The study of galaxy evolution hinges on our ability to interpret multiwavelength galaxy
observations in terms of their physical properties. To do this, we rely on spectral energy …

We present deep 1.4 GHz source counts from∼ 5 deg2 of the continuum Early Science data
release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration survey …

We use the Galaxy and Mass Assembly (GAMA) and the Deep Extragalactic Visible Legacy
Survey (DEVILS) observational data sets to calculate the cosmic star formation rate (SFR) …

Active galactic nuclei (AGN) are typically identified through radio, mid-infrared, or X-ray
emission or through the presence of broad and/or narrow emission lines. AGN can also …

Gas-phase metallicities of galaxies are typically measured through auroral or nebular
emission lines, but metallicity also leaves an imprint on the overall spectral energy …

We present the first look at star formation histories of galaxy components using ProFuse, a
new technique to model the 2D distribution of light across multiple wavelengths using …

We consider the effect of including an active galactic nuclei (AGN) component when fitting
spectral energy distributions of 109 spectroscopically confirmed z≈ 3.5–12.5 galaxies with …

We use two independent galaxy-formation simulations, flares, a cosmological
hydrodynamical simulation, and shark, a semi-analytic model, to explore how well the JWST …

Traditionally, the far-ultraviolet (FUV) to far-infrared (FIR) and radio spectral energy
distributions (SEDs) of galaxies have been considered separately despite the common …

We give an overview and describe the rationale, methods, and first results from NIRCam
images of the JWST" Prime Extragalactic Areas for Reionization and Lensing …