Using a large galaxy group catalogue constructed from the Sloan Digital Sky Survey Data
Release 2, we investigate the correlation between various galaxy properties and halo mass …

We have studied the morphology–density relation and morphology–cluster-centric-radius
relation using a volume-limited sample (0.05< z< 0.1, Mr*<− 20.5) of the Sloan Digital Sky …

We analyse the observed correlation between galaxy environment and Hα emission-line
strength, using volume-limited samples and group catalogues of 24 968 galaxies at 0.05< z< …

We investigate how environment affects satellite galaxies using their location within the
projected phase space of their host haloes from the Wang et al.'s group catalogue. Using the …

We investigate the environmental dependence of star formation and the morphology of
galaxies in the local universe based on a volume-limited sample constructed from the data …

Using the stellar ages and metallicities of galaxies in the Sloan Digital Sky Survey (SDSS)
obtained by and the SDSS galaxy group catalogue of, we study how the stellar ages and …

The environment within dark matter haloes can quench the star formation of galaxies.
However, environmental effects beyond the virial radius of haloes (≳ 1 Mpc) are less …

A series of high-resolution ΛCDM cosmological N-body simulations are used to study the
properties of galaxy-size dark halos as a function of global environment. We analyze halos …

We show by means of a high-resolution N-body simulation how the mass assembly histories
of galaxy-sized cold dark matter (CDM) halos depend on environment. Halos in high-density …

We assess the effects of galaxy–galaxy interactions on star formation (SF) by analysing pairs
in groups and clusters of galaxies with virial masses in the range 1013–1015 M⊙ extracted …