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Table B.2.

Substructure of clusters.

(1) (2) (3) (4) (5) (6) (7) (8) (9)
No. Ngal R.A. Dec. Distmed zmed logSFRmed Dn(4000)med ID
A1656
1 295 194.9 27.75 67.02 0.022 -1.75 1.72 1;SE
2 60 194.8 28.89 73.24 0.024 -1.52 1.67 3,4;N
3 119 195.5 28.10 63.75 0.020 -1.75 1.72 SE
4 48 193.2 27.37 70.84 0.023 -1.62 1.64 W
5 158 194.2 27.48 74.49 0.024 -1.53 1.65 2,3;W
A1367
1 178 176.1 19.84 65.34 0.021 -1.54 1.60 1
2 67 176.3 20.32 74.84 0.024 -1.18 1.46 2
A1185
1 91 167.7 28.69 99.0 0.032 -1.26 1.62 1
2 23 168.0 27.57 105.1 0.034 -1.53 1.76 3
3 27 166.8 28.66 100.0 0.032 -0.56 1.25 2
4 60 167.7 28.26 108.5 0.035 -1.01 1.57

Notes. Columns are as follows: (1): Component number; (2): Number of galaxies in a component; (3-4): Median Right Ascension (R.A.) and Declination (Dec.) of galaxies in a component (in degrees); (5): Median uncorrected distance of galaxies in a component, Distmed, in h−1 Mpc; (6): Median observed redshift of galaxies in a component, zmed; (7): Median value of star formation rate of galaxies in a component, logSFRmed; (8): Median value of Dn(4000) index of galaxies in a component, Dn(4000)med; (9): identification of a component with structures from other studies. Numbers are numbers of partner clusters from WH24m catalogue (Table B.1). W, N, and SE denotes endpoints of filaments as identified in HyeongHan et al. (2024).

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