pyccl.massfunction module¶
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pyccl.massfunction.
halo_bias
(cosmo, halo_mass, a, overdensity=200)[source]¶ Tinker et al. (2010) halo bias
Parameters: Returns: Halo bias.
Return type: float or array_like
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pyccl.massfunction.
massfunc
(cosmo, halo_mass, a, overdensity=200)[source]¶ Tinker et al. (2010) halo mass function, dn/dlog10M.
Parameters: Returns: Halo mass function; dn/dlog10M.
Return type: float or array_like
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pyccl.massfunction.
massfunc_m2r
(cosmo, halo_mass)[source]¶ Converts smoothing halo mass into smoothing halo radius.
Note
This is R=(3M/(4*pi*rho_m))^(1/3), where rho_m is the mean matter density.
Parameters: - cosmo (
Cosmology
) – Cosmological parameters. - halo_mass (float or array_like) – Halo masses; Msun.
Returns: Smoothing halo radius; Mpc.
Return type: float or array_like
- cosmo (