Table 1.
Best-fit values and marginalised errors of the parameters in the modified Schechter functions derived from fitting to our measurements only (based on the de-blended catalogue in COSMOS).
| Redshift range | ϕ* | L* | N |
|---|---|---|---|
| 0.0 < z < 0.3 |  |
 |
2932 |
| 0.3 < z < 0.45 |  |
 |
7990 |
| 0.45 < z < 0.6 |  |
 |
9113 |
| 0.6 < z < 0.8 |  |
 |
18660 |
| 0.8 < z < 1.0 |  |
 |
26469 |
| 1.0 < z < 1.2 |  |
 |
21127 |
| 1.2 < z < 1.7 |  |
 |
36380 |
| 1.7 < z < 2.0 |  |
 |
15491 |
| 2.0 < z < 2.5 |  |
 |
13429 |
| 2.5 < z < 3.0 |  |
 |
9323 |
| 3.0 < z < 4.2 |  |
 |
5037 |
| 4.2 < z < 5.0 |  |
 |
1369 |
| 5.0 < z < 6.0 |  |
 |
599 |
 |
|||
 |
|||
Notes. The faint-end slope parameter α and the bright-end Gaussian width parameter σ are assumed to be independent of redshift. The last column N shows the number of galaxies above the completeness limit in the corresponding redshift bin.
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