Table 1
Twenty-three possible orbital solutions for the period of HIP41378 d.
| Orbital period [d] | TESS | RM 2019 | RM 2019+2022 |
|---|---|---|---|
| 1113.4465 | ✓ | ✗ | ✗ |
| 556.7233 | ✓ | ✓ | ✗ |
| 371.1488 | ✓ | ✗ | ✗ |
| 278.3616 | ✓ | ✓ | ✓ |
| 222.6893 | ✗ | ✗ | ✗ |
| 185.5744 | ✓ | ✓ | ✗ |
| 159.0638 | ✗ | ✗ | ✗ |
| 139.1808 | ✗ | ✓ | ✓ |
| 123.7163 | ✗ | ✗ | ✗ |
| 111.3447 | ✗ | ✓ | ✗ |
| 101.2224 | ✓ | ✗ | ✗ |
| 92.7872 | ✓ | ✓ | ✓ |
| 85.6497 | ✗ | ✗ | ✗ |
| 79.5319 | ✗ | ✓ | ✗ |
| 74.2298 | ✗ | ✗ | ✗ |
| 69.5904 | ✗ | ✓ | ✓ |
| 65.4969 | ✗ | ✗ | ✗ |
| 61.8581 | ✗ | ✓ | ✗ |
| 58.6024 | ✗ | ✗ | ✗ |
| 55.6723 | ✗ | ✓ | ✓ |
| 53.0213 | ✗ | ✗ | ✗ |
| 50.6112 | ✗ | ✓ | ✗ |
| 48.4107 | ✗ | ✗ | ✗ |
Notes. Values are taken from Becker et al. (2019). The orbital solutions that would have led to a transit during one of the sectors when TESS observed HIP41378 are indicated with ✗, while those compatible with no transit detection in TESS data have a ✓ Similarly, orbital solutions compatible with the RM detection in the 2019 event alone and both the 2019 and 2022 events have a ✓while those that are not compatible with those observations have an ✗. The adopted solution is highlighted in bold face.
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