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Table 2.

Orbital parameters.

ID γ P KA ω e
[km s−1] [d] [km s−1] [rad]
CD-35 15144 1.8936 ± 0.0004 172.53244 ± 0.00003 23.289 ± 0.001 3.026 ± 0.011 0.821 ± 0.012
HD 4457 37.0 (⋆) 9000 < P < 15 000 2.8 < KA < 3.2 2.2 < ω < 3.2 0.32 < e < 0.37
HD 24706 −1.47 ± 0.04 1493 ± 337 6.75 ± 0.02 3.178 ± 0.008 0.401 ± 0.005
HD 96118 −18.86 ± 0.31 336.660 ± 0.011 21.53 ± 0.34 0.11 ± 0.41 0.007 ± 0.007
HD 127124 11.4 (⋆) 9000 < P < 11 000 3.7 < KA < 4.6 0.13 < ω < 0.17 0.78 < e < 0.83
HD 160346 21.943 ± 0.001 83.7282 ± 0.0004 5.694 ± 0.004 2.445 ± 0.001 0.2051 ± 0.0003
HD 178445 −5.21 ± 0.01 62.8201 ± 0.0006 15.51 ± 0.01 1.345 ± 0.003 0.374 ± 0.001
HD 219630 −2.16 ± 0.01 6521 ± 54 3.74 ± 0.01 0.137 ± 0.005 0.383 ± 0.002
PM J21214-6655 5.94 ± 0.12 549 ± 29 5.37 ± 0.20 5.601 ± 0.019 0.659 ± 0.023
PX Vir −1.960 ± 0.013 216.483 ± 0.020 12.91 ± 0.02 5.157 ± 0.005 0.256 ± 0.002
Ross 193 −44.40 ± 0.15 23.99 ± 0.10 4.51 ± 0.33 4.64 ± 0.21 0.461 ± 0.090
Wolf 414 −7.34 ± 0.01 4419.7 ± 9.8 3.46 ± 0.02 5.12 ± 0.06 0.315 ± 0.003

Notes. The columns are, from left to right, star ID, systemic RV (γ), orbital period (P), Doppler semi-amplitude for the primary component (KA), periastron argument (ω), and eccentricity (e).

(⋆)

Systemic velocity estimated from the best relative peak of the 3D density diagram for ℱ from the vgrid task.

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