How do galaxies populate Dark Matter halos ?

@inproceedings{Guo2009HowDG,
  title={How do galaxies populate Dark Matter halos ?},
  author={Qi Guo and Simon White and Cheng Li and Michael Boylan-Kolchin},
  year={2009}
}
For any assumed standard stellar Initial Mass Function, the Sloan Digital Sky Survey (SDSS) gives a precise determination of the abundance of galaxies as a function of their stellar mass over the full stellar mass range 108M⊙ < M∗ < 10 12M⊙. Within the concordance ΛCDM cosmology, the Millennium simulations give precise halo abundances as a function of mass and redshift for all halos within which galaxies can form. Under the plausible hypothesis that the stellar mass of a galaxy is an increasing… CONTINUE READING
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