Table 1.
Properties of the SUPER AGNs considered in this paper.
| ID | RA | Dec | z | z[OIII] | H | K | rH | rK | Log (LBol/erg s−1) | Log (L5100/erg s−1) |
|---|---|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| X_N_160_22 | 02:04:53.81 | −06:04:07.82 | 2.445 | 2.442 | 19.22 | 18.79 | 0.5 | 0.4 | 46.74 ± 0.02 | 45.83 ± 0.06 |
| X_N_81_44 | 02:17:30.95 | −04:18:23.66 | 2.311 | 2.317 | 18.78 | 18.43 | 0.45 | 0.4 | 46.80 ± 0.03 | 45.75 ± 0.06 |
| X_N_53_3 | 02:20:29.84 | −02:56:23.41 | 2.434 | 2.433 | 20.60 | – | – | 0.2 | 46.21 ± 0.03 | – |
| X_N_66_23 | 02:22:33.64 | −05:49:02.73 | 2.386 | 2.385 | 20.56 | 20.33 | 0.35 | 0.45 | 46.04 ± 0.02 | 45.63 ± 0.06 |
| X_N_35_20 | 02:24:02.71 | 05:11:30.82 | 2.261 | 2.261 | 22.07 | 21.70 | 0.15 | 0.2 | 45.44 ± 0.02 | 43.95 ± 0.06 |
| X_N_12_26 | 02:25:50.09 | −03:06:41.16 | 2.471 | 2.472 | 19.83 | 19.53 | 0.4 | 0.35 | 46.52 ± 0.02 | 45.53 ± 0.06 |
| X_N_44_64 | 02:27:01.46 | −04:05:06.73 | 2.252 | 2.244 | 21.31 | 20.77 | – | 0.2 | 45.51 ± 0.07 | – |
| X_N_4_48 | 02:27:44.63 | −03:42:05.46 | 2.317 | 2.315 | 19.57 | 20.43 | 0.25 | 0.35 | 46.16 ± 0.02 | 45.05 ± 0.06 |
| X_N_102_35 | 02:29:05.94 | 04:02:42.99 | 2.190 | 2.190 | 18.76 | 18.19 | 0.15 | 0.15 | 46.82 ± 0.02 | 45.52 ± 0.06 |
| X_N_115_23 | 02:30:05.66 | −05:08:14.10 | 2.342 | 2.340 | 19.79 | 19.26 | 0.35 | 0.4 | 46.49 ± 0.02 | 45.55 ± 0.06 |
| cid_166 | 09:58:58.68 | +02:01:39.22 | 2.448 | 2.461 | 18.55 | 18.23 | 0.3 | 0.45 | 46.93 ± 0.02 | 45.83 ± 0.06 |
| cid_1605 | 09:59:19.82 | +02:42:38.73 | 2.121 | 2.118 | 20.63 | 20.14 | 0.2 | 0.2 | 46.03 ± 0.02 | 44.84 ± 0.06 |
| cid_346 | 09:59:43.41 | +02:07:07.44 | 2.194 | 2.217 | 19.24 | 18.95 | 0.35 | 0.40 | 46.66 ± 0.02 | 45.61 ± 0.06 |
| cid_1205 | 10:00:02.57 | +02:19:58.68 | 2.255 | 2.257 | 21.64 | 20.72 | 0.15 | 0.6 | 45.75 ± 0.17 | 44.91 ± 0.06 |
| cid_467 | 10:00:24.48 | +02:06:19.76 | 2.288 | 2.285 | 19.34 | 18.91 | 0.2 | 0.2 | 46.53 ± 0.04 | 45.25 ± 0.06 |
| J1333+1649 | 13:33:35.79 | 16:49:03.96 | 2.089 | 2.099 | 15.72 | 15.49 | 0.55 | 0.5 | 47.91 ± 0.02 | 47.32 ± 0.06 |
| J1441+0454 | 14:41:05.54 | +04:54:54.96 | 2.059 | 2.080 | 17.15 | 16.53 | 0.50 | 0.55 | 47.55 ± 0.02 | 46.66 ± 0.06 |
| J1549+1245 | 15:49:38.73 | +12:45:09.20 | 2.365 | 2.368 | 15.92 | 15.34 | 0.50 | 0.65 | 47.73 ± 0.04 | 47.16 ± 0.06 |
| S82X1905 | 23:28:56.35 | −00:30:11.74 | 2.263 | 2.273 | 19.72 | 19.15 | 0.4 | 0.35 | 46.50 ± 0.02 | 45.55 ± 0.06 |
| S82X1940 | 23:29:40.28 | −00:17:51.68 | 2.351 | 2.350 | 20.80 | 20.15 | 0.3 | 0.3 | 46.03 ± 0.02 | 44.98 ± 0.06 |
| S82X2058 | 23:31:58.62 | −00:54:10.44 | 2.308 | 2.315 | 19.79 | 19.29 | 0.3 | 0.35 | 46.39 ± 0.02 | 45.54 ± 0.06 |
Notes. Columns give the following information: (1) target identification, (2–3) celestial coordinates, (4) redshift from archival optical spectra, (5) redshift from the peak location of the [OIII]λ5008 in the integrated spectra, (6–7) 2MASS photometric data, (8–9) the radius (in arcsec) of the circular aperture centred on the target used to extract the spectrum for the H and K bands, (10) logarithm of the bolometric luminosity derived from SED fitting (Circosta et al. 2018), and (11) logarithm of the extinction-corrected luminosity at 5100 Å derived from the best-fit values of the power-law model representing the AGN continuum (see Sect. 3).
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