Characterizing the relationship between stars, gas, and metals in galaxies is a critical
component of understanding the cosmic baryon cycle. We compile contemporary censuses …

We introduce the simba simulations, the next generation of the mufasa cosmological galaxy
formation simulations run with gizmo's meshless finite mass hydrodynamics. simba includes …

We present predictions for the evolution of the galaxy dust-to-gas ratio (DGR) and dust-to-
metal ratio (DTM) from z= 0→ 6, using a model for the production, growth, and destruction of …

ABSTRACT In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make
available our full spectroscopic redshift sample. This includes 248 682 galaxy spectra, and …

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 …

We present detailed implementations of (i) binary stellar evolution (BSE; using binary_c) and
(ii) dust production and destruction into the cosmological semi-analytic galaxy evolution …

The physical mechanisms that link the termination of star formation in quiescent galaxies
and the evolution of their baryonic components, stars, and the interstellar medium (ISM; dust …

To study the dust evolution in the cosmological structure formation history, we perform a
smoothed particle hydrodynamic simulation with a dust enrichment model in a cosmological …

Aims. The dust content of normal galaxies and the dust mass density (DMD) at high-z (z> 4)
are unconstrained given the source confusion and the sensitivity limitations of previous …

We analyse the physical properties of 121 SNR≥ 5 sub-millimetre galaxies (SMGs) from the
STUDIES 450 μ m survey. We model their UV-to-radio spectral energy distributions using …