Table 5
Expected number counts with different LF assumption
| LF(1) | LF(2) | |||
| Redshift | Blank | A2667 | Blank | A2667 |
|
|
||||
| AB < 25.5 | ||||
| [6.0,7.0] | 0.5 (1) | 1.5 (2) | 2.9 (3) | 4.2 (3) |
| [7.0,8.0] | <0.1 (1) | 0.3 (1) | 1.5 (2) | 2.3 (2) |
| (*) | 0.1 (1) | 0.5 (1) | ||
| [8.0,9.0] | <0.1 (1) | 0.1 (1) | 0.8 (1) | 1.4 (2) |
| (*) | <0.1 (1) | 0.2 (1) | ||
| [9.0,11.0] | <0.1 (1) | 0.1 (1) | 0.6 (1) | 1.3 (2) |
|
|
||||
| AB < 26.0 | ||||
| [6.0,7.0] | 3.1 (3) | 5.4 (4) | 8.5 (5) | 10.5 (5) |
| [7.0,8.0] | 0.4 (1) | 1.1 (2) | 4.9 (3) | 6.4 (4) |
| (*) | 0.8 (1) | 1.9 (2) | ||
| [8.0,9.0] | <0.1 (1) | 0.3 (1) | 2.9 (3) | 4.0 (3) |
| (*) | 0.3 (1) | 0.7 (1) | ||
| [9.0,11.0] | <0.1 (1) | 0.1 (1) | 2.8 (2) | 4.3 (3) |
Notes. Number counts are computed for sources with AB < 25.5 and AB < 26.0 expected in the field of A2667, with and without the presence of a lensing cluster, for different redshift bins and for two different LFs: Bouwens et al. (2008) (1) and Beckwith et al. (2006) (2) (see text). Error bars in number counts, including Poisson uncertainty and field-to-field variance, are given in brackets.
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