Table 1
Radio-loud BAL quasar sample.
| RA(J2000) | Dec(J2000) | z | BI | S1.4 GHz | logL1.4 GHz | S4.9 GHz | S8.4 GHz | αfit | log RI | log Pjet | |||
| h m s | ° ′ ″ | (km s-1) | (mJy) | (W Hz-1) | (mJy) | (mJy) | (W Hz-1) | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | |||
|
|
|||||||||||||
| 08 11 02.931 | 50 07 24.52 | 1.84 | 371 | 24.9 | 26.8 | 10.9 | 11.9 | 0.41 | 2.1 | 38.7 | |||
| 08 42 24.395 | 06 31 16.78 | 2.46 | 1974 | 51.0 | 27.4 | 25.6 | 21.2 | 0.49 | 2.8 | 39.3 | |||
| 08 56 41.566 | 42 42 53.94 | 3.06 | 295 | 20.0 | 27.2 | 20.5 | 13.7 | 0.19 | 1.8 | 39.2 | |||
| 10 40 59.802 | 05 55 24.78 | 2.44 | 4290 | 42.2 | 27.3 | 8.1 | 3.8 | 1.34 | 2.5 | 39.2 | |||
| 13 33 25.080 | 47 29 35.36 | 2.62 | 152 | 44.7 | 27.4 | − | − | − | 2.1 | 39.3 | |||
| 14 01 26.163 | 52 08 34.63 | 2.97 | 70 | 37.1 | 27.4 | − | − | − | 2.0 | 39.4 | |||
| 14 57 56.263 | 57 44 46.90 | 2.13 | 17 | 78.9 | 27.4 | − | − | − | 2.7 | 39.3 | |||
| 21 07 57.683 | -06 20 10.49 | 0.65 | 559 | 20.4 | 25.5 | − | − | − | 1.4 | 37.6 | |||
| 22 38 43.578 | 00 16 48.05 | 3.47 | 13 | 36.9 | 27.6 | − | − | − | 2.2 | 39.6 | |||
| 22 48 00.717 | -09 07 44.93 | 2.11 | 16 | 36.7 | 27.1 | − | − | − | 2.3 | 39.0 | |||
Notes. Description of the columns: (1) and (2) source coordinates (J2000) extracted from FIRST; (3) redshift as measured from the SDSS; (4) balnicity index taken from Trump et al. (2006); (5) total flux density at 1.4 GHz extracted from FIRST; (6) log of the radio luminosity at 1.4 GHz; (7) and (8) total flux density at 4.9 GHz and 8.4 GHz taken from DiPompeo et al. (2011); (9) spectral index using linear fit to all available radio data taken from DiPompeo et al. (2011); (10) radio-loudness, the radio-to-optical (i-band) ratio of the quasar core (Kimball et al. 2011b), which were calculated from z, S1.4 GHz, Mi taken from Trump et al. (2006), and the assumption of a radio core spectral index of 0 and an optical spectral index of −0.5, (11) jet power at 1.4 GHz calculated using formula from Sikora et al. (2013; see also Sect. 3.3).
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