Table 5.
Spatial extents of the outflow and narrow components measured from Paα/Brγ and [Si VI].
| QSO2 | FWHMseeing | Line | FWHMout | rout | FWHMnar | rnar | ||
|---|---|---|---|---|---|---|---|---|
| [arcsec] | [arcsec] | [arcsec] | [kpc] | [arcsec] | [arcsec] | [kpc] | ||
| J0802+25 | 0.74 | Paα | 0.97 ± 0.03 | 0.63 ± 0.06 | 0.96 ± 0.09 | 1.16 ± 0.03 | 0.90 ± 0.04 | 1.37 ± 0.06 |
| [Si VI] | 0.65 ± 0.03* | < 0.738 | < 1.13 | 0.87 ± 0.03 | 0.46 ± 0.07 | 0.70 ± 0.10 | ||
| J0945+17 | 1.01 | Paα | 1.37 ± 0.04 | 0.93 ± 0.06 | 2.13 ± 0.15 | 1.54 ± 0.02 | 1.17 ± 0.04 | 2.67 ± 0.08 |
| [Si VI] | 1.54 ± 0.18 | 1.17 ± 0.25 | 2.67 ± 0.57 | 1.50 ± 0.05 | 1.11 ± 0.08 | 2.55 ± 0.18 | ||
| J1034+60 | 1.25 | Brγ | 1.78 ± 0.18 | 1.27 ± 0.28 | 1.26 ± 0.28 | 2.25 ± 0.10 | 1.87 ± 0.12 | 1.87 ± 0.12 |
| [Si VI] | 1.65 ± 0.09 | 1.08 ± 0.23 | 1.07 ± 0.23 | 1.98 ± 0.03 | 1.54 ± 0.04 | 1.53 ± 0.04 | ||
| J1440+53 | 0.85 | Brγ | 0.95 ± 0.09** | 0.43 ± 0.23 | 0.32 ± 0.17 | 1.05 ± 0.02 | 0.62 ± 0.04 | 0.46 ± 0.03 |
| [Si VI] | 0.76 ± 0.10 | < 0.846 | < 0.62 | 0.94 ± 0.02 | 0.41 ± 0.05 | 0.30 ± 0.04 | ||
| J1455+35 | 0.64 | Paα | 0.77 ± 0.12 | 0.43 ± 0.22 | 0.70 ± 0.35 | 0.90 ± 0.03 | 0.63 ± 0.04 | 1.03 ± 0.07 |
| [Si VI] | 0.47 ± 0.07 | < 0.64 | < 1.04 | 0.86 ± 0.05 | 0.58 ± 0.08 | 0.94 ± 0.13 | ||
| J1713+57 | 1.10 | Paα | 1.25 ± 0.08 | 0.59 ± 0.18 | 1.21 ± 0.36 | 1.25 ± 0.03 | 0.59 ± 0.07 | 1.21 ± 0.15 |
| [Si VI] | 1.26 ± 0.17 | 0.61 ± 0.45 | 1.25 ± 0.93 | 1.40 ± 0.09 | 0.86 ± 0.15 | 1.77 ± 0.31 | ||
Notes. Column 2 presents the seeing FWHM measured from the K-band spectra of the standard stars shown in Table 2. In the case of J0802+25 FWHMseeing is the average value measured from the stars HD 76619 and HD 233594. Columns 3–5 show the FWHM of the continuum-subtracted spatial profile of the outflow component and corresponding seeing deconvolved spatial extent (in arcseconds and kiloparsecs). Columns 6–8 are the same, but for the narrow component. * Using only the red wing of the line because of blend with H2 1-0S(3) on the blue side of the line. ** Using only the blue wing of the line because the redshifted outflow component is not spatially resolved.
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