Table C.1.
Parameter constraints for the probe combinations considered in this work: 3 × 2 pt, cosmic shear (CS) and galaxy-galaxy lensing (GGL), cosmic shear and galaxy clustering (GC), and galaxy clustering by itself.
| Parameter | 3 × 2 pt | 3 × 2 pt | GC | GC | CS+GGL | CS+GGL | CS+GC | CS+GC |
|---|---|---|---|---|---|---|---|---|
| (joint) | (marginal) | (joint) | (marginal) | (joint) | (marginal) | (joint) | (marginal) | |
| S8 |
 |
 |
 |
 |
 |
 |
 |
 |
| h2Ωc | 0.123 |
 |
 |
 |
 |
 |
 |
 |
| h2Ωb | 0.0225 | – |
 |
– | 0.0258 | – |
 |
– |
| h |
 |
 |
 |
 |
 |
– |
 |
 |
| ns | 0.901 | – |
 |
– | 0.947 | – |
 |
– |
| Abary |
 |
– | 3.13 | – | 3.13 | – | ||
| AIA |
 |
 |
 |
 |
 |
 |
||
 |
 |
 |
 |
 |
 |
 |
||
 |
 |
 |
 |
 |
 |
 |
||
 |
 |
 |
 |
 |
 |
 |
||
 |
 |
 |
 |
 |
 |
 |
||
 |
 |
 |
 |
 |
 |
 |
||
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
0.968 | – |
 |
 |
 |
 |
 |
 |
 |
7.87 | – |
 |
 |
 |
 |
 |
 |
 |
 |
 |
||
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
 |
– |
 |
 |
 |
 |
 |
 |
 |
 |
– |
 |
 |
 |
 |
– |
 |
– |
 |
– | ||
| Ωm |
 |
 |
 |
 |
 |
 |
 |
 |
| σ8 |
 |
 |
 |
 |
 |
 |
 |
 |
| σ12 |
 |
 |
 |
 |
 |
 |
0.734 |
 |
| S12 |
 |
 |
 |
 |
 |
 |
 |
 |
| As |
 |
 |
 |
 |
 |
– |
 |
 |
| 100θMC | 1.05 |
 |
 |
 |
 |
 |
 |
 |
Notes. We refer the reader to Asgari et al. (2021a) for cosmic shear-only constraints. For each probe, the first column lists the MAP value with the PJ-HPD CI. If the PJ-HPD CI could not be robustly determined, no uncertainty estimate is provided. The second column for each probe lists the maximum of the marginal posterior, together with the marginal HPD CI. Parameter for which the marginal probability at either prior edge exceeds 13% of the peak probability are deemed unconstrained (see Appendix A of Asgari et al. 2021a), and are denoted by a dash. Finally, parameters that are not sampled are left blank.
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