We report 18 dust continuum detections (≥ 3.3 σ) at∼ 88 and 158 out of 49 ultraviolet (UV)-
bright galaxies (M UV<− 21.3 mag) at> 6.5, observed by the Cycle-7 Atacama Large …

We present new multifrequency Atacama Large Millimeter/submillimeter Array (ALMA)
continuum observations of the massive [], UV-luminous [] galaxy REBELS-25 in Bands 3, 4 …

We present measurements of the CO luminosity functions (LFs) and the evolution of the
cosmic molecular gas density out to z∼ 6 based on an 8.5 arcmin 2 spectral scan survey at …

Gaseous outflows are key phenomena in the evolution of galaxies, as they affect star
formation (either positively or negatively), eject gas from the core or disc, and directly cause …

We make use of ultra-deep 3 GHz Karl G. Jansky Very Large Array (VLA) observations of the
COSMOS field from the multiband COSMOS-XS survey to infer radio luminosity functions …

As the primary fuel for star formation, molecular gas plays a key role in galaxy evolution. A
number of techniques have been used for deriving the mass of molecular reservoirs in the …

Abstract The MeerKAT Absorption Line Survey (MALS) has observed 391 telescope
pointings at the L band (900–1670 MHz) at δ≲+ 20. We present radio continuum images …

By combining high-sensitivity LOFAR 150 MHz, uGMRT 400 MHz and 1250 MHz, GMRT
610 MHz, and VLA 5 GHz data in the ELAIS-N1 field, we study the radio spectral properties …

Mapping the average active galactic nucleus (AGN) luminosity across galaxy populations
and over time reveals important clues regarding the interplay between supermassive black …

Radio free–free emission is considered to be one of the most reliable tracers of star
formation in galaxies. However, as it constitutes the faintest part of the radio spectrum …