Table A.1
Epoch of the VLT/UVES observations and the adopted instrument setups.
UT date | Age | UT start | Exptime | Inst. setup | Slit | R |
---|---|---|---|---|---|---|
(d) | (h) | (s) | (″) | |||
2017/08/17 | 56 | 01:59 | 1000 | DIC1 346+564 | 0.4/0.3 | 65000/95-100000 |
2017/08/17 | 56 | 02:21 | 500 | DIC2 437+760 | 0.4/0.3 | 65000/95-100000 |
2017/08/23 | 64 | 02:20 | 1100 | DIC1 346+564 | 0.8 | 60000 |
2017/08/23 | 64 | 02:43 | 400/300 | DIC2 437+760 | 0.8 | 60000 |
2017/09/17 | 89 | 01:24 | 1100 | DIC1 346+564 | 0.8 | 60000 |
2017/09/17 | 89 | 01:51 | 400 | DIC2 437+760 | 0.8 | 60000 |
2017/10/30 | 132 | 00:34 | 1100 | DIC1 346+564 | 0.4/0.3 | 65000/95-100000 |
2017/10/30 | 132 | 00:59 | 400 | DIC2 437+760 | 0.4/0.3 | 65000/95-100000 |
Notes. In all cases the CCD readout was “fast readout,” “low gain,” and un-binned. In Cols. 4, 6, and 7, whenever two values are given, the first refers to the blue arm and the second to the red arm. The resolving power (R) of the red arm also depends on the CCD, within the 2 CCD mosaic (e.g., 95 000 and 100 000).
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