ATLAS Fields observed by 2dF. For the NGC-F2A data in the bottom row, the blue and red arm of the spectra were reduced and analysed separately. Here we show what fields were observed, for how long, the seeing on each field, and what percentage of the data we were able to make spectroscopic QSO IDs on.
| Field . | RA (deg) . | Dec (deg) . | Date . | Exposure . | Seeing . | IDs . | Total Exp. . | Comments . |
|---|---|---|---|---|---|---|---|---|
| NGC-F1 | 196.9 | −16.0 | 18/2/2021 | 1 × 30 min + 4 × 20 min | 2|${^{\prime\prime}_{.}}$|1 | – | – | – |
| NGC-F1 | 196.9 | −16.0 | 09/3/2021 | 1 × 25 min + 2 × 30 min | 1|${^{\prime\prime}_{.}}$|4 | – | – | – |
| NGC-F1 | 196.9 | −16.0 | 15/3/2021 | 3 × 30 min | 4|${^{\prime\prime}_{.}}$|0 | 66.8 per cent | 4.75 h | – |
| NGC-F2 | 211.6 | −16.0 | 09/3/2021 | 18.3 + 25 + 15.3 min | 1|${^{\prime\prime}_{.}}$|5 | 60.2 per cent | – | – |
| NGC-F2 | 211.6 | −16.0 | 15/3/2021 | 3 × 25 min | 4|${^{\prime\prime}_{.}}$|0 | 35 (54) per cent | 2.25 h | – |
| NGC-F2A | 211.6 | −16.0 | 07/4/2021 | 4 × 20 min | 2|${^{\prime\prime}_{.}}$|5 | 43 per cent | 1.33 h | Moon |
| Field . | RA (deg) . | Dec (deg) . | Date . | Exposure . | Seeing . | IDs . | Total Exp. . | Comments . |
|---|---|---|---|---|---|---|---|---|
| NGC-F1 | 196.9 | −16.0 | 18/2/2021 | 1 × 30 min + 4 × 20 min | 2|${^{\prime\prime}_{.}}$|1 | – | – | – |
| NGC-F1 | 196.9 | −16.0 | 09/3/2021 | 1 × 25 min + 2 × 30 min | 1|${^{\prime\prime}_{.}}$|4 | – | – | – |
| NGC-F1 | 196.9 | −16.0 | 15/3/2021 | 3 × 30 min | 4|${^{\prime\prime}_{.}}$|0 | 66.8 per cent | 4.75 h | – |
| NGC-F2 | 211.6 | −16.0 | 09/3/2021 | 18.3 + 25 + 15.3 min | 1|${^{\prime\prime}_{.}}$|5 | 60.2 per cent | – | – |
| NGC-F2 | 211.6 | −16.0 | 15/3/2021 | 3 × 25 min | 4|${^{\prime\prime}_{.}}$|0 | 35 (54) per cent | 2.25 h | – |
| NGC-F2A | 211.6 | −16.0 | 07/4/2021 | 4 × 20 min | 2|${^{\prime\prime}_{.}}$|5 | 43 per cent | 1.33 h | Moon |
ATLAS Fields observed by 2dF. For the NGC-F2A data in the bottom row, the blue and red arm of the spectra were reduced and analysed separately. Here we show what fields were observed, for how long, the seeing on each field, and what percentage of the data we were able to make spectroscopic QSO IDs on.
| Field . | RA (deg) . | Dec (deg) . | Date . | Exposure . | Seeing . | IDs . | Total Exp. . | Comments . |
|---|---|---|---|---|---|---|---|---|
| NGC-F1 | 196.9 | −16.0 | 18/2/2021 | 1 × 30 min + 4 × 20 min | 2|${^{\prime\prime}_{.}}$|1 | – | – | – |
| NGC-F1 | 196.9 | −16.0 | 09/3/2021 | 1 × 25 min + 2 × 30 min | 1|${^{\prime\prime}_{.}}$|4 | – | – | – |
| NGC-F1 | 196.9 | −16.0 | 15/3/2021 | 3 × 30 min | 4|${^{\prime\prime}_{.}}$|0 | 66.8 per cent | 4.75 h | – |
| NGC-F2 | 211.6 | −16.0 | 09/3/2021 | 18.3 + 25 + 15.3 min | 1|${^{\prime\prime}_{.}}$|5 | 60.2 per cent | – | – |
| NGC-F2 | 211.6 | −16.0 | 15/3/2021 | 3 × 25 min | 4|${^{\prime\prime}_{.}}$|0 | 35 (54) per cent | 2.25 h | – |
| NGC-F2A | 211.6 | −16.0 | 07/4/2021 | 4 × 20 min | 2|${^{\prime\prime}_{.}}$|5 | 43 per cent | 1.33 h | Moon |
| Field . | RA (deg) . | Dec (deg) . | Date . | Exposure . | Seeing . | IDs . | Total Exp. . | Comments . |
|---|---|---|---|---|---|---|---|---|
| NGC-F1 | 196.9 | −16.0 | 18/2/2021 | 1 × 30 min + 4 × 20 min | 2|${^{\prime\prime}_{.}}$|1 | – | – | – |
| NGC-F1 | 196.9 | −16.0 | 09/3/2021 | 1 × 25 min + 2 × 30 min | 1|${^{\prime\prime}_{.}}$|4 | – | – | – |
| NGC-F1 | 196.9 | −16.0 | 15/3/2021 | 3 × 30 min | 4|${^{\prime\prime}_{.}}$|0 | 66.8 per cent | 4.75 h | – |
| NGC-F2 | 211.6 | −16.0 | 09/3/2021 | 18.3 + 25 + 15.3 min | 1|${^{\prime\prime}_{.}}$|5 | 60.2 per cent | – | – |
| NGC-F2 | 211.6 | −16.0 | 15/3/2021 | 3 × 25 min | 4|${^{\prime\prime}_{.}}$|0 | 35 (54) per cent | 2.25 h | – |
| NGC-F2A | 211.6 | −16.0 | 07/4/2021 | 4 × 20 min | 2|${^{\prime\prime}_{.}}$|5 | 43 per cent | 1.33 h | Moon |
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