Table A.1.
Radio-loud AGNs discovered to date at z ≥ 5.5.
| Name | z (Ref) | S1.4 GHz | ανr (Ref) | R |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| J034141−004812 | 5.68 (1) | 2.09 | 0.75* (1) | 178.0 ± 40.5 |
| J083643+005453 | 5.77 (2) | 1.11 | 0.89 ± 0.29 (8) | 11.9 ± 0.3 |
| J090132+161506 | 5.63 (1) | 3.90 | 0.75* (1) | 91.4 ± 8.8 |
| J142738+331241 | 6.12 (3) | 1.03 | 0.62 ± 0.17 (8) | 53.3 ± 4.1 |
| J142952+544717 | 6.21 (4) | 2.95 | 0.79 ± 0.04 (8) | 109.2 ± 8.9 |
| J160937+304147 | 6.14 (1) | 0.48 | 0.75* (1) | 28.3 ± 8.6 |
| J205321+004706 | 5.92 (5) | 0.43 | 0.75* (1) | 44.1 ± 18.7 |
| J222843+011031 | 5.95 (6) | 1.32 | 0.8 (1) | 61.3 ± 20.9 |
| J232936−152016a | 5.84 (7) | 14.90 | 0.97 ± 0.12 (7) | 1169.5 ± 300.5 |
Notes. Column (1): object name; for the object denoted with a the reported values of ανr and R are the median of the results of Bañados et al. (2018); Col. (2): redshift from the literature and reference; Col. (3): observed radio flux density at 1.4 GHz in mJy; Col. (4): radio spectral index and reference. For objects denoted with an *, ανr have been assumed by Bañados et al. (2015); Col. (5): radio loudness as defined in Kellermann et al. (1989).
References. 1 = Bañados et al. (2015), 2 = Fan et al. (2001), 3 = McGreer et al. (2006), 4 = Willott et al. (2010), 5 = Jiang et al. (2009), 6 = Zeimann et al. (2011), 7 = Bañados et al. (2018), 8 = Coppejans et al. (2017).
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