hmf.alternatives.wdm.MassFunctionWDM.rho_gtm¶
- property MassFunctionWDM.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.