Table 3.
Properties of the final quasar sample.
| Name | RA | Dec | z | log FUV | log FX | Group | ΓX | DM |
|---|---|---|---|---|---|---|---|---|
| 030341.04−002321.9 | 45.92103 | −0.38942 | 3.235 | −27.00 ± 0.04 | −31.38 ± 0.04 | 1 | 1.87 ± 0.12 | 46.42 ± 0.31 |
| 030449.85−000813.4 | 46.20775 | −0.13708 | 3.296 | −26.98 ± 0.01 | −31.24 ± 0.03 | 1 | 1.99 ± 0.29 | 45.62 ± 0.20 |
| 090508.88+305757.3 | 136.28702 | 30.96593 | 3.034 | −26.97 ± 0.01 | −31.14 ± 0.02 | 1 | 2.12 ± 0.09 | 44.90 ± 0.17 |
Notes. This table is presented in its entirety at the CDS; a portion is shown here for guidance. Fluxes are in units of log(erg s−1 cm−2 Hz−1). The Group column flags the different sub-samples: 1 = XMM–Newtonz ≃ 3 sample, 2 = new XMM–Newtonz ≃ 4 quasar, 3 = High−z sample, 4 = XXL, 5 = SDSS – 4XMM, 6 = SDSS – Chandra, 7 = local AGN. The column DM reports the distance moduli (with uncertainties) to reproduce Fig. 9.
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