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astrolibR (version 0.1)

ldist: Integrand for luminosity distance calculation

Description

Integrand for luminosity distance calculation

Usage

ldist(z, q0, lambda0)

Arguments

z
redshift, positive scalar or vector
q0
deceleration parameter, scalar
lambda0
cosmological constant normalized to the closure density

Value

Details

Used in place of the Mattig formula when the cosmological constant is non-zero.

Examples

Run this code
ldist(3.0, 0.5, 0.7)

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