Table 4
Example of the content of the input file STARNAME_PID_III.X-JJJJ_MJD_nnnnn.mmm: here we consider HD190073_PID_081.C-0410_MJD_54609.411 (the file structure is explained in the text).
| FORS1.2008-05-23T09:36:34.552.fits | 180 | 315.0 | 1/8 | 200176637 |
| FORS1.2008-05-23T09:41:07.012.fits | 200 | 45.0 | 2/8 | 200176637 |
| FORS1.2008-05-23T09:45:27.830.fits | 250 | 45.0 | 3/8 | 200176637 |
| FORS1.2008-05-23T09:51:10.408.fits | 250 | 315.0 | 4/8 | 200176637 |
| FORS1.2008-05-23T09:56:21.302.fits | 250 | 315.0 | 5/8 | 200176637 |
| FORS1.2008-05-23T10:02:03.889.fits | 250 | 45.0 | 6/8 | 200176637 |
| GRIS_600B 0.40 1797 | ||||
| Norma III 4136 × 40961 × 1 200Kps/low_gain | ||||
Notes. From the file list one can infer that last two exposures of the observing series have been dropped (either because the observing series was interrupted, or because the frames were discarded due to some problem, e.g. saturation).
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