Table A.3: Radial velocities of likely binaries or non members. For these stars, each of the three RV measurements is given. Fields with blanks indicate that problems were present with the cross-correlation profile of these objects.

Object
$V_{\rm rad}^1$ $\Delta V_{\rm rad}^1$ $V_{\rm rad}^2$ $\Delta V_{\rm rad}^2$ $V_{\rm rad}^3$ $\Delta V_{\rm rad}^3$

342
17.74 0.72 57.20 1.45 40.75 0.73
364 36.93 0.43 36.58 1.18 36.48 0.74
437 45.87 0.65 45.54 0.83 45.68 0.52
455 38.07 0.50 14.62 1.24 33.41 0.47
571 31.73 0.49 31.07 0.66 31.47 0.56
574 42.88 0.46 42.91 0.85 42.08 0.62
681 24.14 0.80 56.70 1.22 59.70 0.85
713 35.34 0.46 35.03 0.64 34.91 0.33
756 46.24 0.50 45.54 0.77 45.47 0.41
880 39.62 6.67 / / 33.55 5.81
905 34.78 0.35 37.30 1.02 74.65 0.89
917 18.66 0.86 15.59 1.36 / /
971 36.13 0.51 36.13 0.70 36.22 0.63
986 16.54 0.53 27.69 0.84 49.08 0.68
1010 17.22 0.97 30.77 0.63 34.29 0.75
1091 27.59 3.27 27.03 0.62 25.77 0.78
1108 15.92 1.00 / / / /
1161 35.53 0.65 35.49 1.21 22.45 1.55
1163 10.10 0.66 65.99 1.32 70.80 1.24
1342 37.97 0.69 28.40 1.06 34.93 0.65
1397 35.43 1.12 34.91 0.85 34.88 0.54
1424 54.44 1.62 57.22 1.31 56.04 1.58
1480 22.86 1.02 25.56 1.09 28.27 0.48
1680 37.65 1.29 35.65 0.96 32.27 0.81
1706 35.79 1.05 35.40 0.90 35.77 0.61
1778 29.59 1.30 29.92 2.96 31.19 1.26
1842 30.09 0.69 29.88 1.20 30.52 0.47
1862 31.31 0.63 30.29 2.03 31.27 0.43
1957 21.17 0.52 20.15 0.83 21.21 0.57
2016 21.64 0.46 25.96 0.94 65.63 0.66
2017 126.58 0.84 125.09 1.62 126.01 0.63


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