Table 4.

We show the best-fitting value of r0 for each M − z bin with the corresponding error, χ2 and p-value. We correct for varying β(z) according to equation (4). We fit between 5 < s (h−1 Mpc) < 55, each bin having 10 df.. We include measurements of ξ20 (Section 6.4), bias and dark matter halo mass (Section 6.4.1).

Redshift rangezAbsolute magnitude rangeMi(z = 2)Best r0χ2p-valueξ20bMDM × 1012h−1 M
(median)Mi(z = 2)(median)
0.3 < z < 0.80.53−23.5 < Mi < −22.3−23.06|$4.2^{+0.65}_{-0.8}$|11.960.290.18 ± 0.06
0.8 < z < 1.40.99−23.5 < Mi < −22.3−23.18|$5.65^{+1.0}_{-1.2}$|5.950.820.39 ± 0.111.79 ± 0.29|$3.60_{- 2.19}^{+ 3.54}$|
0.3 < z < 0.80.63−24.5 < Mi < −23.5−23.93|$4.05^{+0.8}_{-1.05}$|8.70.560.25 ± 0.081.13 ± 0.21|$0.71_{- 0.62}^{+ 1.60}$|
0.8 < z < 1.41.10−24.5 < Mi < −23.5−24.04|$5.65^{+0.7}_{-0.8}$|8.910.540.29 ± 0.081.58 ± 0.24|$1.40_{- 0.90}^{+ 1.55}$|
1.4 < z < 1.91.61−24.5 < Mi < −23.5−24.15|$7.1^{+0.8}_{-0.9}$|10.770.380.40 ± 0.102.39 ± 0.33|$2.87_{- 1.43}^{+ 2.08}$|
1.9 < z < 2.92.02−24.5 < Mi < −23.5−24.31|$9.1^{+2.7}_{-3.65}$|9.260.511.08 ± 0.434.79 ± 0.96|$17.17_{- 9.23}^{+13.35}$|
0.3 < z < 0.80.69−25.5 < Mi < −24.5−24.84|$4.4^{+1.5}_{-2.1}$|13.00.220.37 ± 0.151.51 ± 0.34|$3.62_{- 2.92}^{+ 6.18}$|
0.8 < z < 1.41.07−25.5 < Mi < −24.5−25.09|$4.3^{+0.7}_{-0.75}$|13.980.170.21 ± 0.061.29 ± 0.21|$0.42_{- 0.33}^{+ 0.72}$|
1.4 < z < 1.91.65−25.5 < Mi < −24.5−24.99|$5.6^{+0.7}_{-0.85}$|8.840.550.36 ± 0.082.28 ± 0.27|$2.10_{- 0.96}^{+ 1.35}$|
1.9 < z < 2.92.11−25.5 < Mi < −24.5−25.07|$6.55^{+0.95}_{-1.1}$|5.520.850.33 ± 0.112.60 ± 0.44|$1.36_{- 0.81}^{+ 1.33}$|
0.8 < z < 1.41.21−28.5 < Mi < −25.5−25.94|$5.85^{+0.6}_{-0.6}$|9.080.520.34 ± 0.071.84 ± 0.21|$2.27_{- 1.06}^{+ 1.52}$|
1.4 < z < 1.91.67−28.5 < Mi < −25.5−26.27|$5.85^{+0.35}_{-0.4}$|16.980.070.37 ± 0.042.35 ± 0.15|$2.28_{- 0.59}^{+ 0.71}$|
1.9 < z < 2.92.19−28.5 < Mi < −25.5−26.58|$6.2^{+0.45}_{-0.5}$|7.630.670.39 ± 0.052.91 ± 0.20|$1.90_{- 0.51}^{+ 0.62}$|
Redshift rangezAbsolute magnitude rangeMi(z = 2)Best r0χ2p-valueξ20bMDM × 1012h−1 M
(median)Mi(z = 2)(median)
0.3 < z < 0.80.53−23.5 < Mi < −22.3−23.06|$4.2^{+0.65}_{-0.8}$|11.960.290.18 ± 0.06
0.8 < z < 1.40.99−23.5 < Mi < −22.3−23.18|$5.65^{+1.0}_{-1.2}$|5.950.820.39 ± 0.111.79 ± 0.29|$3.60_{- 2.19}^{+ 3.54}$|
0.3 < z < 0.80.63−24.5 < Mi < −23.5−23.93|$4.05^{+0.8}_{-1.05}$|8.70.560.25 ± 0.081.13 ± 0.21|$0.71_{- 0.62}^{+ 1.60}$|
