Table 1: General information on the observed stars.
HIP Cmp1 GJ2 CCDM3 Extra Ident. mV Sp $\rho$ (Hp) $\theta$ (Hp) $\pi$ $\sigma$($\pi$)
Nr   Nr     (mag)   ( $\hbox{$^{\prime\prime}$ }$) ( $\hbox{$^\circ$ }$) (mas) (mas)

473		 AB 4 00057+4548 BD +45 4408 9.01 K7 6.041 178.3 85.10 2.74
2552 Aa-B 22 00325+6714 BD +66 34 10.29 M2 4.147 163.4 97.4 2.4
3937 AB 3060 00506+2449 LDS 3203 11.69 M3.5 2.080 316. 83.20 9.08
10531/29 AB 90 02157+6740 HD 13579 7.18 K2V 18.580 337.3 55.15 1.25
13642 AB 9105 02556+2652 HD 18143 7.58 G5 5.538 220.3 43.71 1.26
15844 AB 140 03241+2347 WOR 4 10.38 M1 2.247 347.1 50.54 4.66
17666 AB 1064 03470+4126 HD 23439 8.18 K1V 7.307 54.2 40.83 2.24
17749/50 A-BC 153 03480+6841 HD 23189 9.07 K0 17.11 14. 57.53 2.68
18512 AB 157 03575-0110 HD 24916 8.00 K4V 11.078 17.3 63.41 2.00
21088 AB 169.1 04312+5858 STI 2051 10.82 M4 8.350 69.4 180.66 0.86
54952 AC 420 11153+7328 HD 97584 7.63 K5 6.619 321.0 68.13 1.18
56 809 AB 9370 11387+4506 HD 101177 6.44 G0V 9.224 249.5 42.94 0.95
63253 AB 490 12577+3514 BD +36 2322 10.50 M0.5 15.990 225.8 55.277 3.15
65011/12 BC 507 13192+3507 BD +35 2436 9.52 M0.5 17.650 129.2 75.96 3.31
65343 AB 509 13235+2914 HD 116495 8.90 K5 1.313 77.8 53.97 2.13
66077 AB 516 13327+1649 VYS 6 11.38 M2.5 - - 61.56 5.76
66492 AB 520 13379+4808 BD +48 2138 9.76 M0 2.166 311.9 45.66 2.72
67422 AB 528 13491+2659 HD 120476 7.04 K2 3.456 166.5 73.257 1.33
79492 AB 615.1 16134+1331 HD 145958 6.68 G8V 4.139 352.2 41.05 1.58
83020 AB 649.1 16578+4722 HD 153557 7.83 K3V 4.915 61.0 55.71 1.21
83988/96 AB 659 17102+5430 HD 155674 8.80 K0 22.189 133.6 47.14 1.88
86282 AB 9596 17378+2257 BD +23 3151 9.89 K5 4.265 185.5 42.06 2.86
87768 AB 698 17557+1830 BD +18 3497 9.23 K5 18.788 46.7 43.40 2.21
91768/72 AB 725 18428+5937 HD 173739 8.91 M3V 13.34 170.4 280.28 2.57
94336 AB 9648 19121+4951 HD 179958 6.57 G4V 7.648 207.8 40.16 0.83
97241 AB 4122 19458+3223 CRI 24 10.86 M1 12.765 338.9 87.57 4.80
97292 AB 767 19464+3201 HD 331161 10.28 M1 4.866 133.7 73.86 1.96
106694 AB 834 21366+3927 VYS 10 10.20 M0 1.783 283.6 46.80 3.37
110526 AB 856 22235+3228 WOR 11 11.40 M3 1.772 199.0 62.18 10.01
110640 AB 857.1 22248+2233 BD +21 4747 8.82 M0 1.613 228. 46.74 1.66
110893 AB 860 22281+5741 HD 239960 9.59 M3 3.400 128.3 249.52 3.03
1 Component identification.
2 Gliese & Jahreiss (1991).
3 Dommanget & Nys (2002).
4 Revised Hipparcos parallax (Söderhjelm 1999).
5 The alternative Hipparcos parallax solution is adopted.
6 Van Altena et al. (1995).
7 The ground-based and Hipparcos parallaxes are slightly discrepant (2 $\sigma$-level).


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