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Table 3.
Millennium luminosity-limited galaxy samples.
| Sample | Mr | Ngal | r0 | ξ6 |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| Mill.18b | −18.0 | 829 725 | 5.45 ± 0.05 | 0.907 |
| Mill.19b | −19.0 | 1 022 303 | 5.70 ± 0.03 | 0.954 |
| Mill.20b | −20.0 | 1 209 900 | 5.60 ± 0.04 | 0.955 |
| Mill.21b | −21.0 | 568 705 | 5.44 ± 0.06 | 0.902 |
| Mill.22b | −22.0 | 98 575 | 6.54 ± 0.18 | 1.176 |
| Mill.23b | −23.0 | 5414 | 12.8 ± 1.46 | 3.574 |
| Mill.20.0t | −20.0 | 1 882 809 | 5.79 ± 0.04 | 0.952 |
| Mill.20.5t | −20.5 | 1 183 825 | 5.81 ± 0.04 | 0.956 |
| Mill.21.0t | −21.0 | 672 909 | 5.81 ± 0.06 | 0.956 |
| Mill.21.5t | −21.5 | 309 580 | 6.13 ± 0.09 | 1.033 |
| Mill.22.0t | −22.0 | 104 204 | 6.84 ± 0.18 | 1.271 |
| Mill.23.0t | −23.0 | 5629 | 12.9 ± 1.44 | 3.766 |
Notes. The columns show the (1) sample name; (2) the absolute r-magnitude limit, Mr; (3) the number of galaxies in a sample; (4) the correlation length of the sample r0 in h−1 Mpc; and (5) the correlation function amplitude at ξ6.
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