activity
20052012
most citedThe effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas

956 citations · 3.8k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.CO2012★ 32 cited

Physical properties of simulated galaxy populations at z=2 - II. Effects of cosmology, reionization and ISM physics

Marcel R. Haas, Joop Schaye, C. M. Booth +4

We use hydrodynamical simulations from the OWLS project to investigate the dependence of the physical properties of galaxy populations at redshift 2 on the assumed star formation l…

astro-ph.CO2012★ 71 cited

Physical properties of simulated galaxy populations at z=2 - I. Effect of metal-line cooling and feedback from star formation and AGN

Marcel R. Haas, Joop Schaye, C. M. Booth +4

We use hydrodynamical simulations from the OWLS project to investigate the dependence of the physical properties of galaxy populations at redshift 2 on metal-line cooling and feedb…

astro-ph.CO2012★ 31 cited

LOFAR insights into the epoch of reionization from the cross power spectrum of 21cm emission and galaxies

R. P. C. Wiersma, B. Ciardi, R. M. Thomas +18

Using a combination of N-body simulations, semi-analytic models and radiative transfer calculations, we have estimated the theoretical cross power spectrum between galaxies and the…

astro-ph.CO2011★ 290 cited

Cosmological simulations of the formation of the stellar haloes around disc galaxies

Andreea S. Font, Ian G. McCarthy, Robert A. Crain +4

We use the Galaxies-Intergalactic Medium Interaction Calculation (GIMIC) suite of cosmological hydrodynamical simulations to study the formation of stellar spheroids of Milky Way-m…

astro-ph.CO2011★ 58 cited

The effect of variations in the input physics on the cosmic distribution of metals predicted by simulations

Robert P. C. Wiersma, Joop Schaye, Tom Theuns

[Abridged] We investigate how a range of physical processes affect the cosmic metal distribution using a suite of cosmological, hydrodynamical simulations. Focusing on z = 0 and 2,…

astro-ph.CO2010★ 64 cited

Absorption signatures of warm-hot gas at low redshift: OVI

Thorsten Tepper-Garcia, Philipp Richter, Joop Schaye +4

We investigate the origin and physical properties of OVI absorbers at low redshift (z = 0.25) using a subset of cosmological, hydrodynamical simulations from the OverWhelmingly Lar…