User Guide
Reference
c_light_kms
print_cosmology()
set_cosmology()
H()
E()
inv_E()
DM()
DA()
DL()
dV()
dVdtau()
init_dist_measures()
dm()
dl()
da()
dv()
dvdtau()
E_to_F()
F_to_E()
dFnu_to_dEnu()
choose_source_evolution_function()
sfr_evolution()
opz_evolution()
sfr()
Development
Dimensionless Hubble parameter E(z) = H(z)/H0.
Computes the normalized expansion rate assuming flat Lambda CDM cosmology.
z (float or array_like) – Redshift(s) at which to evaluate E(z).
Dimensionless Hubble parameter E(z) = sqrt(Omega_m*(1+z)^3 + Omega_k*(1+z)^2 + Omega_lambda).
float or ndarray