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Table C.1.
Fits to the redshift dependence of the response of the galaxy power spectrum.
| z | 
|
R0 | R1 |
|---|---|---|---|
| 0.1 | 4.06 | 5.00 | −0.97 |
| 0.2 | 4.48 | 5.29 | −0.83 |
| 0.3 | 4.79 | 5.24 | −0.47 |
| 0.4 | 4.98 | 5.10 | −0.13 |
| 0.5 | 5.08 | 4.95 | 0.14 |
| 0.6 | 5.12 | 4.78 | 0.34 |
| 0.7 | 5.10 | 4.62 | 0.50 |
| 0.8 | 5.06 | 4.45 | 0.63 |
| 0.9 | 4.98 | 4.29 | 0.72 |
| 1.0 | 4.89 | 4.13 | 0.78 |
| 1.1 | 4.79 | 4.00 | 0.82 |
| 1.2 | 4.70 | 3.91 | 0.82 |
| 1.3 | 4.63 | 3.86 | 0.80 |
| 1.4 | 4.59 | 3.85 | 0.77 |
| 1.5 | 4.61 | 3.89 | 0.75 |
| 1.6 | 4.70 | 3.97 | 0.76 |
| 1.7 | 4.87 | 4.09 | 0.80 |
| 1.8 | 5.13 | 4.26 | 0.90 |
| 1.9 | 5.49 | 4.46 | 1.06 |
Notes. Column 1 gives the start of the redshift bin, of width Δz = 0.1. Column 2 gives values for the scale independent model 
, while Cols. 3 and 4 give values for the linear model Rℓ = R0 + R1 × (ℓ/ℓ0) with ℓ0 = 1000.
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