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Table 2.
Detected emission lines.
| Emission-line | EW0 | FWHM | Δv |
|---|---|---|---|
| [Å] | [km s−1] | [km s−1] | |
| Lyα | 62 ± 3 | 313 ± 24 | +195 ± 20 |
O I |
0.56 ± 0.09 | 140 ± 20 | 1 ± 18 |
Si II |
0.56 ± 0.08 | 140 ± 20 | −1 ± 20 |
C II |
0.68 ± 0.20 | 140 ± 20 | 0 ± 17 |
Si II |
0.66 ± 0.19 | 140 ± 20 | −2 ± 21 |
| C IV1548.19 |
 |
110 ± 40 | +51 ± 19 |
| C IV1550.77 |
 |
110 ± 40 | +51 ± 19 |
Notes. Properties of the emission lines detected in the integrated MUSE spectrum of ID53. Δv lists the velocity offset with respect to the systemic redshift of zsys = 4.7745 ± 0.0004. The Lyα flux and width are obtained from Leclercq et al. (2017).
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