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Table 1.
VLT/X-shooter observations used in this paper.
| Object | RA (J2000) | Dec (J2000) | Date | Exp. time (s) |
Seeing | Remarks | ||
|---|---|---|---|---|---|---|---|---|
| (hh:mm:ss.ss) | (dd:mm:ss.s) | (dd-mm-yyyy) | UVB | VIS | NIR | (″) | ||
| S1 | 05:38:31.62 | −69:02:14.6 | 30-11-2012 | 4 × 670 | 4 × 700 | 4 × 50 | 0.7 | |
| S1-SE | 05:38:32.25 | −69:02:14.0 | 30-11-2012 | 4 × 670 | 4 × 700 | 4 × 50 | 1.0 | |
| S2 | 05:38:33.09 | −69:06:11.7 | 28-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 1.2 | |
| S3 | 05:38:34.05 | −69:04:52.2 | 26-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 1.4 | |
| S3-K | 05:38:34.69 | −69:04:50.0 | 27-01-2013 | 4 × 700 | 8 × 330 | 4 × 50 | 2.1 | |
| S4 | 05:38:34.60 | −69:05:56.8 | 28-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 1.2 | |
| S5-A,B,C,D,E,F | 05:38:39.68 (1) | −69:05:37.9 (1) | 26-01-2013 | 4 × 700 | 8 × 330 | 4 × 50 | 0.8 | 6 objects on slit |
| S6 | 05:38:41.36 | −69:03:54.0 | 24-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 1.5 | |
| S7-A,B | 05:38:46.84 (2) | −69:05:05.4 (2) | 24-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 2.2 | 2 objects on slit |
| S8 | 05:38:48.17 | −69:04:11.7 | 28-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 0.8 | 2 unresolved objects |
| S9 | 05:38:49.27 | −69:04:44.4 | 24-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 1.5 | |
| S10-A,BC | 05:38:56.31 (3) | −69:04:16.1 (3) | 29-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 1.5 | S10-B&C unresolved |
| S10-K | 05:38:58.38 | −69:04:21.6 | 28-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 1.2 | |
| S10-SW-A,B | 05:38:52.72 (4) | −69:04:37.5 (4) | 28-01-2013 | 4 × 670 | 4 × 700 | 4 × 50 | 1.3 | 2 objects on slit |
| R135 | 05:38:33.62 | −69:04:50.4 | 14-01-2013 | 2 × 210 | 2 × 240 | 2 × 50 | 1.2 | Wolf-Rayet star |
Notes. All observations were carried out under ESO program 090.C-0346(A). The object names are the same as defined by Walborn et al. (2013), where we introduced additional letters if multiple or additional objects were identified on the X-shooter slit.
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