Table 3: Published photometric data for the eclipsing binaries and the comparison stars. N is the total number of observations used to form the mean values, and $\sigma $ is the rms error (per observation) in mmag.
Object Reference V $\sigma $ b-y $\sigma $ m1 $\sigma $ c1 $\sigma $ N(${\it uvby}$) $\beta $ $\sigma $ N($\beta $)
AD Boo HH75 9.370   0.348   0.153   0.419   1      
  L02 9.399   0.335   0.161   0.446   1 2.645   1
HD 128369 O83 7.965 3 0.298 3 0.122 5 0.453 5 5 2.643 2 3
HD 129430 O93 6.401 4 0.590 2 0.293 2 0.413 3 1      
HD 128185 O83 7.925 4 0.387 6 0.163 2 0.420 3 4 2.604 8 3
SW CMa L02 9.121   0.108   0.221   1.026   1 2.860   1
  WK83 9.15   0.095   0.209   1.036   1 2.863   1
V636 Cen O83, OP84 8.713 6 0.407 5 0.220 9 0.259 7 1 2.601 7 1
  O85 8.706 7 0.426 3 0.197 5 0.276 8 3      
  O93 8.720 2 0.414 3 0.205 6 0.284 8 3      
VZ Hya WK83 9.660 30 0.333 1 0.146 1 0.368 4 2 2.624 7 2
HD 72528 O83, OP84 7.335 6 0.328 4 0.181 6 0.381 6 1 2.617 7 1
HD 71615 O83, OP84 7.949 5 0.249 4 0.141 6 0.520 7 1 2.685 7 1
HD 72782 O83 7.648 6 0.103 5 0.193 9 0.947 15 2      
  J96                   2.840 9 2
WZ Oph HH75 9.095 7 0.377 32 0.119 42 0.367 10 2      
HD 155193 O83 7.010 5 0.352 3 0.168 4 0.419 4 1      
  O94 7.020 4 0.350 3 0.163 4 0.429 4 1      
  P69 7.020   0.348   0.168   0.418   2      
HD 154931 O83 7.263 9 0.385 7 0.192 0 0.372 7 2      
  O94 7.251 4 0.396 3 0.167 4 0.378 5 1      
  P69 7.250   0.392   0.179   0.365   2      
References are: HH75 = Hilditch & Hill (1975); J96 = Jordi et al. (1996); O83 = Olsen (1983); O93 = Olsen (1993); O94 = Olsen (1994b); OP83 = Olsen & Perry (1984); P69 = Perry (1969); WK83 = Wolf & Kern (1983); L02 = Lacy (2002). The two WK83 observations of VZ Hya are done near phase 0.00. Two WK83 observations of SW CMa inside eclipses have not been included. Two HH75 observations of WZ Oph inside eclipses have not been included.

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