Nearby galaxies offer unique laboratories allowing multi-wavelength spatially resolved
studies of the interstellar medium, star formation and nuclear activity across a broad range of …

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 …

Context. Measuring how the physical properties of galaxies change across cosmic times is
essential to understand galaxy formation and evolution. With the advent of numerous ground …

Source classifications, stellar masses, and star-formation rates are presented for≈ 80 000
radio sources from the first data release of the Low Frequency Array Two-metre Sky Survey …

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 …

The dust-to-stellar mass ratio (M dust/M⋆) is a crucial, albeit poorly constrained, parameter
for improving our understanding of the complex physical processes involved in the …

Aims. We leverage the largest available Atacama Large Millimeter/submillimeter Array
(ALMA) survey from the archive (A 3 COSMOS) to study infrared luminosity function and dust …

Recent works have suggested that energy balance spectral energy distribution (SED) fitting
codes may be of limited use for studying high-redshift galaxies for which the observed …

Context. Over the past few years the Atacama Large Millimeter Array (ALMA) has detected
dust-rich galaxies whose cold dust emission is spatially disconnected from the ultraviolet …

We present an optical to near-infrared (NIR) selected astronomical catalogue covering 1270
deg2. This is the first attempt to systematically combine data from 23 of the premier …