Table 6.
Baseline of assumed systematic errors for the reconstruction of biasing functions.
| Source | RMS error |
|---|---|
| Redshift bias (sources and lenses) | 2.0% |
| Width of p(z) (sources and lenses) | 5.0% |
| Ωm | 4.3% |
| Ωb | 4.8% |
| w | 6.2% |
| H0 | 2.3% |
| ns | 0.5% |
| σ8 | 2.6% |
| Aia | 170% |
| F(k, z) | 30.0% |
Notes. The resulting systematic RMS uncertainties of b(k) and r(k) amplitudes are within [6.8%,13.5%] and [5.2%,8.5%], respectively (see text). Correlated errors on cosmological parameters Ωm to σ8 are the posterior constraints from Planck Collaboration XIII (2016) for a flat wCDM model. The IA parameter is 
from Heymans et al. (2013). The baryon transfer function F(k, z) is from Chisari et al. (2018); we use as fiducial values their Fig. 11, but randomly perturb F(k, z) by δF(k, z) = δ × (F(k, z)−1) with a normally distributed amplitude δ of the quoted RMS variance.
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