Table 2. Clustering properties of four subsamples with different flux density S90 in the AKARI All-Sky Survey North.
From: Clustering of far-infrared galaxies in the AKARI All-Sky Survey North
limiting S90 [Jy] | Number of galaxies | Median z | A w [deg] | r0 [h−1 Mpc] | γ |
|---|---|---|---|---|---|
0.2 | 8472 | 0.030 |
| 4.49 ± 0.74 | 1.8 ± 0.1 |
0.5 | 5493 | 0.029 | −0.16 ± 0.02 | 4.24 ± 0.41 | 1.9 ± 0.1 |
1.0 | 2233 | 0.022 |
| 4.44 ± 0.54 | 1.9 ± 0.2 |
1.5 | 1282 | 0.018 |
| 4.8 ± 0.36 |
|
