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Table B.2.

Extracted frequencies for Cl NGC 2264 VAS 219.

Designation f ASRa05 ϕ S/N cross-ref
(d−1) (mmag) ()
F1 2.09926(5) 4.07(1) 0.2272(5) 7.37 SRa01, TESS
F2 1.92554(6) 3.34(1) 0.9149(6) 7.05 SRa01, TESS
F3 1.36574(7) 2.77(1) 0.3421(7) 6.44 SRa01, TESS
F4 0.04759(7) 2.51(1) 0.8480(8) 5.93
F5 0.1993(1) 1.88(1) 0.126(1) 4.57
F6 2.0562(1) 1.96(1) 0.103(1) 5.22 SRa01, TESS
F7 1.3392(1) 1.88(1) 0.290(1) 4.94 SRa01
F8 2.1481(1) 1.88(1) 0.521(1) 6.10 SRa01
F9 3.4281(1) 1.62(1) 0.416(1) 9.91 SRa01
F10 1.8049(1) 1.58(1) 0.302(1) 5.32 SRa01, TESS
F11 3.7810(1) 1.50(1) 0.301(1) 13.95 SRa01
F12 0.1087(1) 1.57(1) 0.929(1) 5.00
F13 1.6359(1) 1.45(1) 0.303(1) 5.01 SRa01
F14 0.5601(1) 1.49(1) 0.277(1) 4.19 SRa01
F15 2.4539(1) 1.34(1) 0.327(1) 5.88 SRa01
F16 1.5451(2) 1.24(1) 0.416(2) 5.10 SRa01
F17 0.1662(2) 1.00(1) 0.329(2) 4.26
F18 1.0608(2) 1.11(1) 0.554(2) 3.74 SRa01
F19 0.3389(2) 1.03(1) 0.218(2) 4.10 SRa01
F20 2.3782(2) 1.01(1) 0.961(2) 5.07
F21 0.0773(2) 1.77(1) 0.278(2) 8.98
F22 1.8715(2) 1.00(1) 0.119(2) 4.93
F23 1.9070(2) 0.89(1) 0.316(2) 5.51
F24 1.6848(3) 0.72(1) 0.751(3) 4.26

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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