Table 9
Main results of our analysis for sources without measured redshift.
| Source | Redshift | Detected | Redshift | Flux (erg cm-2 s-1 Å-1) | Power law index | Flux ratio | mR(galaxy) |
| spectroscopic | line type | imaging | 10 000 Å | 5500 Å | |||
|
|
|||||||
| KUV 00311–1938 | 0.506 ≤ z ≤ 1.54 | Int | ≥0.47 | 4.0(±0.2) × 10-16 | −1.14 ± 0.14 | ≥18 | ≤19.7 |
| BZB J0816–1311 | 0.288 ≤ z ≤ 1.56 | Int | ≥0.33 | 2.0(±0.1) × 10-16 | −1.24 ± 0.15 | ≥10 | ≤ 19.5 |
| PKS 0447–439 | z ≤ 1.51 | None | ≥0.175 | 38.7(±1.6) × 10-16 | −1.32 ± 0.09 | ≥20 | ≤16.7 |
Notes. The columns contain from left to right: (1) source name; (2) spectroscopic limits on redshifts (lower limits based on intervening systems and upper-limits on the non detection of Lyα); (3) detected line type, “Int” for intervening system; (4) limits on redshifts based on the imaging method proposed by Sbarufatti et al. (2005) (for MR = − 22.5); (5) the flux at 10 000 Å; (6) UVB–NIR power law slope; (7) limits on the jet/galaxy ratio at 5500 Å in the determined rest frame that assumes a redshift at 0.506, 0.288, and 0.175, respectively, for KUV 00311–1938, BZB J0816–1311, and PKS 0447–439; and (8) upper limit to the apparent magnitude of the host galaxy.
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