Table 1
Summary of the ESPRESSO observations.
# | Calendar | UT obs. | Texp | Nobs (in/out) | Airmass (a) | S∕N (b) | Telescope | PID (c) | ||
---|---|---|---|---|---|---|---|---|---|---|
night | window | [s] | Continuum (d) | Na core | Hα core | |||||
1 | 2018-10-31 | 00:51–04:37 | 500 | 24 (13/11) | 1.21–1.20–1.98 | 34–46 | 2–7 | 13–19 | VLT-UT3 | i |
2 | 2018-11-07 | 00:05–04:24 | 800 | 18 (9/9) | 1.22–1.20–2.17 | 38–57 | 3–10 | 15–24 | VLT-UT3 | ii |
3 | 2018-11-14 | 00:23–04:13 | 800 | 16 (8/8) | 1.20–1.20–2.46 | 37–61 | 4–10 | 15–26 | VLT-UT2 | ii |
Notes. (a) First and third values refer to the airmass at the beginning and at the end of the observation. The second value gives the minimum airmass. (b) The two figures correspond to the minimum and maximum S/N, respectively. (c) PID i and ii refer to ESO programs 0102.D-0789 (PI: H. Cegla) and 0102.C-0493 (PI: G. Chen), respectively. (d) The signal-to-noise ratio (S/N) of the continuum was measured at around 590 nm.
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