Table 2.

Observations and predictions for bright subsamples

Statistic	1	2	3	4	5	6	7
sm	0.79	1.11  ± 0.06	1.15  ± 0.06	0.78  ± 0.04	5.3	0.5	−0.4
	0.79	1.06  ± 0.05	1.13  ± 0.06	0.77  ± 0.04	4.9	0.9	−0.8
〈m〉	21.29	21.08  ± 0.06	21.05  ± 0.08	21.25  ± 0.05	−3.7	−0.4	−1.0
	21.29	21.14  ± 0.05	21.06  ± 0.06	21.23  ± 0.05	−2.8	−0.9	−1.1
β	1.34	2.58  ± 0.30	2.70  ± 0.44	1.26  ± 0.20	4.1	0.3	−0.3
	1.43	2.53  ± 0.37	2.78  ± 0.32	1.32  ± 0.25	3.0	0.5	−0.5
ρ1	−0.78	−0.58  ± 0.05	−0.53  ± 0.07	−0.79  ± 0.02	4.5	−0.4	0.2
	−0.77	−0.57  ± 0.05	−0.52  ± 0.06	−0.79  ± 0.02	3.7	0.8	−0.7
ρ2	−0.13	0.20  ± 0.07	0.22  ± 0.10	−0.15  ± 0.06	4.7	0.2	−0.4
	−0.10	0.19  ± 0.09	0.23  ± 0.07	−0.14  ± 0.08	3.2	0.4	−0.5
σ1	1.17	1.13  ± 0.05	1.15  ± 0.07	1.18  ± 0.04	−0.8	0.2	0.3
	1.13	1.09  ± 0.06	1.11  ± 0.04	1.14  ± 0.05	−0.8	0.3	0.2
σ2	0.74	0.96  ± 0.05	0.99  ± 0.07	0.73  ± 0.04	4.4	0.5	−0.3
	0.74	0.91  ± 0.04	0.97  ± 0.05	0.71  ± 0.03	4.4	1.0	−0.8

For each statistic, the upper line is for the subsample of 242 galaxies apparently brighter than magnitude 22.5 and with 0.1 < z ≤ 1.65, and the lower line is for the subsample of 237 galaxies further limited by the constraint z ≤ 1.1.