cl_cmbl_bm Namespace Reference

Classes
class	Power_Spectra

Variables
	cosmo = csmm.FlatLambdaCDM(70.,0.3,Tcmb0=2.725)
	cosmo_h = cosmo.clone(H0=100)
	c = c.to(u.km/u.second)
	cosmo_fid
dictionary	pk_params = {'non_linear':1,'kmax':30,'kmin':1.e-4,'nk':5000}
	PS = Power_Spectra()
	l
	cl2
	n_zl
	log_zl
	True
	zl_min
	zl_max
	pk_func
	fontsize
	fmt

Variable Documentation

cl_cmbl_bm.c = c.to(u.km/u.second)

Definition at line 12 of file cl_cmbl_bm.py.

Referenced by nlohmann::detail::serializer< BasicJsonType >.dump_float(), nlohmann::detail::lexer< BasicJsonType >.get_token_string(), tkEH_0(), u_nfw_c(), and window_function().

cl_cmbl_bm.cl2

Definition at line 103 of file cl_cmbl_bm.py.

cl_cmbl_bm.cosmo = csmm.FlatLambdaCDM(70.,0.3,Tcmb0=2.725)

Definition at line 10 of file cl_cmbl_bm.py.

Referenced by a_of_chi(), ccl_angular_cl_native(), ccl_cosmology_create(), ccl_cosmology_create_flat_lcdm(), ccl_sigmaR(), ccl_sigmaV(), chi_integrand(), compare_bbks(), compare_bcm(), compare_cls(), compare_corr(), compare_correlation_3d(), compare_distances(), compare_distances_hiz(), compare_distances_hiz_mnu(), compare_distances_mnu(), compare_eh(), compare_emu(), compare_emu_nu(), compare_growth(), compare_growth_hiz(), compare_halomod(), compare_massfunc(), compare_sigmam(), compute_chi(), dfzero(), fzero(), growth_change(), growth_ode_system(), growth_rate(), main(), one_halo_integral(), two_halo_integral(), window_lensing(), window_magnification(), and write_Pk_CLASS().

cl_cmbl_bm.cosmo_fid

Initial value:

= dict({'h':0.7,'Omb':0.0,'Omd':0.3,'s8':0.8,'Om':0.3,
                'As':2.12e-09,'mnu':0.,'Omk':0.,'tau':0.06,'ns':0.96})

Definition at line 14 of file cl_cmbl_bm.py.

cl_cmbl_bm.cosmo_h = cosmo.clone(H0=100)

Definition at line 11 of file cl_cmbl_bm.py.

cl_cmbl_bm.fmt

Definition at line 112 of file cl_cmbl_bm.py.

Referenced by Catch::StringMaker< T[SZ]>.convert().

cl_cmbl_bm.fontsize

Definition at line 108 of file cl_cmbl_bm.py.

cl_cmbl_bm.l

Definition at line 103 of file cl_cmbl_bm.py.

Referenced by __ctest_spherical_bessel_tests_compare_gsl_run(), ccl_tracer_corr_legendre(), compare_cls(), compute_spectra(), compute_w_theta(), anonymous_namespace{chameleon.cpp}::ChiSolver< T >.correct_sol(), emuInit(), anonymous_namespace{main.cpp}.init_and_run_app(), MultiGridSolver< NDIM, T >.l_operator(), main(), spectra(), test_angpow_precision(), tkEH_0(), transfer_rsd(), MultiGridSolver< NDIM, T >.upd_operator(), anonymous_namespace{chameleon.cpp}::ChiSolver< T >.upd_operator(), and write_cl_single().

cl_cmbl_bm.log_zl

Definition at line 103 of file cl_cmbl_bm.py.

cl_cmbl_bm.n_zl

Definition at line 103 of file cl_cmbl_bm.py.

cl_cmbl_bm.pk_func

Definition at line 103 of file cl_cmbl_bm.py.

Referenced by cl_cmbl_bm.Power_Spectra.cl_z().

dictionary cl_cmbl_bm.pk_params = {'non_linear':1,'kmax':30,'kmin':1.e-4,'nk':5000}

Definition at line 16 of file cl_cmbl_bm.py.

cl_cmbl_bm.PS = Power_Spectra()

Definition at line 102 of file cl_cmbl_bm.py.

cl_cmbl_bm.True

Definition at line 103 of file cl_cmbl_bm.py.

cl_cmbl_bm.zl_max

Definition at line 103 of file cl_cmbl_bm.py.

cl_cmbl_bm.zl_min

Definition at line 103 of file cl_cmbl_bm.py.