Table 2: Number of stars observed (N) and mean internal errors ($\sigma $) as a function of apparent visual magnitude.
V range V (b-y) m1 c1 H$_{\beta }$
  N $\sigma $ N $\sigma $ N $\sigma $ N $\sigma $ N $\sigma $
8-9 3 0.029 3 0.028 3 0.029 2 0.004    
9-10 8 0.008 7 0.007 6 0.008 7 0.007 2 0.001
10-11 22 0.003 22 0.002 22 0.003 22 0.005 10 0.009
11-12 28 0.004 28 0.022 26 0.003 26 0.005 14 0.016
12-13 114 0.004 114 0.003 114 0.004 114 0.005 56 0.009
13-14 199 0.003 199 0.003 198 0.004 197 0.006 75 0.015
14-15 240 0.020 239 0.005 238 0.006 237 0.009 63 0.016
15-16 277 0.007 277 0.010 275 0.011 269 0.018 57 0.019
16-17 299 0.011 299 0.015 272 0.021 233 0.031 10 0.016
17-18 307 0.021 306 0.029 245 0.041 109 0.043 1 0.033
18-19 259 0.040 259 0.058 130 0.073 46 0.059    
19-20 75 0.093 75 0.125 18 0.141 12 0.106    
Total 1831   1828   1547   1274   288  

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