Table A.3.
Derived line parameters from our optical spectra.
| Candidate | Spectral features | Observed wavelength (Å) | Redshift |
|---|---|---|---|
| 59 | CIV | 5015.26 ± 1.26 | 2.238 ± 0.001 |
| CIII | 6164.46 ± 4.63 | 2.230 ± 0.002 | |
| 35 | MgII | 5600.17 ± 5.47 | 1.001 ± 0.002 |
| 06 | [OII] | 5013.71 ± 0.05 | 0.345 ± 0.001 |
| [NeIII] | 5204.39 ± 0.05 | 0.345 ± 0.001 | |
| Hβ | 6537.28 ± 0.03 | 0.344 ± 0.001 | |
| [OIII] | 6670.21 ± 0.06 | 0.345 ± 0.001 | |
| [OIII] | 6734.62 ± 0.02 | 0.345 ± 0.001 | |
| 47 | [OII] | 5341.68 ± 0.06 | 0.433 ± 0.001 |
| Hβ | 6957.91 ± 0.08 | 0.431 ± 0.001 | |
| [OIII] | 7098.02 ± 1.77 | 0.431 ± 0.001 | |
| [OIII] | 7169.62 ± 1.19 | 0.432 ± 0.001 | |
| 26 | MgII | 5546.48 ± 1.00 | 0.982 ± 0.001 |
| 18 | MgII | 5141.63 ± 0.74 | 0.837 ± 0.001 |
Notes. For the doublet [OII] that is unresolved in our data we adopted a rest wavelength of 3727.89 Å averaging the central wavelengths of the two components in 1:2 ratio, approximately proportional to the flux ratio of the two components. The wavelength and redshift errors reflect only random uncertainties.
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