Table 1
Sample of the 11 radio-loud BAL QSOs studied in this paper.
| Name | SDSS name | RA | Dec | z | S 1.4 | BAL |
| (J2000) | (J2000) | (mJy/beam) | Type | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
|
|
||||||
| 0044+00 | J004444.06+001303.5 | 00 44 44.0657 | +00 13 03.560 | 2.28 | 53.1 | – |
| 0756+37 | J075628.25+371455.6 | 07 56 28.24 | +37 14 55.6 | 2.51 | 239.4 | – |
| 0816+48 | J081618.99+482328.4 | 08 16 18.9960 | +48 23 28.469 | 3.57 | 68.3 | – |
| 0849+27 | J084914.27+275729.7 | 08 49 14.2716 | +27 57 29.709 | 1.73 | 52.8 | Hi |
| 1014+05 | J101440.35+053712.6 | 10 14 40.3561 | +05 37 12.682 | 2.01 | 55.0 | Hi |
| 1102+11 | J110206.66+112104.9 | 11 02 06.6617 | +11 21 04.900 | 2.35 | 82.3 | – |
| 1237+47 | J123717.44+470807.0 | 12 37 17.44 | +47 08 07.0 | 2.27 | 78.5 | FeLo |
| 1304+13 | J130448.06+130416.6 | 13 04 48.0594 | +13 04 16.590 | 2.57 | 49.6 | – |
| 1327+03 | J132703.21+031311.2 | 13 27 03.21 | +03 13 11.2 | 2.83 | 60.7 | – |
| 1406+34 | J140653.84+343337.3 | 14 06 53.84 | +34 33 37.3 | 2.56 | 164.4 | – |
| 1603+30 | J160354.15+300208.6 | 16 03 54.1534 | +30 02 08.705 | 2.03 | 53.7 | Hi |
Notes.Columns 3–5 are respectively RA, Dec and redshift as measured from the SDSS. For phase-referenced sources we give the coordinates of the brightest component peak, derived from our VLBI observations. Column 6 gives the peak flux density at 1.4 GHz from the FIRST catalogue (Becker et al. 1995; White et al. 1997). The last column is the BAL type as given in Bruni et al. (2012): a hyphen indicates that it could not be determined.
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