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 select galaxies from the IllustrisTNG hydrodynamical simulations (at 0≤ z≤ 2) and
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …

We use the IllustrisTNG hydrodynamical simulations to show how the fractions of quenched
galaxies vary across different environments and cosmic time, and to quantify the role AGN …

Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift - IOPscience
This site uses cookies. By continuing to use this site you agree to our use of cookies. To find …

Galaxies fall into two clearly distinct types:'blue-sequence'galaxies that are rapidly forming
young stars, and 'red-sequence'galaxies in which star formation has almost completely …

The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼
5 - IOPscience This site uses cookies. By continuing to use this site you agree to our use of …

We present a catalog of 10,718 objects in the COSMOS field, observed through multi-slit
spectroscopy with the Deep Imaging Multi-Object Spectrograph (DEIMOS) on the Keck II …

Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent
Galaxies - IOPscience This site uses cookies. By continuing to use this site you agree to our …

The variation of galaxy stellar masses and colour types with the distance to projected cosmic
filaments are quantified using the precise photometric redshifts of the COSMOS2015 …

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 …