The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical
property of the system, including the star-formation history, metal content, abundance …

By compiling a comprehensive census of literature studies, we investigate the evolution of
the main sequence (MS) of star-forming galaxies (SFGs) in the widest range of redshift (0< …

We present a method to flexibly and self-consistently determine individual galaxies' star
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …

Context. Feedback from accreting supermassive black holes (SMBHs) is often identified as
the main mechanism responsible for regulating star formation in active galactic nucleus …

In this paper, we investigate how massive central galaxies cease their star formation by
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …

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 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 …

We explore the simple inter-relationships between mass, star formation rate, and
environment in the SDSS, zCOSMOS, and other deep surveys. We take a purely empirical …

The main sequence (MS) of star-forming (SF) galaxies plays a fundamental role in driving
galaxy evolution and our efforts to understand it. However, different studies find significant …

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 …