A survey for pulsating subdwarf B stars with the Nordic Optical Telescope

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Table 6:

Details from the discovery runs for the four new sdBVs.
Target	Run	N_p	$\Delta t$	$\sigma$	$A_{\rm max}$
	ID		s	mma	mma
HE 2151-1001	S2	120	30	0.58	2.20
	S3	73	30	1.05	2.35
HS 2125+1105	S2	67	35	1.75	6.45
	ST	95	30	0.95	3.56
	S3	116	42	0.72	3.42
	S3	433	30	0.40	4.35
	S3	541	30	0.33	3.84
	S4	89	28	1.17	4.76
PG 1033+201	T7	118	20	1.01	4.95
HE 1450-0957	S6	125	30	0.90	6.81

Notes. ``Run ID'' refers to the identifiers listed in Table 1, $N_{\rm p}$ is the number of points for the specific sequence, $\Delta t$ is the sampling time interval, $\sigma$ is the mean noise level in the FT, and $A_{\rm max}$ is the amplitude of the highest peak.

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