Table 2.

The kurtosis parameter of the stellar mass distribution of the BGGs in observations and SAMs, which are determined with respect to the normal distribution.

Subsample IDmean zobservationsG11DLB07B06
S-I0.22−0.12 ± 0.530.02 ± 0.15−0.19 ± 0.151.00 ± 0.08
S-II0.25−0.07 ± 0.63−0.34 ± 0.22−0.05 ± 0.240.05 ± 0.17
S-III0.551.11 ± 0.560.63 ± 0.20−0.20 ± 0.200.20 ± 0.12
S-IV0.841.69 ± 0.460.07 ± 0.20−0.01 ± 0.140.19 ± 0.12
S-V1.151.74 ± 0.670.48 ±0.25−0.25 ± 0.260.08 ± 0.20
Subsample IDmean zobservationsG11DLB07B06
S-I0.22−0.12 ± 0.530.02 ± 0.15−0.19 ± 0.151.00 ± 0.08
S-II0.25−0.07 ± 0.63−0.34 ± 0.22−0.05 ± 0.240.05 ± 0.17
S-III0.551.11 ± 0.560.63 ± 0.20−0.20 ± 0.200.20 ± 0.12
S-IV0.841.69 ± 0.460.07 ± 0.20−0.01 ± 0.140.19 ± 0.12
S-V1.151.74 ± 0.670.48 ±0.25−0.25 ± 0.260.08 ± 0.20
Table 2.

The kurtosis parameter of the stellar mass distribution of the BGGs in observations and SAMs, which are determined with respect to the normal distribution.

Subsample IDmean zobservationsG11DLB07B06
S-I0.22−0.12 ± 0.530.02 ± 0.15−0.19 ± 0.151.00 ± 0.08
S-II0.25−0.07 ± 0.63−0.34 ± 0.22−0.05 ± 0.240.05 ± 0.17
S-III0.551.11 ± 0.560.63 ± 0.20−0.20 ± 0.200.20 ± 0.12
S-IV0.841.69 ± 0.460.07 ± 0.20−0.01 ± 0.140.19 ± 0.12
S-V1.151.74 ± 0.670.48 ±0.25−0.25 ± 0.260.08 ± 0.20
Subsample IDmean zobservationsG11DLB07B06
S-I0.22−0.12 ± 0.530.02 ± 0.15−0.19 ± 0.151.00 ± 0.08
S-II0.25−0.07 ± 0.63−0.34 ± 0.22−0.05 ± 0.240.05 ± 0.17
S-III0.551.11 ± 0.560.63 ± 0.20−0.20 ± 0.200.20 ± 0.12
S-IV0.841.69 ± 0.460.07 ± 0.20−0.01 ± 0.140.19 ± 0.12
S-V1.151.74 ± 0.670.48 ±0.25−0.25 ± 0.260.08 ± 0.20
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close