Table 1
References for the observational data.
| Planet | Reference |
|---|---|
| GJ 436b | Knutson et al. (2011) (1) |
| Knutson et al. (2014) | |
| Morello et al. (2015) (2) | |
| Lothringer et al. (2018) | |
| GJ 1214b | Fraine et al. (2013) (3) |
| Kreidberg et al. (2014) (4) | |
| GJ 3470b | Benneke et al. (2019) |
| HAT-P-1b(*) | Wakeford et al. (2013) |
| Nikolov et al. (2014) | |
| HAT-P-11b | Chachan et al. (2019) |
| HAT-P-12b | Wong et al. (2020) |
| HAT-P-26b | Wakeford et al. (2017) |
| HD 97658b | Guo et al. (2020) (5) |
| HD 189733b(*) | Pont et al. (2013) |
| McCullough et al. (2014) | |
| Sing et al. (2016) | |
| HD 209458b(*) | Sing et al. (2016) |
| WASP-6b | Carter et al. (2020) |
| WASP-12b(*) | Sing et al. (2013) |
| Kreidberg et al. (2015) | |
| Sing et al. (2016) | |
| WASP-17b | Sing et al. (2016) |
| WASP-19b(*) | Huitson et al. (2013) |
| Sing et al. (2016) | |
| WASP-31b | Sing et al. (2015) |
| Sing et al. (2016) | |
| WASP-39b | Sing et al. (2016) |
| Fischer et al. (2016) | |
| Wakeford et al. (2018) |
Notes. (*) Planet samples with masses larger than half Jupiter mass, for which disequilibrium retrieval with fixed Tint is additionally performed. (1) The average of three measurements at the Spitzer 8.0 μm band is used, excluding the observed transit on UT 2009 February 2 due to the possible stellar activity effect. (2) The results presented in Table 6 are used. (3)The “simultaneous” fit results are used. (4)The “divide-white” fit results are used. (5)Following the approach of this study, we do not include the HST/STIS data points for our retrieval due to their large discrepancy at long wavelengths. Also, the results derived using the “logarithmic visit-long trend” are used.
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