Table 2.
Emission line properties of the QSO as constrained from our best fit of the spectrum (Fig. 5).
| Kinematics | |||
|---|---|---|---|
| Δv [km s−1]a | σ [km s−1] | ||
| BLR | −410 ± 40 | 4160 ± 60 | |
| Narrow | −240 ± 20 | 660 ± 30 | |
| Outflow | −1420 ± 120 | 1360 ± 80 | |
| Emission line fluxesb | |||
| Line | BLR | Narrowc | Outflowc |
| Hβ | 220 ± 10 | 50 ± 4 | 40 ± 5 |
| [O III] | – | 8 ± 3 | 20 ± 4 |
| Hα | 520 ± 20 | 180 ± 30 | 130 ± 20 |
| [N II] | – | 72 ± 15 | 160 ± 50 |
Notes. The top table reports the velocity shift and velocity dispersion of the emission lines, while their fluxes are reported in the bottom table. aRelative to z = 4.6943 (Carniani et al. 2013). bIn units of 10−17 erg s−1 cm−2. cThese measurements should be taken with caution due to the degeneracies in the fitting.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.