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This article has an erratum: [https://doi.org/10.1051/0004-6361/201015427e]


Table 8

Solution parameters and companion masses for stars with orbits that have significances above 1-σ.

Object Sol. Norb σΛ a sin i a M2 M2 (3-σ) arel Null prob. Significance
type (mas) (mas) (mas) (MJ) (MJ) (mas) (%) (%)

HD 17289 1 2.1 7.2 1.29 (386, 700) 32.0 0.32 7e-29 >99.9
HD 30501 5 0.6 3.3 10.44 (65, 132) 147.7 0.79 0.005 99.9
HD 43848a 9 0.5 4.2 2.32 (59,150) 90.8 1.09 4e-8 >99.9
HD 43848b 9 0.5 4.2 4.93 (73,179) 91.7 1.07 1e-8 >99.9
HD 53680 1 0.7 5.7 9.73 (159, 301) 160.7 0.82 3e-16 >99.9
HD 164427A 5 11.1 2.4 0.49 (101, 482) 12.8 1.15 0.003 99.7
HIP 103019 5 1.2 7.1 3.33 (118,280) 53.4 1.13 4e-10 >99.9
HD 3277 5 24.8 3.6 0.58 (143, 600) 9.4 1.00 5e-4 97.7
HD 131664 5 0.6 4.7 0.88 (44,153) 60.3 0.77 2e-5 97.9
HD 154697 7 0.6 3.1 6.26 (81, 235) 89.2 1.60 1e-6 96.0
HD 174457 5 1.3 3.2 1.77 (65,190) 35.2 1.22 12.3 95.9
HD 190228 5 1.0 3.5 0.13 (10,99) 32.9 1.08 0.3 95.4
HD 74014 5 0.1 2.5 9.84 (51, 1568) 235.4 1.34 19.9 80.6
HD 168443 5 0.6 1.9 1.25 (18,67) 75.9 1.53 3.6 75.0
HD 191760 5 1.6 3.3 0.46 (39,659) 16.0 1.39 27.6 77.5

Notes. The top 6 orbits have high significance 99.7% and are therefore fully characterised. The bottom 3 orbits are of low significance (1-σ–2-σ) and represent the formal solution. The remaining 5 orbits have moderate significance (2-σ–3-σ) and provide lower and upper mass-limits for the companions.

(a)

Final solution at lower eccentricity.

(b)

Formal solution at higher eccentricity.

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