Table 2: New photometric data for the eclipsing binaries and the comparison stars. For the eclipsing binaries, the ${\it uvby}\beta $ information is the mean values outside eclipses, see also Fig 1. N is the total number of observations used to form the mean values, and $\sigma $ is the rms error (per observation) in mmag. See also Table 3.
Object Sp. type V $\sigma $ b-y $\sigma $ m1 $\sigma $ c1 $\sigma $ N (uvby) $\beta $ $\sigma $ N ($\beta $)
AD Boo F6+G0 9.379 7 0.322 4 0.186 10 0.431 14 14 2.647 8 16
HD 128369 F5 7.959 8 0.281 3 0.149 8 0.455 11 17 2.640 8 15
HD 129430 G8III-IV 6.402 5 0.581 2 0.311 6 0.385 9 5 2.573 3 3
HD 128185 F8V 7.925 11 0.373 5 0.183 10 0.402 12 13 2.606 8 14
HW CMa A8 9.190 6 0.128 3 0.228 10 0.839 14 6 2.853 10 95
SW  CMa A8 9.149 9 0.094 8 0.210 9 1.013 7 12 2.865 10 104
HD 56341 A0V 6.358 8 -0.001 2 0.127 5 1.098 7 17 2.861 6 53
HD 53123 B9V 7.156 13 -0.020 5 0.112 7 0.878 9 10 2.805 8 51
HD 55271 B5V 6.950 14 0.005 2 0.060 8 0.290 6 2 2.520 10 9
V636 Cen F8/G0V 8.704 11 0.410 4 0.205 7 0.285 18 16 2.594 12 57
HD 124829 F2 8.466 6 0.266 4 0.143 6 0.516 6 16 2.682 6 16
HD 125444 A6V 7.557 12 0.111 4 0.176 7 0.918 5 10 2.814 9 34
VZ Hya F5+F6 8.953 4 0.300 4 0.166 7 0.389 9 9 2.640 9 83
HD 72528 F7V 7.330 3 0.337 2 0.177 3 0.388 6 8 2.628 8 33
HD 71615 F0 7.946 3 0.233 4 0.176 7 0.516 8 9 2.692 8 34
HD 72782 A2 7.641 10 0.109 2 0.183 3 0.947 11 5 2.831 7 61
WZ Oph F8 9.096 7 0.366 5 0.145 7 0.375 5 11 2.627 8 11
HD 155193 F8IV 7.007 7 0.338 4 0.185 5 0.405 6 12 2.623 7 12
HD 154931 G0 7.258 7 0.384 4 0.189 6 0.361 4 12 2.600 8 13


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