Table 1
Selected systems for observational follow-ups to detect transit timing shifts driven by wave breaking.
| Planet | EEP | fcrit |
[date] |
[s] |
|---|---|---|---|---|
| HAT-P-23 b | ![]() |
0% |
a
|
a
|
| HATS-18 b | ![]() |
20.6 % | 2021.4 ± 0.3 | ![]() |
| HIP 65 A b | ![]() |
0 % | 2033.2 ± 0.4a | 42.9 ± 2.5a |
| NGTS-10 b | ![]() |
0 % | 2027.0 ± 0.3a |
a
|
| TOI-1937 b | ![]() |
23.1 % | ![]() |
36 ± 6 |
| WASP-4 b | ![]() |
28.1 % | ![]() |
![]() |
| WASP-19 A b | ![]() |
0 % |
a
|
a
|
| WASP-43 b | ![]() |
0 % |
a
|
a
|
| WASP-103 b | ![]() |
0.47 % | ![]() |
![]() |
| HATS-9 b | ![]() |
100 % | ![]() |
![]() |
| TOI-1855 b | ![]() |
59.9 % | ![]() |
![]() |
| TOI-2337 b | ![]() |
95.6 % | ![]() |
![]() |
| WASP-135 b | ![]() |
87.3 % | ![]() |
![]() |
| WASP-163 A b | ![]() |
100 % | ![]() |
![]() |
Notes. (a)Calculated using the formal Q′WB estimate obtained without satisfying the Mcrit < Mp criterion, which results in fcrit = 0%. If wave breaking is indeed inactive, no measurable 5-minute transit-time shift is expected on practical observational timescales.
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