We examine the effect of using different halo finders and merger tree building algorithms on galaxy properties predicted using the GALFORM semi-analytical model run on a high resolution, large volume dark matter simulation. The halo finders/tree builders HBT, ROCKSTAR, SUBFIND, and VELOCI RAPTOR differ in their definitions of halo mass, on whether only spatial or phase-space information is used, and in how they distinguish satellite and main haloes; all of these features have some impact on the model galaxies, even after the trees are post-processed and homogenized by GALFORM. The stellar mass function is insensitive to the halo and merger tree finder adopted. However, we find that the number of central and satellite galaxies in GALFORM doe...
We present a clustering comparison of 12 galaxy formation models [including semi-analytic models (SA...
We examine whether large-scale environment affects the mass assembly history of central galaxies. To...
We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 hal...
A halo merger tree forms the essential backbone of a semi-analytic model for galaxy formation and ev...
Merger tree codes are routinely used to follow the growth and merger of dark matter haloes in simula...
Merger trees are routinely used to follow the growth and merging history of dark matter haloes and s...
We present a new Monte Carlo algorithm to generate merger trees describing the formation history of ...
Merging haloes with similar masses (i.e. major mergers) pose significant challenges for halo finders...
We develop a hybrid galaxy formation model that uses outputs from an N-body simulation to follow the...
We use the Millennium Simulation data base to compare how different versions of the Durham and Munic...
Tracking the formation and evolution of dark matter haloes is a critical aspect of any analysis of c...
We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 hal...
We present predictions for the two-point correlation function of galaxy clustering as a function of ...
We apply the model relating halo concentration to formation history proposed by Ludlow et al. to mer...
We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 hal...
We present a clustering comparison of 12 galaxy formation models [including semi-analytic models (SA...
We examine whether large-scale environment affects the mass assembly history of central galaxies. To...
We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 hal...
A halo merger tree forms the essential backbone of a semi-analytic model for galaxy formation and ev...
Merger tree codes are routinely used to follow the growth and merger of dark matter haloes in simula...
Merger trees are routinely used to follow the growth and merging history of dark matter haloes and s...
We present a new Monte Carlo algorithm to generate merger trees describing the formation history of ...
Merging haloes with similar masses (i.e. major mergers) pose significant challenges for halo finders...
We develop a hybrid galaxy formation model that uses outputs from an N-body simulation to follow the...
We use the Millennium Simulation data base to compare how different versions of the Durham and Munic...
Tracking the formation and evolution of dark matter haloes is a critical aspect of any analysis of c...
We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 hal...
We present predictions for the two-point correlation function of galaxy clustering as a function of ...
We apply the model relating halo concentration to formation history proposed by Ludlow et al. to mer...
We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 hal...
We present a clustering comparison of 12 galaxy formation models [including semi-analytic models (SA...
We examine whether large-scale environment affects the mass assembly history of central galaxies. To...
We present a comparison of 14 galaxy formation models: 12 different semi-analytical models and 2 hal...