**Table 2:** Photometric data for the eclipsing binaries and the comparison stars in the *uvby* and $\beta$ standard systems. For the eclipsing binaries, the *uvby* information is given at maximum light level outside eclipses. The $\beta$ information is the mean values outside eclipses. N is the total number of observations used to form the mean values, and $\sigma$ is the rms error (per observation) in mmag.
Object	Sp. type	V	$\sigma$	b-y	$\sigma$	m₁	$\sigma$	c₁	$\sigma$	N(uvby)	$\beta$	$\sigma$	N( $\beta$ )
DWCar	B1V+B1V	9.675	5	0.067	5	0.046	8	-0.017	8	7	2.528	7	7
HD 93191	A0	8.488	5	-0.011	3	0.157	4	0.824	4	2	2.804	5	2
HD 92072	B5V	7.044	4	-0.052	5	0.131	8	0.394	5	3	2.720	5	2
HD 92288	B6V	7.902	4	-0.033	1	0.130	2	0.482	4	3	2.705	2	2
BFCen	B8	8.513	10	0.046	8	0.063	15	0.136	11	4	2.616	6	2
HD 100942	B8/B9V	7.770	16	0.026	5	0.114	8	0.708	7	16	2.797	6	7
HD 101466	A0IV	7.322	26	0.045	4	0.123	8	1.062	5	19	2.851	9	6
ACVel	B3IV	8.869	8	0.118	3	0.044	4	0.309	1	4	2.637	5	4
HD 93943	B9.5IV-V	5.863	27	0.016	5	0.129	8	1.016	4	11	2.843	8	3
HD 92757	B9.5V	6.820	3	-0.029	2	0.180	1	0.945	2	3	2.891	4	2
HD 92155	B3V	6.430	1	-0.079	1	0.121	0	0.328	1	2	2.653	6	2
NSV 5783	B5V	8.679	8	0.011	4	0.107	9	0.391	6	8	2.695	2	4
HD 108925	A3V	6.477		0.068		0.183		1.141		1	2.842	7	2
HD 109808	A1/A2V	6.948	4	0.073	3	0.193	6	0.905	4	2	2.853	1	2

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