The study of galaxy protoclusters is beginning to fill in unknown details of the important
phase of the assembly of clusters and cluster galaxies. This review describes the current …

We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …

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 …

Using a compilation of 25 studies from the literature, we investigate the evolution of the star-
forming galaxy (SFG) main sequence (MS) in stellar mass and star formation rate (SFR) out …

ABSTRACT We introduce the First Light And Reionisation Epoch Simulations (FLARES), a
suite of zoom simulations using the EAGLE model. We resimulate a range of overdensities …

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 …

We explore a large uniformly selected sample of Hα selected star-forming galaxies (SFGs) at
z= 0.40, 0.84, 1.47, 2.23 to unveil the evolution of the star formation rate (SFR) function and …

To search for dust-obscured star-formation activity in the early Universe, it is essential to
obtain a deep and wide submillimeter/millimeter map. The advent of the Atacama Large …

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 present results on the star formation rate (SFR) versus stellar mass (M*) relation (ie, the"
main sequence") among star-forming galaxies at 1.37≤ z≤ 2.61 using the MOSFIRE Deep …