Table 2
Properties of the detected background or foreground galaxies in the observed field.
| ID | RA (J2000) | Dec (J2000) | F775W | z | QF | z prev | IDref. |
|
|
|||||||
| 35 | 22:48:43.394 | –44:32:47.28 | 23.33 | 0.153 | 1 | – | – |
| 36 | 22:48:41.195 | –44:31:44.24 | 23.47 | 0.160 | 1 | – | – |
| 37 | 22:48:39.980 | –44:32:24.75 | 22.14 | 0.459 | 1 | – | – |
| 38 | 22:48:41.767 | –44:31:56.80 | 18.79 | 0.607 | 1 | 0.610 | 878 (3) |
| 39 | 22:48:45.288 | –44:32:16.38 | 22.86 | 0.611 | 1 | – | – |
| 40 | 22:48:44.260 | –44:32:22.46 | 24.09 | 0.652 | 1 | – | – |
| 41 | 22:48:43.019 | –44:32:31.90 | 26.73 | 0.698 | 1 | – | – |
| 42 | 22:48:43.233 | –44:32:38.65 | 25.31 | 0.714 | 1 | – | 667 (3) |
| 43a | 22:48:41.302 | –44:31:49.86 | 26.21 | 1.035 | 1 | – | 7a (2) |
| 43b | 22:48:42.234 | –44:32:10.13 | – | 1.035 | 1 | – | 7b (2) |
| 43c | 22:48:43.366 | –44:32:19.16 | – | 1.035 | 1 | – | 7c (2) |
| 44 | 22:48:41.407 | –44:32:28.61 | 23.09 | 1.269 | 2 | 1.270 | (1) |
| 45 | 22:48:42.125 | –44:32:44.08 | 23.77 | 1.269 | 9 | 1.269 | A (6) |
| 46a | 22:48:45.223 | –44:32:23.88 | 22.05 | 1.428 | 1 | 1.429 | 6a/2.1 (1, 2, 5, 6) |
| 46b | 22:48:42.199 | –44:31:57.29 | – | 1.428 | 1 | 1.429 | 6b/2.2 (2, 5) |
| 46c | 22:48:41.781 | –44:31:42.39 | 22.63 | 1.428 | 1 | 1.429 | 6c/2.3 (2, 5, 6) |
| 47 | 22:48:42.477 | –44:32:46.77 | 24.85 | 1.477 | 9 | – | – |
| 48 | 22:48:38.723 | –44:32:18.05 | – | 2.577 | 9 | 2.576 | (4) |
| 49a | 22:48:42.011 | –44:32:27.69 | 25.50 | 3.116 | 1 | 3.117 | 11.1 (2, 6) |
| 49b | 22:48:41.564 | –44:32:24.01 | 25.33 | 3.116 | 1 | 3.110 | 11b (1, 2) |
| 50 | 22:48:38.939 | –44:32:17.85 | 24.14 | 3.117 | 1 | – | – |
| 51 | 22:48:41.764 | –44:32:28.47 | 25.72 | 3.228 | 1 | – | – |
| 52a | 22:48:42.984 | –44:32:19.08 | 26.92 | 4.113 | 1 | – | – |
| 52b | 22:48:43.593 | –44:32:21.71 | 26.32 | 4.113 | 1 | – | – |
| 53a | 22:48:43.449 | –44:32:04.56 | – | 6.107 | 1 | 6.107-6.110 | ID2/6.2 (1, 2, 5, 6) |
| 53b | 22:48:45.827 | –44:32:14.62 | – | 6.107 | 1 | 6.107-6.110 | ID3/6.3 (1, 2, 5, 6) |
| 53c | 22:48:44.177 | –44:32:07.14 | – | 6.107 | 9 | – | – |
|
|
|||||||
| 54 | 22:48:44.579 | –44.32.18.78 | 23.35 | ? | – | – | |
| 55 | 22:48:40.581 | –44:32:25.44 | 23.03 | ? | – | – | |
| 56 | 22:48:41.320 | –44:32:35.30 | 23.24 | ? | – | – | |
| 57 | 22:48:43.978 | –44:32:37.88 | 22.54 | ? | – | – | |
| 58 | 22:48:41.465 | –44:32:43.63 | 22.91 | ? | – | – | |
|
|
|||||||
| 60 | 22:48:43.184 | –44:32:08.16 | – | ? | – | – | |
| 61 | 22:48:41.908 | –44:32:13.18 | – | ? | – | – | |
| 62 | 22:48:43.673 | –44:32:18.89 | 22.89 | ? | – | – | |
| 63 | 22:48:44.371 | –44:32:26.35 | 23.27 | ? | – | – | |
| 64 | 22:48:44.534 | –44:32:18.92 | 23.35 | ? | – | – | |
Notes. The columns are the same as the first eight columns in Table 1, but the redshifts and IDs in the seventh and eighth column refer to different studies (1 = Balestra et al. 2013; 2 = Monna et al. 2014; 3 = Gómez et al. 2012; 4 = Balestra et al. in prep.; 5 = Richard et al. 2014a; 6 = Johnson et al. 2014). We added a quality flag in column six: 9 means that the redshift is based on a single emission line, although for [O ii] the profile is also taken into account. Galaxies with IDs 54-58 show flat and featureless continuums, and are identified in the 3D datacube. Because of the featureless continuum, we are unable to determine the redshift for these galaxies. Sources with IDs higher than 60 are only seen in several narrowband images created with the MUSE data and are not found in the 3D datacube. Therefore, they do not have an extracted spectrum or redshift determination.
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