Table B.1
Prior parameter distributions* of the global fit with the PyMC3 and exoplanet packages (see Section 3.3).
| Parameter | HAT-P-33 | HAT-P-49 | HD 89345 | |
|---|---|---|---|---|
| Instrument Offsets | ||||
| 〈RV〉SOPHIE | [ms−1] | 𝒩 (23236.35, 1.0) | 𝒩(14511.75, 1.0) | 𝒩(2312.0, 1.0) |
| 〈RV〉HIRES | [ms−1] | 𝒩 (13.65, 1.0) | 𝒩(1.35, 1.0) | |
| 〈RV〉TRES | [ms−1] | 𝒩(45.5, 1.0) | ||
| 〈RV〉HARPS | [ms−1] | 𝒩(2357.5, 1.0) | ||
| 〈RV〉HARPS-N | [ms−1] | 𝒩(2350.2, 1.0) | ||
| 〈RV〉FIES | [ms−1] | 𝒩(-5.4, 1.0) | ||
| 〈RV〉APF | [ms−1] | 𝒩(-2.0, 1.0) | ||
| Keplerian Parameters** | ||||
| T0 | [BTJD] | 𝒩 (6684.86508, 0.00027) | 𝒩(6975.61736, 0.00050) | 𝒩(8740.81147, 0.00044) |
| ln P | 𝒩 (1.2454442, 1.9 10−7) | 𝒩(0.9901187, 4.5 10−7) | 𝒩(2.4693193, 5.6 10−7) | |
| ln K | 𝒩 (4.3567, 0.1538) | 𝒩(5.2402, 0.1161) | 𝒩(2.2502, 0.0885) | |
 |
𝒩 (0.42400562, 0.13834369) | 𝒩(-0.11585252, 0.16083117) | ||
 |
𝒩 (0.0148066, 0.25613424) | 𝒩(0.43540578, 0.07368543) | ||
| White noise | ||||
| σSET | [ms−1] | 𝒩+(0, 50.0) | 𝒩+(0, 50.0) | 𝒩+(0, 50.0) |
| Linear trend (m · t [BTJD] + b) | ||||
| m | [ms−1 d−1] | 𝒩(0.0, 0.1) | 𝒩(0.0, 0.1) | 𝒩(0.0, 0.1) |
| b | [ms−1] | 𝒩(0.0, 1.0) | 𝒩(0.0, 1.0) | 𝒩(0.0, 1.0) |
Notes.(*) 𝒩(μ, σ) indicates a normal distribution with mean μ and standard deviation σ; and 𝒩+(0, σ) a half-normal distribution with mean 0 and standard deviation σ. (**) The values for the prior distributions of parameters K, 
sin ω, and 
are taken from Wang et al. (2017b); for parameters T0, ln P, and ln K, the values are taken from this work (STELLA, cf. Sect. 2.2.1).
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