Table C.1
HD 55693 model statistics.
| ln P-ln 𝒵 | ln 𝒵 |  |
BIC |  |
RMS | |
|---|---|---|---|---|---|---|
| WN (K0) | 11.48±0.01 | -235.28±0.01 | 0.25 | 474.19±0.01 | 1.09±0.01 | 3.54±0.01 |
| WN (K1) | 23.68±0.03 | -218.95±0.01 | 0.43 | 439.29±0.06 | 1.16±0.01 | 2.54±0.01 |
| WN (K2) | 33.97±0.30 | -214.29±0.10 | 0.09 | 431.53±0.45 | 1.22±0.16 | 2.11±0.01 |
| MA (K0) | 13.84±0.10 | -227.94±0.11 | 0.07 | 463.64±0.01 | 1.11±0.01 | 3.15±0.01 |
| MA (K1) | 22.13±0.09 | -213.12±0.05 | 0.09 | 439.57±0.16 | 1.18±0.07 | 2.41±0.02 |
| MA (K2) | 33.70±0.86 | -212.91±0.18 | 0.10 | 438.18±1.67 | 1.36±0.01 | 2.06±0.02 |
| SA (K0) | 3.48±0.06 | -217.79±0.06 | 0.09 | 438.89±0.07 | 1.16±0.04 | 2.73±0.01 |
| SA (K1) | 25.99±0.12 | -213.49±0.08 | 0.08 | 437.04±0.17 | 1.23±0.05 | 2.27±0.01 |
| SA (K2) | 35.54±1.51 | -213.29±0.04 | 0.09 | 439.69±3.01 | 1.05±0.22 | 1.99±0.08 |
| SAMA (K0) | -1.23±0.22 | -215.74±0.20 | 0.10 | 440.54±0.28 | 1.22±0.06 | 2.60±0.01 |
| SAMA (K1) | 32.22±0.05 | -213.38±0.01 | 0.09 | 440.59±1.66 | 1.27±0.02 | 2.12±0.15 |
| SAMA (K2) | 41.57±0.28 | -212.03±0.07 | 0.11 | 433.97±0.54 | 1.27±0.04 | 1.85±0.01 |
| 𝒢𝒫 rot(K0) | 28.01±0.01 | -235.17±0.01 | 0.22 | 463.06±0.02 | 1.09±0.011 | 2.68±0.01 |
| 𝒢𝒫 rot(K1) | 31.10±0.59 | -211.76±0.12 | 0.10 | 432.21±1.16 | 0.40±0.074 | 0.81±0.05 |
| 𝒢𝒫 rot+SHO(K0) | 27.55±0.13 | -214.70±0.12 | 0.18 | 436.34±0.13 | 0.41±0.010 | 0.81±0.04 |
Notes. Runs from different models: (Kn) denotes the number of Keplerian signals. In descending order: white noise only (WN), exponentially weighted moving average (MA), stellar activity linearly correlated (SA), stellar-activity plus moving average (SAMA), Gaussian Process with a rotation kernel (𝒢𝒫 rot), and GP with a rotation kernel plus a simple harmonic oscillator (𝒢𝒫 rot+SHO).
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