Table 2
Suitability of the single Keplerian model alone, i.e. assuming that no other sources of variability exist.
|
< 0.05 | < 0.01 | < 0.005 | < 0.001 |
|
|
||||
| No. of stars | 101 | 83 | 79 | 72 |
| Fraction | 54% | 44% | 42% | 39% |
| Confidence C | > 95% | > 99% | > 99.5% | > 99.9% |
Notes. Second row: number of stars for which the chi-square probability of the single Keplerian model is less than the values given in the first row. Third row: fraction of the 187 stars in our version 2 sample. Last row: confidence 
with which the single Keplerian model can be rejected.
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