Table 13.
Impact of RSDs.
| Ωm, 0 | Ωb, 0 | w0 | wa | h | ns | σ8 | ||
|---|---|---|---|---|---|---|---|---|
 (GCph) |
No RSD | 36% | 24% | 34% | 35% | 14% | 32% | 18% |
| With RSD | 32% | 20% | 29% | 29% | 13% | 27% | 17% | |
| Δθ/σθ (GCph) | No RSD | −0.65 | −0.64 | −1.02 | 1.20 | 0.05 | 1.04 | 0.17 |
| With RSD | −0.75 | −0.63 | −0.83 | 0.86 | 0.25 | 1.05 | 0.09 | |
 (GCph + WL + GGL) |
No RSD | 1% | < 1% | 2% | 2% | < 1% | < 1% | 1% |
| With RSD | 1% | < 1% | 2% | 2% | < 1% | < 1% | 1% | |
| Δθ/σθ (GCph + WL + GGL) | No RSD | 6.90 | 2.89 | 4.58 | −2.82 | 1.16 | −4.39 | −4.56 |
| With RSD | 6.95 | 2.82 | 4.62 | −2.98 | 1.07 | −4.22 | −4.73 | |
Notes. Impact of magnification in the GCph and GCph + WL + GGL analyses, including or neglecting RSDs, for our baseline cosmology. In the results labelled as ‘with RSD’, we add the contribution of RSDs both in the Fisher analysis that includes magnification and the one that neglects it. Vice versa, the results denoted as ‘no RSD’ completely neglect RSDs, and they correspond to the analysis presented in Sect. 5.
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