Table D.4
GJ 699 FWHM ESPRESSO parameter comparison.
| Parameter | Prior | WN(K3) | 𝒢𝒫 grot(K0) | 𝒢𝒫 rot(K0) | 𝒢𝒫 rot(K1) | 𝒢𝒫 rot+Mag(a) | 𝒢𝒫 rot+Mag(b) |
|---|---|---|---|---|---|---|---|
| Offsets and Jitter | |||||||
| γE18 | ~ 𝒰 (-10.5,10..5) | ![]() |
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| γE19 | ~ 𝒰 (-10.5,10.5) | ![]() |
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| σE18 | ~ 𝒩 (0.5,1) | ![]() |
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| σE19 | ~ 𝒩 (0.5,1) | ![]() |
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| P1 | ~ 𝒰 (50,300) | ![]() |
- | - | ![]() |
- | - |
| K1 | ~ 𝒰 (0,6.60) | ![]() |
- | - | ![]() |
- | - |
| ϕ1 | ~ 𝒰 (0,2π) | ![]() |
- | - | ![]() |
- | - |
| e1 | ~ 𝒩 (0,0.1) | ![]() |
- | - | ![]() |
- | - |
| ω1 | ~ 𝒰 (0,2π) | ![]() |
- | - | ![]() |
- | - |
| P2 | ~ 𝒰 (50, 300) | ![]() |
- | - | - | - | - |
| K2 | ~ 𝒰 (0, 6.60) | ![]() |
- | - | - | - | - |
| ϕ2 | ~ 𝒰 (0, 2π) | ![]() |
- | - | - | - | - |
| e2 | ~ 𝒩 (0, 0.1) | ![]() |
- | - | - | - | - |
| ω2 | ~ 𝒰 (0, 2π) | ![]() |
- | - | - | - | - |
| P3 | ~ 𝒰 (1,5000) | ![]() |
- | - | - | - | - |
| K3 | ~ 𝒰 (0, 6.60) | ![]() |
- | - | - | - | - |
| ϕ3 | ~ 𝒰 (0, 2π) | ![]() |
- | - | - | - | - |
| e3 | ~ 𝒩 (0, 0.1) | ![]() |
- | - | - | - | - |
| ω3 | ~ 𝒰 (0, 2π) | ![]() |
- | - | - | - | - |
| 𝒢𝒫 grotρ | ~ 𝒰 (50, 300) | - | ![]() |
- | - | - | - |
| 𝒢𝒫 grotτ | ~ 𝒰 (50, 600) | - | ![]() |
- | - | - | - |
| 𝒢𝒫 grotA1 | ~ 𝒩 (3.3, 3.3) | - | ![]() |
- | - | - | - |
| 𝒢𝒫 grotA2 | ~ 𝒩 (3.3, 6.6) | - | ![]() |
- | - | - | - |
| 𝒢𝒫 rotρ | ~ 𝒰 (50, 300) | - | - | ![]() |
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| 𝒢𝒫 rotσ | ~ 𝒩 (3.3, 3.3) | - | - | ![]() |
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| 𝒢𝒫 rotQ0 | ~𝒰 (0, 100) | - | - | ![]() |
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| 𝒢𝒫 rotδQ | ~ 𝒰 (0, 100) | - | - | ![]() |
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| 𝒢𝒫 rot f | ~ 𝒰 (0, 1) | - | - | ![]() |
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| Pmag | ~ 𝒰 (1,5000) | - | - | - | - | ![]() |
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| A1mag | ~ 𝒰 (0, 6.6) | - | - | - | - | ![]() |
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| A2mag | ~ 𝒰 (0, 6.6) | - | - | - | - | ![]() |
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| ϕ1mag | ~ 𝒰 (0, 2π) | - | - | - | - | ![]() |
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| ϕ2mag | ~ 𝒰 (0, 2π) | - | - | - | - | ![]() |
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Notes. Runs from different models: (Kn) denotes the number of Keplerian signals. In descending order: white noise only (WN), Gaussian process with a rotation kernel (𝒢𝒫 rot), and GP with a rotation kernel and a magnetic cycle (𝒢𝒫rot+Mag). This last model was tested with two different priors for the magnetic cycle: (a) 𝒰 (0.5, 5000), and (b) 𝒰 (800, 5000).
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