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Table B.6

Orbital fits for the 40 single stellar companions in the M-dwarf regime with M sin i larger than 90MJ and lower than 0.52 M⊙, ordered by values of M2 sin i.

Name Period K e ω Tp –2.4 × 106 γS+ γS σO−C,S+ σO−C,S f(m) M2 sin i a2
(day) (ms−1) (°) (day) (kms−1) (kms−1) (ms−1) (ms−1) (10−6 M⊙) (MJup) (AU)
90 MJ < M sin i < 0.52 M⊙; M-dwarfs
BD+281779 46.31706 ± 0.00022 7789.2 ± 8.0 0.61773 ± 0.00058 −68.975 ± 0.069 56469.8643 ± 0.0041 −18.018 ± 0.010 −18.0317 ± 0.0095 3.69 8.09 1103.0 ± 2.4 90.8 ± 2.9 0.2396 ± 0.0037
HD62923 175.221 ± 0.013 3200.1 ± 5.9 0 (a) – 58237.6304 ± 0.2650 8.3432 ± 0.0049 1.07 594.9 ± 3.3 91.8 ± 3.0 0.642 ± 0.010
HD156111 39.43957 ± 0.00060 7754.8 ± 1.6 0.65053 ± 0.00013 65.798 ± 0.027 57520.1329 ± 0.0024 −48.6374 ± 0.0025 3.66 834.83 ± 0.59 92.0 ± 3.1 0.2259 ± 0.0037
HD103913 2322 ± 10 1534 ± 11 0.4129 ± 0.0075 −175.16 ± 0.54 56892.6 ± 4.8 7.101 ± 0.018 7.092 ± 0.016 6.65 12.3 656 ± 18 98.1 ± 3.4 3.659 ± 0.061
HD225239 701.49 ± 0.55 3532.9 ± 6.4 0.7561 ± 0.0014 −34.07 ± 0.15 56996.16 ± 0.20 4.817 ± 0.010 8.16 898.2 ± 4.3 100.5 ± 3.2 1.588 ± 0.025
HD133621 448.60 ± 0.17 3039.8 ± 3.0 0.35583 ± 0.00090 63.39 ± 0.27 56846.11 ± 0.46 −49.1224 ± 0.0037 2.99 1065.6 ± 3.2 101.8 ± 3.5 1.156 ± 0.019
HD73636 155.284 ± 0.025 3550.2 ± 6.6 0.2874 ± 0.0011 81.85 ± 0.35 55201.78 ± 0.23 −16.515 ± 0.054 −16.5011 ± 0.0080 14.1 7.04 632.6 ± 3.6 102.7 ± 3.4 0.620 ± 0.010
HD101305 1677.4 ± 2.6 2099.9 ± 4.0 0.4911 ± 0.0020 −118.60 ± 0.19 58309.0 ± 2.2 12.5904 ± 0.0047 5.11 1063.3 ± 6.9 106.1 ± 3.6 2.843 ± 0.046
HD106888 365.606 ± 0.060 3211 ± 43 0.4629 ± 0.0038 −81.9 ± 1.1 55572.69 ± 0.73 −5.518 ± 0.053 −5.546 ± 0.047 8.33 18.8 872 ± 34 108.3 ± 3.8 1.071 ± 0.017
BD+192536 178.543 ± 0.025 4779 ± 50 0.1254 ± 0.0037 −144.9 ± 1.5 56892.99 ± 0.88 −3.302 ± 0.052 −3.314 ± 0.041 3.26 2.35 1972 ± 59 108.5 ± 3.7 0.5888 ± 0.0093
HD212733 89.85646 ± 0.00015 6379.5 ± 1.3 0.43071 ± 0.00017 −105.221 ± 0.033 55060.6477 ± 0.0058 11.6822 ± 0.0022 11.6802 ± 0.0088 5.61 10.5 1776.78 ± 0.89 112.0 ± 3.8 0.3841 ± 0.0063
