Fast Methods for Cosmological Simulations
FastSim serves as a tool for quick N-body simulations in modified gravity.
cl_cmblx_bm.Power_Spectra Member List

This is the complete list of members for cl_cmblx_bm.Power_Spectra, including all inherited members.

__init__(self, cosmo_params=cosmo_fid, pk_params=pk_params, cosmo=cosmo, cosmo_h=None)cl_cmblx_bm.Power_Spectra
ccl_pk_bbks(self, z, cosmo_params=None, pk_params=None)cl_cmblx_bm.Power_Spectra
cl_z(self, z=[], l=np.arange(3000)+1, pk_params=None, cosmo_h=None, cosmo=None, pk_func=None)cl_cmblx_bm.Power_Spectra
cosmocl_cmblx_bm.Power_Spectra
cosmo_hcl_cmblx_bm.Power_Spectra
cosmo_paramscl_cmblx_bm.Power_Spectra
DZ_int(self, z=[0], cosmo=None)cl_cmblx_bm.Power_Spectra
g_kappa_cl(self, pk_func=None, zs=[1100], p_zs=[1], zg=[1], p_zg=[1], bias_g=1, pk_params=None, cosmo_h=None, l=np.arange(0, 3001))cl_cmblx_bm.Power_Spectra
kappa_cl(self, zl_min=1.e-4, zl_max=1100, n_zl=10, log_zl=False, pk_func=None, zs1=[1100], p_zs1=[1], zs2=[1100], p_zs2=[1], pk_params=None, cosmo_h=None, l=np.arange(0, 3001))cl_cmblx_bm.Power_Spectra
pk_paramscl_cmblx_bm.Power_Spectra
Rho_crit(self, cosmo_h=None)cl_cmblx_bm.Power_Spectra
sigma_crit(self, zl=[], zs=[], cosmo_h=None)cl_cmblx_bm.Power_Spectra