activity
20092013
most citedOn the evolution of the HI column density distribution in cosmological simulations

512 citations · 823 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2013★ 14 cited

The effect of recombination radiation on the temperature and ionization state of partially ionized gas

Milan Raičević, Andreas H. Pawlik, Joop Schaye +1

A substantial fraction of all ionizing photons originate from radiative recombinations. However, in radiative transfer calculations this recombination radiation is often assumed to…

astro-ph.CO2013★ 106 cited

The impact of local stellar radiation on the HI column density distribution

Alireza Rahmati, Joop Schaye, Andreas H. Pawlik +1

It is often assumed that local sources of ionizing radiation have little impact on the distribution of HI in the post-reionization Universe. While this is a good assumption for the…

astro-ph.CO2012★ 512 cited

On the evolution of the HI column density distribution in cosmological simulations

Alireza Rahmati, Andreas H. Pawlik, Milan Raičević +1

We use a set of cosmological simulations combined with radiative transfer calculations to investigate the distribution of neutral hydrogen in the post-reionization Universe. We ass…

astro-ph.CO2010★ 27 cited

Modelling recombinations during cosmological reionization

Milan Raičević, Tom Theuns

An ionization front expanding into a neutral medium can be slowed-down significantly by recombinations. In cosmological numerical simulations the recombination rate is often comput…

astro-ph.CO2010★ 40 cited

The galaxies that reionized the Universe

Milan Raičević, Tom Theuns, Cedric Lacey

The Durham GALFORM semi-analytical galaxy formation model has been shown to reproduce the observed rest-frame 1500Å luminosity function of galaxies well over the whole redshift ran…

astro-ph.CO2009★ 124 cited

Cosmological Radiative Transfer Comparison Project II: The Radiation-Hydrodynamic Tests

Ilian T. Iliev, Daniel Whalen, Garrelt Mellema +14

The development of radiation hydrodynamical methods that are able to follow gas dynamics and radiative transfer self-consistently is key to the solution of many problems in numeric…