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Table 2:

Extract of the CPMDS catalogue of common proper motion double stars with angular separations smaller than 2 $\hbox {$^\prime $ }$.
$\alpha_{2000}$ $\delta_{2000}$ Identification $\rho $ $\sigma_{\rho}$ $\theta$ $\sigma_{\theta}$ Mag P Mag S $\mu^*_{\alpha} P$ $\mu_{\delta} P$ $\sigma_{\mu^*_\alpha} P$ $\sigma_{\mu_\delta} P$ No $\mu^*_{\alpha} S$ $\mu_{\delta} S$ $\sigma_{\mu^*_\alpha} S$ $\sigma_{\mu_\delta} S$ No Epoch Class $\beta $  
h m s $^\circ$ $^\prime$ $^{\prime\prime}$     $^{\prime\prime}$ $^\circ$ mag. mas/yr   mas/yr   yr      
0 2 20.009 +16 08 46.97 1692 1685 30.58 0.06 185.82 0.10 15.427 15.781 19.5 -12.5 4.8 3.8 7 8 21.6 -15.4 3.8 3.9 6 6 1994.94 I 0.35  
0 2 46.393 +16 47 8.27 2010 1993 77.72 0.06 335.41 0.04 15.464 15.697 16.1 -25.5 4.4 3.6 9 8 13.9 -23.1 4.0 5.2 4 3 1994.94 II 0.19  
0 3 44.683 +11 33 34.22 2710 2680 76.30 0.07 335.59 0.05 15.490 16.088 17.5 -11.6 4.7 3.6 6 7 14.3 -14.4 3.8 3.9 4 4 1992.78 I 0.44  
0 5 24.297 +16 19 44.44 3857 3820 89.14 0.04 336.94 0.02 8.770 8.982 33.9 -31.3 2.1 2.1 9 9 34.9 -30.1 2.1 2.1 9 9 1996.57 I 0.01  
0 12 34.144 +11 18 0.44 8713 8668 79.13 0.05 253.32 0.04 15.007 15.597 -10.7 -12.3 3.5 3.5 9 9 -13.6 -14.3 3.5 3.5 7 8 1995.18 I 0.60  
0 13 41.298 +15 37 1.46 9457 9535 96.90 0.06 115.02 0.04 15.038 16.107 18.2 -20.5 3.5 3.6 9 9 19.7 -19.0 3.8 3.9 4 4 1993.95 II 0.03  
0 14 23.006 +16 42 59.12 9941 9955 95.29 0.06 12.97 0.03 15.906 16.347 11.7 -15.3 3.6 3.7 4 4 14.2 -14.8 3.6 3.7 4 4 1995.72 I 0.05  


 

Table 3: Extract of high proper motion CPM stars with angular separations greater than 2 $\hbox {$^\prime $ }$ and smaller than 5 $\hbox {$^\prime $ }$.
$\alpha_{2000}$ $\delta_{2000}$ Identification $\rho $ $\sigma_{\rho}$ $\theta$ $\sigma_{\theta}$ Mag P Mag S $\mu^*_{\alpha} P$ $\mu_{\delta} P$ $\sigma_{\mu^*_\alpha} P$ $\sigma_{\mu_\delta} P$ No $\mu^*_{\alpha} S$ $\mu_{\delta} S$ $\sigma_{\mu^*_\alpha} S$ $\sigma_{\mu_\delta} S$ No Epoch Class $\beta $  
h m s $^\circ$ $^\prime$ $^{\prime\prime}$     $^{\prime\prime}$ $^\circ$ mag. mas/yr   mas/yr   yr      
1 32 31.117 +16 45 24.74 57224 57397 247.92 0.04 79.21 0.01 13.625 14.963 35.1 -51.2 5.5 5.5 7 7 34.2 -50.8 5.5 5.5 7 7 1998.81 I 0.12  
1 47 39.162 +16 42 31.12 65958 65844 209.45 0.04 228.38 0.01 10.224 11.236 89.6 -54.6 2.0 2.0 7 7 89.3 -54.5 2.0 2.0 12 12 1997.53 I 0.12  
2 55 52.221 +14 55 11.50 107836 107938 286.74 0.06 30.23 0.01 14.719 15.576 18.1 -48.3 5.0 5.1 11 11 20.5 -47.4 5.3 5.3 4 4 1996.92 I 0.04  
3 5 52.711 +13 1 40.23 114294 114392 184.33 0.05 138.04 0.02 12.991 14.485 -39.2 -66.4 5.1 5.1 7 7 -41.6 -62.2 5.0 5.1 10 10 1998.14 I 0.22  
3 16 12.555 +13 1 52.68 120872 120882 229.30 0.05 2.49 0.01 14.087 14.907 47.3 -31.5 5.0 5.0 8 8 51.7 -31.4 5.0 5.0 7 7 1998.48 I 0.05  
3 30 5.302 +12 58 28.71 129571 129567 162.78 0.06 180.96 0.02 15.334 15.665 31.2 -50.5 5.0 5.0 9 9 33.5 -48.4 5.1 5.1 4 4 1998.20 IV 0.03  
4 28 34.466 +15 57 44.13 171052 171309 268.36 0.06 74.97 0.01 5.906 11.975 111.9 -23.0 2.2 2.2 6 6 108.2 -25.1 5.8 5.9 6 6 1996.16 V 0.47  


 

Table 4: Extract of our measurements of the 926 WDS double stars.

$\alpha_{2000}$ 		$\delta_{2000}$ WDS $\rho $ $\sigma_{\rho}$ $\theta$ $\sigma_{\theta}$ MagP MagS Epoch No
h m s $^\circ$ $^\prime$ $^{\prime\prime}$   $^{\prime\prime}$ $^\circ$ mag. year  
0 00 13.8 +16 40 57 00003+1642 26.629 0.015 61.54 0.03 9.6 13.1 1999.1 10
0 01 13.1 +13 58 29 00012+1357 11.653 0.016 204.02 0.06 10.6 11.2 1999.0 8
0 05 24.2 +16 19 44 00054+1620 89.141 0.044 336.94 0.02 8.8 9.0 1998.6 8
0 09 37.4 +11 46 12 00096+1145 289.248 0.022 42.69 0.00 10.5 10.8 1997.7 9
0 09 51.8 +11 24 58 00099+1125 31.534 0.029 167.73 0.04 8.5 11.2 1998.8 7


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