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< …

As they grow, galaxies can transition from irregular/spheroidal with 'bursty'star formation
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …

We analyse scaling relations and evolution histories of galaxy sizes in TNG100, part of the
IllustrisTNG simulation suite. Observational qualitative trends of size with stellar mass, star …

We investigate the burstiness of star formation and the ionizing efficiency of a large sample
of galaxies at 0.7< z< 1.5 using HST grism spectroscopy and deep ultraviolet (UV) imaging …

The Star Formation Main Sequence in the Hubble Space Telescope Frontier Fields -
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Understanding the variability of galaxy star formation histories (SFHs) across a range of time-
scales provides insight into the underlying physical processes that regulate star formation …

We present a comparison of galaxy atomic and molecular gas properties in three recent
cosmological hydrodynamic simulations, namely SIMBA, EAGLE, and IllustrisTNG, versus …

The star formation histories (SFHs) of galaxies contain imprints of the physical processes
responsible for regulating star formation during galaxy growth and quenching. We improve …

We use the simba cosmological galaxy formation simulation to investigate the relationship
between major mergers (4: 1), starbursts, and galaxy quenching. Mergers are identified via …

We analyze the far-infrared (FIR) properties of∼ 5000 star-forming galaxies at z< 4.5, drawn
from the deepest, super-deblended catalogs in the GOODS-N and COSMOS fields. We …