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Table 1.

Observational data.

Date range PI VLT Instrument Setup Slit (a) Binning Ttot(b) IQ (c) R(d)
[″] [s] [″] [×103]
09–28/11/2018 Ledoux UT3 ESPRESSO SingleUT-HR ... 2 × 1 24 110 0.89 132.0/146.0

21–26/08/2017 Bergeron UT2 UVES B390+R564 0.8 1 × 1 21 000 0.83 58.8/59.4/58.3
21–24/09/2009 Molaro UT2 UVES B390+R580 0.7 1 × 1 33 870 0.92 64.8/73.4/65.5
20/09/2009 Molaro UT2 UVES B437+R760 0.7 1 × 1 16 200 0.78 64.9/72.5/67.3
22/09/2009 Molaro UT2 UVES (B420+)R700 0.7 1 × 1 15 000 1.18 (...)/72.5/67.3
29/06/2001 Bergeron UT2 UVES B437+R860 1.0 2 × 2 3 600 0.53 60.3/57.3/56.1
15–24/08/2001 Bergeron UT2 UVES B437+R860 1.0 2 × 2 18 000 0.87 48.1/48.7/45.7
16–24/08/2001 Bergeron UT2 UVES B346+R580 1.0 2 × 2 21 600 0.55 58.6/66.3/59.3

Notes.

(a)

Slit width.

(b)

Total on-source exposure time.

(c)

Image Quality from the Shack-Hartmann sensor of the VLT active optics at 650 nm at the airmass of observations.

(d)

Resolving power measured from emission lines in ThAr calibration frames. The listed values correspond to the Blue and Red arm spectra, respectively, for ESPRESSO, and to the Blue, Lower-Red, and Upper-Red spectra for UVES. For the latter instrument, the effect of an IQ smaller than the slit width in some cases is taken into account.

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