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Table 1.
Priors on the free parameters employed in our Bayesian analyses.
Cosmology | |
Ωm | [0.1, 0.7] |
As | [5 × 10−10, 5 × 10−9] |
h | [0.55, 0.90] |
Ωb | [0.03, 0.07] |
ns | [0.87, 1.07] |
Mν | [0.0559, 0.400] eV |
Baryons | |
log Mc | [9.0, 15.0] log(h−1 M⊙) |
log η | [ − 0.7, 0.7] |
log β | [ − 1.0, 0.7] |
log Mz0,cen | [9.0, 13.0] log(h−1 M⊙) |
log θinn | [ − 2.00, −0.53] |
log θout | [ − 0.48, 0.00] |
log Minn | [9.0, 13.5] log(h−1 M⊙) |
Intrinsic alignment | |
a1 | [ − 5, 5] |
η1 | [ − 5, 5] |
a2 | [ − 5, 5] |
η2 | [ − 5, 5] |
bta | [0, 2] |
Photo-z shift | |
![]() |
𝒩(0.000, 0.018) |
![]() |
𝒩(0.000, 0.015) |
![]() |
𝒩(0.000, 0.011) |
![]() |
𝒩(0.000, 0.017) |
Shear calibration | |
m1 | 𝒩(−0.0063, 0.0091) |
m2 | 𝒩(−0.0198, 0.0078) |
m3 | 𝒩(−0.0241, 0.0076) |
m4 | 𝒩(−0.0369, 0.0076) |
Notes. The intrinsic alignment parameters a2, η2, and bta were fixed to 0 in our fiducial run. We also imposed a prior on the combination of parameters Ωbh2 ∈ [0.009, 0.040].
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