activity
19962016
most citedThe Cores of Dwarf Galaxy Halos

623 citations · 1.7k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2016★ 20 cited

Evidence for a Localised Source of the Argon in the Lunar Exosphere

Jacob A. Kegerreis, Vincent R. Eke, Richard J. Massey +3

We perform the first tests of various proposed explanations for observed features of the Moon's argon exosphere, including models of: spatially varying surface interactions; a sour…

astro-ph.EP2015★ 10 cited

The effect of craters on the lunar neutron flux

V. R. Eke, K. E. Bower, S. Diserens +8

The variation of remotely sensed neutron count rates is measured as a function of cratercentric distance using data from the Lunar Prospector Neutron Spectrometer. The count rate,…

astro-ph2004★ 396 cited

Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue

V. R. Eke, C. M. Baugh, S. Cole +25

The construction of a catalogue of galaxy groups from the 2-degree Field Galaxy Redshift Survey (2dFGRS) is described. Groups are identified by means of a friends-of-friends percol…

astro-ph2003★ 500 cited

Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS

Michael Balogh, Vince Eke, Chris Miller +34

We analyse the observed correlation between galaxy environment and H-alpha emission line strength, using volume-limited samples and group catalogues of 24968 galaxies drawn from th…

astro-ph2002★ 47 cited

Measuring Sigma8 with Cluster Lensing : Biases from Unrelaxed Clusters

Graham P. Smith, Alastair C. Edge, Vincent R. Eke +3

We use gravitational lens models and X-ray spectral analysis of ten X-ray luminous galaxy clusters at z~0.2 to study the impact of cluster substructure on attempts to normalize the…

astro-ph1999★ 40 cited

Cosmological parameters from cluster abundances, CMB and IRAS

S. L. Bridle, V. R. Eke, O. Lahav +5

We combine information on cosmological parameters from cluster abundances, CMB primordial anisotropies and the IRAS 1.2 Jy galaxy redshift survey. We take as free parameters the pr…