Table 3.
Properties of the [NeII]12.8, [NeV]14.3, and H20-0S(5) emission lines derived from the fits with Gaussian components.
| QSO2 | [NeII]12.8 | [NeV]14.3 | H20-0S(5) | ||||||
|---|---|---|---|---|---|---|---|---|---|
| L[NeII] | FWHM | vs | L[NeV] | FWHM | vs | LS(5) | FWHM | vs | |
| (1041 erg s−1) | (km s−1) | (km s−1) | (1041 erg s−1) | (km s−1) | (km s−1) | (1041 erg s−1) | (km s−1) | (km s−1) | |
| J1010 | 3.50±0.22 | 410±10 | 0±3 | 0.14±0.03 | 390 | 40±20 | 0.18±0.01 | 340±30 | –30±10 |
| 3.92±0.19 | 1220±60 | 10±10 | 0.66±0.05 | 1600±100 | 170±50 | … | … | … | |
| J1100 | 3.78±0.16 | 360±10 | 0±3 | 8.88±0.15 | 339±4 | 28±1 | 0.53±0.06 | 510±60 | –10±20 |
| 4.63±0.17 | 1360±60 | 60±20 | 8.57±0.19 | 1470±40 | 120±10 | … | … | … | |
| J1356 | 1.30±0.05 | 300±10 | 200±5 | 0.81±0.08 | 360±25 | 140±6 | 0.90±0.02 | 470±10 | –10±4 |
| 1.95±0.06 | 290±10 | –200±3 | 0.73±0.04 | 220±10 | –270±4 | … | … | … | |
| 1.50±0.08 | 1640±90 | –100±30 | 4.23±0.09 | 1450±30 | 14±8 | … | … | … | |
| J1430 | 4.65±0.17 | 320±6 | 0±1 | 3.04±0.11 | 420±8 | 56±2 | 0.50±0.01 | 500±10 | 20±4 |
| 6.12±0.15 | 900±20 | –13±4 | 2.94±0.10 | 1150±40 | 80±7 | … | … | … | |
| J1509 | 5.57±0.09 | 386±4 | 0±1 | 3.07±0.08 | 420±8 | 7±2 | 0.59±0.02 | 390±10 | 25±5 |
| 4.05±0.09 | 1390±40 | –140±10 | 6.48±0.09 | 1560±30 | –220±8 | … | … | … | |
Notes. The peak of the narrow component of [NeII] has been set as zero velocity (vs = 0 km s−1), so vs of any other component is relative to it. In J1356, where two narrow components were fitted to the atomic lines, the average of their two peak wavelengths corresponds to zero velocity. FWHMs are corrected from instrumental broadening, calculated following Eq. (1) in Argyriou et al. (2023). FWHMs without errors have been fixed.
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