Table 1
The sample of 25 radio-loud BAL QSOs studied in this paper.
Name | RA | Dec | z | AI | S 1.4 | BAL |
(J2000) | (J2000) | (km s-1) | (mJy) | Type | ||
|
||||||
0044+00 | 00 44 44.06 | +00 13 03.5 | 2.28 | 11701 | 53.1 | – |
0756+37 | 07 56 28.24 | +37 14 55.6 | 2.51 | 330 | 239.4 | – |
0816+48 | 08 16 18.99 | +48 23 28.4 | 3.57 | 260 | 68.3 | – |
0842+06 | 08 42 24.38 | +06 31 16.8 | 2.45 | 26901 | 48.1 | – |
0849+27 | 08 49 14.27 | +27 57 29.7 | 1.73 | 540 | 52.8 | Hi |
0905+02 | 09 05 52.41 | +02 59 31.5 | 1.82 | 130 | 43.5 | Hi |
0929+37 | 09 29 13.97 | +37 57 43.0 | 1.91 | 2170 | 43.2 | Hi |
1014+05 | 10 14 40.35 | +05 37 12.6 | 2.01 | 250 | 55.0 | Hi |
1040+05 | 10 40 59.80 | +05 55 24.4 | 2.44 | 49201 | 40.2 | – |
1054+51 | 10 54 16.51 | +51 23 26.1 | 2.34 | 22201 | 32.0 | – |
1102+11 | 11 02 06.66 | +11 21 04.9 | 2.35 | 506 | 82.3 | – |
1103+11 | 11 03 34.79 | +11 14 42.4 | 1.73 | 380 | 148.0 | FeLo |
1129+44 | 11 29 38.47 | +44 03 25.1 | 2.21 | 1430 | 41.1 | Hi |
1159+01 | 11 59 44.82 | +01 12 06.9 | 2.00 | 22601 | 266.5 | FeLo |
1159+06 | 11 59 01.75 | +06 56 19.1 | 2.19 | 3645 | 116.6 | Hi |
1229+09 | 12 29 09.64 | +09 38 10.1 | 2.65 | 230 | 66.2 | – |
1237+47 | 12 37 17.44 | +47 08 07.0 | 2.27 | 13001 | 78.5 | FeLo |
1304+13 | 13 04 48.06 | +13 04 16.6 | 2.57 | 640 | 49.6 | – |
1327+03 | 13 27 03.21 | +03 13 11.2 | 2.83 | 190 | 60.7 | – |
1335+02 | 13 35 11.90 | +02 53 09.5 | 1.85 | 210 | 105.3 | Hi |
1337−02 | 13 37 01.40 | −02 46 30.3 | 3.06 | 590 | 43.3 | – |
1404+07 | 14 04 33.01 | +07 28 47.2 | 2.86 | 120 | 131.1 | – |
1406+34 | 14 06 53.84 | +34 33 37.3 | 2.56 | 350 | 164.4 | – |
1603+30 | 16 03 54.15 | +30 02 08.7 | 2.03 | 1355 | 53.7 | Hi |
1624+37 | 16 24 53.47 | +37 58 06.6 | 3.38 | 10201 | 56.1 | – |
Notes. Columns 2–7 give the optical coordinates and redshifts from SDSS, the absorption index for the C iv line (width of at least 1000 km s-1), the FIRST peak flux densities, and the type.
Balnicity index BI > 0 following Weymann et al. (1991).
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