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Table A.1.
Priors and posteriors on planet parameters. We note that Pi refers to the instantaneous period that best fits the 2021 measurements, and is different from Pmean, which minimizes the scatter of the TTVs of all observations between 2018–2021.
| AU Mic b | AU Mic c | |
|---|---|---|
| PRIORS | ||
| D | 𝒩(0.003, 0.001) | 𝒩(0.0015, 0.0004) |
| W[h] | 𝒩(3.656, 0.203) | 𝒩(3.892, 0.4) |
| b | 𝒰(0.00, 0.30) | 𝒰(0.3, 0.7) |
| Pi[d] | 𝒩(8.463000, 0.003) | 𝒩(18.8590, 0.0030) |
| T0 | 𝒩(9447.52630, 0.004) | 𝒩(9436.0350, 0.0072) |
| POSTERIORS | ||
| D | 0.00187 ± 0.00008 | 0.00098 ± 0.00010 |
| W[h] | 3.514 ± 0.026 | 4.290 ± 0.307 |
| b | 0.17 ± 0.10 | 0.58 ± 0.13 |
| Pi[d] | 8.46353 ± 0.00024 | 18.8602 ± 0.0026 |
| T0 | 9447.52634 ± 0.00046 | 9436.036 ± 0.004 |
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