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Table 3

Low-mass binary stars and brown dwarf candidates analysed in this study.

Period ω K T 0 γ SOPHIE O−C O−C+ a m2sini
Name Eccentricity
[day] [°] [m/s] [BJD−2 400 000] [km s-1] [km s-1] [m/s] [m/s] [AU] [MJup]

Low-mass binary stars

HD 6664B 1718 ± 11 0.289 ± 0.002 138.9 ± 0.5 1417 ± 4 56 227 ± 2 6.898 ± 0.009 6.932 ± 0.007 14.6 7.0 2.80 ± 0.09 80 ± 5
BD+73 0275B 1423.20 ± 0.14 0.81386 ± 0.00038 120.62 ± 0.09 1624.9 ± 1.3 57 326.15 ± 0.04 −26.0352 ± 0.0035 −26.0297 ± 0.0014 11.3 4.3 2.31 ± 0.06 44 ± 3
HD 50761B 2092 ± 11 0.377 ± 0.007 23.89 ± 0.01 7.4 3.5 ± 0.2
HD 51813B 0.735 ± 0.003 37.07 ± 0.02 11.2 13.7 2.6 ± 0.1 46 ± 4
HD 56709B 2499.0 ± 5.6 0.106 ± 0.006 153 ± 4 896 ± 4 −22.296 ± 0.007 −22.278 ± 0.006 11.4 12.4 4.03 ± 0.11 72 ± 4
HD 134169B 67.8578 ± 0.0038 0.10300 ± 0.00053 −5.02 ± 0.48 4184.9 ± 2.4 56 243.940 ± 0.090 18.9395 ± 0.0017 4.0 0.324 ± 0.008 83 ± 4
Brown dwarf candidates to solar-type stars with projected masses between 10 and 80 MJup

HD 283668b 2558 ± 8 0.577 ± 0.011 −94.6 ± 1.2 67.80 ± 0.011 67.79 ± 0.02 10.8 4.7 3.30 ± 0.11 53 ± 4
HD 39392b 0.394 ± 0.008 −31.9 ± 1.3 56 322 ± 1 −64.632 ± 0.002 10.0 1.08 ± 0.03 13.2 ± 0.8
HD 77065b 0.69 397 ± 0.00036 105.972 ± 0.065 2817.1 ± 1.6 56 881.239 ± 0.006 6.3822 ± 0.0009 5.1 0.438 ± 0.013 41 ± 2
BD+26 1888b 536.78 ± 0.25 0.2675 ± 0.0016 1.3 ± 0.7 805.1 ± 1.3 56 548.3 ± 0.9 −14.8843 ± 0.0012 4.7 1.19 ± 0.05 26 ± 2
HD 122562b 0.71 ± 0.01 55 935 ± 2 8.0 3.5 4.1 ± 0.2 24 ± 2
HD 132032b 274.33 ± 0.24 0.0844 ± 0.0024 −0.9 ± 0.9 1950.7 ± 2.2 56 238.0 ± 0.7 −8.118 ± 0.005 3.2 0.87 ± 0.02 70 ± 4
HD 134113b 201.680 ± 0.004 0.891 ± 0.002 163.0 ± 0.2 56 808.54 ± 0.05 −60.2027 ± 0.0015 9.7 0.638 ± 0.010
HD 160508b 178.9049 ± 0.0074 0.5967 ± 0.0009 −168.83 ± 0.13 1825.3 ± 2.7 55 998.70 ± 0.03 22.2054 ± 0.0035 22.2440 ± 0.0020 11.0 6.9 0.68 ± 0.02 48 ± 3
BD+24 4697b 145.081 ± 0.016 0.50048 ± 0.00043 66.35 ± 0.09 2728.4 ± 1.6 55 986.042 ± 0.037 −36.5913 ± 0.0016 3.5 0.50 ± 0.08 53 ± 3

Notes.

(†)

These objects contain data from Latham et al. (2002) where HD 77065 is published as G9-42 and HD 134133 as G66-65.

(‡)

The uncertainties in stellar mass were included in the uncertainty calculation of m2sini.

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