Description Usage Arguments Value Author(s) References See Also
Calculates transverse comoving distance
| 1 | comovdist.trans(z = 1, c = 3E8, H = 70, M = 0.3, L = 1-M, K = 1-M-L, units = "Mpc")
 | 
| z | redshift | 
| c | speed of light (m/s) | 
| H | Hubble constant (km/s/Mpc) | 
| M | Omega M - matter | 
| L | Omega L - energy | 
| K | Omega K - curvature | 
| units | output units [Mpc/ly/m] | 
Transverse comoving distance in indicated units to the given redshift with the given cosmology.
Lee Kelvin <lee.kelvin@uibk.ac.at>
Hogg D. W., 1999, ArXiv Astrophysics e-prints, arXiv:astro-ph/9905116
The astronomy package: astro.
Add the following code to your website.
For more information on customizing the embed code, read Embedding Snippets.