Table 2: Variability data for the $\gamma$ Doradus stars. Frequencies are in d^-1, amplitudes in mmag and phases in degrees. The quoted errors on the frequencies, amplitude ratios and phase differences are standard deviations on the values determined from extensive simulations (see text).
ID $\nu_{i}$ $\nu$ A_B S/N_B A_I/A_B $\phi_{I}-\phi_{B}$

V11 $\nu_{1}$ 1.165(1) 7.93 6.78 0.41(4) -1(5)

$\nu_{2}$ 1.270(1) 5.12 4.37 0.40(6) 6(8)

$\nu_{3}$ 1.400(2) 8.58 7.34 0.40(3) 3(5)

V12 $\nu_{1}$ 1.395(4) 9.26 5.84 0.70(6) 30(6)

V13 $\nu_{1}$ 0.830(1) 8.10 6.00 0.39(4) 13(6)

V14 $\nu_{1}$ 0.758(4) 2.130 4.57 0.68(13) 33(12)

$\nu_{2}$ 0.870(1) 17.750 38.08 0.43(2) -8(2)

$\nu_{3}$ 0.927(1) 4.090 8.77 0.31(8) 88(18)

V15 $\nu_{1}$ 0.495(4) 3.60 3.16 0.46(13) 35(17)

$\nu_{2}$ 0.614(1) 14.93 13.10 0.48(2) 4(2)

$\nu_{3}$ 1.130(1) 6.28 5.51 0.45(4) 131(5)

V16 $\nu_{1}$ 0.474(20) 9.599 5.02 0.29(3) 14(13)

$\nu_{2}$ 0.795(1) 20.603 10.78 0.52(2) -13(2)

$\nu_{3}$ 0.918(3) 11.459 6.00 0.49(4) 1(4)

$\nu_{4}$ 1.730(13) 6.144 3.21 0.73(11) -4(8)

V17 $\nu_{1}$ 0.136(1) 10.875 7.64 0.68(4) 21(3)

$\nu_{2}$ 0.606(1) 28.233 19.85 0.46(2) 4(2)

$\nu_{3}$ 0.645(7) 15.658 11.01 0.51(3) -11(3)

$\nu_{4}$ 1.268(1) 7.362 5.17 0.55(5) -3(5)

$\nu_{5}$ 1.537(2) 7.213 5.07 0.35(11) 28(15)

$\nu_{6}$ 2.439(1) 5.711 4.01 0.65(8) -2(7)

V18 $\nu_{1}$ 0.206(1) 8.939 9.51 0.80(4) -15(3)

$\nu_{2}$ 0.674(2) 3.767 4.01 0.96(11) -14(6)

V19 $\nu_{1}$ 0.156(1) 7.190 6.13 0.56(4) 1(4)

$\nu_{2}$ 0.442(2) 15.774 13.44 0.51(2) 1(2)

$\nu_{3}$ 0.583(1) 20.767 17.70 0.39(2) 0(3)

$\nu_{4}$ 1.344(3) 6.928 5.90 0.51(5) -27(5)

$\nu_{5}$ 1.593(5) 6.902 5.88 0.51(6) 5(6)

V20 $\nu_{1}$ 0.842(25) 7.610 11.23 0.43(5) -28(7)

$\nu_{2}$ 0.883(1) 9.963 14.70 0.66(5) -2(3)

$\nu_{3}$ 1.701(16) 3.011 4.44 0.47(8) -28(11)

V21 $\nu_{1}$ 0.503(1) 5.069 3.50 0.53(9) 4(15)

$\nu_{3}$ 0.648(1) 17.793 12.30 0.40(2) -15(2)

$\nu_{3}$ 1.740(1) 5.434 3.76 0.60(5) 29(6)

V22 $\nu_{1}$ 0.700(1) 14.214 6.18 0.44(3) -8(4)

$\nu_{2}$ 1.378(1) 12.684 5.52 0.42(3) 2(4)

V23 $\nu_{1}$ 1.168(3) 9.616 6.35 0.47(4) 1(5)

$\nu_{2}$ 1.260(3) 14.415 9.52 0.52(3) 12(3)

V24 $\nu_{1}$ 0.916(1) 14.458 12.25 0.45(3) 16(5)

V25 $\nu_{1}$ 1.178(1) 14.747 10.84 0.60(3) 12(2)

$\nu_{2}$ 1.987(2) 7.055 5.19 0.50(5) -18(8)

