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Table 1.

Overview of the measured parameter values for our binary stars with detected γ Dor-type pulsations and tidal perturbations.

KIC 3228863 KIC 3341457 KIC 4947528 KIC 9108579 KIC 12785282 V456 Cyg(1)
TIC 394179296 137094904 169560376 273583841 406997952 15795549
Eclipsing y n n n y y
mKepler (mag) 11.816 13.873 13.910 11.560 13.518
νorb (d−1) 1.36809332(4) 1.8932976(5) 2.0121190(1) 0.85497202(16) 1.26782902(13) 1.122091(8)
νrot, nc (d−1) 1.371(3) 1.865(1) 2.03(2) 0.847(7) 1.264(3) 1.113(5)
Π0 (s) 4370(100) 3870(40) 4390(310) 4240(160) 4214(30) 4300(50)
Pulsating component Primary Unknown Unknown Unknown Primary Secondary

k 0 0 0 0 0 0
m 1 1 1 1 1 1
nmin −61 −72 −42 −47 −56 −31
nmax −28 −41 −21 −40 −19 −18
nspan 34 32 22 8 38 14
Tidal perturbations y y y n y y

k −2 −2 0
m −1 −1 2
nmin −24 −53 −61
nmax −18 −33 −49
nspan 7 21 13
Tidal perturbations n y y

Notes. The middle and bottom sections contain the relevant parameters for the first and (if detected) second g-mode period-spacing pattern of each target, respectively. The νrot, nc parameter is the near-core rotation frequency, measured from asteroseismic modelling. The nspan parameter indicates the total number of radial orders that the g-mode pulsations within the detected period-spacing patterns span. The ‘tidal perturbation’ parameter indicates when tidal perturbations were detected for any pulsation in a g-mode period-spacing pattern.

References. (1) studied by Van Reeth et al. (2022b).

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