Table B.2.
Parameters derived with SPECIES for the stars included in interferometric and asteroseismology works.
| HIP | HD | log g | Radius | Mass | Age | References |
|---|---|---|---|---|---|---|
| (cgs) | (R⊙) | (M⊙) | (Gyr) | |||
| 343 | 225197 | 2.44 ± 0.12 | 11.21 |
1.38 |
3.26 |
7 |
| 655 | 344 | 2.36 ± 0.11 | 11.25 |
1.27 |
4.24 |
7 |
| 3137 | 3750 | 2.38 ± 0.13 | 9.97 |
1.61 |
1.99 |
1 |
| 4293 | 5457 | 2.69 ± 0.09 | 9.07 |
1.50 |
2.47 |
7 |
| 4587 | 5722 | 2.69 ± 0.08 | 10.58 |
2.07 |
1.11 |
1 |
| 8102 | 10700 | 4.33 ± 0.06 | 0.83 |
0.77 |
13.04 |
3, 5 |
| 8928 | 11977 | 2.72 ± 0.08 | 10.64 |
2.29 |
0.82 |
1 |
| 9440 | 12438 | 2.65 ± 0.08 | 9.82 |
1.86 |
1.09 |
1 |
| 10234 | 13468 | 2.64 ± 0.08 | 10.57 |
2.00 |
1.19 |
1 |
| 11791 | 15779 | 2.75 ± 0.10 | 9.90 |
2.18 |
1.03 |
1 |
| 13147 | 17652 | 2.56 ± 0.08 | 10.15 |
1.87 |
1.16 |
1 |
| 16537 | 22049 | 4.40 ± 0.06 | 0.72 |
0.80 |
0.59 |
3 |
| 19849 | 26965 | 4.33 ± 0.06 | 0.77 |
0.75 |
12.18 |
3 |
| 69673 | 124897 | 1.67 ± 0.10 | 24.76 |
0.91 |
9.87 |
2 |
| 79672 | 146233 | 4.36 ± 0.05 | 1.04 |
1.03 |
3.92 |
3 |
| 89962 | 168723 | 3.01 ± 0.08 | 5.54 |
1.57 |
1.89 |
2 |
| 92968 | 175679 | 2.88 ± 0.10 | 12.63 |
3.04 |
0.35 |
2 |
| 95124 | 181342 | 3.13 ± 0.10 | 5.31 |
1.64 |
2.00 |
8 |
| 95222 | 181907 | 2.43 ± 0.10 | 11.20 |
1.45 |
2.68 |
2 |
| 98036 | 188512 | 3.61 ± 0.07 | 3.00 |
1.37 |
3.02 |
2, 5 |
| 102014 | 196737 | 2.71 ± 0.11 | 9.89 |
1.48 |
2.61 |
7 |
| 103836 | 200073 | 2.75 ± 0.09 | 7.84 |
1.03 |
8.79 |
7 |
| 105854 | 203949 | 2.46 ± 0.16 | 10.75 |
0.97 |
11.50 |
4, 7 |
| 110813 | 212771 | 3.38 ± 0.07 | 4.33 |
1.57 |
1.95 |
4, 8 |
| 114775 | 219263 | 2.70 ± 0.12 | 8.62 |
1.43 |
3.26 |
7 |
| 116630 | 222076 | 3.17 ± 0.12 | 4.28 |
1.28 |
4.54 |
6 |
Notes. Some stars in the list do not belong to the EXPRESS programme, but were included to test the method.
References. (1) Gallenne et al. (2018); (2) Morel et al. (2014); (3) Tsantaki et al. (2013); (4) Campante et al. (2019); (5) Rains et al. (2020); (6) Jiang et al. (2020); (7) Aguirre et al. (2020); (8) North et al. (2017).
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