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Table B.1

Parameter posteriors of our best model on all data, against the same set up on ESPRESSO data alone.

Parameter name Symbol Unit Prior Posterior

All-data ESPRESSO
LTF parameters
Period Pcyc d U(1000,2000)$\mathcal{U}\left(1000, 2000\right)$ 168040+50$1680^{+50}_{-40}$ 1720210+190$1720^{+190}_{-210}$
RV phase ϕcyc, 0 U(0,1)$\mathcal{U}\left(0, 1\right)$(w) 0.8430.129+0.118$0.843^{+0.118}_{-0.129}$ 0.8720.177+0.149$0.872^{+0.149}_{-0.177}$
RV semi-amplitude kcyc, 0 m s-1 U(0,10)$\mathcal{U}\left(0, 10\right)$ 0.510.33+0.35$0.51^{+0.35}_{-0.33}$ 0.540.37+0.47$0.54^{+0.47}_{-0.37}$
FWHM phase ϕcyc, 1 U(0,1)$\mathcal{U}\left(0, 1\right)$(w) 0.4290.089+0.085$0.429^{+0.085}_{-0.089}$ 0.4480.132+0.145$0.448^{+0.145}_{-0.132}$
FWHM semi-amplitude kcyc, 1 m s-1 U(0,10)$\mathcal{U}\left(0, 10\right)$ 2.731.32+1.51$2.73^{+1.51}_{-1.32}$ 2.341.44+1.68$2.34^{+1.68}_{-1.44}$
S-index phase ϕcyc, 2 U(0,1)$\mathcal{U}\left(0, 1\right)$(w) 0.5480.248+0.252$0.548^{+0.252}_{-0.248}$ 0.8540.268+0.342$0.854^{+0.342}_{-0.268}$
S-index semi-amplitude kcyc, 2 U(0,0.1)$\mathcal{U}\left(0, 0.1\right)$ 0.0190.013+0.019$0.019^{+0.019}_{-0.013}$ 0.0230.016+0.025$0.023^{+0.025}_{-0.016}$
RV zero-order correction α0 m s-1 N(μlm,200σlm)$\mathcal{N}(\mu_\text{lm},200\sigma_\text{lm})$ 0.470.83+0.85$0.47^{+0.85}_{-0.83}$ 0.601.27+1.25$0.60^{+1.25}_{-1.27}$
FWHM zero-order correction α1 m s-1 N(μlm,200σlm)$\mathcal{N}(\mu_\text{lm},200\sigma_\text{lm})$ 3.893.23+3.28$3.89^{+3.28}_{-3.23}$ 4.115.25+5.05$4.11^{+5.05}_{-5.25}$
S-index zero-order correction α2 N(μlm,200σlm)$\mathcal{N}(\mu_\text{lm},200\sigma_\text{lm})$ 0.050±0.048$0.050\pm 0.048$ 0.0510.077+0.075$0.051^{+0.075}_{-0.077}$
Dataset parameters
ESPRESSO19 RV offset O1,0 m s-1 N(0,5σ0)$\mathcal{N}(0,5\sigma_0)$ 1.06±0.74$-1.06\pm 0.74$ 1.170.94+0.93$-1.17^{+0.93}_{-0.94}$
HIRES RV offset O2,0 m s-1 N(0,5σ0)$\mathcal{N}(0,5\sigma_0)$ 0.001.01+1.00$0.00^{+1.00}_{-1.01}$
HARPS RV offset O3,0 m s-1 N(0,5σ0)$\mathcal{N}(0,5\sigma_0)$ 0.051.12+1.13$-0.05^{+1.13}_{-1.12}$
ESPRESSO19 FWHM offset O1,1 m s-1 N(0,5σ1)$\mathcal{N}(0,5\sigma_1)$ 4.632.21+2.30$-4.63^{+2.30}_{-2.21}$ 5.043.20+3.02$-5.04^{+3.02}_{-3.20}$
HARPS FWHM offset O3,1 m s-1 N(0,5σ1)$\mathcal{N}(0,5\sigma_1)$ 0.194.10+4.30$-0.19^{+4.30}_{-4.10}$
ESPRESSO19 S-index offset O1,2 N(0,5σ2)$\mathcal{N}(0,5\sigma_2)$ (6.223.38+3.44)×102$\left(-6.22^{+3.44}_{-3.38}\right)\times 10^{-2}$ (6.574.84+4.55)×102$\left(-6.57^{+4.55}_{-4.84}\right)\times 10^{-2}$
HIRES S-index offset O2,2 N(0,5σ2)$\mathcal{N}(0,5\sigma_2)$ (4.635.44+5.39)×102$\left(-4.63^{+5.39}_{-5.44}\right)\times 10^{-2}$
HARPS S-index offset O3,2 N(0,5σ2)$\mathcal{N}(0,5\sigma_2)$ (0.075.77+6.09)×102$\left(0.07^{+6.09}_{-5.77}\right)\times 10^{-2}$
ESPRESSO18 RV jitter J0,0 m s-1 exp[N(lnσ0,lnσ0)]$\exp[\mathcal{N}(\ln\sigma_0,\ln\sigma_0)]$ 1.820.35+0.47$1.82^{+0.47}_{-0.35}$ 1.820.36+0.48$1.82^{+0.48}_{-0.36}$
