Table 1.
Main characteristics of MUSE observations.
| FoV | Seeing | Integration(h) | RA (J2000) | Dec (J2000) | ESO programme | |
|---|---|---|---|---|---|---|
| A1689 | 1′ × 1′ | 0.9″−1.1″ | 1.8 | 197°52′39″ | −1°20′42″ | 60.A-9100(A) |
| A2390 | 1′ × 1′ | 0.75″ | 2 | 328°23′53″ | 17°41′48″ | 094.A-0115(B) |
| A2667 | 1′ × 1′ | 0.62″ | 2 | 357°54′50″ | −26°05′03″ | 094.A-0115(A) |
| A2744 (a) | 2′ × 2′ | 0.58″ | 16.5 | 3°35′14″ | −30°23′54″ | 094.A-0115(B) |
| A2744 (b) | 1′ × 1′ | 0.58″ | 2 | 3°35′14″ | −30°23′54″ | 094.A-0115(B) |
Notes. The A2744 field was splitted in two (part a and part b) because of the additional pointing covering the centre of the 2 × 2 MUSE mosaic. For A1689 and A2390, the seeing was measured on the white light image obtained from the final datacube. For A2667 and A2744, the seeing was obtained by fitting a MUSE reconstructed F814W image with a seeing convolved HST F814W image (see Patricio et al. 2018 for A2667 and Mahler et al. 2018 for A2744).
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