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 …

We review the properties of the established Scaling Relations (SRs) of galaxies and active
galactic nuclei (AGN), focusing on their origin and expected evolution back in time, providing …

We present a catalog of 182 galaxy clusters detected through the Sunyaev–Zel'dovich (SZ)
effect by the Atacama Cosmology Telescope in a contiguous 987.5 deg 2 field. The clusters …

We study the effects of the local environment and stellar mass on galaxy properties using a
mass complete sample of quiescent and star-forming systems in the COSMOS field at …

In this paper, we investigate environment-driven gas depletion in satellite galaxies, taking
full advantage of the atomic hydrogen (H i) spectral stacking technique to quantify the gas …

We explore the structures of protoclusters and their relationship with high-redshift clusters
using the Millennium Simulation combined with a semi-analytic model. We find that …

We study the dependence of star formation quenching on galaxy mass and environment, in
the Sloan Digital Sky Survey (SDSS; z∼ 0.1) and the All-Wavelength Extended Groth Strip …

We present a study of metal-enriched halo gas traced by Mg ii and C iv absorption at z< 2 in
the MUSE Analysis of Gas around Galaxies survey and the Quasar Sightline and Galaxy …

We study the dependence of the galaxy content of dark matter halos on large-scale
environment and halo formation time using semi-analytic galaxy models applied to the …

We present the∼ 800 star formation rate maps for the Sydney-AAO Multi-object Integral field
spectrograph (SAMI) Galaxy Survey based on H α emission maps, corrected for dust …