HD18450 25.037329 ± 0.000015 9351.19 ± 0.98 0.07884 ± 0.00014 27.109 ± 0.087 56747.6986 ± 0.0060 37.8288 ± 0.0018 1.17 2101.50 ± 0.70 114.6 ± 3.8 0.1616 ± 0.0026
HD144286 316.7767 ± 0.0067 3871.5 ± 5.4 0.12729 ± 0.00062 −40.48 ± 0.46 56625.65 ± 0.34 −53.8401 ± 0.0064 2.82 1858.5 ± 7.6 117.6 ± 3.9 0.905 ± 0.015
HD212029 771.02 ± 0.28 3533.8 ± 6.6 0.4978 ± 0.0011 2.88 ± 0.22 57504.95 ± 0.46 −107.529 ± 0.011 8.39 2300 ± 12 122.1 ± 4.1 1.616 ± 0.026
HD104289 2389.0 ± 1.5 1790 ± 11 0.2935 ± 0.0037 80.1 ± 2.1 57862.9 ± 8.1 −19.4205 ± 0.0097 5.26 1241 ± 26 125.8 ± 4.5 3.818 ± 0.064
HD156728 4097 ± 79 1792 ± 12 0.321 ± 0.011 103.32 ± 0.72 57093.9 ± 6.5 −0.8480 ± 0.0093 3.01 2074 ± 27 126.5 ± 4.5 5.08 ± 0.11
HD204613 876.84 ± 0.41 3297 ± 44 0.0413 ± 0.0030 −54 ± 12 56524 ± 30 −90.816 ± 0.043 −90.779 ± 0.061 2.31 8.54 3248 ± 130 151.7 ± 5.5 1.858 ± 0.030
HD109157 300.212 ± 0.025 6860.5 ± 3.7 0.62565 ± 0.00062 137.84 ± 0.11 56777.730 ± 0.047 6.0473 ± 0.0073 5.47 4767.9 ± 8.2 153.1 ± 5.0 0.864 ± 0.013
HD167215 3460.5 ± 3.2 3354 ± 97 0.7635 ± 0.0062 163.72 ± 0.26 55146.05 ± 0.69 −42.82 ± 0.13 −42.82 ± 0.13 3.72 8.94 3645 ± 198 167.5 ± 6.3 4.783 ± 0.075
HD40647 8078 ± 872 2318 ± 50 0.506 ± 0.011 30.4 ± 3.5 57284 ± 30 −13.612 ± 0.072 −13.629 ± 0.073 13.0 14.1 6693 ± 1152 172 ± 11 7.82 ± 0.58
HD193554 (b) 797.69 ± 0.18 4115.2 ± 9.1 0.3136 ± 0.0017 140.25 ± 0.65 57365.6 ± 1.2 7.5276 ± 0.0098 fixed 6.37 17.2 4870 ± 77 173.6 ± 6.0 1.751 ± 0.029
HD15292 2087 ± 58 3052 ± 20 0.325 ± 0.011 24.07 ± 0.28 59802 ± 57 −40.173 ± 0.036 0.9 5202 ± 184 176.5 ± 6.2 3.325 ± 0.081
HD110376 1282.2 ± 3.3 4088 ± 119 0.246 ± 0.027 −68.4 ± 2.9 57424 ± 32 −10.62 ± 0.21 3.56 8264 ± 581 177.7 ± 7.1 2.262 ± 0.036
HD87899 1527 ± 16 5199 ± 99 0.6734 ± 0.0028 −178 ± 30 55211.8 ± 2.7 33.76 ± 0.12 11.0 8986 ± 523 195.3 ± 7.8 2.627 ± 0.048
HD207992 (b) 2090 ± 12 4792 ± 33 0.638 ± 0.012 −62.8 ± 1.5 55894 ± 12 −55.261 ± 0.051 fixed 0.19 32.5 10860 ± 236 206.8 ± 7.3 3.238 ± 0.054
HD5470 (b) 7788 ± 50 2041.3 ± 3.4 0.3557 ± 0.0031 −124.62 ± 0.50 53155.6 ± 5.9 −3.874 ± 0.013 fixed 8.17 14.7 5601 ± 27 208.5 ± 6.9 8.57 ± 0.14
