Table B.3.
Extracted frequencies for Cl⋆ NGC 2264 VAS 230.
| Designation | f | ASRa01 | ϕ | S/N | cross ref |
|---|---|---|---|---|---|
| (d−1) | (mmag) | ( ) |
|||
| F1 | 8.1866(4) | 0.77(1) | 0.336(3) | 6.71 | SRa05, TESS |
| F2 | 8.4660(6) | 0.62(1) | 0.730(3) | 9.10 | SRa05, TESS |
| F3 | 8.5591(8) | 0.42(1) | 0.891(4) | 7.98 | SRa05, TESS |
| F4 | 11.8419(9) | 0.35(1) | 0.175(6) | 10.87 | SRa05, TESS |
| F5 | 8.385(1) | 0.29(1) | 0.464(6) | 6.33 | TESS |
| F6 | 2.3203(7) | 0.58(1) | 0.282(4) | 4.18 | SRa05 |
| F7 | 2.2407(6) | 0.54(1) | 0.650(4) | 5.07 | SRa05 |
| F8 | 2.1643(6) | 0.49(1) | 0.718(3) | 4.15 | SRa05 |
| F9 | 3.3006(8) | 0.46(1) | 0.275(5) | 5.48 | SRa05 |
Notes. The values in parentheses give the 1σ uncertainty as reported by the standard error estimates formulated by Montgomery & O’Donoghue (1999). The amplitudes (ASRa01) are determined from the CoRoT SRa01 data. The last column (cross ref) marks the frequencies that can also be detected in the CoRoT SRa05 and TESS data. The first five frequencies are the p-modes and the second four frequencies are the g-modes; both are sorted by decreasing amplitude.
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