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One simulation to fit them all - changing the background parameters of a cosmological N-body simulation
Raul E. Angulo, Simon D. M. White
We demonstrate that the output of a cosmological N-body simulation can, to remarkable accuracy, be scaled to represent the growth of large-scale structure in a cosmology with param…
There's no place like home? Statistics of Milky Way-mass dark matter halos
Michael Boylan-Kolchin, Volker Springel, Simon D. M. White +1
We present an analysis of the distribution of structural properties for Milky Way-mass halos in the Millennium-II Simulation (MS-II). This simulation of structure formation within…
Dark matter response to galaxy formation
Patricia B. Tissera, Simon D. M. White, Susana Pedrosa +1
We have resimulated the six galaxy-sized haloes of the Aquarius Project including metal-dependent cooling, star formation and supernova feedback. This allows us to study not only h…
Evolution of the Early-Type Galaxy Fraction in Clusters since z = 0.8
Luc Simard, Douglas Clowe, Vandana Desai +13
We study the morphological content of a large sample of high-redshift clusters to determine its dependence on cluster mass and redshift. Quantitative morphologies are based on bulg…
Autocorrelations of stellar light and mass in the low-redshift Universe
Cheng Li, Simon D. M. White
The final data release of the Sloan Digital Sky Survey (SDSS) provides reliable photometry and spectroscopy for about half a million galaxies with median redshift 0.09. Here we use…
Star formation and AGN activity in SDSS cluster galaxies
Anja von der Linden, Vivienne Wild, Guinevere Kauffmann +2
We investigate the recent and current star formation activity of galaxies as function of distance from the cluster center in a sample of 521 SDSS clusters at z<0.1. We show that wh…