HD78536 11.345932 ± 0.000041 17029 ± 12 0 (a) – 58018.4661 ± 0.0042 −11.507 ± 0.041 −11.567 ± 0.044 7.85 0.88 5805 ± 12 213.7 ± 6.9 0.1109 ± 0.0017
HD153376 (b) 4878 ± 37 3907 ± 59 0.7952 ± 0.0053 113.54 ± 0.65 59193 ± 38 −45.629 ± 0.085 fixed 2.15 6.89 6732 ± 80 236.8 ± 8.1 6.49 ± 0.11
HD24505 11268 ± 99 3294.9 ± 3.5 0.7974 ± 0.0014 157.952 ± 0.066 56995.36 ± 0.56 −13.5624 ± 0.0070 7.03 9169 ± 362 238.2 ± 7.8 10.89 ± 0.18
HD146735 13932 ± 3864 2161 ± 85 0.507 ± 0.068 84.1 ± 7.4 70233 ± 3911 −16.845 ± 0.089 4.20 9364 ± 2296 244 ± 22 12.7±2.4
BD+362641 17.312171 ± 0.000071 43330 ± 1702 0.8456 ± 0.0053 15.24 ± 0.32 54646.2032 ± 0.0051 −1.1 ± 2.2 1.59 21934 ± 1555 251 ± 11 0.1322 ± 0.0021
HD161479 10.2417625 ± 0.0000035 24175 ± 48 0.02316 ± 0.00062 69.3 ± 3.5 54102.9 ± 5.0 −17.095 ± 0.056 −17.079 ± 0.062 36.0 42.6 14982 ± 90 268.7 ± 9.1 0.1012 ± 0.0016
HD155228 432.976 ± 0.022 7429 ± 70 0.5309 ± 0.0025 −149.51 ± 0.42 57639.10 ± 0.88 16.40 ± 0.11 3.34 11177 ± 364 268.9 ± 9.5 1.278 ± 0.020
BD+680971 1134.141 ± 0.057 10749 ± 678 0.8303 ± 0.0044 −39.2 ± 1.9 56979.3 ± 1.0 −8.26 ± 0.79 9.54 25268 ± 3986 276 ± 17 2.207 ± 0.036
HD147487 533.228 ± 0.070 7370 ± 47 0.2134 ± 0.0022 −176.59 ± 0.51 57462.6 ± 1.0 −63.967 ± 0.052 2.21 20624 ± 368 279.7 ± 9.3 1.378 ± 0.021
HD108436 2720 ± 142 4970 ± 217 0.241 ± 0.081 −30.3 ± 3.2 57996 ± 54 −68.27 ± 0.40 3.78 31121 ± 3534 305 ± 14 4.02 ± 0.16
HD13014 3451 ± 390 4881 ± 482 0.4911 ± 0.0047 137.5 ± 4.2 57268 ± 28 0.72 ± 0.51 5.01 27555 ± 12207 366 ± 52 5.22 ± 0.46
HD60846 6027 ± 891 8397 ± 2360 0.824 ± 0.030 −4.59 ± 0.45 62514 ± 889 50.0 ± 3.0 5.92 62968 ± 41381 448 ± 95 7.43 ± 0.77
HD85533 31214 ± 30144 3907 ± 355 0.61 ± 0.13 −57 ± 17 58008 ± 98 −26.17 ± 0.57 −26.21 ± 0.57 5.19 10.9 91085 ± 54942 453 ± 89 22 ± 13
BD+132550 2537 ± 17 6679.1 ± 5.6 0 (a) – 60080 ± 16 −10.872 ± 0.016 8.30 78330 ± 544 463 ± 16 4.159 ± 0.065

Notes. The explanations are identical to Table B.5. (a)With an eccentricity of 0, the time of periastron passage is ill-defined. In this case, Tp indicates the time of primary transit. (b)We fixed the γ of the S+ and S− dataset at a common value.

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