Table 5.
Binaries from Gaia DR3 in the sample of stars with anomalous peaks, reported by Colman et al. (2017).
| KIC | Ppeak | Porb | e |
|---|---|---|---|
| [d] | [d] | ||
| Possible physical associations | |||
| 2449020 | 0.83 | 310 ± 2 | 0.29 ± 0.05 |
| 10936814 | 4.45 | 665 ± 6 | 0.02 ± 0.03 |
| 7596350 | 0.26 | 647 ± 11 | 0.04 ± 0.04 |
| Presumed chance alignments | |||
| 5556726 | 0.48 | 172 ± 1 | 0.24 ± 0.02 |
| 12117138 | 4.40 | 685 ± 18 | 0.39 ± 0.03 |
| Confirmed chance alignments | |||
| 2167774 | 0.35 | 137.0 ± 0.2 | 0.21 ± 0.06 |
| 1872210 | 0.67 | 540 ± 6 | 0.20 ± 0.07 |
Notes. The period and eccentricity of the orbit is taken from Gaia DR3 TBO. Ppeak is the period of the dominant anomalous peak, reported by Colman et al. (2017). The categorisation of the anomalous peak, given by the authors is reported.
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