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19942009
most citedThe redshift dependence of the structure of massive LCDM halos

510 citations · 5.9k across the 44 of their papers we have counts for

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Showing 2006Show all

12 papers · 1 filter

astro-ph2006374 cited

Assembly bias in the clustering of dark matter haloes

Liang Gao, Simon D. M. White

We use a very large simulation of structure growth in a LCDM universe -- the Millennium Simulation -- to study assembly bias, the fact that the large-scale clustering of haloes of…

astro-ph2006337 cited

How special are Brightest Group and Cluster Galaxies?

Anja von der Linden, Philip N. Best, Guinevere Kauffmann +1

We use the Sloan Digital Sky Survey to construct a sample of 625 brightest group and cluster galaxies (BCGs) together with control samples of non-BCGs matched in stellar mass, reds…

astro-ph2006224 cited

The build-up of the colour-magnitude relation in galaxy clusters since z~0.8

Gabriella De Lucia, Bianca M. Poggianti, Alfonso Aragon-Salamanca +11

Using galaxy clusters from the ESO Distant Cluster Survey, we study how the distribution of galaxies along the colour-magnitude relation has evolved since z~0.8. While red-sequence…

astro-ph2006271 cited

The high redshift galaxy population in hierarchical galaxy formation models

Manfred G. Kitzbichler, Simon D. M. White

We compare observations of the high redshift galaxy population to the predictions of the galaxy formation model of Croton et al. (2006) and De Lucia & Blaizot (2006). This model, i…

astro-ph2006135 cited

The clustering of narrow-line AGN in the local Universe

Cheng Li, Guinevere Kauffmann, Lan Wang +3

We have analyzed the clustering of ~ 90,000 narrow-line AGN drawn from the Data Release 4 (DR4) of the SDSS. We compute the cross-correlation between AGN and a reference sample of…

astro-ph2006111 cited

Asymmetries in the inner regions of LCDM haloes

liang Gao, Simon D. M. White

Many galaxies display warps, lopsided images, asymmetric rotation curves or other features which suggest that their immediate dynamical environment is neither static nor in equilib…