Table B.1.
Extracted frequencies for Cl⋆ NGC 2264 VAS 196.
| Designation | f | ASRa05 | ϕ | S/N | cross-ref |
|---|---|---|---|---|---|
| (d−1) | (mmag) | ( ) |
|||
| F1 | 0.88674(8) | 1.344(7) | 0.4615(9) | 7.83 | SRa01, TESS |
| F2 | 1.3564(1) | 1.029(7) | 0.434(1) | 9.75 | SRa01, TESS |
| F3 | 1.3217(1) | 0.762(7) | 0.353(2) | 10.99 | SRa01, TESS |
| F4 | 1.4819(2) | 0.519(7) | 0.621(2) | 10.99 | SRa01 |
| F5 | 0.9083(2) | 0.451(7) | 0.062(2) | 5.84 | SRa01 |
| F6 | 0.1569(4) | 0.289(7) | 0.750(4) | 4.06 | |
| F7 | 1.2874(4) | 0.248(7) | 0.657(5) | 5.07 | |
| F8 | 2.7511(5) | 0.212(7) | 0.660(6) | 7.14 | SRa01 |
| F9 | 1.4420(5) | 0.233(7) | 0.558(5) | 6.22 |
Notes. The values in parentheses give the 1σ uncertainty as reported by the standard error estimates formulated by Montgomery & O’Donoghue (1999). The amplitudes (ASRa05) are determined from the CoRoT SRa05 data. The last column (cross-ref) marks the frequencies that can also be detected in the CoRoT SRa01 and TESS data.
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