Table 5
The measured flux densities (in mJy) for the sample of 25 radio-loud BAL QSOs.
| Name | comp. | S 1.4 | S 2.6 | S 4.85 | S 4.86 | S 8.35 | S 8.46 | S 10.5 | S 22 | S 43 | LS |
|
|
|||||||||||
| 0044+00 | 54.76 ± 0.11* | 54.8 ± 2.91 | 30.9 ± 1.01 | 34.2 ± 1.8 | 24.0 ± 1.01 | 25.5 ± 0.6 | 26.9 ± 3.91 | 9.5 ± 2.7 | 4.9 ± 1.8 | <8 | |
| 0756+37 | 213 ± 14 | 266.0 ± 3.11 | 209.6 ± 2.61 | 226.2 ± 2.0 | 131.5 ± 3.01 | 142.1 ± 1.8 | 113.6 ± 5.21 | 56.2 ± 2.4 | <8.4 | <8 | |
| 0816+48 | 304 ± 21 | 45.8 ± 1.41 | 31.8 ± 1.01 | 31.4 ± 0.5 | 18.4 ± 0.81 | 19.5 ± 0.5 | 15.3 ± 2.61 | <5.7 | – | 217 | |
| 0842+06 | 45.9 ± 7.5 | 45.7 ± 1.91 | 30.7 ± 1.71 | 29.5 ± 0.4 | <541 | 20.9 ± 0.5 | 15.4 ± 4.61 | 6.9 ± 1.4 | – | <8 | |
| 0849+27 | 67.08 ± 0.30* | 49.4 ± 1.71 | 32.0 ± 1.51 | – | 21.3 ± 1.01 | – | 17.2 ± 2.21 | – | – | 173-382 | |
| A | 7.84 ± 0.15* | – | – | – | – | – | – | – | – | ||
| B | 4.47 ± 0.15* | – | – | – | – | – | – | – | – | ||
| C | 53.95 ± 0.15* | – | – | – | – | – | – | – | – | ||
| D | 0.82 ± 0.15* | – | – | – | – | – | – | – | – | ||
| 0905+02 | 32.8 ± 8.5 | 87.0 ± 3.52 | 47.8 ± 2.72 | – | 27.9 ± 1.12 | 28.5 ± 1.4 | <1352 | 8.8 ± 1.9 | – | <8 | |
| 0929+37 | 38.9 ± 4.9 | 29.4 ± 1.82 | 29.1 ± 1.42 | 32.0 ± 0.5 | 26.0 ± 1.32 | 29.3 ± 0.5 | 20.7 ± 7.22 | 19.1 ± 1.4 | 6.9 ± 2.5 | <8 | |
| 1014+05 | 57.9 ± 3.3 | 37.4 ± 3.33 | 33.1 ± 2.23 | 34.5 ± 0.6 | – | 25.1 ± 0.5 | 17.9 ± 3.03 | 12.6 ± 2.2 | – | <8 | |
| 1040+05 | 42.20 ± 0.23* | – | – | 37.2 ± 1.4 | – | 5.2 ± 0.4 | – | – | – | <19 | |
| 1054+51 | 38.8 ± 3.4 | 32.1 ± 1.91 | 16.7 ± 1.11 | 15.9 ± 0.5 | 8.6 ± 0.71 | 9.5 ± 0.6 | 7.9 ± 3.21 | <12.6 | – | <19 | |
| 1102+11 | 98.4 ± 7.9 | 79.2 ± 2.43 | 36.4 ± 2.43 | 39.8 ± 0.8 | 18.6 ± 0.72 | 19.9 ± 0.7 | 16.1 ± 5.02 | <4.2 | – | <19 | |
| 1103+11 | 250.43 ± 0.21* | 150.9 ± 2.21 | 95.5 ± 2.11 | 100.9 ± 0.8 | 65.9 ± 1.11 | 75.0 ± 0.8 | 58.4 ± 3.81 | 43.6 ± 1.8 | – | 69 | |
| A | 76.14 ± 0.15* | – | – | 21.2 ± 0.3 | – | 10.2 ± 0.3 | – | – | – | ||
| C | 174.29 ± 0.15* | – | – | 79.7 ± 0.7 | – | 64.8 ± 0.7 | – | – | – | ||
| 1129+44 | 42.1 ± 7.4 | 72.1 ± 1.61 | 41.3 ± 1.51 | 38.5 ± 2.5 | 23.9 ± 6.61 | 26.6 ± 1.7 | 19.5 ± 3.91 | 3.1 ± 1.2 | – | <19 | |
