Table 3: Published ${uvby}\beta$ photometry 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. References are: GO76 = Grønbech & Olsen (1976), GO77 = Grønbech & Olsen (1977), HM80 = Heck & Manfroid (1980), K98 = Kaltcheva (1998), KOC00 = Kaltcheva et al. (2000), K78 = Kilkenny (1978), K81 = Kilkenny (1981), K92 = Knude (1992), LPLM90 = Landolt et al. (1990), S85 = Shobbrook (1985), SHL92 = Slawson et al. (1992), TAT95 = Twarog & Anthony-Twarog (1995), WK83 = Wolf & Kern (1983).
Object Ref. Sp. type V $\sigma$ b-y $\sigma$ m1 $\sigma$ c1 $\sigma$ N(uvby) $\beta $ $\sigma$ N($\beta $)
DWCar - B1V+B1V                        
HD 93191 - A0                        
HD 92072 K98 B5V 7.119   -0.030   0.085   0.433     2.715    
  LPLM90   7.068 12 -0.046 4 0.115 8 0.423 8 17 2.702 8 15
HD92288 KOC00 B6V 7.893 17 -0.012 3 0.102 1 0.500 4 2 2.705 1 2
  LPLM90   7.904 5 -0.022 2 0.099 7 0.525 12 3 2.708 4 3
BFCen WK83 B8 8.54   0.054   0.029   0.172   1 2.609   1
  S85   8.62   0.058   0.010   0.150   4 2.619   3
HD 100942 KOC00 B8/B9V 7.762 2 0.011 3 0.138 5 0.698 11 3 2.800 7 1
HD 101466 KOC00 A0IV 7.318 3 0.034 8 0.143 8 1.052 0 2 2.858 7 1
  SHL92   7.35               2      
ACVel WK83 B3IV 8.88   0.155   -0.013   0.331   1 2.629   1
HD 93943 GO76,77 B9.5IV-V 5.865 8 0.018 7 0.122 10 1.029 1 2 2.848 5 3
HD 92757 - B9.5V                        
HD 92155 HM80 B3V 6.432 4 -0.069 2 0.096 6 0.356 6 6 2.654 4 5
NSV5783 K92 B5V 8.674   0.029   0.060   0.428     2.714    
  K81                     2.696   2
  K78   8.69   0.023   0.075   0.410   3      
HD 108925 GO76, 77 A3V 6.448 8 0.087 8 0.153 4 1.172 3 2 2.853 9 3
  TAT95   6.452 2 0.081 4 -   -   4      
  SHL92   6.44               1      
HD 109808 SHL92 A1/A2V 6.934                      

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