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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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