Table 3.

The skewness value of the stellar mass distribution of the BGGs in observations and SAMs which are computed with the normal distribution.

Subsample IDmean zobservationsG11DLB07B06
S-I0.22−0.64 ± 0.27−0.37 ± 0.07−0.18 ± 0.07−0.64 ± 0.04
S-II0.25−0.35 ± 0.32−0.31 ± 0.12−0.11 ± 0.12−0.58 ± 0.09
S-III0.55−0.77 ± 0.26−0.28 ± 0.09−0.28 ± 0.10−0.58 ± 0.06
S-IV0.84−1.07 ± 0.23−0.31 ± 0.10−0.40 ± 0.07−0.55 ± 0.06
S-V1.15−1.24 ± 0.34−0.44 ± 0.13−0.15 ± 0.13−0.53 ± 0.10
Subsample IDmean zobservationsG11DLB07B06
S-I0.22−0.64 ± 0.27−0.37 ± 0.07−0.18 ± 0.07−0.64 ± 0.04
S-II0.25−0.35 ± 0.32−0.31 ± 0.12−0.11 ± 0.12−0.58 ± 0.09
S-III0.55−0.77 ± 0.26−0.28 ± 0.09−0.28 ± 0.10−0.58 ± 0.06
S-IV0.84−1.07 ± 0.23−0.31 ± 0.10−0.40 ± 0.07−0.55 ± 0.06
S-V1.15−1.24 ± 0.34−0.44 ± 0.13−0.15 ± 0.13−0.53 ± 0.10
Table 3.

The skewness value of the stellar mass distribution of the BGGs in observations and SAMs which are computed with the normal distribution.

Subsample IDmean zobservationsG11DLB07B06
S-I0.22−0.64 ± 0.27−0.37 ± 0.07−0.18 ± 0.07−0.64 ± 0.04
S-II0.25−0.35 ± 0.32−0.31 ± 0.12−0.11 ± 0.12−0.58 ± 0.09
S-III0.55−0.77 ± 0.26−0.28 ± 0.09−0.28 ± 0.10−0.58 ± 0.06
S-IV0.84−1.07 ± 0.23−0.31 ± 0.10−0.40 ± 0.07−0.55 ± 0.06
S-V1.15−1.24 ± 0.34−0.44 ± 0.13−0.15 ± 0.13−0.53 ± 0.10
Subsample IDmean zobservationsG11DLB07B06
S-I0.22−0.64 ± 0.27−0.37 ± 0.07−0.18 ± 0.07−0.64 ± 0.04
S-II0.25−0.35 ± 0.32−0.31 ± 0.12−0.11 ± 0.12−0.58 ± 0.09
S-III0.55−0.77 ± 0.26−0.28 ± 0.09−0.28 ± 0.10−0.58 ± 0.06
S-IV0.84−1.07 ± 0.23−0.31 ± 0.10−0.40 ± 0.07−0.55 ± 0.06
S-V1.15−1.24 ± 0.34−0.44 ± 0.13−0.15 ± 0.13−0.53 ± 0.10
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