Study of a sample of faint Be stars in the exofield of CoRoT - II. Pulsation and outburst events: Time series analysis of photometric variations

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Volume 613 (May 2018)

A&A, 613 (2018) A70

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Table 1

Some basic characteristics of the CoRoT data.

CoRoT ID	No	V	Run	t_o	Pts.	Sampl.	Δ T	Δf	N_f	A_min	Cross references to sections,
		mag					d	c d⁻¹		ppm	figures and tables
CoRoT 101486436	1	12.33	LRC1	2691.75311	25596	S1	152.007	0.0016	74	39	Sect. 8.1.1; Sect. B.1; Fig. 2; Fig. 31; Table 7
CoRoT 102595654	2	13.82	LRA1	2852.43938	21415	S1	131.463	0.0019	10	81	Sect. B.2; Fig. 10; Table 8
CoRoT 102656190	4	13.89	LRA1	2852.43932	22034	S1	131.463	0.0019	95	71	Sect. 8.1.2; Sect. B.3; Fig. 13; Table 9
CoRoT 102672979	5	11.47	LRA1	2852.43930	22034	S1	131.463	0.0019	48	94	Sect. 7.1; Sect. B.4; Fig. 4; Fig. 21; Fig. 22;
											Table 10
CoRoT 102686433	6	13.48	LRA1	2852.43929	22034	S1	131.463	0.0019	84	153	Sect. 8.2.1; Sect. 8.2.1; Sect. 7.2; Sect. B.5;
											Fig. 3; Fig. 23; Fig. 24; Fig. 32; Table 11
CoRoT 102719279	9	14.07	IR1	2590.05584	86563	S1, S2	57.446	0.0044	24	1769	Sect. B.6; Fig. 6; Fig. 25; Table 12
			LRA1	2852.43929	22034	S1	131.463	0.0019	64	941	Sect. 8.2.2; Sect. 7.3; Sect. B.6; Fig. 6;
											Fig. 25; Fig. 26; Fig. 27; Table 12
			LRA6	4394.27693	206592	S2	76.618	0.0032	42	805	Fig. 7; Fig. B.1, Fig. B.2, Fig. B.3, Table 13
CoRoT 102725623	11	15.17	IR1	2590.05583	9662	S1	57.441	0.0044	2	273	Sect. B.7; Fig. 11; Table 14
			LRA1	2852.43927	22034	S1	131.463	0.0019	8	186	Sect. B.7; Fig. 11; Table 14
CoRoT 102728404	12	11.93	LRA1	2852.43930	338782	S2	131.462	0.0019	62	112	Sect. B.8; Fig. B.4; Table 15
CoRoT 102766835	14	13.20	IR1	2590.05585	9662	S1	57.441	0.0044	23	710	Sect. B.9; Fig. 8; Table 16
			LRA1	2853.94531	348702	S2	131.462	0.0019	68	411	Sect. 8.3.1; Sect. B.9; Fig. 8; Table 16
CoRoT 102785204	16	12.06	LRA1	2853.94533	338782	S2	131.462	0.0019	30	622	Sect. B.10; Fig. B.5; Table 17
CoRoT 102785480	17	12.90	LRA1	2853.94534	338782	S2	131.462	0.0019	114	199	Sect. 8.2.3; Sect. B.11;Fig. 9; Fig. 28;
											Fig. 29; Table 18
CoRoT 102825808	18	14.42	IR1	2590.05587	9662	S1	57.441	0.0044	44	135	Sect. B.12; Fig. 12; Table 19
CoRoT 102829773	19	15.21	IR1	2593.07642	9178	S1	54.421	0.0046	26	194	Sect. B.13; Fig. B.6; Table 20
CoRoT 102847615	20	13.87	IR1	2593.18500	147021	S1	54.315	0.0046	7	99	Sect. B.14; Fig. B.7; Table 21
CoRoT 102904910	22	14.02	IR1	2590.05590	9662	S1	57.441	0.0044	32	181	Sect. B.15; Fig. 5; Fig. 30; Table 22

Notes. No = sequence number in Table 1 of Paper I; t_o = CoRoT time of phase 0 (heliocentric JD with origin on 01/01/2000 at 12h00 UT); Pts. = number of data points; Sampl. = sampling: S1 = 512 sec., S2 = 32 sec.; Δ T = total duration of CoRoT observations; Δf = 1∕4ΔT frequency accuracy; N_f = number of identified frequencies; A_min is the lower amplitude detected in ppm units; d = days.

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