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Table 2
Timing results of the perturbed circular orbit fit for the Kepler-87 b and Kepler-87 c planets.
| Best-fit time of | Median time of | Residuals from | 1σ |
| mid transit | mid transit | linear ephemeris | error |
| (BJD-2 454 833) | (BJD-2 454 833) | [d] | [d] |
|
|
|||
| Kepler-87 b | |||
|
|
|||
| 165.1564 | 165.1576 | 0.0056 |
|
| 279.8881 | 279.8884 | 0.0001 | ± 0.0017 |
| 394.6166 | 394.6161 | −0.0086 | ± 0.0016 |
| 509.3531 | 509.3527 | −0.0083 | ± 0.0014 |
| 624.1031 | 624.1034 | 0.0060 | ± 0.0014 |
| 738.8414 | 738.8409 | 0.0071 |
|
| 853.5690 | 853.5700 | −0.0001 |
|
| 968.3024 | 968.3010 | −0.0055 | ± 0.0020 |
| 1197.7846 | 1197.7845 | 0.0053 | ± 0.0015 |
| 1312.5218 | 1312.5223 | 0.0068 |
|
| 1541.9800 | 1541.9798 | −0.0085 |
|
|
|
|||
| Kepler-87 c | |||
|
|
|||
| 286.0894 | 286.0900 | −0.1606 |
|
| 477.6302 | 477.6292 | 0.1467 |
|
| 860.0537 | 860.0483 | 0.1022 |
|
| 1242.3155 | 1242.3152 | −0.0945 |
|
Notes. Residuals are calculated relative to the best-fit linear solution.
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