Table 1
Spectroscopically observed objects.
| Slit | RA (J2000.0) | Dec (J2000.0) |
|
Redshift/velocity | Comment |
| (1) | (2) | (3) | (4) | (5) | (6) |
|
|
|||||
| 1 | 04:49:12.445 | –43:48:26.81 | 20.52 | z = 0.2023 ± 0.0002 | (a+e) merger |
| 2 | 04:49:15.279 | –43:48:18.28 | 20.85 | v = −112 ± 30 km s-1 | (a) star |
| 3 | 04:49:14.687 | –43:50:09.11 | 21.89 | z = 0.5677 ± 0.0001 | (a+e) |
| 4 | 04:49:24.655 | –43:50:10.06 | 14.69 | PKS 0447-439 | |
| 5 | 04:49:22.458 | –43:49:36.00 | 22.46 | z = 0.3463 ± 0.0002 [*] | (a) |
| 6 | 04:49:21.540 | –43:50:32.75 | 22.15 | z = 0.3438 ± 0.0001 [*] | (e) spiral? |
| 7 | 04:49:20.393 | –43:49:08.37 | 22.73 | z = 0.3055 ± 0.0002 | (a) |
| 8 | 04:49:23.399 | –43:50:28.13 | 21.55 | z = 0.3458 ± 0.0001 [*] | (e) interacting |
| 9 | 04:49:23.929 | –43:49:15.51 | 22.87 | z = 0.3153 ± 0.0005 | (a) interacting |
| 10 | 04:49:19.931 | –43:50:33.49 | 20.28 | z = 0.1942 ± 0.0001 | (a+e) |
| 11 | 04:49:30.571 | –43:51:44.91 | 18.70 | v = 303 ± 10 km s-1 | (a) star |
| 12 | 04:49:31.161 | –43:50:18.97 | 21.54 | z = 0.3401 ± 0.0001 [*] | (a) elongated-interacting |
| 13 | 04:49:32.131 | –43:47:59.12 | 21.61 | z = 0.3406 ± 0.0001 [*] | (a) |
| 14 | 04:49:28.429 | –43:52:22.24 | 21.81 | z = 0.3398 ± 0.0001 [*] | (a) |
| 15 | 04:49:27.931 | –43:52:26.44 | 20.79 | z = 0.4155 ± 0.0001 | (a+e) |
| 16 | 04:49:33.070 | –43:49:27.06 | 22.21 | ? | (a+e) spiral-interacting |
| 17 | 04:49:29.962 | –43:49:59.50 | 20.90 | z = 0.0156 ± 0.0001 | (e) elongated |
| 18 | 04:49:26.109 | –43:50:45.69 | 22.35 | z = 0.4076 ± 0.0001 | (a+e) |
| 19 | 04:49:27.256 | –43:49:17.23 | 22.17 | z = 0.3463 ± 0.0002 [*] | (a) |
| 20 | 04:49:34.382 | –43:52:33.67 | 21.71 | z = 0.4133 ± 0.0001 | (a) |
| 21 | 04:49:35.463 | –43:47:52.18 | 21.40 | z = 0.3761 ± 0.0002 | (e+a) spiral? |
| 22 | 04:49:36.763 | –43:49:36.69 | 21.78 | v = 150 ± 20 km s-1 | (a) ? |
Notes. Column 1 gives the slit numbers; Cols. 2 and 3 show RA and Dec (J2000.0); Col. 4 shows the total g′ integrated magnitude; Col. 5 lists the measured redshifts or radial velocity; and Col. 6 indicates whether the redshift was computed using absorption (a), emission lines (e), or both (a+e). This last column also gives a brief description of the observed object.
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