halomod.integrate_corr.dxdz

halomod.integrate_corr.dxdz(z, cosmo=FlatLambdaCDM(name='Planck18', H0=<Quantity 67.66 km / (Mpc s)>, Om0=0.30966, Tcmb0=<Quantity 2.7255 K>, Neff=3.046, m_nu=<Quantity [0., 0., 0.06] eV>, Ob0=0.04897))[source]

Derivative of comoving distance with redshift [Mpc/h].