Cosmological Parameters from Spherical Harmonic Analyses

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Paris Conference 2 pages uuencoded postscript file- figure available upon request

Scientific paper

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.

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