ESPRESSO19 RV jitter J1,0 m s-1 exp[N(lnσ0,lnσ0)]$\exp[\mathcal{N}(\ln\sigma_0,\ln\sigma_0)]$ 0.850.22+0.21$0.85^{+0.21}_{-0.22}$ 1.010.23+0.20$1.01^{+0.20}_{-0.23}$
HIRES RV jitter J2,0 m s-1 exp[N(lnσ0,lnσ0)]$\exp[\mathcal{N}(\ln\sigma_0,\ln\sigma_0)]$ 1.200.65+0.71$1.20^{+0.71}_{-0.65}$
HARPS RV jitter J3,0 m s-1 exp[N(lnσ0,lnσ0)]$\exp[\mathcal{N}(\ln\sigma_0,\ln\sigma_0)]$ 2.210.36+0.43$2.21^{+0.43}_{-0.36}$
ESPRESSO18 FWHM jitter J0,1 m s-1 Ulog(103,103)$\mathcal{U}_{\log}\left(10^{-3}, 10^{3}\right)$ 1.020.27+0.34$1.02^{+0.34}_{-0.27}$ 1.000.26+0.34$1.00^{+0.34}_{-0.26}$
ESPRESSO19 FWHM jitter J1,1 m s-1 Ulog(103,103)$\mathcal{U}_{\log}\left(10^{-3}, 10^{3}\right)$ 1.820.29+0.34$1.82^{+0.34}_{-0.29}$ 1.780.31+0.35$1.78^{+0.35}_{-0.31}$
HARPS FWHM jitter J3,1 m s-1 Ulog(103,103)$\mathcal{U}_{\log}\left(10^{-3}, 10^{3}\right)$ 4.250.62+0.77$4.25^{+0.77}_{-0.62}$
ESPRESSO18 S-index jitter J0,2 Ulog(103,103)$\mathcal{U}_{\log}\left(10^{-3}, 10^{3}\right)$ (1.270.45+0.55)×102$\left(1.27^{+0.55}_{-0.45}\right)\times 10^{-2}$ (1.460.51+0.58)×102$\left(1.46^{+0.58}_{-0.51}\right)\times 10^{-2}$
ESPRESSO19 S-index jitter J1,2 Ulog(103,103)$\mathcal{U}_{\log}\left(10^{-3}, 10^{3}\right)$ (4.770.54+0.62)×102$\left(4.77^{+0.62}_{-0.54}\right)\times 10^{-2}$ (4.730.65+0.66)×102$\left(4.73^{+0.66}_{-0.65}\right)\times 10^{-2}$
HIRES S-index jitter J2,2 Ulog(103,103)$\mathcal{U}_{\log}\left(10^{-3}, 10^{3}\right)$ (3.140.59+0.75)×102$\left(3.14^{+0.75}_{-0.59}\right)\times 10^{-2}$
HARPS S-index jitter J3,2 Ulog(103,103)$\mathcal{U}_{\log}\left(10^{-3}, 10^{3}\right)$ (0.430.27+0.64)×102$\left(0.43^{+0.64}_{-0.27}\right)\times 10^{-2}$
Stellar-activity hyperparameters
Timescale τ d Ulog(20,104)$\mathcal{U}_{\log}\left(20, 10^{4}\right)$ 27782+109$277^{+109}_{-82}$ 227109+281$227^{+281}_{-109}$
Period Prot d U(40.1,64.1)$\mathcal{U}(40.1,64.1)$ 48.7±0.3$48.7\pm 0.3$ 48.51.0+0.6$48.5^{+0.6}_{-1.0}$
Sinescale (harmonic complexity) η Ulog(102,102)$\mathcal{U}_{\log}\left(10^{-2}, 10^{2}\right)$ 0.530.10+0.13$0.53^{+0.13}_{-0.10}$ 0.940.32+0.78$0.94^{+0.78}_{-0.32}$
RV amplitude A0 m s-1 U(103,103)$\mathcal{U}(-10^3,10^3)$ 1.450.26+0.30$1.45^{+0.30}_{-0.26}$ 2.210.69+2.05$2.21^{+2.05}_{-0.69}$
RV gradient amplitude B0 m s-1 d-1 U(103,103)$\mathcal{U}(-10^3,10^3)$ 19.93.2+4.0$19.9^{+4.0}_{-3.2}$ 23.17.3+23.3$23.1^{+23.3}_{-7.3}$
FWHM amplitude A1 m s-1 Ulog(103,103)$\mathcal{U}_{\log}\left(10^{-3}, 10^{3}\right)$ 7.260.86+1.13$7.26^{+1.13}_{-0.86}$ 9.762.78+9.10$9.76^{+9.10}_{-2.78}$
S-index amplitude A2 m s-1 Ulog(103,103)$\mathcal{U}_{\log}\left(10^{-3}, 10^{3}\right)$ 0.1060.012+0.015$0.106^{+0.015}_{-0.012}$ 0.1330.042+0.137$0.133^{+0.137}_{-0.042}$

Notes. (w)Wrapped parameter. Reported uncertainties reflect the 16th and the 84th percentiles. Offsets are defined relative to ESPRESSO18. The standard deviation of measurements in physical quantity j is denoted σj.

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