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Table 3

Results of the fitting to the observed radial velocities.

KOI K e ω Vsys Mcompsinia inc.b FM c a F-testd
(km s-1) (deg) (km s-1) (M) (deg) (MJup) (AU)

Group A Eclipsing binaries

0340 B 16.28 ± 0.11 0.5138 ± 0.0059 239.71 ± 0.58 84.007 ± 0.045 0.2144 ± 0.0058 89.95 7.000 ± 0.091 0.1614 ± 0.0054 > 100
0371 B 8.252 ± 0.086 0.4070 ± 0.0081 94.75 ± 0.47 56.855 ± 0.081 0.445 ± 0.014 89.95 23.15 ± 0.82 1.424 ± 0.047 > 100
0686 B 6.3 ± 1.7 0.52 ± 0.15 63 ± 12 31.30 ± 0.65 0.089 ± 0.018 89.38 0.88 ± 0.45 0.259 ± 0.015 > 100
3853 B 26.98 ± 0.48 0.3956 ± 0.0084 130.8 ± 1.3 75.19 ± 0.15 0.527 ± 0.043 50.42 35.5 ± 2.2 0.175 ± 0.014 > 100
3853 C 2.1 ± 1.3 0.56 ± 0.20 312 ± 21 75.19 ± 0.15 0.030 ± 0.016 0.011 ± 0.019 0.171 ± 0.014 > 100

Group C Unsolved cases

1463 B > 3.3 > 0.18 [80,200] [28.5,25.5] > 0.183 ± 0.030 89.95 > 4.15 2.15 ± 0.19 > 100
3890 B > 2.5 > 0.33 [0,82] [28.7,24.2] > 0.097 ± 0.014 89.95 > 0.27 0.676 ± 0.040 3.6

Notes.

(a)

Companion mass assuming primary mass from Huber et al. (2014), see Table 2.

(b)

Orbital inclination provided by the Kepler team.

(c)

Mass function, defined as: . This parameter is directly obatined from the RV fit and does not depend on the primary mass.

(d)

F-test comparing the significance of the RV model to a straight line.

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