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Table 4

Inferred parameters from the MCMC runs.

Parameter Unit GJ 832 b GJ 674 b Ross 128 b Ross 128 b Ross 128 b

HARPS All HARPS All HARPS All HARPS RedDots HARPS All + CARMENES
K (m s−1) 17.20.6+0.6$17.2_{ - 0.6}^{ + 0.6}$ 8.680.12+0.11$8.68_{ - 0.12}^{ + 0.11}$ 1.410.14+0.14$1.41_{ - 0.14}^{ + 0.14}$ 1.450.24+0.24$1.45_{ - 0.24}^{ + 0.24}$ 1.410.13+0.13$1.41_{ - 0.13}^{ + 0.13}$
P (d) 380895+111$3808_{ - 95}^{ + 111}$ 4.695020.00003+0.00003$4.69502_{ - 0.00003}^{ + 0.00003}$ 9.85560.0011+0.0012$9.8556_{ - 0.0011}^{ + 0.0012}$ 9.850.08+0.08$9.85_{ - 0.08}^{ + 0.08}$ 9.85560.0011+0.0011$9.8556_{ - 0.0011}^{ + 0.0011}$
esinω$\sqrt e \sin \omega $ 0.100.10+0.14$ - 0.10_{ - 0.10}^{ + 0.14}$ 0.3270.021+0.020$0.327_{ - 0.021}^{ + 0.020}$ 0.140.19+0.16$0.14_{ - 0.19}^{ + 0.16}$ 0.270.30+0.23$0.27_{ - 0.30}^{ + 0.23}$ 0.140.19+0.15$0.14_{ - 0.19}^{ + 0.15}$
ecosω$\sqrt e \cos \omega $ 0.070.14+0.12$0.07_{ - 0.14}^{ + 0.12}$ 0.3670.017+0.019$ - 0.367_{ - 0.017}^{ + 0.019}$ 0.410.15+0.10$0.41_{ - 0.15}^{ + 0.10}$ 0.350.28+0.18$0.35_{ - 0.28}^{ + 0.18}$ 0.370.16+0.10$0.37_{ - 0.16}^{ + 0.10}$
t0 (BJD) 2450989659+773$2450989_{ - 659}^{ + 773}$ 2453160.260.04+0.04$2453160.26_{ - 0.04}^{ + 0.04}$ 2453584.50.9+0.8$2453584.5_{ - 0.9}^{ + 0.8}$ 2459202.51.2+1.2$2459202.5_{ - 1.2}^{ + 1.2}$ 2453584.51.0+0.8$2453584.5_{ - 1.0}^{ + 0.8}$

e 0.0360.023+0.030$0.036_{ - 0.023}^{ + 0.030}$ 0.2420.013+0.012$0.242_{ - 0.013}^{ + 0.012}$ 0.210.10+0.09$0.21_{ - 0.10}^{ + 0.09}$ 0.270.18+0.19$0.27_{ - 0.18}^{ + 0.19}$ 0.180.09+0.09$0.18_{ - 0.09}^{ + 0.09}$
ω (rad) 0.91.0+1.2$ - 0.9_{ - 1.0}^{ + 1.2}$ 2.410.05+0.05$2.41_{ - 0.05}^{ + 0.05}$ 0.30.5+0.4$0.3_{ - 0.5}^{ + 0.4}$ 0.60.8+0.6$0.6_{ - 0.}^{ + 0.6}$ 0.30.5+0.4$0.3_{ - 0.5}^{ + 0.4}$
M sin i M 2478+8$247_{ - 8}^{ + 8}$ 10.950.14+0.14$10.95_{ - 0.14}^{ + 0.14}$ 1.400.13+0.13$1.40_{ - 0.13}^{ + 0.13}$ 1.390.23+0.21$1.39_{ - 0.23}^{ + 0.21}$ 1.410.13+0.12$1.41_{ - 0.13}^{ + 0.12}$
a (au) 3.660.06+0.07$3.66_{ - 0.06}^{ + 0.07}$ 0.038670870.00000015+0.00000015$0.03867087_{ - 0.00000015}^{ + 0.00000015}$ 0.0496400.000004+0.000004$0.049640_{ - 0.000004}^{ + 0.000004}$ 0.04960.0003+0.0003$0.0496_{ - 0.0003}^{ + 0.0003}$ 0.0496390.000004+0.000004$0.049639_{ - 0.000004}^{ + + 0.000004}$

