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19962022
most citedThe 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications

2.1k citations · 10.3k across the 61 of their papers we have counts for

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astro-ph2008★ 117 cited

Galaxy morphology in the LambdaCDM cosmology

O. H. Parry, V. R. Eke, C. S. Frenk

We investigate the origins of galaxy morphology (defined by bulge-to-total K-band luminosity) in the LambdaCDM cosmology using two galaxy formation models ,based on the Millennium…

astro-ph2006★ 151 cited

The baryon fraction of LambdaCDM haloes

Robert A. Crain, Vincent R. Eke, Carlos S. Frenk +4

We investigate the baryon fraction in dark matter haloes formed in non-radiative gas-dynamical simulations of the LambdaCDM cosmogony. By combining a realisation of the Millennium…

astro-ph2006★ 488 cited

The spin and shape of dark matter haloes in the Millennium simulation of a LambdaCDM universe

Philip Bett, Vincent Eke, Carlos S. Frenk +3

We investigate the spins and shapes of over a million dark matter haloes identified at z=0 in the Millennium simulation. Our sample spans halo masses ranging from dwarf galaxies to…

astro-ph2005★ 68 cited

Galaxy Groups in the 2dFGRS: the number density of groups

V. R. Eke, C. M. Baugh, S. Cole +2

The abundance of galaxy clusters as a function of mass is determined using the 2dFGRS Percolation-Inferred Galaxy Group (2PIGG) catalogue. This is used to estimate the amplitude of…

astro-ph2005★ 220 cited

The effects of feedback on the morphology of galaxy discs

Takashi Okamoto, Vince R. Eke, Carlos S. Frenk +1

We have performed hydrodynamic simulations of galaxy formation in a LCDM universe. We have followed galaxy formation in a dark matter halo, chosen to have a relatively quiet recent…

astro-ph2005★ 2.1k cited

The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications

S. Cole, W. J. Percival, J. A. Peacock +28

We present a power spectrum analysis of the final 2dF Galaxy Redshift Survey, employing a direct Fourier method. The sample used comprises 221,414 galaxies with measured redshifts.…