Table 2.
Variability properties of the extragalactic FXT candidates detected and/or discussed in this work obtained by the G–L method, ordered by subsample and date.
| FXT | Odds ratio | Prob. | Var. index |
|---|---|---|---|
| (1) | (2) | (3) | (4) |
| 15 | 10.18 | 0.99 | 9 |
| 16 | 93.73 | 1.0 | 10 |
| 17 | 9.09 | 0.99 | 8 |
| 18 | 8.67 | 0.99 | 8 |
| 19 | 167.0 | 1.0 | 10 |
| 20 | 34.47 | 1.0 | 10 |
| 21 | 6.19 | 0.99 | 8 |
| 22 | 29.56 | 1.0 | 9 |
Notes. Column 1: shorthand identifier (FXT #) used throughout this work. Column 2: logarithmic odds ratio (ratio of obtaining the observed distribution versus obtaining a flat distribution) for variability signal. Column 3: variable signal probability (the probability that the flux calculated from the source region is not constant throughout the observation). Column 4: variability index (ratio of obtaining the observed distribution versus obtaining a flat distribution).
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