A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey.

The large-scale structure in the distribution of galaxies is thought to arise from the gravitational instability of small fluctuations in the initial density field of the Universe. A key test of this hypothesis is that forming superclusters of galaxies should generate a systematic infall of other ga...

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Bibliographic Details
Main Authors:	Peacock, J, Cole, S, Norberg, P, Baugh, C, Bland-Hawthorn, J, Bridges, T, Cannon, R, Colless, M, Collins, C, Couch, W, Dalton, G, Deeley, K, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Frenk, C, Glazebrook, K, Jackson, C, Lahav, O, Lewis, I, Lumsden, S, Maddox, S, Percival, W, Peterson, B
Format:	Journal article
Language:	English
Published:	2001

A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey.

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