MOST observations of the young open cluster NGC 2264

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Volume 502 / No 1 (July IV 2009)

A&A, 502 1 (2009) 239-252

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Table 6:

Pulsation frequencies, amplitudes, S IGS PEC significances (sig) and signal-to-noise values (S/N) of the four new candidate PMS pulsators obtained with S IGS PEC and P ERIOD04 where the respective last digit frequency errors calculated according to Kallinger et al. (2008c) are given in parentheses.
Var ID	#	freq		amp	sig	S/N
		[c/d]	[ $\mu$ Hz]	[mmag]
V1	f1	19.60(1)	226.8(1)	2.802	17.10	6.7
	f2	10.93(1)	126.5(1)	2.792	14.38	4.0
	f3	12.03(1)	139.2(1)	2.680	15.57	4.7
	f4	9.80(2)	113.3(2)	1.788	7.63	4.0
	f5	21.03(2)	243.3(2)	1.764	7.54	4.5
	f6	16.80(2)	194.3(2)	1.717	7.22	4.1
	f7	13.56(2)	156.9(2)	1.684	6.92	4.0
V2	f1	61.497(4)	711.52(5)	14.689	127.90	18.6
	f2	58.030(5)	671.41(6)	10.751	68.61	9.8
V3	f1	34.706(4)	401.55(5)	3.705	100.36	11.4
	f2	21.59(2)	249.8(2)	0.999	7.84	3.8
	f3	34.38(2)	397.7(2)	0.872	5.84	4.4
	f4	68.34(2)	790.7(2)	0.830	5.55	4.0
V4	f1	35.216(4)	407.45(5)	9.463	104.19	16.1
	f2	32.912(9)	380.8(1)	4.566	26.41	7.2
	f3	32.612(9)	377.3(1)	4.494	23.26	6.6

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