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Table 5

Parameters from transit light curve analysis, both with and without gravity darkening (GD).

Parameter (i) no GD (ii) GD λ free (iii) GD λ fixed
Fitted parameters:

Orbital period Porb (d) 1.2198747 ± 0.0000012 1.2198769 ± 0.0000011 1.219876280.00000102+0.00000095$1.21987628_{ - 0.00000102}^{ + 0.00000095}$
Transit epoch T0 (BJDTDB − 2450000) 8792.63255 ± 0.00053 8792.63167 ± 0.00049 8792.63188 ± 0.00045
Scaled semi-major axis a/R 3.60662822790.045+0.036$3.6066282279_{ - 0.045}^{ + 0.036}$ 3.5510.035+0.029$3.551_{ - 0.035}^{ + 0.029}$ 3.5120.024+0.022$3.512_{ - 0.024}^{ + 0.022}$
Radius ratio Rp/R 0.10918 ± 0.00098 0.107120.00074+0.00076$0.10712_{ - 0.00074}^{ + 0.00076}$ 0.10696 ± 0.00083
Transit impact parameter b 0.100.08+0.10$0.10_{ - 0.08}^{ + 0.10}$ 0.0700.056+0.073$0.070_{ - 0.056}^{ + 0.073}$ 0.0640.058+0.075$0.064_{ - 0.058}^{ + 0.075}$
Limb-darkening coefficient и+ 0.8010.090+0.087$0.801_{ - 0.090}^{ + 0.087}$ 0.8020.091+0.086$0.802_{ - 0.091}^{ + 0.086}$ 0.7370.087+0.090$0.737_{ - 0.087}^{ + 0.090}$
Limb-darkening coefficient u 0.630.16+0.21$ - 0.63_{ - 0.16}^{ + 0.21}$ 0.530.22+0.29$ - 0.53_{ - 0.22}^{ + 0.29}$ −0.26 ± 0.28
Longitude of ascending node Ω* 23822+17$238_{ - 22}^{ + 17}$ 201.5 (fixed)
Stellar inclination i (deg) 10912+15$109_{ - 12}^{ + 15}$ 100.5 ± 8.4
White noise level σw (ppm) 214±5 214±5 214±6
Red noise level σr (ppm) 16517 ± 227 16468 ± 218 16471 ±247
Derived parameters:

Semi-major axis a (au) 0.02603 ± 0.00040 0.02603 ± 0.00040 0.02603 ± 0.00040
Orbital inclination angle ip (degrees) 88.31.7+1.2$88.3_{ - 1.7}^{ + 1.2}$ 88.81.2+0.8$88.8_{ - 1.2}^{ + 0.8}$ 88.91.2+0.8$88.9_{ - 1.2}^{ + 0.8}$
Transit duration T14 (h) 2.893 ± 0.022 2.9430.022+0.027$2.943_{ - 0.022}^{ + 0.027}$ 2.979 ± 0.016
Planet radius Rp (RJup ) 1.724 ± 0.042 1.692 ± 0.039 1.689 ± 0.039
Sky-projected stellar obliquity λ (deg) 14817+22$ - 148_{ - 17}^{ + 22}$ −111.5 (fixed)
True obliquity ψ (deg) 13915+12$139_{ - 15}^{ + 12}$ 111.30.7+0.2$111.3_{ - 0.7}^{ + 0.2}$
Relative Bayesian information criterion (BIC) 0 +4.1 –5.3

Notes. The best ephemeris for planning future observations is not listed in this table, but rather in Section 7.2.

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