Table A.1.
Sources characterized with a redshift in our VLT/MUSE survey (extract).
| ID | Object | RA | DEC | Impact Parameter | rAB | Mr | z | class | reliability | |
|---|---|---|---|---|---|---|---|---|---|---|
| J2000 | J2000 | (arcsec) | (kpc) | |||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| 1 | J161938.98+254318.7 | 244.91242 | 25.72186 | 22 | - | 18.6 | - | 0.0000 | Star | a |
| 2 | J161939.97+254330.2 | 244.91654 | 25.72506 | 9 | - | 17.7 | - | 0.0000 | Star | a |
| 3 | J161939.31+254247.9 | 244.91379 | 25.71331 | 41 | - | 24.3 | - | 0.0000 | Star | a |
| 4 | J161943.25+254351.5 | 244.93021 | 25.73097 | 45 | - | 22.0 | - | 0.0000 | Star | a |
| 5 | J161941.26+254353.0 | 244.92192 | 25.73139 | 29 | - | 21.0 | - | 0.0000 | Star | a |
| 6 | J161942.90+254324.2 | 244.92875 | 25.72339 | 32 | - | 23.1 | - | 0.0000 | Star | a |
| 7 | J161942.22+254324.9 | 244.92592 | 25.72358 | 23 | - | 20.7 | - | 0.0000 | Star | a |
| 8 | J161940.07+254315.6 | 244.91696 | 25.72100 | 12 | - | 21.5 | - | 0.0000 | Star | a |
| 9 | J161937.79+254401.3 | 244.90746 | 25.73369 | 52 | - | 24.4 | - | 0.0000 | Star | a |
| 10 | J161943.46+254344.9 | 244.93108 | 25.72914 | 44 | - | 19.0 | - | 0.0000 | Star | a |
| 11 | J161937.77+254333.0 | 244.90737 | 25.72583 | 38 | 74 | 23.2 | -15.5 | 0.1016 | SF | b |
| 12 | J161939.24+254336.1 | 244.91350 | 25.72669 | 21 | 47 | 18.0 | -21.2 | 0.1248 | non-SF | a |
| 13 | J161937.79+254254.9 | 244.90746 | 25.71525 | 48 | 128 | 23.1 | -16.1 | 0.1456 | SF | b |
| 14* | J161938.25+254321.0 | 244.90937 | 25.72250 | 31 | 103 | 18.8 | -21.6 | 0.1891 | non-SF | a |
| 15 | J161940.53+254325.6 | 244.91887 | 25.72378 | 0 | 0 | 16.3 | -24.5 | 0.2685 | QSO | a⊥ |
Notes. The full list of 40 sources is available in the VizieR (CDS) database. (⊥): Redmonster did not converge to a z on these sources; redshifts were assigned by a visual inspection. (*): Nearby galaxy to a reported BLA. Sources were classified according to their spectral type. SF galaxies show strong emission lines and a blue continuum and non-SF galaxies show a strong red continuum and an absence of emission lines. Columns (5) and (6) shows the impact parameter of each source to the QSO sight-line, in arcseconds and kiloparsecs, respectively. Sources where r is undefined were not detected by SExtractor and we used MUSELET to identify them and include them in the survey. The uncertainties in the redshift measurements in the column (9) are of the order of ∼0.0001.
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