Fast Methods for Cosmological Simulations
FastSim serves as a tool for quick N-body simulations in modified gravity.
cl_cmblx_bm.py File Reference

Go to the source code of this file.

Classes

class  cl_cmblx_bm.Power_Spectra
 

Namespaces

 cl_cmblx_bm
 

Variables

 cl_cmblx_bm.c = c.to(u.km/u.second)
 
 cl_cmblx_bm.cosmo_fid
 
 cl_cmblx_bm.cosmo
 
 cl_cmblx_bm.cosmo_h = cosmo.clone(H0=100)
 
dictionary cl_cmblx_bm.pk_params = {'non_linear':0,'kmax':1E3,'kmin':5.e-5,'nk':5000}
 
 cl_cmblx_bm.PS = Power_Spectra()
 
 cl_cmblx_bm.zg
 
 cl_cmblx_bm.l
 
 cl_cmblx_bm.cl_g_cmb
 
 cl_cmblx_bm.pk_func
 
 cl_cmblx_bm.ccl_pk_bbks
 
 cl_cmblx_bm.zs
 
 cl_cmblx_bm.p_zs
 
 cl_cmblx_bm.p_zg
 
 cl_cmblx_bm.bias_g
 
 cl_cmblx_bm.fmt
 
float cl_cmblx_bm.sigz1 = 0.15
 
 cl_cmblx_bm.zav = np.linspace(0,10.,10000)
 
int cl_cmblx_bm.pza = 1
 
dictionary cl_cmblx_bm.za = {'z':zav,'pz':pza}
 
 cl_cmblx_bm.n_zl
 
 cl_cmblx_bm.zs2
 
 cl_cmblx_bm.p_zs2
 
 cl_cmblx_bm.zl_max