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 study the star-forming (SF) population of galaxies within a sample of 209 IR-selected
galaxy clusters at 0.3≤ z≤ 1.1 in the ELAIS-N1 and XMM-LSS fields, exploiting the first …

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 combine orbital information from N-body simulations with an analytic model for star
formation quenching and SDSS observations to infer the differential effect of the …

We present the stellar mass functions (SMFs) of passive and star-forming galaxies with a
limiting mass of 10 10.1 M⊙ in four spectroscopically confirmed Spitzer Adaptation of the …

We analyse the evolution of environmental quenching efficiency, the fraction of quenched
cluster galaxies that would be star-forming if they were in the field, as a function of redshift in …

We present the first public data release of the GOGREEN (Gemini Observations of Galaxies
in Rich Early Environments) and GCLASS (Gemini CLuster Astrophysics Spectroscopic …

We present molecular gas reservoirs of 18 galaxies associated with the XMMXCS J2215. 9–
1738 cluster at z= 1.46. From Band 7 and Band 3 data of the Atacama Large Millimeter …

We used the time since infall (TSI) of galaxies, obtained from the Yonsei Zoom-in Cluster
Simulation, and the star formation rate (SFR) from the Sloan Digital Sky Survey Data …

We present the first results from a galaxy population study in the highest redshift galaxy
clusters identified in the 2500 deg 2 South Pole Telescope Sunyaev Zel'dovich effect (SPT …