We investigate the dependence of galaxy structure on a variety of galactic and
environmental parameters for∼ 500 000 galaxies at z< 0.2, taken from the Sloan Digital Sky …

ABSTRACT From the Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5), we extract a
sample of 4594 galaxies at redshifts 0.02< z< 0.03, complete down to a stellar mass of M …

Using the IllustrisTNG simulations, we investigate the connection between galaxy
morphology and star formation in central galaxies with stellar masses in the range 109 …

We present in this paper a detailed analysis of the effect of environment on the star formation
activity of galaxies within the Early Data Release (EDR) of the Sloan Digital Sky Survey …

We investigate the dependence of physical properties of galaxies brighter than M r=-18.0+ 5
log h in the Sloan Digital Sky Survey (SDSS) on environment, as measured by local density …

We present a study of the spectroscopic and photometric properties of galaxies in six nearby
clusters. We perform a partial correlation analysis on our data set to investigate whether the …

The effect of environment on galaxy formation poses one of the best constraints on the
interplay between mass assembly and star formation in galaxies. We present here a detailed …

To break the degeneracy among galactic stellar components, we extract kinematic structures
using the framework that was described in Du et al. For example, the concept of stellar halos …

The distribution of galaxy morphological types is a key test for models of galaxy formation
and evolution, providing strong constraints on the relative contribution of different physical …

Abstract We use the Millennium Simulation, a 10 billion particle simulation of the growth of
cosmic structure, to construct a new model of galaxy clustering. We adopt a methodology …