Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

In order to investigate the effects of galaxy mergers throughout the interaction sequence, we
present a study of 10 800 galaxies in close pairs and a smaller sample of 97 post-mergers …

Radio emission is a key indicator of star formation activity in galaxies, but the radio
luminosity–star formation relation has to date been studied almost exclusively at frequencies …

We measure the merger fraction of massive galaxies using the UltraVISTA/COSMOS
catalog, complemented with the deeper, higher resolution 3DHST+ CANDELS catalog …

The total infrared (IR) luminosity is very useful for estimating the star formation rate (SFR) of
galaxies, but converting the IR luminosity into an SFR relies on assumptions that do not hold …

Galaxy spectral energy distribution (SED) modelling is a powerful tool, but constraining how
well it is able to infer the true values for galaxy properties (eg the star formation rate) is …

Context. Nearly a dozen star-forming galaxies have been detected in γ-rays by the Fermi
observatory in the last decade. A remarkable property of this sample is the quasi-linear …

In this paper, we introduce the Local Volume TiNy Titans sample (LV-TNT), which is a part of
a larger body of work on interacting dwarf galaxies: TNT. This LV-TNT sample consists of 10 …

Context. Extragalactic fast X-ray transients (FXRTs) are short flashes of X-ray photons of
unknown origin that last a few seconds to hours. Aims. Our ignorance about their physical …

We present the evolution of dust and molecular gas properties in a sample of 11 z∼ 0.03
starburst to post-starburst (PSB) galaxies selected to span an age sequence from ongoing …