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Table 5

Model restitution of the chosen observational constraints plus quantities of interest.

Model T eff L [Fe/H] log g R ⟨ Δν ν max r02 rr01/10 X C ΔY/ ΔZ M cc R zc Mpsini
[K] [L] [dex] [dex] [R] [μHz] [μHz] [M] [R] [MJupiter]

A1 6116. 2.053 0.22 4.29 1.28 101.33 2127. 0.074 0.033 0.28 2.0 0.032 0.767 1.17 ± 0.03
A2a 6050. 2.063 0.22 4.28 1.31 98.13 2061. 0.081 0.034 0.33 2.0 0.024 0.798 1.18 ± 0.03
A2b 6053. 2.063 0.22 4.28 1.31 98.14 2089. 0.088 0.035 0.40 2.0 0.019 0.819 1.19 ± 0.03
A2c 6067. 2.082 0.21 4.28 1.31 98.26 2083. 0.086 0.034 0.38 2.0 0.021 0.813 1.19 ± 0.03
A3 6024. 2.066 0.22 4.28 1.32 98.15 2086. 0.086 0.034 0.39 1.5 0.017 0.813 1.20 ± 0.03
A4 6110. 2.055 0.22 4.28 1.28 98.13 2035. 0.084 0.035 0.33 3.3 0.035 0.809 1.14 ± 0.03
A5 6116. 2.053 0.22 4.32 1.28 104.16 2253. 0.083 0.033 0.38 1.0 0.011 0.785 1.22 ± 0.05
A6 6043. 2.081 0.23 4.29 1.32 98.29 2095. 0.083 0.034 0.37 1.5 0.021 0.801 1.20 ± 0.03
A7 6020. 2.102 0.23 4.29 1.34 98.29 2124. 0.084 0.034 0.39 0.8 0.014 0.800 1.23 ± 0.03

Notes. Models listed here were optimized with the reference physics (set A, different cases, see Sect. 3 and Tables 2 and 3). As explained in the text, in cases 2b, 2c, 4, and 7 the optimization considers individual frequencies and separations that were corrected for near-surface effects while in cases 5 and 6 the optimization is based on un-corrected separation ratios r02 and rr01 /10. In case 1 no seismic constraints are considered. In cases 1, 5, and 6, we nevertheless chose to list below a corrected value of ⟨ Δν, i.e. a value corrected for surface effects a posteriori, after the optimized model was obtained. In cases 2a and 3, the scaling values of ⟨ Δν are given, while in case 2c, we list Δνasym. Models without reference options are presented in the appendix.

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