**Table 4:** Pulsational amplitude and phases for spectral lines in 10 Aql. False alarm probabilities (FAP) were computed assuming no a priori knowledge of the presence of possible frequencies. The FAP values in parentheses are for a pre-selected (photometric) frequency.
	26 Jul. 1997
Line (Å)	$\nu$ (c d^-1)	P (min)	K (m s^-1)	$\phi$	FAP
$\lambda$ 5069.43	107.5	13.39 $\pm$ 0.67	153.7 $\pm$ 42.3	0.37 $\pm$ 0.044	0.12 (0.0015)
$\lambda$ 5069.43	122.9	11.72 $\pm$ 0.51	152.0 $\pm$ 42.5	0.37 $\pm$ 0.045	0.14 (0.002)
$\lambda$ 5104.44	124.0	11.61 $\pm$ 0.29	175.1 $\pm$ 27.8	0.38 $\pm$ 0.031	1.5 $\times$ 10^-3
$\lambda$ 5373.01	125.1	11.51 $\pm$ 0.53	63.0 $\pm$ 21.0	0.71 $\pm$ 0.053	0.51 (0.016)
$\lambda$ 5471.40	123.9	11.62 $\pm$ 0.38	262.7 $\pm$ 47.6	0.60 $\pm$ 0.028	<10^-5
$\lambda$ 5730.34	124.0	11.61 $\pm$ 0.29	236.7 $\pm$ 45.0	0.60 $\pm$ 0.026	<10^-5
	11 Aug. 1998
$\lambda$ 5069.43	127.7	11.28 $\pm$ 0.38	215.5 $\pm$ 40.8	0.32 $\pm$ 0.030	4.4 $\times$ 10^-4
$\lambda$ 5104.44	125.2	11.50 $\pm$ 0.91	68.5 $\pm$ 27.8	0.32 $\pm$ 0.062	0.85 (0.075)
$\lambda$ 5373.01	124.6	11.56 $\pm$ 0.42	301.3 $\pm$ 63.1	0.55 $\pm$ 0.033	2.7 $\times$ 10^-3
$\lambda$ 5471.40	124.8	11.54 $\pm$ 0.18	398.0 $\pm$ 43.9	0.55 $\pm$ 0.016	<10^-5
$\lambda$ 5730.34	122.1	11.79 $\pm$ 0.59	112.6 $\pm$ 30.6	0.64 $\pm$ 0.042	0.19 (0.01)
	13 Aug. 1998
$\lambda$ 5069.43	125.1	11.51 $\pm$ 0.72	99.6 $\pm$ 47.6	0.37 $\pm$ 0.079	0.96 (0.08)
$\lambda$ 5104.44	125.1	11.51 $\pm$ 0.56	92.0 $\pm$ 30.0	0.31 $\pm$ 0.075	0.41 (0.012)
$\lambda$ 5373.01	122.3	11.77 $\pm$ 0.90	121.0 $\pm$ 41.2	0.60 $\pm$ 0.049	0.55 (0.014)
$\lambda$ 5471.40	125.2	11.50 $\pm$ 0.32	199.0 $\pm$ 40.0	0.54 $\pm$ 0.032	2.7 $\times$ 10^-4
$\lambda$ 5730.34	126.3	11.40 $\pm$ 0.40	82.9 $\pm$ 24.4	0.55 $\pm$ 0.046	0.21 (0.004)

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