Table 1
Properties of our target galaxies.
Source id1 | RA (J2000) | Dec (J2000) | V (2) | [4.5]3 | Mask4 | z spec 5 | Quality6 |
|
|||||||
26113 | 02:16:49.49 | –05:14:41.01 | 24.73 ± 0.11 | 22.26 ± 0.10 | 2 | ? | |
27497 | 02:16:37.35 | –05:14:01.73 | 23.16 ± 0.10 | 22.56 ± 0.10 | 2 | ? | |
30555 | 02:16:47.57 | –05:12:33.97 | 23.45 ± 0.10 | 21.69 ± 0.10 | 2 | 2.640 | a |
31369 | 02:16:48.60 | –05:12:11.51 | 24.45 ± 0.11 | 22.97 ± 0.10 | 2 | 0.569 | em |
33199 | 02:16:38.56 | –05:11:30.00 | 24.94 ± 0.12 | 22.06 ± 0.10 | 2 | ? | |
34743 | 02:16:38.62 | –05:10:43.03 | 23.73 ± 0.11 | 22.02 ± 0.10 | 2 | 3.186 | a |
36718 | 02:16:50.81 | –05:09:49.88 | 24.14 ± 0.11 | 21.35 ± 0.10 | 2 | 3.209 | b |
37262 | 02:16:51.08 | –05:09:33.06 | 24.04 ± 0.11 | 23.37 ± 0.10 | 2 | 2.934 | b |
38729 | 02:16:39.44 | –05:08:51.60 | 24.45 ± 0.11 | 23.00 ± 0.10 | 2 | 2.611 | a |
86032 | 02:17:19.47 | –04:48:09.77 | 24.35 ± 0.11 | 21.86 ± 0.10 | 1 | 2.696 | c |
86588 | 02:17:29.47 | –04:47:51.52 | 24.98 ± 0.12 | 22.25 ± 0.10 | 1 | ? | |
89190 | 02:17:19.80 | –04:46:22.59 | 24.99 ± 0.12 | 22.18 ± 0.10 | 1 | ? | |
92077 | 02:17:33.44 | –04:44:44.35 | 23.57 ± 0.10 | 23.07 ± 0.10 | 1 | > 3.930† | c |
93334 | 02:17:32.06 | –04:43:59.80 | 24.40 ± 0.11 | 23.14 ± 0.10 | 1 | ? | |
94370 | 02:17:35.01 | –04:43:18.91 | 24.40 ± 0.11 | 22.84 ± 0.10 | 1 | 2.076 | em/c |
94971 | 02:17:35.57 | –04:42:59.59 | 24.87 ± 0.10 | 21.42 ± 0.10 | 1 | 3.100 | em/a |
95692 | 02:17:35.95 | –04:42:33.64 | 22.57 ± 0.10 | 20.13 ± 0.10 | 1 | 3.284 | a |
96259 | 02:17:31.46 | –04:42:10.74 | 25.00 ± 0.12 | 21.85 ± 0.10 | 1 | ? | |
|
|||||||
25668 | 02:16:47.93 | –05:14:54.43 | 24.35 ± 0.11 | 24.18 ± 0.10 | 2 | 3.437 | em |
97267 | 02:17:34.97 | –04:41:29.23 | 24.46 ± 0.11 | 22.76 ± 0.10 | 1 | 3.090 | c |
Notes. Properties of our target galaxies. Mask fillers that appeared to have zspec > 2.5 are included below the line.
redshift quality flag: (a) secure redshift, (b) very likely redshift but not completely secure, (c) plausible redshift but not secure, (em) redshift based on a single emission line.
Because we only see the Lyman α forest, we are unable to determine the redshift and can only give a lower limit, see also Sect. 3.2.
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