Table 6
Properties of CIVλ1549 emission line derived from parametric model fits (see Sect. 3.2).
| SDSS Name |  |
 ,a |
REWCIV | FWHMCIV | LCIV |
|---|---|---|---|---|---|
| (Å) | (km s−1) | (Å) | (km s−1) | (1045 erg s−1) | |
| J0745+4734 | 1548 ± 1 | 190 ± 120 | 31.0  |
4320 ± 120 | 8.3  |
| J0801+5210 | 1535 ± 1 | 2720 ± 180 | 16.5 ± 0.6 | 10930  |
2.9 ± 0.1 |
| J0900+4215 | 1546 ± 1 | 560  |
31.6  |
4200 ± 150 | 6.4  |
| J0958+2827 | 1520 ± 1 | 5640 ± 180 | 19.0 ± 4.0 | 9970  |
1.7 ± 0.2 |
| J1106+6400 | 1534 ± 1 | 2870  |
20.6 ± 0.3 | 7830 ± 160 | 2.8 ± 0.1 |
| J1111+1336 | 1540 ± 1 | 1920 ± 130 | 20.0 ± 1.0 | 8210  |
3.0 ± 0.2 |
| J1157+2724b | 1529  |
3840  |
71.0  |
7620  |
0.9 ± 0.1 |
| J1201+0116 | 1531 ± 1 | 3390 ± 130 | 17.4 ± 0.9 | 8460  |
1.8 ± 0.1 |
| J1201+1206 | 1544 ± 1 | 980  |
37.0  |
5110 ± 110 | 4.4  |
| J1236+6554 | 1532 ± 1 | 3360 ± 110 | 19.9  |
7380  |
2.9 ± 0.1 |
| J1326–0005b | 1549 ± 1 | –50  |
82.0  |
2110  |
17.0 ± 2.0 |
| J1421+4633 | 1523 ± 1 | 5010  |
16.0 ± 2.0 | 10240  |
2.1 ± 0.2 |
| J1422+4417 | 1525 ± 1 | 4670 ± 230 | 20.0 ± 3.0 | 12410  |
5.9 ± 0.1 |
| J1521+5202 | 1511 ± 1 | 7420 ± 200 | 8.3 ± 0.6 | 11500  |
2.1 ± 0.1 |
| J1538+0855 | 1538 ± 1 | 2190 ± 110 | 20.8 ± 0.2 | 5160  |
4.0 ± 0.1 |
| J1549+1245b | 1547 ± 1 | 370  |
23.0 ± 1.0 | 5720  |
3.8  |
| J2123–0050 | 1537 ± 1 | 2330  |
12.4  |
6700  |
1.7 ± 0.1 |
| J2346–0016 | 1532 ± 1 | 3380  |
13.0 ± 2.0 | 8600  |
1.2 ± 0.1 |
Notes. Objects in boldface belong to the [OIII]sample. (a)Velocity shifts of the CIV emission line are calculated from the peak of the multiple Gaussians modeling the CIV profile, with respect to the systemic redshift (see Fig. 2). (b) Sources J1157+2724and J1549+1245 are classified as BAL QSOs according to the Balnicity Index (BI, Weymann et al. 1991) while J1326–0005 is classified according to the modified absorption index (AI1000> 100, Bruni et al. 2012), a more conservative version of the Hall et al. (2002) AI definition. A detailed analysis of the BAL properties of the WISSH QSOs will be presented in a forthcoming paper (Bruni et al. in prep). For these objects the strong absorption in the CIV emission line affects the spectral parameters.
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.