CRAC (version 1.0)

distance.luminosity: Compute the luminosity distance [Mpc/h]

Description

Compute the luminosity distance [Mpc/h]

Usage

distance.luminosity(z, cosmo, z0 = 0, ...)

Arguments

z

redshift upper limit

cosmo

cosmological parameter list

z0

redshift lower limit

...

pass to integrate() to control integration accuracy.

Value

Luminosity distance from $z_0(=0)$ to $z$ [Mpc/h]

References

Equation (20) in [H99]

See Also

distance.angular,distance.comoving

Examples

distance.luminosity(0.1,parameter.fidcosmo)