hmf.mass_function.hmf.MassFunction.rho_gtm

property MassFunction.rho_gtm

Mass density in haloes >m, len=len(m) [units \(M_\odot h^2 Mpc^{-3}\)]

In the case that m does not extend to sufficiently high masses, this routine will auto-generate dndm for an extended mass range.

In the case of the ff.Behroozi fit, it is impossible to auto-extend the mass range except by the power-law fit, thus one should be careful to supply appropriate mass ranges in this case.