Table 3.
Model parameters, split into cosmological and nuisance ones, with the latter further divided into the two bias models described in Sect. 3.
Parameter | Prior | |
---|---|---|
Cosmology | ||
h | 𝒰 [0.55, 0.85] | |
ωc | 𝒰 [0.08, 0.16] | |
Eulerian bias expansion | ||
Bias | b1 | 𝒰 [0.25, 4] |
b2 | 𝒰 [−10, 10] | |
![]() |
𝒰 [−4, 4] or fixed to Eq. (37) | |
bΓ3 | 𝒰 [−8, 8] or fixed to Eq. (36) | |
Counterterm | c0 [(Mpc/h)2] | 𝒰 [−100, 100] |
Shot-noise | αP, 1 | 𝒰 [−1, 2] |
αP, 2 [(Mpc/h)2] | 𝒰 [−5, 5] or fixed to 0 | |
Hybrid Lagrangian bias expansion | ||
Bias |
![]() |
𝒰 [−1, 3] |
![]() |
𝒰 [−3, 3] | |
![]() |
𝒰 [−10, 10] | |
![]() |
𝒰 [−10, 10] | |
Shot-noise | αP, 1 | 𝒰 [−1, 1] |
Notes. The nuisance parameters consist of bias parameters, EFTofLSS counterterm, and shot-noise terms. For each parameter, the imposed prior is specified in the last column of the table. The letter 𝒰 stands for a uniform distribution, with edges identified by the first and second element of the pair, respectively.
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