**Table 2:** Variability data for the $\gamma$ Doradus stars. Frequencies are in d^-1, amplitudes in mmag and phases in degrees. The quoted errors on the frequencies, amplitude ratios and phase differences are standard deviations on the values determined from extensive simulations (see text).
ID	$\nu_{i}$	$\nu$	A_B	S/N_B	A_I/A_B	$\phi_{I}-\phi_{B}$
V11	$\nu_{1}$	1.165(1)	7.93	6.78	0.41(4)	-1(5)
	$\nu_{2}$	1.270(1)	5.12	4.37	0.40(6)	6(8)
	$\nu_{3}$	1.400(2)	8.58	7.34	0.40(3)	3(5)
V12	$\nu_{1}$	1.395(4)	9.26	5.84	0.70(6)	30(6)
V13	$\nu_{1}$	0.830(1)	8.10	6.00	0.39(4)	13(6)
V14	$\nu_{1}$	0.758(4)	2.130	4.57	0.68(13)	33(12)
	$\nu_{2}$	0.870(1)	17.750	38.08	0.43(2)	-8(2)
	$\nu_{3}$	0.927(1)	4.090	8.77	0.31(8)	88(18)
V15	$\nu_{1}$	0.495(4)	3.60	3.16	0.46(13)	35(17)
	$\nu_{2}$	0.614(1)	14.93	13.10	0.48(2)	4(2)
	$\nu_{3}$	1.130(1)	6.28	5.51	0.45(4)	131(5)
V16	$\nu_{1}$	0.474(20)	9.599	5.02	0.29(3)	14(13)
	$\nu_{2}$	0.795(1)	20.603	10.78	0.52(2)	-13(2)
	$\nu_{3}$	0.918(3)	11.459	6.00	0.49(4)	1(4)
	$\nu_{4}$	1.730(13)	6.144	3.21	0.73(11)	-4(8)
V17	$\nu_{1}$	0.136(1)	10.875	7.64	0.68(4)	21(3)
	$\nu_{2}$	0.606(1)	28.233	19.85	0.46(2)	4(2)
	$\nu_{3}$	0.645(7)	15.658	11.01	0.51(3)	-11(3)
	$\nu_{4}$	1.268(1)	7.362	5.17	0.55(5)	-3(5)
	$\nu_{5}$	1.537(2)	7.213	5.07	0.35(11)	28(15)
	$\nu_{6}$	2.439(1)	5.711	4.01	0.65(8)	-2(7)
V18	$\nu_{1}$	0.206(1)	8.939	9.51	0.80(4)	-15(3)
	$\nu_{2}$	0.674(2)	3.767	4.01	0.96(11)	-14(6)
V19	$\nu_{1}$	0.156(1)	7.190	6.13	0.56(4)	1(4)
	$\nu_{2}$	0.442(2)	15.774	13.44	0.51(2)	1(2)
	$\nu_{3}$	0.583(1)	20.767	17.70	0.39(2)	0(3)
	$\nu_{4}$	1.344(3)	6.928	5.90	0.51(5)	-27(5)
	$\nu_{5}$	1.593(5)	6.902	5.88	0.51(6)	5(6)
V20	$\nu_{1}$	0.842(25)	7.610	11.23	0.43(5)	-28(7)
	$\nu_{2}$	0.883(1)	9.963	14.70	0.66(5)	-2(3)
	$\nu_{3}$	1.701(16)	3.011	4.44	0.47(8)	-28(11)
V21	$\nu_{1}$	0.503(1)	5.069	3.50	0.53(9)	4(15)
	$\nu_{3}$	0.648(1)	17.793	12.30	0.40(2)	-15(2)
	$\nu_{3}$	1.740(1)	5.434	3.76	0.60(5)	29(6)
V22	$\nu_{1}$	0.700(1)	14.214	6.18	0.44(3)	-8(4)
	$\nu_{2}$	1.378(1)	12.684	5.52	0.42(3)	2(4)
V23	$\nu_{1}$	1.168(3)	9.616	6.35	0.47(4)	1(5)
	$\nu_{2}$	1.260(3)	14.415	9.52	0.52(3)	12(3)
V24	$\nu_{1}$	0.916(1)	14.458	12.25	0.45(3)	16(5)
V25	$\nu_{1}$	1.178(1)	14.747	10.84	0.60(3)	12(2)
	$\nu_{2}$	1.987(2)	7.055	5.19	0.50(5)	-18(8)

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