Most simulations published here do not take hydrodynamics and star formation into account. However, given a catalog of dark matter halos and their merging histories, it is possible to compute properties of galaxies that would reside in these dark matter halos using semi-analytical recipes.
Within the CosmoSim database, you can find data from following semi-analytical codes:
- Galacticus: Benson 2012, Galacticus table description
- SAGE: Croton et al. 2016, SAGE table description
- SAG: Cora et al., in prep., SAG table description
Currently CosmoSim has galaxy properties for the MDPL2 simulation.
These tables are based on the MDPL2.Rockstar dark matter halo catalog and the merger tree information therein. If you use any of the data, please cite following paper:
Knebe et al. (2017), submitted to MNRAS
in addition to the corresponding code papers above.