Frank C. van den Bosch

TL;DR: In this article, the authors used a statistical approach to determine the relationship between the stellar masses of galaxies and the masses of the dark matter halos in which they reside and obtained a parameterized stellar-to-halo mass (SHM) relation by populating halos and subhalos in an N-body simulation with galaxies and requiring that the observed stellar mass function be reproduced.

TL;DR: Yang et al. as discussed by the authors used a modified version of the halo-based group finder developed by Yang et al., to select galaxy groups from the Sloan Digital Sky Survey (SDSS DR4).

TL;DR: Yang et al. as discussed by the authors used a modified version of the halo-based group finder to select galaxy groups from the Sloan Digital Sky Survey (SDSS DR4), and obtained 301237 groups in a broad dynamic range.

TL;DR: In this paper, a parameterized stellar-to-halo mass (SHM) relation was derived by populating halos and subhalos in an N-body simulation with galaxies and requiring that the observed stellar mass function be reproduced.

TL;DR: In this paper, the effects of changes in the cosmological parameters between the Wilkinson Microwave Anisotropy Probe (WMAP) 1st, 3rd and 5th year results on the structure of dark matter haloes were investigated.