Impact of gaps in the asteroseismic characterization of pulsating stars - I. The efficiency of pre-whitening

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Volume 614 (June 2018)

A&A, 614 (2018) A40

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Table 2

Statistical parameters of the gap distribution for the light curves observed by CoRoT used in this paper.

Star ID	Duty cycle (%)	(h)	(h)	σ(τ_g) (h)	Mode (h)






HD50844	88.69	1.751	0.173	0.126	0.266
HD174936	88.83	0.409	0.162	0.116	0.267
HD174966	89.55	0.409	0.175	0.099	0.267
HD181555	88.95	2.516	0.175	0.125	0.267
HD49434	88.44	13.858	0.182	0.359	0.258
HD172189	89.07	7.031	0.079	0.162	0.009
HD174532	87.18	5.280	0.072	0.265	0.009
HD174589	87.22	5.289	0.072	0.266	0.009
HD51722	89.30	3.476	0.106	0.150	0.009
HD51359	88.90	3.476	0.094	0.138	0.009
HD50870	89.78	3.476	0.102	0.142	0.009
HD170699	88.46	4.044	0.067	0.139	0.009
GSC00144–03031	88.46	7.636	0.066	0.227	0.009
HD41641	78.78	144.249	0.119	2.552	0.009
HD48784	88.55	1.582	0.161	0.137	0.267

Notes. In columns 3–5, τ_g refers to theduration of the gaps in hours, where column 3 is the maximum, column 4 is the mean duration, column 5 is the standard deviation of the gap distribution, and the last column is the most frequent gap duration.

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