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Table 4

Fitted Keplerian orbits and planetary parameters for the two multi-planetary systems, with 1σ error bars.

Parameters HIP 65407b HIP 65407c HD 141399b HD 141399c HD 141399d HD 141399e

P [days] 28.125 ± 0.019 67.30 ± 0.08 94.44 ± 0.05 201.99 ± 0.08 1069.8 ± 6.7
e 0.14 ± 0.07 0.12 ± 0.04 0.04 ± 0.02 0.048 ± 0.009 0.074 ± 0.025 0.26 ± 0.22
ω [°] 50 ± 150 −19 ± 25 −90 ± 80 −140 ± 40 −140 ± 30 −10 ± 20
T0 [BJD] 56 990.8 ± 2.5 57 047 ± 6 56 998 ± 15 56 838 ± 10 56 923 ± 65 58 900 ± 800
K [m s-1] 30.5 ± 1.6 41.5 ± 1.9 19.23 ± 0.47 44.20 ± 0.50 22.63 ± 0.59 8.8 ± 0.9
Mp sin i [MJup] 0.428 ± 0.032 0.784 ± 0.054 0.451 ± 0.030 1.33 ± 0.08 1.18 ± 0.08 0.66 ± 0.10
a [AU] 0.177 ± 0.005 0.316 ± 0.008 0.415 ± 0.011 0.689 ± 0.020 2.09 ± 0.06 5.0 ± 1.5
Vr, SOPHIE [km s-1] −8.748 ± 0.005 −21.566 ± 0.002
Vr, SOPHIE + [km s-1] −8.720 ± 0.003 −21.548 ± 0.001
N 65 139
σO−C, SOPHIE [m s-1] 11.9 12.8
σO−C, SOPHIE + [m s-1] 7.5 4.8
RV drift [m s-1 yr-1] [−0.6; + 7.8 ] [−1.3; + 2.4 ]
Span [days] 1517 2566
Mp max [ M ] 8.11 2.25 0.22 0.12 0.04

Notes.

(‡)

Time of possible transits.

(†)

Using the stellar mass and its uncertainty from Table 2.

(∗)

Stability analyses of HD 141399e provide Pe = 3370 ± 90 days and ee< 0.1 (see Sect. 5.2.2).

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