D.L: Luminosity distance
In cosmoFns: Functions for Cosmological Distances, Times, Luminosities, Etc
D.L R Documentation
Luminosity distance
Description
Function computes luminosity distance in a flat cosmology.
Usage
D.L(z, omega.m = 0.27, omega.lambda = 0.73, H.0 = 71)
Arguments
z
Redshift
omega.m
Omega matter parameter
omega.lambda
Omega lambda parameter
H.0
Hubble constant in km/s/Mpc
Value
Luminosity distance in Mpc
Author(s)
A. Harris
References
Hogg (2000), arXiv:astro-ph/9905116, equation (21)
Examples
D.L(2.3)
cosmoFns documentation built on May 9, 2022, 9:10 a.m.
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| D.L | R Documentation |
Luminosity distance
Description
Function computes luminosity distance in a flat cosmology.
Usage
D.L(z, omega.m = 0.27, omega.lambda = 0.73, H.0 = 71)
Arguments
z |
Redshift |
omega.m |
Omega matter parameter |
omega.lambda |
Omega lambda parameter |
H.0 |
Hubble constant in km/s/Mpc |
Value
Luminosity distance in Mpc
Author(s)
A. Harris
References
Hogg (2000), arXiv:astro-ph/9905116, equation (21)
Examples
D.L(2.3)
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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