A Spherical Harmonic Approach to Redshift Distortion and a Measurement of Omega from the 1.2 Jy IRAS Redshift Survey

Astronomy and Astrophysics – Astrophysics

Scientific paper

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8 pages--uuencoded postscript file

Scientific paper

We present a formalism for analysing redshift distortions based on a
spherical harmonic expansion of the density field. We use a maximum likelihood
estimator for the combination of density and bias parameters, $\Omega^0.6/b$.
We test the method with $N$-body simulations and apply it to the 1.2 Jy IRAS
redshift survey.

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