Table 1
Results from the Sérsic fits for those 13 UCDs that have half-light radii larger than the resolution limit of 23 pc.
| Name | Namealt | RA | Dec | V | Reff | n | (V−I) | v |
| (h:m:s) | (°:′:′′) | (mag) | (pc) | mag | (km s-1) | |||
|
|
||||||||
| UCD-FORS 1 | 1_0630 | 3:38:56.14 | –35:24:49.0 | 20.31 ± 0.004 | 28.10 ± 0.16 | 3.32 ± 0.06 | 1.02 ± 0.07 | 666 ± 48 |
| UCD-FORS 2 | Y99025 a | 3:38:58.55 | –35:26:26.0 | 20.21 ± 0.012 | 34.68 ± 0.76 | 4.85 ± 0.17 | 0.96 ± 0.04 | 1070 ± 38 |
| UCD-FORS 4 | 2_2115 | 3:38:49.18 | –35:21:42.1 | 20.96 ± 0.003 | 23.70 ± 0.15 | 2.44 ± 0.05 | 1.19 ± 0.07 | 864 ± 79 |
| UCD-FORS 32 | UCD6 | 3:38:05.04 | –35:24:09.7 | 19.15 ± 0.001 | 33.27 ± 0.07 | 0.94 ± 0.01 | 1.13 ± 0.11 | 1220 ± 45 |
| UCD-FORS 36 | UCDm | 3:38:06.48 | –35:23:03.8 | 20.00 ± 0.002 | 25.06 ± 0.08 | 4.09± 0.04 | 1.00 ± 0.04 | 1442 ± 123 |
| UCD-FORS 45 | UCD28 | 3:38:10.73 | –35:25:46.2 | 19.97 ± 0.003 | 33.83 ± 0.14 | 3.81 ± 0.03 | 1.29 ± 0.04 | 1715 ± 90 |
| UCD-FORS 48 | UCD31 | 3:38:16.51 | –35:26:19.3 | 20.60 ± 0.008 | 25.88 ± 0.29 | 4.41 ± 0.13 | 0.95 ± 0.05 | 899 ± 85 |
| UCD-FORS 50 | 1_2095 | 3:38:33.82 | –35:25:57.0 | 20.61 ± 0.007 | 24.05 ± 0.24 | 4.56 ± 0.13 | 1.10 ± 0.04 | 1223 ± 221 |
| UCD-FORS 52 | 2_2127 | 3:38:11.69 | –35:27:16.2 | 20.81 ± 0.02 | 44.41 ± 2.47 | 9.05 ± 0.38 | 1.16 ± 0.06 | 1443 ± 131 |
| UCD-FORS 56 | Y10056 | 3:38:38.77 | –35:25:55.2 | 21.18 ± 0.033 | 36.72 ± 2.37 | 5.44 ± 0.42 | 1.26 ± 0.07 | 1062 ± 105 |
| UCD-FORS 71 | Y10048 | 3:38:35.23 | –35:25:39.2 | 22.05 ± 0.015 | 24.85 ± 0.51 | 2.71 ± 0.20 | 1.09 ± 0.04 | 1601 ± 30 |
| UCD-FORS 81 | UCD2 b | 3:38:06.29 | –35:28:58.8 | 19.31 ± 0.048 | 37.82 ± 2.58 | 2.03 ± 0.33 | 1.13 ± 0.11 | 1249 ± 37 |
| UCD-FORS 84 | 2_2072 c | 3:38:14.69 | –35:33:40.7 | 20.77 ± 0.001 | 41.85 ± 0.11 | 1.96 ± 0.01 | 0.89 ± 0.05 | 1448 ± 176 |
Notes. The (V−I) colors and radial velocities are taken from the respective original samples. The provided errors on Reff and n are those given by GALFIT, which should be taken with caution because close to the resolution limit these errors might be underestimated. The alternative object names from the literature are from the following sources: for UCDx Firth et al. (2007), X−xxxMieske et al. (2002, 2004), Yxxx references Richtler et al. (2008). Some of these objects were also presented in Richtler et al. (2005) with the following names: .
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