Table 1.
Forty BAL QSOs from the WISSH sample.
| ID | SDSS ID | z | AI | AI1000 | BI | vmin | vmax | Type |
|---|---|---|---|---|---|---|---|---|
| [km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| 0045+14 | SDSS004527.68+143816.1 | 1.992 | 7762 | 7718 | 7016 | 1300 | 16 000 | LoBAL |
| 0216−09 | SDSS021646.94−092107.2 | 3.691 | 2335 | 1940 | 1170 | 8770 | 18 800 | HiBAL |
| 0414+06 | SDSS041420.90+060914.2 | 2.614⋆ | 10 806 | 10 285 | 7415 | 1140 | 13 750 | HiBAL |
| 0747+27 | SDSS074711.14+273903.3 | 4.110 | 209 | 12 | 0 | 2940 | 12 680 | BAL |
| 0928+53 | SDSS092819.29+534024.1 | 4.390 | 9217 | 8327 | 8327 | 3430 | 19 050 | BAL |
| 0959+13 | SDSS095937.11+131215.4 | 4.061 | 29 | 0 | 0 | 13 800 | 15 700 | BAL |
| 1013+56 | SDSS101336.37+561536.3 | 3.633 | 127 | 0 | 0 | 3460 | 11 650 | HiBAL |
| 1025+24 | SDSS102541.78+245424.2 | 2.382 | 3059 | 2866 | 2356 | 7260 | 13 750 | LoBAL |
| 1048+44 | SDSS104846.63+440710.8 | 4.347 | 11 125 | 10 720 | 9044 | 2060 | 17 840 | BAL |
| 1051+31 | SDSS105122.46+310749.3 | 4.243 | 203 | 14 | 0 | 9920 | 11 800 | BAL |
| 1103+10 | SDSS110352.74+100403.1 | 3.590 | 357 | 38 | 0 | 1530 | 6160 | HiBAL |
| 1110+19 | SDSS111017.13+193012.5 | 2.498 | 2680 | 2532 | 0 | 590 | 4900 | HiBAL |
| 1110+48 | SDSS111038.63+483115.6 | 2.957 | 145 | 0 | 0 | 14 360 | 15 440 | HiBAL |
| 1122+16 | SDSS112258.77+164540.3 | 3.024 | 8061 | 7861 | 7312 | 6610 | 17 670 | LoBAL |
| 1130+07 | SDSS113017.37+073212.9 | 2.654 | 25 | 0 | 0 | 10 710 | 12 140 | HiBAL |
| 1157+27 | SDSS115747.99+272459.6 | 2.217⋆ | 5641 | 4948 | 4021 | 2000 | 17 200 | HiBAL |
| 1204+33 | SDSS120447.15+330938.7 | 3.596 | 5282 | 5117 | 3531 | 1620 | 10 590 | LoBAL |
| 1210+17 | SDSS121027.62+174108.9 | 3.604⋆ | 5903 | 5595 | 5116 | 5840 | 14 750 | HiBAL |
| 1215−00 | SDSS121549.81−003432.1 | 2.707 | 1679 | 1289 | 399 | 5800 | 20 640 | HiBAL |
| 1237+06 | SDSS123714.60+064759.5 | 2.781 | 872 | 187 | 0 | 4200 | 19 810 | HiBAL |
| 1245+01 | SDSS124551.44+010505.0 | 2.798 | 3707 | 3530 | 1939 | 1300 | 12 300 | HiBAL |
| 1250+20 | SDSS125050.88+204658.7 | 3.570 | 890 | 824 | 0 | 350 | 3820 | HiBAL |
| 1305+05 | SDSS130502.28+052151.1 | 4.071 | 246 | 42 | 0 | 19 500 | 22 550 | HiBAL |
| 1326−00 | SDSS132654.96−000530.1 | 3.303⋆ | 2275 | 1960 | 0 | 0 | 3850 | HiBAL |
| 1328+58 | SDSS132827.06+581836.8 | 3.133 | 322 | 131 | 0 | 3500 | 5400 | HiBAL |
| 1422+44 | SDSS142243.02+441721.2 | 3.648⋆ | 310 | 0 | 0 | 15 410 | 22 780 | HiBAL |
| 1447+10 | SDSS144709.24+103824.5 | 3.699 | 6179 | 4484 | 65 | 370 | 23 520 | HiBAL |
| 1451+14 | SDSS145125.31+144136.0 | 3.102 | 4848 | 4340 | 3586 | 6000 | 13 400 | HiBAL |
| 1506+52 | SDSS150654.55+522004.7 | 4.068 | 5147 | 4938 | 4396 | 12 970 | 23 130 | HiBAL |
| 1513+08 | SDSS151352.52+085555.7 | 2.897 | 1293 | 820 | 0 | 200 | 4800 | HiBAL |
| 1544+41 | SDSS154446.34+412035.7 | 3.548 | 4808 | 4663 | 4270 | 9580 | 23 500 | HiBAL |
| 1549+12 | SDSS154938.72+124509.1 | 2.365⋆ | 4918 | 4425 | 1735 | 0 | 6470 | HiBAL |
| 1555+10 | SDSS155514.85+100351.3 | 3.512 | 6992 | 6490 | 5576 | 7090 | 16 000 | LoBAL |
| 1633+36 | SDSS163300.13+362904.8 | 3.576 | 377 | 241 | 90 | 18 700 | 24 800 | HiBAL |
| 1639+28 | SDSS163909.10+282447.1 | 3.801 | 366 | 259 | 0 | 22 300 | 28 460 | HiBAL |
| 1650+25 | SDSS165053.78+250755.4 | 3.338 | 3675 | 3516 | 2913 | 5000 | 13 100 | HiBAL |
| 2123−00 | SDSS212329.46−005052.9 | 2.282⋆ | 107 | 0 | 0 | 13500 | 24 600 | HiBAL |
| 2238−08 | SDSS223808.07−080842.1 | 3.122 | 4300 | 3889 | 2228 | 1500 | 19 000 | HiBAL |
| 0947+14 | SDSS094734.19+142116.9 | 3.040 | 795 | 685 | 548 | 41 250 | 46 040 | HiBAL |
| 1538+08 | SDSS153830.55+085517.0 | 3.567⋆ | 439 | 318 | 130 | 38 300 | 47 000 | HiBAL |
Notes. The first 38 objects are identified through absorption features between the Si IV and C IV emission lines, and the last 2 objects from features blue-wards of Si IV. Absorption index estimates are given in Cols. 4−6. In the last column, the BAL type is reported: objects with a C IV BI > 0 are set in bold face, while “BAL” means that the spectrum coverage does not allow a proper HiBAL/LoBAL classification. Redshifts with an asterisk are taken from Vietri et al. (2018).
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