0.8 < z < 1.41.10−24.5 < Mi < −23.5−24.04|$5.65^{+0.7}_{-0.8}$|8.910.540.29 ± 0.081.58 ± 0.24|$1.40_{- 0.90}^{+ 1.55}$|
1.4 < z < 1.91.61−24.5 < Mi < −23.5−24.15|$7.1^{+0.8}_{-0.9}$|10.770.380.40 ± 0.102.39 ± 0.33|$2.87_{- 1.43}^{+ 2.08}$|
1.9 < z < 2.92.02−24.5 < Mi < −23.5−24.31|$9.1^{+2.7}_{-3.65}$|9.260.511.08 ± 0.434.79 ± 0.96|$17.17_{- 9.23}^{+13.35}$|
0.3 < z < 0.80.69−25.5 < Mi < −24.5−24.84|$4.4^{+1.5}_{-2.1}$|13.00.220.37 ± 0.151.51 ± 0.34|$3.62_{- 2.92}^{+ 6.18}$|
0.8 < z < 1.41.07−25.5 < Mi < −24.5−25.09|$4.3^{+0.7}_{-0.75}$|13.980.170.21 ± 0.061.29 ± 0.21|$0.42_{- 0.33}^{+ 0.72}$|
1.4 < z < 1.91.65−25.5 < Mi < −24.5−24.99|$5.6^{+0.7}_{-0.85}$|8.840.550.36 ± 0.082.28 ± 0.27|$2.10_{- 0.96}^{+ 1.35}$|
1.9 < z < 2.92.11−25.5 < Mi < −24.5−25.07|$6.55^{+0.95}_{-1.1}$|5.520.850.33 ± 0.112.60 ± 0.44|$1.36_{- 0.81}^{+ 1.33}$|
0.8 < z < 1.41.21−28.5 < Mi < −25.5−25.94|$5.85^{+0.6}_{-0.6}$|9.080.520.34 ± 0.071.84 ± 0.21|$2.27_{- 1.06}^{+ 1.52}$|
1.4 < z < 1.91.67−28.5 < Mi < −25.5−26.27|$5.85^{+0.35}_{-0.4}$|16.980.070.37 ± 0.042.35 ± 0.15|$2.28_{- 0.59}^{+ 0.71}$|
1.9 < z < 2.92.19−28.5 < Mi < −25.5−26.58|$6.2^{+0.45}_{-0.5}$|7.630.670.39 ± 0.052.91 ± 0.20|$1.90_{- 0.51}^{+ 0.62}$|
Table 4.

We show the best-fitting value of r0 for each M − z bin with the corresponding error, χ2 and p-value. We correct for varying β(z) according to equation (4). We fit between 5 < s (h−1 Mpc) < 55, each bin having 10 df.. We include measurements of ξ20 (Section 6.4), bias and dark matter halo mass (Section 6.4.1).

Redshift rangezAbsolute magnitude rangeMi(z = 2)Best r0χ2p-valueξ20bMDM × 1012h−1 M
(median)Mi(z = 2)(median)
0.3 < z < 0.80.53−23.5 < Mi < −22.3−23.06|$4.2^{+0.65}_{-0.8}$|11.960.290.18 ± 0.06
0.8 < z < 1.40.99−23.5 < Mi < −22.3−23.18|$5.65^{+1.0}_{-1.2}$|5.950.820.39 ± 0.111.79 ± 0.29|$3.60_{- 2.19}^{+ 3.54}$|
0.3 < z < 0.80.63−24.5 < Mi < −23.5−23.93|$4.05^{+0.8}_{-1.05}$|8.70.560.25 ± 0.081.13 ± 0.21|$0.71_{- 0.62}^{+ 1.60}$|
0.8 < z < 1.41.10−24.5 < Mi < −23.5−24.04|$5.65^{+0.7}_{-0.8}$|8.910.540.29 ± 0.081.58 ± 0.24|$1.40_{- 0.90}^{+ 1.55}$|
1.4 < z < 1.91.61−24.5 < Mi < −23.5−24.15|$7.1^{+0.8}_{-0.9}$|10.770.380.40 ± 0.102.39 ± 0.33|$2.87_{- 1.43}^{+ 2.08}$|
1.9 < z < 2.92.02−24.5 < Mi < −23.5−24.31|$9.1^{+2.7}_{-3.65}$|9.260.511.08 ± 0.434.79 ± 0.96|$17.17_{- 9.23}^{+13.35}$|
0.3 < z < 0.80.69−25.5 < Mi < −24.5−24.84|$4.4^{+1.5}_{-2.1}$|13.00.220.37 ± 0.151.51 ± 0.34|$3.62_{- 2.92}^{+ 6.18}$|
