Cosmological Parameters from Spherical Harmonic Analyses
Astrophysics
2007-05-23 v1
Abstract
In the rest of this volume Lahav and Fisher have presented the method of Spherical Harmonic Analysis (SHA) and its use in estimating cosmologically interesting parameters. Here I demonstrate the use of SHA in cross-correlating galazy catalogues and present an estimate of the ratio of the optical and IRAS galaxy bias parameters; b_O/b_I ~ 1.7.
Cite
@article{arxiv.astro-ph/9309031,
title = {Cosmological Parameters from Spherical Harmonic Analyses},
author = {Caleb. A. Scharf},
journal= {arXiv preprint arXiv:astro-ph/9309031},
year = {2007}
}
Comments
Paris Conference 2 pages uuencoded postscript file- figure available upon request