Table 1.
Details of the MUSE observation of the HzRG sample.
| HzRG | Redshift | UT date | Program ID | Mode | Exp. time total | Seeing |
|---|---|---|---|---|---|---|
| z(†) | (dd/mm/yyyy) | hours | arcsec (*) | |||
| MRC 0943-242 | 2.9230 | 21/02/2014 | 60.A-9100(A) | WFM-NOAO-E | 5.21 | 0.65 (a) |
| – | – | 15/12/2015-18/01/2016 | 096.B-0752(A) | – | – | – |
| MRC 0316-257 | 3.1238 | 15/01-17/01/2015 | 094.B-0699(A) | WFM-NOAO-N | 4.24 | 0.61 (b) |
| TN J0205+2242 | 3.5060 | 03/12-08/12/2015 | 096.B-0752(B) | WFM-NOAO-N | 4.24 | 0.73 |
| TN J0121+1320 | 3.5190 | 06/10/2015 | 096.B-0752(C) | WFM-NOAO-N | 5.30 | 0.83 |
| – | – | 08/08-28/08/2016 | 097.B-0323(C) | – | – | – |
| 4C+03.24 | 3.5828 | 17/06-18/06/2017 | 60.A-9100(G) | WFM-AO-N | 1.25 | 0.63 |
| 4C+19.71 | 3.5892 | 08/06-02/09/2016 | 097.B-0323(B) | WFM-NOAO-N | 5.83 | 1.03 |
| TN J1338-1942 | 4.0959 | 30/04-06/05/2014 | 60.A-9100(B) | WFM-NOAO-N | 8.93 | 0.77 (a) |
| – | – | 30/06/2014 | 60.A-9318(A) | – | – | – |
| 4C+04.11 | 4.5077 | 03-15/12/2015 | 096.B-0752(F) | WFM-NOAO-N | 4.24 | 0.88 |
Notes.
The redshifts are determined from the He IIλ1640 Å or [C I](1-0) emission line (Kolwa et al. 2023). For MRC0316-257 which is not included in Kolwa et al. (2023), we reported its zsys in this paper based on He II fit from our MUSE data (Appendix E).
The seeing reported here is determined from the fitted 2D Moffat FWHM (full width at half maximum) of a star in the white-light image (5000 − 9000 Å) produced from the combined cube. We note that the stars used are red in colour, i.e. the image quality in the Lyα wavelength should in general be worse than the reported seeing (e.g. larger by 10 to 20%).
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