Table 3.
Candidates from the eclipsing binary Gaia DR3 catalog with at least one oscillating component.
| TIC | Frequency (geom.) | νmax | Δν | Reference for | Data | Comment |
|---|---|---|---|---|---|---|
| [d−1] | [μHz] | [μHz] | seismic values | |||
| 235050452 | 0.09336 ± 0.00002 | 98 ± 10 | 9.2 ± 0.1 | Mackereth et al. (2021) | 6S | Surface or synchronized rotation? |
| 272357503 | 0.99314 ± 0.00001 | 51 ± 13 | 5.7 ± 0.2 | Mackereth et al. (2021) | 23S | |
| 293937699 | 0.26058 ± 0.00006 | 47 ± 4 | 6 ± 20 | Mackereth et al. (2021) | 16S | Eclips. bin., actual period: 65.112 d |
| 33767523 | 0.04607 ± 0.00003 | − | − | − | 18S | Porb = 49.63 ± 0.02, e = 0.33 ± 0.01 |
| 268157208 | 0.02770 ± 0.00008 | 47.49 | 4.804 | Yu et al. (2018) | 1Q, 3S | = KIC 8646982 |
Notes. The first column reports the identifier of the eclipsing binary candidate in the TESS Input Catalogue (TIC). The column “Frequency” specifies the frequency of geometric model of the eclipsing binary light curve. The third and fourth column report the mean seismic parameters νmax and Δν from Mackereth et al. (2021), respectively. Those seismic parameters were extracted from the references shown on the next columns. the column “Data” reports how many Sectors (S) of TESS, or Quarters (Q) of data was available for these systems at the time of the analysis. Comments on the system are provided in the last column: the period reported for TIC 293937699 was redetermined from TESS data; the orbital parameters for TIC 33767523 are reported in the TBO catalog by Gaia Collaboration (2023a).
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