Table 1.
Summary of the target AGN sample.
| ID | RA[J2000] | Dec[J2000] | zspec | SINFONI |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| X_N_128_48 (a) | 02:06:13.54 | −04:05:43.20 | 2.323 | n |
| X_N_81_44 | 02:17:30.95 | −04:18:23.66 | 2.311 | y |
| X_N_53_3 | 02:20:29.84 | −02:56:23.41 | 2.434 | n |
| X_N_6_27 (a) | 02:23:06.32 | −03:39:11.07 | 2.263 | n |
| X_N_44_64 | 02:27:01.46 | −04:05:06.73 | 2.252 | n |
| X_N_102_35 | 02:29:05.94 | −04:02:42.99 | 2.190 | y |
| X_N_104_25 (a) | 02:30:24.46 | −04:09:13.39 | 2.241 | n |
| lid_1852 (a) | 09:58:26.57 | +02:42:30.22 | 2.444 | n |
| lid_3456 (a) | 09:58:38.40 | +01:58:26.83 | 2.146 | n |
| cid_166 | 09:58:58.68 | +02:01:39.22 | 2.448 | y |
| lid_1289 | 09:59:14.65 | +01:36:34.99 | 2.408 | n |
| cid_1605 | 09:59:19.82 | +02:42:38.73 | 2.121 | y |
| cid_337 | 09:59:30.39 | +02:06:56.08 | 2.226 | n |
| cid_346 | 09:59:43.41 | +02:07:07.44 | 2.219 | y |
| cid_357 (a) | 09:59:58.02 | +02:07:55.10 | 2.136 | n |
| cid_451 | 10:00:00.61 | +02:15:31.06 | 2.450 | y |
| cid_1205 | 10:00:02.57 | +02:19:58.68 | 2.255 | y |
| cid_2682 | 10:00:08.81 | +02:06:37.66 | 2.435 | y |
| cid_247 (a) | 10:00:11.23 | +01:52:00.27 | 2.412 | n |
| cid_1215 (a) | 10:00:15.49 | +02:19:44.58 | 2.450 | n |
| cid_467 | 10:00:24.48 | +02:06:19.76 | 2.288 | y |
| cid_852 | 10:00:44.21 | +02:02:06.76 | 2.232 | n |
| cid_970 (a) | 10:00:56.52 | +02:21:42.35 | 2.501 | n |
| cid_971 | 10:00:59.45 | +02:19:57.44 | 2.473 | y |
| cid_38 | 10:01:02.83 | +02:03:16.63 | 2.192 | n |
| lid_206 | 10:01:15.56 | +02:37:43.44 | 2.330 | n |
| cid_1253 | 10:01:30.57 | +02:18:42.57 | 2.147 | y |
Notes. (1) Source identification number from the original source catalogs of Menzel et al. (2016) for the XMM-XXL field, and Civano et al. (2016) for the COSMOS field (see also Sect. 2.1). (2) RA and (3) Dec of optical counterparts: The XMM-XXL targets have an SDSS counterpart whose coordinates are given in Menzel et al. (2016); for the COSMOS field we list the i-band coordinates from Marchesi et al. (2016). (4) Spectroscopic redshift from Menzel et al. (2016) and Marchesi et al. (2016). (5) Good-quality SINFONI data available from SUPER.
These targets were not presented in Circosta et al. (2018).
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