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Table 2
Objects with expected non-circular shadows, indicated by the adopted peculiarity criteria Eqs. (14)–(16).
| KIC (a) | KOI (b) |  |
 |
 |
Notes |
|---|---|---|---|---|---|
| 5 357 901 | 188.01 | 2.70 | 0.38 | 1.08 | Noise problem in D; e < 0.33 |
| 5 794 240 | 254.01 | 2.96 | 1.80 | 1.18 |  |
| 9 595 827 | 217.01 | 0.21 | 1.45 | 2.79 | Noise problem in D |
| 9 941 662 | 13.01 | 1.16 | 6.03 | 4.02 | ≈50% uncertainty of ap |
| 10 748 390 | 3.01 | 4.01 | 0.20 | 0.25 | Noise problem in D;  |
| 10 874 614 | 17.01 | 0.45 | 4.55 | 4.83 | Noise problem in D |
| 11 517 719 | 1416.01 | 2.64 | 3.77 | 2.08 |
Notes. (a) Identification KIC number of host star in the Kepler Input Catalog (Kepler Mission Team 2009). (b) The number of Kepler Object of Interest (KOI).
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