Table 2
Journal of the observations.
| UVB arm | VIS arm | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| Object | MJD | texp | S/N | MJD | texp | S/N | Flux STD | Δt | Comment |
| (s) | (s) | (d) | |||||||
| 2DFS-163 | 59150.059 | 1655 | 139 | 59150.059 | 1725 | 78 | LTT3218 | −0.3 | |
| 59150.078 | 1655 | 166 | 59150.078 | 1725 | 70 | LTT3218 | −0.3 | ||
| 2DFS-999 | 59157.207 | 1655 | 112 | 59157.207 | 1725 | 71 | LTT7987 | +0.2 | |
| 59157.227 | 1655 | 106 | 59157.227 | 1725 | 64 | LTT7987 | +0.2 | ||
| 2DFS-2266 | 59179.160 | 1655 | 125 | 59179.160 | 1725 | 72 | GD 71 | −0.1 | |
| 59179.180 | 1655 | 129 | 59179.180 | 1725 | 73 | GD 71 | −0.1 | ||
| 2DFS-2553 | 59161.117 | 1655 | 141 | 59161.117 | 1725 | 70 | LTT3218 | −0.2 | |
| 59161.160 | 1655 | 145 | 59161.160 | 1725 | 84 | LTT3218 | −0.2 | ||
| 2DFS-3689 | 59186.145 | 1960 | 145 | 59186.145 | 2030 | 63 | FEIGE110 | +0.1 | |
| 59186.168 | 1960 | 115 | 59186.168 | 2030 | 60 | FEIGE110 | +0.1 | ||
| 59400.316 | 1960 | 78 | 59400.316 | 2030 | 45 | EG274 | +0.2 | ||
| 59400.340 | 1960 | 72 | 59400.340 | 2030 | 49 | EG274 | +0.3 | ||
| 2DFS-3694 | 59147.297 | 1200 | 211 | 59147.297 | 1270 | 106 | LTT3218 | −1.1 | |
| 2DFS-3780 | 59195.172 | 1050 | 165 | 59195.172 | 1120 | 103 | FEIGE110 | +0.2 | |
| 59195.188 | 1050 | 154 | 59195.188 | 1120 | 87 | FEIGE110 | +0.2 | ||
| 2DFS-3947 | 59175.199 | 1655 | 147 | 59175.199 | 1725 | 83 | EG21 | +0.1 | |
| 59175.219 | 1655 | 154 | 59175.219 | 1725 | 82 | EG21 | +0.1 | ||
| 2DFS-3954 | 59174.191 | 1960 | 153 | 59174.191 | 2030 | 70 | FEIGE110 | +0.2 | |
| 59174.215 | 1960 | 162 | 59174.215 | 2030 | 90 | FEIGE110 | +0.2 | ||
Notes. The first column gives the target name. Columns 2–4 give the modified Julian date (MJD) at the start of the exposure, the exposure time and the (per pixel) S/N computed in the continuum (see Sect. 4.6) for the UVB arm of the rebin individual spectra (Δλ = 0.02 nm; see Sect. 4.5). Columns 5 to 7 give the same information for the VIS arm. Columns 8 and 9 provide the name of the FLUX standard star used to calibrate the response curve and the time difference (Δt) between the start of the SCIENCE and FLUX observations. The last column contains a flag for additional comments provided in the online version of the table. The full table is available at CDS.
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