Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

Galactic archaeology based on star counts is instrumental to reconstruct the past mass
assembly of Local Group galaxies. The development of new observing techniques and data …

We measure the evolution of the stellar mass function (SMF) from z= 0–1 using multi-
wavelength imaging and spectroscopic redshifts from the PRism MUlti-object Survey …

We extend the phenomenological study of the evolving galaxy population of Peng et
al.(2010) to the central/satellite dichotomy in Yang et al. Sloan Digital Sky Survey (SDSS) …

We present the general real-and redshift-space clustering properties of galaxies as
measured in the first data release of the VIPERS survey. VIPERS is a large redshift survey …

We present the galaxy stellar mass function (GSMF) to redshift z≃ 1, based on the analysis
of about 8500 galaxies with I< 22.5 (AB mag) over 1.4 deg 2, which are part of the …

The influence of a galaxy's environment on its evolution has been studied and compared
extensively in the literature, although differing techniques are often used to define …

We present a multi-wavelength photometric catalog in the COSMOS field as part of the
observations by the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey. The …

We study the stellar mass functions (SMFs) of star-forming and quiescent galaxies in 11
galaxy clusters at 1.0< z< 1.4 drawn from the Gemini Observations of Galaxies in Rich Early …

We outline theoretical predictions for extended emission from Mg ii, tracing cool∼ 104 K gas
in the circumgalactic medium (CGM) of star-forming galaxies in the high-resolution TNG50 …