Table 2.
Summary of MUSE observations analysed on the 12 clusters.
| Cluster | Prog. ID | Obs. date | Exp. time (Mode) | PSF | Teff | Notes |
|---|---|---|---|---|---|---|
| [UT] | [s] | ″ | [h] | |||
| A2744 | 094.A-0115, 095.A-0181, | 2014-09-21 – 2015-11-09 | 40 × 1800 (NOAO) | 0.61 | 3.5–7 | 2 × 2 mosaic |
| 096.A-0496 | ||||||
| A370 | 094.A-0115, 096.A-0710 | 2014-11-20 – 2016-09-28 | 4 × 1800 (NOAO) | 0.66 | 1.5–8.5 | 2 × 2 mosaic |
| 37 × 962 (NOAO) | ||||||
| 24 × 930 (NOAO) | ||||||
| 3 × 953 (NOAO) | ||||||
| MACS0257 | 099.A-0292, 0100.A-0249, | 2017-09-20 – 2019-09-28 | 6 × 1000 (NOAO) | 0.52 | 8 | |
| 0103.A-0157 | 24 × 1000 (AO) | |||||
| MACS0329 | 096.A-0105 | 2016-01-09 – 2016-01-29 | 6 × 1447 (NOAO) | 0.69 | 2.5 | |
| MACS0416 (N) | 094.A-0115, 0100.A-0763 | 2014-12-17 – 2019-03-04 | 4 × 1800 (NOAO) | 0.53 | 17 | |
| 6 × 1670 (NOAO) | ||||||
| 27 × 1670 (AO) | ||||||
| MACS0416 (S) | 094.A-0525 | 2014-10-02 – 2015-02-24 | 50 × 700 (NOAO) | 0.65 | 11–15 | |
| 8 × 667 (NOAO) | ||||||
| Bullet | 094.A-0115 | 2014-12-18 | 4 × 1800 (NOAO) (a) | 0.56 | 2 | |
| MACS0940 | 098.A-0502, 098.A-0502, | 2017-01-30 – 2018-05-13 | 3 × 1000 (NOAO) | 0.57 | 8 | |
| 0101.A-0506 | 30 × 900 (AO) (b) | |||||
| MACS1206 | 095.A-0181, 097.A-0269 | 2015-04-15 – 2016-04-09 | 26 × 1800 (NOAO) (c) | 0.52 | 4–9 | 3 × 1 mosaic |
| RXJ1347 | 095.A-0525, 097.A-0909 | 2015-07-16 – 2018-03-21 | 8 × 1475 (NOAO) | 0.55 | 2–3 | 2 × 2 mosaic |
| 18 × 1345 (AO) | ||||||
| SMACS2031 | 60.A-9100 (d) | 2014-04-30 – 2014-05-07 | 33 × 1200 (NOAO) | 0.79 | 10 | |
| SMACS2131 | 0101.A-0506, 0102.A-0135, | 2018-08-13 – 2019-09-30 | 30 × 900 (AO) | 0.59 | 7 | |
| 0103.A-0157 | ||||||
| MACS2214 | 099.A-0292,0101.A-0506, | 2017-09-21 – 2019-10-22 | 3 × 1000 (NOAO) | 0.55 | 7 | |
| 0103.A-0157, 0104.A-0489 | 27 × 900 (AO) |
Notes. It is important to note that the two datasets on MACS0416 cluster (N)orth and (S)outh have been treated separately. From left to right: MUSE dataset, ESO Programs, range of observing dates, list of exposure times and instrument modes, final image quality of the combined datacube (FWHM at 700 nm), range of effective exposure time per spaxel, notes on multiple pointings (see also Fig. 1).
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