Table 2.
Summary of the remaining orbital periods for HIP 41378 d (assuming no TTV).
| Orbital period [d] | TESS | CHEOPS | RM | emin |
|---|---|---|---|---|
| 1113.4465 ± 0.0034 | ✓ | ✓ | ✗ | ∼0.52 |
| 371.1488 ± 0.0011 | ✓ | ✓ | ✗ | ∼0.21 |
| 278.3616 ± 0.0009 | ✓ | ✗ | ✓ | ∼0.14 |
| 101.2224 ± 0.0003 | ✓ | ✓ | ✗ | ∼0.15 |
Notes. Orbital solutions compatible with no transit in TESS and CHEOPS observations are shown with a check mark (✓), while those incompatible are shown with an ✗. Orbital period values are taken from Becker et al. (2019). The RM column corresponds to the results in Grouffal et al. (2022) for the RM detection of the transit. The last column displays the minimal eccentricity that corresponds to tdur ≈ 12.5 h.
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