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Table 3.
Galaxy groups in this pilot study.
| Group No. | RA J2000 | Dec J2000 | z | Ng |
|---|---|---|---|---|
| 1 | 21 56 59.76 | +28 00 57.6 | 0.069 | 6 |
| 2 | 03 04 02.64 | −12 04 22.8 | 0.013 | 10 |
| 3 | 10 50 21.60 | +00 16 44.4 | 0.039 | 42 |
| 4 | 01 05 19.44 | +36 00 50.4 | 0.072 | 7 |
| 5 | 02 25 57.12 | +36 59 45.6 | 0.036 | 17 |
| 6 | 01 36 51.36 | −14 00 25.2 | 0.040 | 14 |
| 7 | 23 17 25.68 | +29 02 31.2 | 0.023 | 8 |
| 8 | 16 06 24.00 | +15 40 12.0 | 0.040 | 123 |
| 9 | 16 50 22.32 | +23 35 42.0 | 0.036 | 52 |
| 10 | 13 49 18.96 | −07 13 48.0 | 0.025 | 22 |
| 11 | 21 07 18.24 | −47 10 08.4 | 0.017 | 10 |
| 12 | 13 28 56.88 | −28 02 27.6 | 0.033 | 38 |
| 13 | 02 41 01.92 | +08 46 55.2 | 0.021 | 14 |
Notes. The sample is sorted according to the extent value of each group. Then, each group is identified using a sequential number (col. 1) to simplify their discussion in this paper. Ng is the number of galaxies used to estimate the redshift of candidates.
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