Table 2.
SDSS luminosity-limited samples.
| Sample | Mr | Ngal | dmax | r0 | ξ6 |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| SDSS.18b | −18.0 | 16 676 | 135 | 6.41 ± 0.42 | 1.108 |
| SDSS.19b | −19.0 | 49 963 | 211 | 6.31 ± 0.24 | 1.100 |
| SDSS.20b | −20.0 | 105 088 | 323 | 7.20 ± 0.19 | 1.359 |
| SDSS.21b | −21.0 | 98 674 | 486 | 7.93 ± 0.21 | 1.599 |
| SDSS.22b | −22.0 | 9430 | 571 | 11.45 ± 0.99 | 3.304 |
| SDSS.18t | −18.0 | 39 711 | 135 | 6.55 ± 0.28 | 1.156 |
| SDSS.19t | −19.0 | 88 132 | 211 | 6.56 ± 0.19 | 1.165 |
| SDSS.20t | −20.0 | 134 431 | 323 | 7.46 ± 0.17 | 1.447 |
| SDSS.21t | −21.0 | 104 512 | 486 | 8.14 ± 0.21 | 1.675 |
| SDSS.22t | −22.0 | 9525 | 571 | 11.32 ± 0.97 | 3.444 |
Notes. The columns show the (1) sample name; (2) the absolute r-magnitude limit, Mr − 5 log h; (3) the number of galaxies in a sample; (4) the maximum comoving distance dmax in h−1 Mpc; (5) the correlation length of the sample r0 in h−1 Mpc; and (6) the correlation function amplitude ξ6 at r6 = 6 h−1 Mpc.
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