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Table 6

Results of the 2D-DEDICA analysis.

Subclump NS α(J2000), δ(J2000) ρS

TOTmain 219 12 06 11.508 47 57 1.00 103
TOTWNW 102 12 05 49.408 46 44 0.20 29
TOTSEint 38 12 06 24.908 49 37 0.20 16
(TOTESE) 41 12 06 35.008 49 26 0.15 15

R200main 203 12 06 11.508 47 57 1.00 80
R200SEint 30 12 06 24.808 49 40 0.20 17

PASmain 126 12 06 12.208 48 05 1.00 41
PASWNW 44 12 05 51.008 46 30 0.25 12

(HDSrESE) 6 12 06 37.008 49 37 1.00 6
HDSrmain 15 12 06 11.008 47 57 0.67 4

wELG 15 12 06 12.008 47 20 1.00 7

ELGNE 39 12 06 21.808 44 00 1.00 14
ELGNW 30 12 05 57.208 40 38 0.85 11
ELGWNW 24 12 05 42.008 46 34 0.68 9
ELGSE 13 12 06 36.008 52 34 0.58 5
ELGSEext 20 12 06 49.708 54 19 0.43 10
ELGNEext 17 12 06 31.008 38 10 0.31 8
ELGESEext 10 12 06 54.208 48 28 0.31 5

vsELGNE 24 12 06 20.508 44 20 1.00 9
vsELGSEext 15 12 06 49.308 53 13 0.55 4

Notes. Column. 1: subsample/peak ID, labels in parentheses correspond to galaxy peaks that do not completely fulfil the criteria we fixed for galaxy number or density, but are listed here becasue they are discussed in the text; Col. 2: number of assigned member galaxies, NS; Col. 3: RA and Dec of the density peak; Col. 4: relative density with respect to the highest peak, ρS; Col. 5: χ2 value of the peak. For each population, the number of peaks is summarized in Table 4 (Col. 7).

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