Table 1: Variability data for the oscillating BS stars. Frequencies are in d^-1 and amplitudes are given in mmag. The quoted errors on the frequencies are standard deviations on the values determined from extensive simulations (see text).
ID $\nu_{i}$ $\nu$ A_I A_B S/N_B

V1 $\nu_{1}$ 13.630(1) 3.2 6.8 15.1

$\nu_{2}$ 14.684(1) 2.8 5.1 11.2

$\nu_{3}$ 14.716(1) 1.7 2.9 6.4

$\nu_{4}$ 16.688(5) 1.5 2.8 6.2

$\nu_{5}$ 16.896(2) 1.0 2.2 5.0

$\nu_{6}$ 17.043(2) 0.9 1.8 4.0

$\nu_{7}$ 17.672(1) 2.2 4.5 10.0

V2 $\nu_{1}$ 10.854(1) 55.8 121.4 215.0

$\nu_{2}$ 20.141(1) 7.5 14.2 29.5

2 $\nu_{1}$ 21.709(1) 8.5 17.0 35.3

$\nu_{3}$ 30.995(2) 1.2 2.8 5.9

3 $\nu_{1}$ 32.563(3) 1.3 3.1 6.4

V3 $\nu_{1}$ 0.526(1) 3.2 6.9 3.1

$\nu_{2}$ 0.827(6) 4.4 10.4 4.7

$\nu_{3}$ 0.908(3) 4.9 12.2 5.5

$\nu_{4}$ 11.243(2) 1.7 5.8 6.4

$\nu_{5}$ 12.031(1) 7.4 16.8 18.6

$\nu_{6}$ 12.265(1) 25.9 56.2 62.0

$\nu_{7}$ 12.748(5) 2.2 3.9 4.4

$\nu_{8}$ 13.088(1) 10.0 18.2 20.1

$\nu_{9}$ 18.555(4) 2.5 3.7 4.1

$\nu_{10}$ 24.336(5) 1.7 3.2 4.5

$\nu_{11}$ 24.530(2) 2.1 4.3 6.0

V6 $\nu_{1}$ 9.441(3) 0.9 3.7 5.9

$\nu_{2}$ 10.767(1) 5.1 10.9 17.2

$\nu_{3}$ 13.958(3) 1.4 3.1 4.9

V7 $\nu_{1}$ 10.576(1) 6.9 15.3 22.3

V8 $\nu_{1}$ 10.227(2) 2.9 4.5 4.5

$\nu_{2}$ 10.611(1) 4.4 11.1 11.2

$\nu_{3}$ 10.781(1) 5.0 11.7 11.7

$\nu_{4}$ 11.550(2) 4.7 8.3 8.4

$\nu_{5}$ 16.149(2) 3.4 6.8 6.8

$\nu_{6}$ 19.423(2) 3.4 7.2 7.2

$\nu_{7}$ 20.944(3) 1.8 3.4 3.4

**Table 1:** Variability data for the oscillating BS stars. Frequencies are in d^-1 and amplitudes are given in mmag. The quoted errors on the frequencies are standard deviations on the values determined from extensive simulations (see text).
ID	$\nu_{i}$	$\nu$	A_I	A_B	S/N_B
V1	$\nu_{1}$	13.630(1)	3.2	6.8	15.1
	$\nu_{2}$	14.684(1)	2.8	5.1	11.2
	$\nu_{3}$	14.716(1)	1.7	2.9	6.4
	$\nu_{4}$	16.688(5)	1.5	2.8	6.2
	$\nu_{5}$	16.896(2)	1.0	2.2	5.0
	$\nu_{6}$	17.043(2)	0.9	1.8	4.0
	$\nu_{7}$	17.672(1)	2.2	4.5	10.0
V2	$\nu_{1}$	10.854(1)	55.8	121.4	215.0
	$\nu_{2}$	20.141(1)	7.5	14.2	29.5
	2 $\nu_{1}$	21.709(1)	8.5	17.0	35.3
	$\nu_{3}$	30.995(2)	1.2	2.8	5.9
	3 $\nu_{1}$	32.563(3)	1.3	3.1	6.4
V3	$\nu_{1}$	0.526(1)	3.2	6.9	3.1
	$\nu_{2}$	0.827(6)	4.4	10.4	4.7
	$\nu_{3}$	0.908(3)	4.9	12.2	5.5
	$\nu_{4}$	11.243(2)	1.7	5.8	6.4
	$\nu_{5}$	12.031(1)	7.4	16.8	18.6
	$\nu_{6}$	12.265(1)	25.9	56.2	62.0
	$\nu_{7}$	12.748(5)	2.2	3.9	4.4
	$\nu_{8}$	13.088(1)	10.0	18.2	20.1
	$\nu_{9}$	18.555(4)	2.5	3.7	4.1
	$\nu_{10}$	24.336(5)	1.7	3.2	4.5
	$\nu_{11}$	24.530(2)	2.1	4.3	6.0
V6	$\nu_{1}$	9.441(3)	0.9	3.7	5.9
	$\nu_{2}$	10.767(1)	5.1	10.9	17.2
	$\nu_{3}$	13.958(3)	1.4	3.1	4.9
V7	$\nu_{1}$	10.576(1)	6.9	15.3	22.3
V8	$\nu_{1}$	10.227(2)	2.9	4.5	4.5
	$\nu_{2}$	10.611(1)	4.4	11.1	11.2
	$\nu_{3}$	10.781(1)	5.0	11.7	11.7
	$\nu_{4}$	11.550(2)	4.7	8.3	8.4
	$\nu_{5}$	16.149(2)	3.4	6.8	6.8
	$\nu_{6}$	19.423(2)	3.4	7.2	7.2
	$\nu_{7}$	20.944(3)	1.8	3.4	3.4

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