D.M | R Documentation |
Function computes comoving distance in a flat cosmology.
D.M(z, omega.m = 0.27, omega.lambda = 0.73, H.0 = 71)
z |
Redshift |
omega.m |
Omega matter parameter |
omega.lambda |
Omega lambda parameter |
H.0 |
Hubble constant in km/s/Mpc |
Comoving distance in Mpc
For flat universe, omega.k = 0
, so transverse and line-of-sight
comoving distances are equal.
A. Harris
Hogg (2000), arXiv:astro-ph/9905116, equations (16) and (15)
D.M(2.3)
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