Table 4.
Results of the t1-asp-3freq, t1-asp-4freq, and t1-asp-5freq exercises.
| Exercise | Parameter | No classical constraint |
1-σ box constraint |
3-σ box constraint |
|||
|---|---|---|---|---|---|---|---|
| m.f. | MC | m.f. | MC | m.f. | MC | ||
| t1-asp-3freq | M (14) | 15.6 | 14.6 |
14 | 14 |
15.6 | 16.4 |
| R (7.48) | 10.18 | 10.78 |
7.50 | 7.50 |
10.18 | 10.49 |
|
| X (0.70) | 0.70 | 0.70 |
0.70 | 0.70 |
0.68 | 0.70 |
|
| Z (0.014) | 0.018 | 0.014 |
0.018 | 0.014 |
0.018 | 0.014 |
|
| αov (0.20) | 0.45 | 0.45 |
0.10 | 0.20 |
0.45 | 0.45 |
|
| Xc (0.288) | 0.237 | 0.182 |
0.283 | 0.283 |
0.237 | 0.221 |
|
| Te (27647) | 26977 | 25532 |
26953 | – | 26977 | – | |
| log g (3.8364) | 3.6150 | 3.5022 |
3.8341 | – | 3.6150 | – | |
| χ2 | 0.0358 | – | 0.0713 | – | 0.0358 | – | |
| t1-asp-4freq | M (14) | 13.8 | 13.9 |
13.8 | 13.8 |
13.8 | 13.9 |
| R (7.48) | 7.45 | 7.47 |
7.45 | 7.45 |
7.47 | 7.68 |
|
| X (0.70) | 0.68 | 0.70 |
0.68 | 0.68 |
0.68 | 0.70 |
|
| Z (0.014) | 0.014 | 0.014 |
0.014 | 0.014 |
0.014 | 0.014 |
|
| αov (0.20) | 0.20 | 0.20 |
0.20 | 0.20 |
0.20 | 0.20 |
|
| Xc (0.288) | 0.274 | 0.279 |
0.274 | 0.275 |
0.274 | 0.279 |
|
| Te (27647) | 27888 | 27901 |
27888 | – | 27888 | – | |
| log g (3.8364) | 3.8330 | 3.8330 |
3.8330 | – | 3.8330 | – | |
| χ2 | 0.2272 | – | 0.2272 | – | 0.2272 | – | |
| t1-asp-5freq | M (14) | 13.8 | 13.8 |
13.8 | 13.8 |
13.8 | 13.8 |
| R (7.48) | 7.45 | 7.46 |
7.45 | 7.45 |
7.45 | 7.46 |
|
| X (0.70) | 0.68 | 0.68 |
0.68 | 0.68 |
0.68 | 0.68 |
|
| Z (0.014) | 0.014 | 0.014 |
0.014 | 0.014 |
0.014 | 0.014 |
|
| αov (0.20) | 0.20 | 0.20 |
0.20 | 0.20 |
0.20 | 0.20 |
|
| Xc (0.288) | 0.274 | 0.275 |
0.274 | 0.275 |
0.274 | 0.275 |
|
| Te (27647) | 27888 | 27888 |
27888 | – | 27888 | – | |
| log g (3.8364) | 3.8330 | 3.8330 |
3.8330 | – | 3.8330 | – | |
| χ2 | 0.4175 | – | 0.4175 | – | 0.4175 | – | |
Notes. ( ‡ )Indicates when the grid resolution is reached and set as the limit to the confidence interval. The m.f. and MC acronyms respectively stand for the analysis based on the input set of observed constraints and that from the method with Monte-Carlo simulations (see Sect. 2). The “no classical constraint“ columns give the results without Te and log g used as constraints. The 1-σ and 3-σ columns gives the results when imposing the solutions to be respectively in the 1-σ and 3-σ boxes on Te and log g. The input stellar parameters of the input model are recalled between brackets in the first column. The M, R, Te, and g parameters are given in M⊙, R⊙, K, and cm s−2, respectively.
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