0.8 < z < 1.41.07−25.5 < Mi < −24.5−25.09|$4.3^{+0.7}_{-0.75}$|13.980.170.21 ± 0.061.29 ± 0.21|$0.42_{- 0.33}^{+ 0.72}$|
1.4 < z < 1.91.65−25.5 < Mi < −24.5−24.99|$5.6^{+0.7}_{-0.85}$|8.840.550.36 ± 0.082.28 ± 0.27|$2.10_{- 0.96}^{+ 1.35}$|
1.9 < z < 2.92.11−25.5 < Mi < −24.5−25.07|$6.55^{+0.95}_{-1.1}$|5.520.850.33 ± 0.112.60 ± 0.44|$1.36_{- 0.81}^{+ 1.33}$|
0.8 < z < 1.41.21−28.5 < Mi < −25.5−25.94|$5.85^{+0.6}_{-0.6}$|9.080.520.34 ± 0.071.84 ± 0.21|$2.27_{- 1.06}^{+ 1.52}$|
1.4 < z < 1.91.67−28.5 < Mi < −25.5−26.27|$5.85^{+0.35}_{-0.4}$|16.980.070.37 ± 0.042.35 ± 0.15|$2.28_{- 0.59}^{+ 0.71}$|
1.9 < z < 2.92.19−28.5 < Mi < −25.5−26.58|$6.2^{+0.45}_{-0.5}$|7.630.670.39 ± 0.052.91 ± 0.20|$1.90_{- 0.51}^{+ 0.62}$|
Redshift rangezAbsolute magnitude rangeMi(z = 2)Best r0χ2p-valueξ20bMDM × 1012h−1 M
(median)Mi(z = 2)(median)
0.3 < z < 0.80.53−23.5 < Mi < −22.3−23.06|$4.2^{+0.65}_{-0.8}$|11.960.290.18 ± 0.06
0.8 < z < 1.40.99−23.5 < Mi < −22.3−23.18|$5.65^{+1.0}_{-1.2}$|5.950.820.39 ± 0.111.79 ± 0.29|$3.60_{- 2.19}^{+ 3.54}$|
0.3 < z < 0.80.63−24.5 < Mi < −23.5−23.93|$4.05^{+0.8}_{-1.05}$|8.70.560.25 ± 0.081.13 ± 0.21|$0.71_{- 0.62}^{+ 1.60}$|
0.8 < z < 1.41.10−24.5 < Mi < −23.5−24.04|$5.65^{+0.7}_{-0.8}$|8.910.540.29 ± 0.081.58 ± 0.24|$1.40_{- 0.90}^{+ 1.55}$|
1.4 < z < 1.91.61−24.5 < Mi < −23.5−24.15|$7.1^{+0.8}_{-0.9}$|10.770.380.40 ± 0.102.39 ± 0.33|$2.87_{- 1.43}^{+ 2.08}$|
1.9 < z < 2.92.02−24.5 < Mi < −23.5−24.31|$9.1^{+2.7}_{-3.65}$|9.260.511.08 ± 0.434.79 ± 0.96|$17.17_{- 9.23}^{+13.35}$|
0.3 < z < 0.80.69−25.5 < Mi < −24.5−24.84|$4.4^{+1.5}_{-2.1}$|13.00.220.37 ± 0.151.51 ± 0.34|$3.62_{- 2.92}^{+ 6.18}$|
0.8 < z < 1.41.07−25.5 < Mi < −24.5−25.09|$4.3^{+0.7}_{-0.75}$|13.980.170.21 ± 0.061.29 ± 0.21|$0.42_{- 0.33}^{+ 0.72}$|
1.4 < z < 1.91.65−25.5 < Mi < −24.5−24.99|$5.6^{+0.7}_{-0.85}$|8.840.550.36 ± 0.082.28 ± 0.27|$2.10_{- 0.96}^{+ 1.35}$|
1.9 < z < 2.92.11−25.5 < Mi < −24.5−25.07|$6.55^{+0.95}_{-1.1}$|5.520.850.33 ± 0.112.60 ± 0.44|$1.36_{- 0.81}^{+ 1.33}$|
0.8 < z < 1.41.21−28.5 < Mi < −25.5−25.94|$5.85^{+0.6}_{-0.6}$|9.080.520.34 ± 0.071.84 ± 0.21|$2.27_{- 1.06}^{+ 1.52}$|
1.4 < z < 1.91.67−28.5 < Mi < −25.5−26.27|$5.85^{+0.35}_{-0.4}$|16.980.070.37 ± 0.042.35 ± 0.15|$2.28_{- 0.59}^{+ 0.71}$|
1.9 < z < 2.92.19−28.5 < Mi < −25.5−26.58|$6.2^{+0.45}_{-0.5}$|7.630.670.39 ± 0.052.91 ± 0.20|$1.90_{- 0.51}^{+ 0.62}$|
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