Table 1.

Comparing LRG HOD model extensions in both redshift bins. The baseline model refers to the standard vanilla 5-parameter model plus velocity bias and incompleteness. A refers to galaxy assembly bias parametrized in terms of halo concentration. B refers to galaxy assembly bias parametrized in terms of the local environment. s refers to 1-halo satellite profile modulations. The AIC scores suggest that none of the extended models are preferred over the baseline model. More details of the best-fits are given in Table 3.

LRG0.4 < z < 0.60.6 < z < 0.8
Modelχ2/d.o.f.AICχ2/d.o.f.AIC
Baseline1.031300.99125
Baseline + A1.051330.98125
Baseline + B1.051330.99126
Baseline + s1.061311.01126
LRG0.4 < z < 0.60.6 < z < 0.8
Modelχ2/d.o.f.AICχ2/d.o.f.AIC
Baseline1.031300.99125
Baseline + A1.051330.98125
Baseline + B1.051330.99126
Baseline + s1.061311.01126
Table 1.

Comparing LRG HOD model extensions in both redshift bins. The baseline model refers to the standard vanilla 5-parameter model plus velocity bias and incompleteness. A refers to galaxy assembly bias parametrized in terms of halo concentration. B refers to galaxy assembly bias parametrized in terms of the local environment. s refers to 1-halo satellite profile modulations. The AIC scores suggest that none of the extended models are preferred over the baseline model. More details of the best-fits are given in Table 3.

LRG0.4 < z < 0.60.6 < z < 0.8
Modelχ2/d.o.f.AICχ2/d.o.f.AIC
Baseline1.031300.99125
Baseline + A1.051330.98125
Baseline + B1.051330.99126
Baseline + s1.061311.01126
LRG0.4 < z < 0.60.6 < z < 0.8
Modelχ2/d.o.f.AICχ2/d.o.f.AIC
Baseline1.031300.99125
Baseline + A1.051330.98125
Baseline + B1.051330.99126
Baseline + s1.061311.01126
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