Table 8.
Spectral windows used to extract spatial profiles of the stellar continuum light (Cols. 2 and 3) and of the outflowing gas (Col. 4) from the X-shooter slit spectra.
| Object | Δλblue | Δλred | Δvout |
|---|---|---|---|
| [Å] | [Å] | [km s−1] | |
| PKS 0252–71 | 4890 ≤ λ ≤ 4923 | 5040 ≤ λ ≤ 5073 | |
| PKS 2135–209 | 4890 ≤ λ ≤ 4923 | 5040 ≤ λ ≤ 5073 | |
| PKS 2313+03 | 4756 ≤ λ ≤ 4806 | 5040 ≤ λ ≤ 5073 | −2000 ≤ v ≤ −800 |
| PKS 1151–34 ( * ) | 4831 ≤ λ ≤ 4839 | 4881 ≤ λ ≤ 4889 | −529 ≤ v ≤ −279 |
| PKS 1814–63 | 4890 ≤ λ ≤ 4923 | 5040 ≤ λ ≤ 5073 | 400 ≤ v ≤ 1000 |
Notes. For PKS 0252–71 and PKS 2135–209 the indicated spectral windows are used to derive the average continuum light spatial profile in the framework of the spectro-astrometry technique employed to extract the outflow spatial extents. For PKS 1814–63 and PKS 2314+03 the indicated spectral windows are used to study the outflow spatial extents following the approach described in Rose et al. (2018) and Spence et al. (2018). The boundaries of the spectral windows are reported in Å for the stellar continuum and as velocity shifts with respect to the rest-frame velocity of the [O III]λ5007 Å emission line for the outflowing gas. For PKS 1151–34 the spatial study has been carried out using the emission of the Hβ and the bands probing the stellar continuum also contain emission of the BLR, to allow subtraction of the BLR emission as well as the continuum emission. ( * )Value reported refer to the Hβ emission line which has been used for this target.
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.