Table 1.
Photometric amplitudes and probabilities of being a contact binary of either late or early type for the objects in our sample.
| KIC/EPIC | a (mag) | σa (mag) | pCBL | pCBE |
|---|---|---|---|---|
| 1026032 | 0.085360 | 0.001293 | 0.0000 | 0.0000 |
| 1026957 | 0.001115 | 0.000429 | 0.0000 | 0.0000 |
| 1432214 | 0.098101 | 0.000707 | 0.0000 | 0.0000 |
| 1571511 | 0.022127 | 0.000116 | 0.0000 | 0.0000 |
| 1572353 | 0.116464 | 0.004660 | 0.9474 | 0.0000 |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
| 212163353 | 0.098400 | – | 0.0000 | 0.0000 |
| 212175535 | 0.080279 | – | 0.9402 | 0.0000 |
Notes. The full table is available at the CDS. For some systems, we were not able to reliably estimate their amplitude uncertainties. In our analysis, we adopted an uncertainty of 4% for these systems (Sect. 3.3).
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