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arxiv: astro-ph/9309027 · v1 · pith:C56KG2FZnew · submitted 1993-09-18 · 🌌 astro-ph

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

classification 🌌 astro-ph
keywords redshiftdensityharmonicirasomegasphericalsurveyanalysing
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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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