In order to produce some predictions for galaxy number densities, we implemented a turnover in stellar mass at high halo masses within the set_halo_properties function in HaloBox.c. However this model is hardcoded and not optimised. It should be properly implemented with flags and parameters.
In order to produce some predictions for galaxy number densities, we implemented a turnover in stellar mass at high halo masses within the
set_halo_propertiesfunction inHaloBox.c. However this model is hardcoded and not optimised. It should be properly implemented with flags and parameters.