NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at 1.5 < z < 4 in the COSMOS field

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Table G.1.

Concentration parameters for all groups.

Structure	Concentration	Prediction^a
HPC1001	$44_{- 42}^{+ 21}$ $44^{+21}_{-42}$	21 ± 4
SBCX3	$13_{- 10}^{+ 16}$ $13^{+16}_{-10}$	20 ± 4
SBCX4	$55_{- 39}^{+ 23}$ $55^{+23}_{-39}$	15 ± 3
SBCX1	$55_{- 44}^{+ 23}$ $55^{+23}_{-44}$	13 ± 3
SBCX7	$33_{- 15}^{+ 21}$ $33^{+21}_{-15}$	13 ± 3
SBC3	$46_{- 46}^{+ 26}$ $46^{+26}_{-46}$	13 ± 3
SBC6	$28_{- 21}^{+ 22}$ $28^{+22}_{-21}$	13 ± 3
SBC4	$60_{- 35}^{+ 19}$ $60^{+19}_{-35}$	10 ± 2

Notes:^apredicted concentration using concentration, halo mass, and redshift relation from Ludlow et al. (2016).

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