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< …

The early release science results from JWST have yielded an unexpected abundance of
high-redshift luminous galaxies that seems to be in tension with current theories of galaxy …

We utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …

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

We use the panchromatic spectral energy distribution (SED)-fitting code Prospector to
measure the galaxy logM*–logSFR relationship (the star-forming sequence) across 0.2< z< …

The recent reported discovery of a low-mass z= 5.2 and an intermediate-mass z= 7.3
quenched galaxy with JWST/NIRSpec is the first evidence of halted star formation above z≈ …

The TNG50 cosmological simulation produces X-ray emitting bubbles, shells, and cavities in
the circumgalactic gas above and below the stellar discs of Milky Way-and Andromeda-like …

The nebular recombination line H α is widely used as a star formation rate (SFR) indicator in
the local and high-redshift Universe. We present a detailed H α radiative transfer study of …

We present an analysis of the instantaneous supermassive black hole (SMBH) accretion
rates in a collection of 1563 post-merger galaxies drawn from the IllustrisTNG simulation …

Using the TNG50 cosmological simulation and observations from the Kilo-Degree Survey
(KiDS), we investigate the connection between galaxy mergers and optical morphology in …