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The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe

This paper is available in a repository.
This paper is available in a repository.

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Postprint: policy unknown
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Abstract

We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias parameter of the galaxies. This parameter quantifies the strength of clustering of the galaxies relative to the mass in the Universe. By analysing 80 million triangle configurations in the wavenumber range 0.1