Table 1.
Observed objects in the field of S5 0716+714 (slit 1).
| Slit | RA | Dec | r′ | z | d [arcmin] | d [kpc] | Inf. |
|---|---|---|---|---|---|---|---|
| 1 | 07:21:53.32 | 71:20:36.5 | – | Blazar | – | – | – |
| 2 | 07:21:51.42 | 71:20:10.5 | 20.03 | 0.2634 | – | – | EL, 0.264 (St, By) |
| 3 | 07:21:42.12 | 71:20:24.0 | 20.55 | 0.2564 | – | – | 0.257 (St, By) |
| 4 | 07:21:46.05 | 71:21:49.5 | 21.28 | 0.2306 | 1.36 | 301 | EL |
| 5 | 07:21:33.85 | 71:20:01.4 | 18.82 | 0.2302 | 1.69 | 374 | – |
| 6 | 07:21:40.73 | 71:21:44.5 | 20.62 | 0.2328 | 1.52 | 337 | – |
| 7 | 07:22:19.07 | 71:20:07.4 | 20.56 | 0.2305 | 1.83 | 407 | – |
| 8 | 07:21:22.73 | 71:21:08.7 | 19.87 | 0.2310 | 2.52 | 559 | – |
| 9 | 07:21:57.15 | 71:18:55.0 | 21.00 | 0.2314 | 1.71 | 380 | – |
| 10 | 07:21:55.50 | 71:19:03.0 | 21.56 | 0.2317 | 1.57 | 349 | – |
| 11 | 07:22:09.02 | 71:19:16.6 | 21.12 | 0.2307 | 1.81 | 403 | – |
| 12 | 07:22:26.15 | 71:21:12.3 | 19.06 | 0.2646 | – | – | 0.2643 (Ke) |
| 13 | 07:22:23.53 | 71:21:44.0 | 19.22 | 0.2291 | 2.63 | 644 | 0.2285 (Ke) |
| 14 | 07:22:23.67 | 71:22:18.6 | 19.60 | 0.2283 | 2.96 | 657 | – |
| 15 | 07:22:09.97 | 71:22:38.9 | 21.14 | 0.4873 | – | – | – |
| 16 | 07:22:08.37 | 71:22:06.3 | 21.29 | 0.2061 | – | – | – |
| 17 | 07:21:38.36 | 71:18:55.8 | 20.54 | 0.2281 | 2.09 | 464 | – |
| 18 | 07:22:06.46 | 71:18:15.1 | 21.42 | – | – | – | – |
| 19 | 07:21:52.25 | 71:22:37.1 | 21.10 | 0.2274 | 2.00 | 443 | EL |
| 20 | 07:21:31.66 | 71:22:52.6 | 20.88 | 0.2323 | 2.84 | 630 | EL |
| 21 | 07:21:22.61 | 71:21:37.8 | 21.08 | 0.2306 | 2.63 | 584 | EL |
| 22 | 07:21:37.08 | 71:20:13.2 | 21.38 | 0.2563 | – | – | EL |
| 23 | 07:21:46.27 | 71:21:48.5 | 23.47 | 0.2312 | 1.36 | 301 | EL |
| 24 | 07:21:54.96 | 71:20:11.2 | – | – | – | – | (0.249 By) |
Notes. We provide the following: Col. 1, slit number; Cols. 2 and 3, RA and Dec (J2000.0); Col. 4, r′ integrated magnitude; and Col. 5, measured redshifts. The projected radius to the blazar is indicated in arcminutes (Col. 6) and in kiloparsecs (Col. 7) for the 15 members of the group. Column 8 indicates if the galaxy spectrum shows emission lines (EL). Also indicated in this column are the redshifts obtained by Stickel et al. (1993, St), Bychkova et al. (2006, By), and Keeney et al. (2018, Ke). We note that the last galaxy in the table was only observed by Bychkova et al. (2006).
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