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
Inverse of dimensionless Hubble parameter, 1/E(z).
Used as integrand for computing comoving distance.
z (float) – Redshift.
1/E(z), where E(z) is the dimensionless Hubble parameter.
float