ldist: Integrand for luminosity distance calculation
In astrolibR: Astronomy Users Library
Description
Usage
Arguments
Details
Value
Examples
Description
Integrand for luminosity distance calculation
Usage
1
ldist(z, q0, lambda0)
Arguments
z
redshift, positive scalar or vector
q0
deceleration parameter, scalar
lambda0
cosmological constant normalized to the closure density
Details
Used in place of the Mattig formula when the cosmological constant is non-zero.
Value
Value of the partial integral
Examples
1
ldist(3.0, 0.5, 0.7)
astrolibR documentation built on May 2, 2019, 3:26 a.m.
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Description Usage Arguments Details Value Examples
Description
Integrand for luminosity distance calculation
Usage
1 | ldist(z, q0, lambda0)
|
Arguments
z |
redshift, positive scalar or vector |
q0 |
deceleration parameter, scalar |
lambda0 |
cosmological constant normalized to the closure density |
Details
Used in place of the Mattig formula when the cosmological constant is non-zero.
Value
Value of the partial integral
Examples
1 | ldist(3.0, 0.5, 0.7)
|
R Package Documentation
Browse R Packages
We want your feedback!
Note that we can't provide technical support on individual packages. You should contact the package authors for that.
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