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Table 2

Percentages of compact groups that lie within the boundaries of galaxy groups in redshift-space.

% of GG ALL CG Dom CG No-Dom CG Real CG CA CG






OBS SAM OBS SAM OBS SAM OBS SAM OBS SAM OBS SAM
ALL GG 100 100 27 ± 5 27 ± 3 34 ± 8 22 ± 4 19 ± 6 32 ± 5 35 ± 6 17 ± 4






Low mass GG 33 40 6 ± 2 11 ± 2 6 ± 4 12 ± 4 6 ± 5 9 ± 2 15 ± 3 6 ± 3
9 ± 2 11 ± 1 11 ± 3 9 ± 2 6 ± 2 13 ± 2 14 ± 2 7 ± 2 *






Int mass GG 33 32 14 ± 5 9 ± 2 19 ± 6 7 ± 3 10 ± 5 11 ± 3 12 ± 4 4 ± 2
9 ± 2 9 ± 1 11 ± 3 7 ± 1 6 ± 2 10 ± 2 11 ± 2 5 ± 1 *






High mass GG 34 28 6 ± 2 7 ± 3 9 ± 5 3 ± 2 3 ± 1 12 ± 3 7 ± 4 7 ± 3
9 ± 2 8 ± 1 12 ± 3 6 ± 1 6 ± 2 9 ± 1 10 ± 2 5 ± 1 *






ALL GG+5 100 100 26 ± 5 22 ± 3 31 ± 9 17 ± 4 20 ± 6 24 ± 5 26 ± 6 15 ± 5






Gaussian GG 50 58 13 ± 4 12 ± 2 16 ± 6 9 ± 3 10 ± 5 14 ± 4 14 ± 5 10 ± 4
13 ± 3 13 ± 2 16 ± 5 10 ± 2 10 ± 3 14 ± 3 15 ± 3 9 ± 3 *






Non-Gaussian GG 12 7 2 ± 1 1 ± 1 3 ± 3 0 ± 1 0 ± 1 1 ± 1 0 ± 1 1 ± 1
3 ± 1 2 ± 1 4 ± 1 1 ± 1 2 ± 1 2 ± 1 2 ± 1 1 ± 1 *






Not classified GG 38 35 11 ± 3 9 ± 2 12 ± 6 8 ± 3 10 ± 4 9 ± 3 12 ± 4 4 ± 3
10 ± 2 8 ± 1 12 ± 3 6 ± 1 8 ± 2 8 ± 2 9 ± 2 5 ± 2 *

Notes. Each column represents a different subsample of CGs, while each row represents a different GG subsample (see Sect. 3.1 for a more detailed description of each subsample). Errors were computed with a bootstrap-resampling technique. For each GG subsample, we have included a second row with the expected percentage of embedded compact groups, which is computed considering the size of the GG subsample as the product of the total percentage, quoted in the first row, and the percentage of the GG sample that represents the corresponding subsample, quoted in the first column. OBS: Results obtained from the observational samples. SAM: Results obtained from the semi-analytical samples.

(*)

Rows with the expected percentages of embedded CGs for each subsample of GGs.

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