Table 1: VRI Photometry of Southern high proper motion stars from the Cerro El Roble proper motion survey.

STAR
$N_{\rm obs}$ V ErrV $\sigma_V$ V-R Err(V-R) $\sigma_{(V-R)}$ V-I Err(V-I) $\sigma_{(V-I)}$ Ref. Remarks

WT98
5 14.023 0.002 0.027 1.203 0.002 0.028 2.627 0.002 0.018 1  
WT110 4 16.932 0.017 0.023 1.193 0.019 0.021 2.700 0.017 0.020 1  
WT121 4 15.587 0.005 0.039 1.274 0.006 0.036 2.884 0.006 0.048 1  
WT133 6 16.021 0.008 0.018 1.350 0.008 0.020 3.064 0.008 0.018 1  
WT135 7 14.161 0.002 0.024 1.099 0.002 0.030 2.338 0.002 0.023 1  
WT143 4 16.325 0.011 0.053 0.805 0.013 0.043 1.518 0.013 0.057 1  
WT178 4 14.919 0.003 0.011 1.402 0.004 0.007 3.121 0.003 0.004 3  
WT233b 6 16.235 0.008 0.042 0.920 0.009 0.029 1.821 0.009 0.023 3 *
WT233f 6 16.901 0.014 0.050 0.469 0.018 0.063 0.993 0.021 0.104 3 *
WT1289 5 16.181 0.011 0.049 1.265 0.012 0.037 2.881 0.011 0.039 5 *
WT1353 4 13.916 0.002 0.028 1.083 0.003 0.009 2.347 0.003 0.009 5  
WT1356 6 16.080 0.009 0.041 1.401 0.009 0.043 3.126 0.009 0.035 5  
WT1463 6 16.159 0.011 0.043 1.261 0.012 0.042 2.827 0.011 0.026 5  
WT1481 6 13.622 0.002 0.017 0.703 0.002 0.019 1.328 0.002 0.011 5  
WT1515 7 14.903 0.004 0.041 1.283 0.004 0.053 2.842 0.004 0.040 5  
WT1530 6 16.882 0.011 0.042 1.417 0.012 0.060 3.110 0.011 0.036 5  
WT1542 6 14.116 0.002 0.035 1.230 0.002 0.045 2.698 0.002 0.037 5  
WT1759 4 15.446 0.007 0.019 0.275 0.010 0.028 0.544 0.011 0.016 6  
WT1760b 4 16.164 0.008 0.029 1.390 0.010 0.036 3.070 0.009 0.025 6 *
WT2390 7 15.215 0.004 0.027 1.168 0.005 0.028 2.569 0.004 0.029 8  
WT2431 6 13.708 0.002 0.024 0.966 0.002 0.024 1.897 0.002 0.017 8  
WT2451 8 15.062 0.003 0.027 1.214 0.004 0.044 2.727 0.003 0.037 8  
WT2461 6 15.264 0.004 0.036 1.183 0.005 0.022 2.669 0.004 0.033 8  
WT2462 4 15.089 0.005 0.016 1.318 0.006 0.020 2.957 0.005 0.015 8  
WT2463 4 15.711 0.006 0.045 1.046 0.007 0.028 2.225 0.006 0.040 8  
WT2475 6 15.899 0.006 0.017 1.386 0.006 0.014 3.082 0.006 0.014 6  
LTT1323 4 13.138 0.001 0.029 1.141 0.001 0.015 2.550 0.001 0.016 2  
LTT1588 7 11.495 0.001 0.011 0.407 0.001 0.007 0.784 0.001 0.006 8 *
LTT1697 6 12.801 0.001 0.022 0.932 0.001 0.006 1.814 0.001 0.015 8  
LTT1848 4 13.012 0.001 0.017 1.029 0.001 0.023 2.128 0.001 0.024 2  
LTT2202 6 14.544 0.003 0.026 0.941 0.003 0.039 1.854 0.003 0.029 8  
LTT2631 5 12.936 0.001 0.010 1.183 0.002 0.011 2.656 0.002 0.015 7  
LTT2856 6 12.587 0.001 0.028 1.068 0.001 0.011 2.290 0.001 0.011 4  
LTT3461 6 11.235 0.001 0.013 0.864 0.001 0.008 1.677 0.001 0.007 7  
LTT3496 6 15.094 0.003 0.029 0.138 0.004 0.019 0.317 0.006 0.029 4  
LTT3553 6 12.590 0.001 0.034 1.081 0.001 0.014 2.383 0.001 0.018 7  
LTT3616 6 11.882 0.001 0.020 1.064 0.001 0.014 2.349 0.001 0.011 7  
LTT3632 6 12.958 0.001 0.014 1.101 0.001 0.017 2.436 0.001 0.030 4  
LTT3725 4 15.650 0.006 0.007 1.171 0.007 0.010 2.653 0.007 0.057 8  
LTT3742 4 13.021 0.001 0.013 1.163 0.001 0.011 2.555 0.002 0.013 8  
LTT3790 4 11.673 0.001 0.006 1.044 0.001 0.009 2.194 0.001 0.015 4  
LTT3791 4 13.202 0.002 0.005 1.240 0.003 0.007 2.756 0.002 0.010 4  
LTT3802 5 11.274 0.001 0.001 0.976 0.001 0.012 1.940 0.001 0.021 7  
LTT3861 6 11.211 0.001 0.008 0.868 0.001 0.010 1.640 0.001 0.014 8  

References to coordinates, proper motions, and finding charts.
[1] Wroblewski, H., & Torres, C. 1989, A&AS, 78, 231
[2] Wroblewski, H., & Torres, C. 1990, A&AS, 83, 317
[3] Wroblewski, H., & Torres, C. 1991, A&AS, 91, 129
[4] Wroblewski, H., & Torres, C. 1992, A&AS, 92, 449
[5] Wroblewski, H., & Torres, C. 1996, A&AS, 115, 481
[6] Wroblewski, H., & Torres, C. 1997, A&AS, 122, 447
[7] Wroblewski, H., & Torres, C. 1998, A&AS, 128, 457
[8] Wroblewski, H., & Costa, E. 2001, A&A, 367, 725.


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