Table 3
Transit times of HIP 41378 c from the global photometric analysis with PYORBIT.
| T0 (BJDTDB) | σT0 (days) | O-C (minutes) | Telescope |
|---|---|---|---|
| 2 457 163.1671 | 0.0035 | 112.25 | K2 |
| 2 457 194.8661 | 0.004 | 92.56 | K2 |
| 2 457 606.9849 | 0.004 | −117.49 | Spitzer |
| 2 458 272.8811 | 0.003 | −218.00 | K2 |
| 2 458 494.8820 | 0.015 | −200.39 | TESS |
| 2 459 509.8919 | 0.0094 | 94.18 | TESS |
| 2 459 541.5800 | 0.017 | 58.80 | TESS |
| 2 459 573.3330 | 0.014 | 116.88 | TESS |
| 2 459 636.7637 | 0.0043 | 124.61 | CHEOPS |
| 2 459 922.1468 | 0.004 | 80.11 | CHEOPS |
| 2 459 985.5543 | 0.0051 | 54.43 | CHEOPS |
| 2 459 985.5541 | 0.0089 | 54.14 | TESS |
| 2 460 270.9410 | 0.015 | 15.11 | TESS |
| 2 460 714.8127 | 0.0069 | −137.00 | TESS |
| 2 460 746.5209 | 0.0028 | −143.43 | CHEOPS |
Notes. The O-C values (third column) are computed with respect to the linear ephemeris: Tref = 2 457 163.089 ± 0.047 BJDTDB. Plin = 31.71266 ± 0.00063 days. The transit times are given in the BJDTDB standard (Eastman et al. 2010); the second column reports the associated 1-σ error.
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