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Table 1.
Local slopes for the source galaxy counts αs and the lens galaxy counts αd given as a function of redshift and as a function of the limiting flux.
| (a) | (b) | (c) | |||
|---|---|---|---|---|---|
| fix zs = 0.99 | fix zd = 0.41 | fix slim, d = 22 | |||
| slim, s | αs | slim, d | αd | zd | αd |
| 22.0 | 2.89 | 19.5 | 2.71 | 0.24 | 0.46 |
| 22.5 | 2.33 | 20.0 | 2.03 | 0.41 | 0.66 |
| 23.0 | 1.75 | 20.5 | 1.56 | 0.51 | 0.98 |
| 23.5 | 1.29 | 21.0 | 1.06 | 0.62 | 1.58 |
| 24.0 | 0.93 | 21.5 | 0.85 | 0.83 | 2.49 |
| 24.5 | 0.68 | 22.0 | 0.66 | ||
| 25.0 | 0.58 | 23.0 | 0.44 | ||
| 26.0 | 0.45 | ||||
Notes. Either redshift or limiting flux is always kept fixed, while the other quantity is varied, as shown below. The limiting flux is given in terms of r-band magnitude.
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