0.07	0.63	8.46
Planetary log (g)	0.01	0.92	8.47
M_p (M_J)	0.09	0.56	8.78
H (km)	−0.17	0.25	8.50
R_s (R_⊙)	−0.40	0.00	7.06
Radius anomaly	−0.25	0.14	6.86

Notes. We show the Pearson correlation coefficient (r), the associated chance probability (p), and the residual variance from an ODR linear fit to the data.

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