Table 5.
Marginalized 1-σ errors in different cosmological scenarios for the galaxy weak lensing (WL) and angular void clustering (V) probes, together with their combinations in the case they are assumed to be independent, WL + V, and when their cross-correlation is included.
| Probe | h | Ωm | Ωb | σ8 | ns | Mν [eV] | w0 | wa | FoM |
|---|---|---|---|---|---|---|---|---|---|
| ΛCDM | |||||||||
| 0.141 | 0.00494 | 0.0244 | 0.00708 | 0.0327 | – | – | – | – | |
| WL | 0.136 | 0.00339 | 0.0236 | 0.00528 | 0.0298 | – | – | – | – |
| 0.215 | 0.252 | 0.0625 | 0.735 | 0.581 | – | – | – | – | |
| V | 0.0398 | 0.0198 | 0.0145 | 0.110 | 0.103 | – | – | – | – |
| 0.107 | 0.00483 | 0.0187 | 0.00655 | 0.0257 | – | – | – | – | |
| WL + V | 0.00735 | 0.00304 | 0.00389 | 0.00363 | 0.00432 | – | – | – | – |
| 0.0216 | 0.00466 | 0.00530 | 0.00575 | 0.0104 | – | – | – | – | |
| WL + V + XC | 0.00604 | 0.00285 | 0.00321 | 0.00338 | 0.00409 | – | – | – | – |
| νΛCDM | |||||||||
| 0.144 | 0.00526 | 0.0265 | 0.0129 | 0.0348 | 0.310 | – | – | – | |
| WL | 0.138 | 0.00342 | 0.0248 | 0.00873 | 0.0304 | 0.229 | – | – | – |
| 0.216 | 0.254 | 0.0667 | 0.812 | 0.707 | 2.46 | – | – | – | |
| V | 0.0402 | 0.0205 | 0.0154 | 0.113 | 0.131 | 0.593 | – | – | – |
| 0.109 | 0.00519 | 0.0203 | 0.0127 | 0.0272 | 0.302 | – | – | – | |
| WL + V | 0.00741 | 0.00309 | 0.00579 | 0.00752 | 0.00461 | 0.202 | – | – | – |
| 0.0216 | 0.00509 | 0.00718 | 0.0124 | 0.0118 | 0.292 | – | – | – | |
| WL + V + XC | 0.00605 | 0.00289 | 0.00505 | 0.00705 | 0.00443 | 0.193 | – | – | – |
| w0waCDM | |||||||||
| 0.141 | 0.0130 | 0.0246 | 0.0152 | 0.0348 | – | 0.147 | 0.552 | 26.9 | |
| WL | 0.138 | 0.00949 | 0.0237 | 0.0104 | 0.0299 | – | 0.121 | 0.426 | 53.9 |
| 0.316 | 0.394 | 0.0793 | 0.804 | 0.674 | – | 2.30 | 6.59 | 0.253 | |
| V | 0.0636 | 0.0934 | 0.0181 | 0.113 | 0.166 | – | 0.390 | 1.55 | 5.11 |
| 0.108 | 0.0128 | 0.0191 | 0.0148 | 0.0279 | – | 0.146 | 0.543 | 27.7 | |
| WL + V | 0.0131 | 0.00744 | 0.00407 | 0.00748 | 0.00461 | – | 0.0912 | 0.296 | 84.7 |
| 0.0244 | 0.0124 | 0.00638 | 0.0139 | 0.0143 | – | 0.144 | 0.526 | 29.3 | |
| WL + V + XC | 0.0105 | 0.00649 | 0.00348 | 0.00650 | 0.00425 | – | 0.0791 | 0.251 | 106 |
| νw0waCDM | |||||||||
| 0.148 | 0.0148 | 0.0270 | 0.0273 | 0.0430 | 0.413 | 0.149 | 0.630 | 20.2 | |
| WL | 0.139 | 0.00950 | 0.0250 | 0.0120 | 0.0305 | 0.231 | 0.122 | 0.429 | 53.6 |
| 0.351 | 0.482 | 0.0801 | 1.26 | 0.710 | 4.21 | 2.43 | 7.98 | 0.148 | |
| V | 0.0676 | 0.0987 | 0.0182 | 0.119 | 0.169 | 0.655 | 0.409 | 1.67 | 4.63 |
| 0.110 | 0.0146 | 0.0204 | 0.0267 | 0.0341 | 0.397 | 0.148 | 0.614 | 20.9 | |
| WL + V | 0.0131 | 0.00747 | 0.00584 | 0.0102 | 0.00492 | 0.203 | 0.0912 | 0.296 | 84.4 |
| 0.0244 | 0.0142 | 0.00721 | 0.0259 | 0.0200 | 0.380 | 0.145 | 0.591 | 22.6 | |
| WL + V + XC | 0.0105 | 0.00652 | 0.00514 | 0.00929 | 0.00463 | 0.182 | 0.0791 | 0.251 | 105 |
Notes. In each probe block, the first row shows the errors for the pessimistic scenario, while the second row corresponds to the optimistic one.
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