Table 8
Main results of our analysis for sources with measured redshift.
| Source | Redshift | Detected | Flux (erg cm-2 s-1 Å-1) | Power law index | Flux ratio | mR(galaxy) | MR (galaxy) |
| line type | 10 000 Å | 5500 Å | |||||
|
|
|||||||
| BZB J0238–3116 | 0.2329 | Abs, Em | 2.66(±0.01) × 10-16 | –1.57 ± 0.02 | 6.0 ± 0.4 | 18.5 ± 0.1 | –22.5 ± 0.1 |
| BZB J0543–5532 | 0.273 | Abs | 4.60(±0.01) × 10-16 | –1.56 ± 0.10 | 25.0 ± 10.0 | 20.0 ± 0.6 | –21.4 ± 0.6 |
| BZB J0505+0415 | 0.424 | Abs | 2.06(±0.02) × 10-16 | –1.42 ± 0.10 | 4.5 ± 0.8 | 18.6 ± 0.2 | –24.2 ± 0.2 |
| RBS 334 | 0.411 | Abs | 2.26(±0.02) × 10-16 | –1.66 ± 0.15 | 5.0 ± 1.6 | 18.7 ± 0.3 | –24.0 ± 0.3 |
| PKS 0301–243 | 0.2657 | Em | 13.7(±0.1) × 10-16 | –1.03 ± 0.02 | ~34 | 18.7 (–0.4) | –23.4 |
Notes. The columns contain from left to right: (1) source name; (2) redshift; (3) detected line type, absorption (Abs) or emission (Em); (4) flux at 10 000 Å; (5) UVB–NIR power law slope; (6) jet/galaxy ratio at 5500 Å in the rest frame; (7) apparent magnitude of the host galaxy before slit loss correction (for PKS 0301-243, we quote the magnitude measured by Falomo & Ulrich 2000 and the upper limit derived following the discussion in Sect. 3); and (8) absolute magnitude of the host galaxy corrected by slit losses considering an effective radius of 10 kpc for all sources, except BZB J0505+0415, for which we used the effective radius from Nilsson et al. (2003), and PKS 0301-243, for which we quote the magnitude measured by Falomo & Ulrich (2000).
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