Table 5.
Kinematic properties of the broad (outflow) component of the whole QSO2 sample.
| Galaxy ID |  |
Δv | Routflow | |
|---|---|---|---|---|
| (SDSS_PA code) | (km s−1) | (km s−1) | (kpc) | |
| (1) | (2) | (3) | (4) | |
| OSIRIS/GTC | ||||
| 0741+3020 Central outflow (a) | 291.82 ± 41.30 | –380.54 ± 107.80 | 4.2±0.4 | |
| 0741+3020 Giant nebula (a) | ∼130 | ∼100 | ∼40 | |
| 0818+3958 (b) | 491.02 ± 61.29 | –568.80 ± 185.75 | < 2.2 | |
| 0834+5534_34 | 948.84 ± 48.78 | 629.20 ± 63.18 | 0.7 ± 0.4 | |
| 0834+5534_145 | 871.51 ± 74.79 | 452.05 ± 56.84 | 0.8 ± 0.3 | |
| 0902+5459_83a | – | – | ||
| 0902+5459_138a | – | – | ||
| 0902+5459_83b | – | – | ||
| 0902+5459_138b | – | – | ||
| 0956+5735 | 624.09 ± 24.36 | 110.76 ± 65.54 | < 3.3 | |
| 1101+4004a | – | – | ||
| 1101+4004b | – | – | ||
| FORS2/VLT | ||||
| J0923+0101 | 708.16 ± 75.19 | –33 ± 49 | 0.16 – 1.0 | |
| J0950+0111 | 696.69 ± 18.69 | –506 ± 35 | 0.38 – 1.1 | |
| J0955+0346 | 1062.02 ± 84.96 | –810 ± 190 | 0.20 – 3.5 | |
| J1014+0244a/pa1 | 652.93 ± 30.59 | –126 ± 53 | 0.20 – 1.0 | |
| J1014+0244a/pa2 | 671.20 ± 48.85 | –72 ± 72 | = | |
| J1153+0326 | 615.97 ± 33.98 | 325 ± 80 | 0.52 – 1.7 | |
| J1247+0152 | 498.30 ± 84.11 | –301 ± 194 | 0.28 – 1.4 | |
| J1307–0214 | 424.80 ± 12.74 | –246 ± 29 | 1.3 ± 0.4 | |
| J1336–0039 | 1055.64 ± 73.49 | –942 ± 112 | 0.19 – 1.0 | |
| J1337–0128 | 543.76 ± 25.49 | –320 ± 16 | 0.19 – 1.7 | |
| J1407+0217 | 709.43 ± 50.98 | –80 ± 33 | 1.0 ± 0.2 | |
| J1413–0142 | 505.52 ± 21.24 | –185 ± 38 | 0.21 – 1.5 | |
| J1430–0050 | 679.69 ± 84.96 | –520 ± 60 | 0.12 – 0.80 | |
| J1546–0005 | 331.35 ± 12.74 | –270 ± 55 | 0.20 – 1.4 | |
Notes. Column (1): SDSS short name. When a system is composed of two galaxies, we identify them with a and b. The information of the slit PA is shown, unless only one slit is used for the observations. The minus means that the broad component (and thus, an outflow) has not been detected. Column (2): mean velocity dispersion. The FORS2/VLT values are taken from the works of Villar-Martín et al. (2011, 2012, 2016). Column (3): velocity offset, computed as the difference between the mean velocity of the broad component and the systemic velocity. Negative values represent blueshifted values, and positive values are redshifted. The FORS2/VLT values are taken from the works of Villar-Martín et al. (2011, 2012, 2016). Column (4): intrinsic radius of the outflow. It has been computed as half the difference between the FWHM of the observed [OIII] flux profile of the broad component and the FWHMseeing computed within the slit, according to the formula: Rout [kpc] = scale [kpc/″] × 
. For the FORS2/VLT data the minimum and maximum radial sizes of the outflows are given (see Table 5 in Villar-Martín et al. 2016, for details).
See Sect. 5.3.
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