onepower.hmi.SOVirial_Mead.mean_density

classmethod SOVirial_Mead.mean_density(z=0, cosmo=FlatLambdaCDM(name='Planck15', H0=<Quantity 67.74 km / (Mpc s)>, Om0=0.3075, Tcmb0=<Quantity 2.7255 K>, Neff=3.046, m_nu=<Quantity [0., 0., 0.06] eV>, Ob0=0.0486))

Get the mean density of the Universe at redshift z, [h^2 Msun / Mpc^3].