How internal structure shapes the metallicity of giant exoplanets

Open Access

Table A.2

List of bulk metallicity estimates found by the study.

Planet Name	Z_DC0.25	Z_DC0.5	Z_DC0.75	Z_DCA	Z_DCA3	Z_CEA
TOI-4010d				0.631 ± 0.002	0.692 ± 0.012
HATS-72b				0.380 ± 0.006	0.405 ± 0.005
WASP-156b				0.720 ± 0.004	0.720 ± 0.050
HAT-P-12b*	0.119 ± 0.048	0.124 ± 0.047	0.124 ± 0.047	0.123 ± 0.047	0.163 ± 0.049	0.129 ± 0.050
TOI-3629b*		0.389 ± 0.028	0.372 ± 0.027	0.427 ± 0.029	0.436 ± 0.027	0.453 ± 0.026
HD332231b*	0.195 ± 0.035	0.214 ± 0.045	0.209 ± 0.043	0.210 ± 0.046	0.267 ± 0.045	0.222 ± 0.049
K2-329b				0.371 ± 0.047	0.375 ± 0.026
WASP-69b				0.085 ± 0.046	0.131 ± 0.046
HAT-P-19b*	0.019 ± 0.014	0.021 ± 0.014	0.021 ± 0.015	0.046 ± 0.017	0.094 ± 0.017	0.048 ± 0.017
TOI-4406b*	0.038 ± 0.025	0.043 ± 0.025	0.043 ± 0.024	0.049 ± 0.021	0.111 ± 0.026	0.051 ± 0.021
TOI-1268b				0.428 ± 0.044	0.421 ± 0.031
K2-287b*	0.229 ± 0.015	0.246 ± 0.024	0.240 ± 0.023	0.270 ± 0.023	0.303 ± 0.023	0.289 ± 0.024
HATS-49b*		0.385 ± 0.027	0.367 ± 0.024	0.406 ± 0.032	0.421 ± 0.024	0.419 ± 0.025
WASP-132b				0.300 ± 0.053	0.332 ± 0.046
TOI-5344b*	0.064 ± 0.034	0.065 ± 0.033	0.064 ± 0.034	0.105 ± 0.033	0.156 ± 0.023	0.108 ± 0.035
TOI-201b*	0.053 ± 0.031	0.084 ± 0.029	0.082 ± 0.029	0.124 ± 0.029	0.169 ± 0.029	0.130 ± 0.031
HATS-75b*	0.184 ± 0.026	0.182 ± 0.025	0.179 ± 0.024	0.220 ± 0.023	0.241 ± 0.021	0.233 ± 0.026
HAT-P-17b*	0.041 ± 0.028	0.038 ± 0.028	0.040 ± 0.028	0.049 ± 0.026	0.083 ± 0.027	0.050 ± 0.026
WASP-84b*	0.124 ± 0.051	0.137 ± 0.046	0.135 ± 0.044	0.135 ± 0.045	0.194 ± 0.044	0.140 ± 0.048
TOI-3714b*	0.121 ± 0.038	0.121 ± 0.035	0.120 ± 0.035	0.153 ± 0.033	0.181 ± 0.030	0.161 ± 0.036
HAT-P-54b*	0.154 ± 0.048	0.162 ± 0.049	0.158 ± 0.048	0.161 ± 0.049	0.194 ± 0.048	0.166 ± 0.051
K2-290c				0.095 ± 0.056	0.126 ± 0.058
TOI-1478b				0.057 ± 0.034	0.096 ± 0.032
K2-140b				0.066 ± 0.036	0.105 ± 0.040
TOI-1811b*	0.099 ± 0.046	0.110 ± 0.042	0.108 ± 0.041	0.141 ± 0.042	0.172 ± 0.038	0.145 ± 0.044
WASP-130b				0.323 ± 0.051	0.349 ± 0.061
TOI-2010b*	0.037 ± 0.028	0.040 ± 0.031	0.062 ± 0.038	0.093 ± 0.065	0.113 ± 0.031	0.074 ± 0.031
TOI-5542b				0.099 ± 0.088	0.184 ± 0.160
HATS-17b				0.428 ± 0.042	0.404 ± 0.031
HATS-74Ab*	0.056 ± 0.030	0.064 ± 0.031	0.063 ± 0.030	0.103 ± 0.041	0.169 ± 0.014	0.106 ± 0.031
Kepler-117c				0.082 ± 0.018	0.076 ± 0.026
TIC237913194b				0.072 ± 0.039	0.109 ± 0.036
HAT-P-15b				0.086 ± 0.042	0.125 ± 0.036
TOI-4515b				0.101 ± 0.055	0.123 ± 0.042
K2-114b				0.255 ± 0.045	0.275 ± 0.044
TOI-4127b				0.064 ± 0.031	0.121 ± 0.030
HATS-76b*	0.046 ± 0.030	0.028 ± 0.014	0.060 ± 0.038	0.107 ± 0.051	0.151 ± 0.042	0.097 ± 0.046
TOI-2180b*	0.096 ± 0.029	0.105 ± 0.030	0.098 ± 0.030	0.106 ± 0.032	0.142 ± 0.028	0.142 ± 0.062
NGTS-20b				0.094 ± 0.044	0.124 ± 0.039
TOI-5153b*	0.067 ± 0.040	0.080 ± 0.045	0.079 ± 0.044	0.123 ± 0.057	0.150 ± 0.054	0.118 ± 0.058
TOI-2589b*	0.034 ± 0.023	0.038 ± 0.026	0.038 ± 0.026	0.054 ± 0.025	0.090 ± 0.032	0.065 ± 0.033
WASP-162b				0.181 ± 0.082	0.198 ± 0.068
TOI-2338b				0.165 ± 0.031	0.165 ± 0.035

Notes. Retrieved bulk metallicities for the following tested models: DC0.25, DC0.5, DC0.75, DCA, DCA3, and CEA. Planet names without the asterisk (*) are missing data from DC and CEA models; hence, the statistical analysis was carried out only for the 21 planets with radius uncertainties smaller than 3% (σ_R < 3%).

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