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## Halo bias parameters from the peak-background split approximation
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The halo bias parameters can be calculated from a halo multiplicity function using the so-called peak-background split (PBS) approximation. See [Desjacques, Jeong & Schmdit, Phys. Rept., 733, 1 (2018)](https://www.sciencedirect.com/science/article/pii/S0370157317304192).
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The halo bias parameters can be calculated from a halo multiplicity function using the so-called peak-background split (PBS) approximation. See Equation (2.16) and Section 3.3 of [Desjacques, Jeong & Schmdit, Phys. Rept., 733, 1 (2018)](https://www.sciencedirect.com/science/article/pii/S0370157317304192).
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The package contains
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-`pbsBias(lnν, MF)` and `pbsBias1(lnν, MF)`: The linear bias parameter from the PBS.
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-`pbsBias2(lnν, MF)`: The second-order bias parameter from the PBS.
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-`pbsBias2(lnν, MF)` and `pbsBias3(lnν, MF)`: The second- and third-order bias parameters from the PBS.
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Here, `MF(lnν)` is any of the halo multiplicity functions from the above list. For example, ``pbsBias(lnν, stMF)`` and ``pbsBias(lnν, x -> tinker10MF(x, z, Δm))``.
*Reference*: Equation (2.14) and Section 3.3 of Desjacques, Jeong & Schmidt, Phys. Rept., 733, 1 (2018)
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# Arguments
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- `lnν::Real`: natural logarithm of a threshold, ν, i.e., `lnν` = log(ν), defined by ν ≡ [δc/σ(R,z)]^2. Here, δc = 1.6865 and σ(R,z) is the r.m.s. mass fluctuation within
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