Table 3
First lines of the online material fits file, reporting the catalog of candidate flares.
| OBS_ID | SRC_NUM | RA | Dec | ST_FLARE | PROB |
|---|---|---|---|---|---|
| 0000110101 | 1 | 64.926 | 55.999 | F | 0.0006 |
| 0000110101 | 6 | 64.996 | 56.225 | F | 0.0002 |
| 0001730201 | 1 | 263.677 | –32.582 | F | 0.02 |
| 0001730201 | 9 | 263.649 | –32.596 | T | 0.99 |
Notes. OBS_ID is the observation identifier of the XMM-Newton observation and SRC_NUM the source number; these two parameters define the “name” of the source. Then, we report the fk5 celestial coordinates, in degrees (RA, Dec). The last two colums are the results of our model: ST_FLARE show if the source is predicted to be a flare, on the basis of the threshold of 0.5 on the resulting probability, PROB.
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