Table C.1
Comparison of the tested periods for HIP 41378 e.
| Planet order | log Z | Δ log Z | ESS |
|---|---|---|---|
| d − e − f | 8855.93 ± 0.40 | 0.0 | 5242 |
| e − d − f | 8849.43 ± 0.40 | −6.50 | 4960 |
| d − f − e | 8841.23 ± 0.38 | −14.70 | 4803 |
Notes. Comparison of the tested orbital periods for HIP 41378 e with photometry and RV data. The columns report, from left to right: the assumed planetary ordering, the Bayesian evidence (log Z) with its uncertainty, the evidence difference Δ log Z relative to the highest-evidence model, and the effective sample size (ESS).
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