ρ (d) 265+10$26_{ - 5}^{ + 10}$ 213+3$21_{ - 3}^{ + 3}$ 7621+20$76_{ - 21}^{ + 20}$ 269152+156$269_{ - 152}^{ + 156}$ 8014+22$80_{ - 14}^{ + 22}$
τ (d) 64+5$6_{ - 4}^{ + 5}$ 6.01.9+2.5$6.0_{ - 1.9}^{ + 2.5}$ 2017+32$20_{ - 17}^{ + 32}$ 5249+89$52_{ - 49}^{ + 89}$ 2724+35$27_{ - 24}^{ + 35}$
σGP,H-pre (d) 1.90.3+0.4$1.9_{ - 0.3}^{ + 0.4}$ 2.750.24+0.28$2.75_{ - 0.24}^{ + 0.28}$ 2.20.4+0.7$2.2_{ - 0.4}^{ + 0.7}$ 2.20.4+0.9$2.2_{ - 0.4}^{ + 0.9}$
σGP,H-post (d) 2.00.3+0.8$2.0_{ - 0.3}^{ + 0.8}$ 2.80.4+0.5$2.8_{ - 0.4}^{ + 0.5}$ 3.81.1+2.0$3.8_{ - 1.1}^{ + 2.0}$ 3.91.2+3.0$3.9_{ - 1.2}^{ + 3.0}$
σGP,H-warmup (d) 2.30.7+1.6$2.3_{ - 0.7}^{ + 1.6}$ 95+11$9_{ - 5}^{ + 11}$ 2.30.8+2.3$2.3_{ - 08}^{ + 2.3}$
σGP,carmenes (d) 1.80.5+0.8$1.8_{ - 0.5}^{ + 0.8}$

sH–pre (m s–1) 0.680.21+0.38$0.68_{ - 0.21}^{ + 0.38}$ 0.480.19+0.16$0.48_{ - 0.19}^{ + 0.16}$ 0.480.25+0.20$0.48_{ - 0.25}^{ + 0.20}$ 0.510.24+0.20$0.51_{ - 0.24}^{ + 0.20}$
sH–post (m s–1) 0.360.22+0.20$0.36_{ - 0.22}^{ + 0.20}$ 0.60.3+0.3$0.6_{ - 0.3}^{ + 0.3}$ 0.50.3+0.4$0.5_{ - 0.3}^{ + 0.4}$ 0.50.3+0.4$0.5_{ - 0.3}^{ + 0.4}$
sH-warmup (m s–1) 1.020.17+0.15$1.02_{ - 0.17}^{ + 0.15}$ 1.050.17+0.16$1.05_{ - 0.17}^{ + 0.16}$ 1.020.17+0.15$1.05_{ - 0.17}^{ + 0.16}$
scarmenes (m s–1) 1.40.4+0.4$1.02_{ - 0.17}^{ + 0.15}$
µH-pre (m s–1) 4.30.5+0.5$4.3_{ - 0.5}^{ + 0.5}$ 5.70.4+0.4$5.7_{ - 0.4}^{ + 0.4}$ 2.30.6+0.5$2.3_{ - 0.6}^{ + 0.5}$ 2.40.6+0.5$2.4_{ - 0.6}^{ + 0.5}$
µH-post (m s–1) 9.22.3+3.0$9.2_{ - 2.3}^{ + 3.0}$ 13.00.6+0.6$13.0_{ - 0.6}^{ + 0.6}$ 4.21.8+1.5$ - 4.2_{ - 1.8}^{ + 1.5}$ 4.01.8+1.6$ - 4.0_{ - 1.8}^{ + 1.6}$
µH-warmup (m s–1) 2.21.2+1.2$2.2_{ - 1.2}^{ + 1.2}$ 25+5$2_{ - 5}^{ + 5}$ 2.31.2+1.2$2.3_{ - 1.2}^{ + 1.2}$
µcarmenes (m s–1) 0.10.6+0.6$0.1_{ - 0.6}^{ + 0.6}$

Notes. In addition to the median of the posterior of the one eccentric planet + GP-SHO models, we give the 16th and 84th percentile confidence interval. The blocks are sorted into the directly inferred orbital elements, derived elements, GP hyperparameters, RV-jitter and -offset.

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