Table 2.
Emission line parameters.
| Line | z | FWHM | L |
|---|---|---|---|
| (km s−1) | (1044 erg s−1) | ||
| Hβ, comp 1 | 2.6252 | 5700 ± 430 | 0.9 |
| Hβ, comp 2 | 2.6273 | 1960 ± 150 | 0.5 |
| [O III]λ5008, broad | 2.6233 | 1600 ± 60 | 1.1 |
| [O III]λ5008, narrow | 2.6309 | 630 ± 50 | 0.6 |
| [O II] | 2.6310 | 950 ± 80 | 0.15 |
| C IV, comp 1 | 2.6149 | 5620 ± 170 | 1.3 |
| C IV, comp 2 | 2.6221 | 2050 ± 50 | 0.6 |
| Leaking Lyα | 2.634 | 600 | 1.4 |
Notes. The apparent peak and FWHM of the leaking Ly-α emission were estimated visually from the non-Gaussian spectral profile and the luminosity from direct integration. For the other lines, these parameters were obtained from fitting the Gaussian profiles as described in the text. Statistical uncertainties on the line luminosities are about 10% for NIR lines and 5% for UVB lines. However, the uncertainty on the absolute flux calibration is about 20%. This has no effect on the line ratios.
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