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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(τg) (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, τg 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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