| 1159+01 | 264.4 ± 9.8 | – | – | 146.1 ± 1.3 | – | 176.6 ± 2.2 | – | 169.2 ± 2.8 | – | <8 | |
| 1159+06 | 159.5 ± 3.1 | 109.5 ± 5.32 | 60.2 ± 2.52 | 58.5 ± 1.1 | 35.8 ± 1.62 | 37.6 ± 0.7 | 26.2 ± 3.32 | 4.6 ± 2.3 | – | <19 | |
| 1229+09 | 81.3 ± 6.6 | 35.8 ± 1.51 | 15.4 ± 2.31 | 17.3 ± 0.5 | 15.7 ± 6.31 | – | 7.5 ± 2.41 | <2.7 | – | <32 | |
| 1237+47 | 74.7 ± 5.9 | – | – | 62.3 ± 1.0 | – | 61.6 ± 1.6 | – | – | – | <19 | |
| 1304+13 | 61.4 ± 4.9 | 37.0 ± 3.03 | 21.4 ± 1.63 | 24.6 ± 0.5 | 15 ± 12 2 | 17.1 ± 0.5 | 14.3 ± 3.52 | 5.3 ± 1.3 | – | <8 | |
| 1327+03 | 163 ± 15 | 92.2 ± 2.71 | 67.7 ± 1.91 | 79.5 ± 1.7 | 52.5 ± 1.21 | 56.5 ± 0.7 | 51.8 ± 3.31 | 28.6 ± 1.8 | – | <8 | |
| 1335+02 | 112.3 ± 5.6 | 96.9 ± 1.71 | 81.9 ± 1.31 | 86.7 ± 1.3 | 63.3 ± 1.41 | 69.4 ± 1.0 | 64.7 ± 3.91 | 88.6 ± 1.7 | <10.5 | <8 | |
| 1337−02 | 47.2 ± 5.3 | 67.3 ± 3.23 | 42.3 ± 2.73 | 42.9 ± 0.8 | – | 16.4 ± 0.5 | – | – | – | <19 | |
| 1404+07 | 187.8 ± 3.6 | 225.9 ± 2.61 | 209.4 ± 2.81 | 206.4 ± 2.3 | 173.6 ± 2.41 | 189.6 ± 2.2 | 160.9 ± 7.51 | 146.9 ± 2.3 | – | <8 | |
| 1406+34 | 165 ± 24 | 246.6 ± 2.91 | 301.5 ± 3.11 | 312.8 ± 3.1 | 263.1 ± 3.41 | 276.3 ± 3.0 | 237 ± 10 1 | 180.1 ± 2.9 | 90.2 ± 3.4 | <4 | |
| 1603+30 | 54.17 ± 0.14* | 34.4 ± 9.93 | 38.8 ± 2.53 | 34.5 ± 2.4 | – | 26.9 ± 0.6 | – | 9.7 ± 1.3 | – | 17 | |
| A | – | – | – | – | – | – | – | 2.4 ± 0.8 | – | ||
| C | – | – | – | – | – | – | – | 7.3 ± 1.0 | – | ||
| 1624+37 | 56.44 ± 0.14* | 35.0 ± 3.01 | 25.8 ± 1.51 | 28.1 ± 3.7 | 22.5 ± 0.71 | 18.2 ± 1.7 | 18.9 ± 5.61 | 7.4 ± 3.1 | – | <19 | |
Notes. Flux densities at 1.4, 4.86, 8.46, 22, and 43 GHz are from the VLA; those at 2.6, 4.85, 8.35, and 10.5 GHz are from the Effelsberg telescope. Asterisked values are taken from the FIRST survey. Superscripts on the errors indicate the run number of the Effelsberg observations, according to the key in Table 3. Column 2 specifies the component of the source being referred to (see Sect. 4.1): if no letter is present the total flux density is given. The last column gives the projected linear size (in kpc) of the resolved sources (in boldface) and the upper limits for unresolved sources (the latter taken from the highest-resolution map with at least a 3-σ detection).
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