Method

NumCosmoClusterPseudoCountsmf_lognormal_integral

Declaration [src]

gdouble
nc_cluster_pseudo_counts_mf_lognormal_integral (
  NcClusterPseudoCounts* cpc,
  NcHaloMassFunction* mfp,
  NcClusterMass* clusterm,
  NcHICosmo* cosmo,
  const gdouble lnMsz,
  const gdouble lnMl,
  const gdouble z
)

Description [src]

Numerically evaluate the integral of the mass function multiplied by the log-normal observable distribution for given SZ and lensing observed masses. This is used in assembling expected counts or likelihoods where a log-normal approximation is sufficient.

Parameters

mfp

Type: NcHaloMassFunction

A NcHaloMassFunction.

The data is owned by the caller of the method.
clusterm

Type: NcClusterMass

A NcClusterMass.

The data is owned by the caller of the method.
cosmo

Type: NcHICosmo

A NcHICosmo.

The data is owned by the caller of the method.
lnMsz

Type: const gdouble

Logarithm base e of SZ mass.

lnMl

Type: const gdouble

Logarithm base e of lensing mass.

z

Type: const gdouble

Spectroscopic redshift.

Return value

Type: gdouble

Value of the integral (dimensionless).