Table A.2
Frequencies for Star B.
| Degree | Frequency (μHz) | 1-σ error (μHz) |
|
|
||
| 0 | 1895.30 | 0.33 |
| 0 | 1998.14 | 0.33 |
| 0 | 2101.33 | 0.34 |
| 0 | 2206.00 | 0.19 |
| 0 | 2309.40 | 0.39 |
| 0 | 2412.25 | 0.51 |
| 0 | 2517.48 | 0.70 |
| 0 | 2620.37 | 0.82 |
|
|
||
| 1 | 1840.59 | 0.28 |
| 1 | 1942.22 | 0.34 |
| 1 | 2046.03 | 0.33 |
| 1 | 2149.80 | 0.19 |
| 1 | 2254.19 | 0.23 |
| 1 | 2358.27 | 0.32 |
| 1 | 2461.65 | 0.59 |
| 1 | 2565.83 | 0.56 |
| 1 | 2672.28 | 0.12 |
|
|
||
| 2 | 1888.50 | 0.48 |
| 2 | 1991.24 | 0.79 |
| 2 | 2094.36 | 0.48 |
| 2 | 2198.06 | 0.39 |
| 2 | 2301.19 | 0.56 |
| 2 | 2405.91 | 1.06 |
| 2 | 2509.17 | 3.41 |
Notes. The first column is the spherical harmonic degree. The second column is the temporal frequency. The third column is the 1-σ uncertainty quoted when the mode is fitted. All modes were correctly detected and fitted. Please note that in order to get the frequencies at the source, one must add –10-4ν to the observed frequencies which takes into account the stellar radial velocity of the star.
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