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 …

In this paper, we investigate the relationship between 150 MHz luminosity and the star-
formation rate–the SFR-L 150 MHz relation–using 150 MHz measurements for a near …

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 …

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 …

It is well known that supermassive black holes (SMBHs) and their host galaxies co-evolve. A
manifestation of this co-evolution is the correlation that has been found between the SMBH …

We use approximately 1800 X-ray active galactic nuclei (AGN) in the eROSITA Final
Equatorial-Depth Survey (eFEDS) that span over two orders of magnitude in X-ray …

We explore the properties of the host galaxies of X-ray selected AGN in the COSMOS field
using the Chandra Legacy sample and the LEGA-C survey VLT optical spectra. Our main …

It is still a matter of intense debate how supermassive black holes (SMBHs) grow and the
role played by feedback from active galactic nuclei (AGN) in the coevolution of SMBHs and …

In this work, our aim is to investigate the star formation rate (SFR) of the host galaxies of
active galactic nuclei (AGNs) in the early Universe. To this end, we constructed a sample of …

We report the identification of radio (0.144–3 GHz) and mid-, far-infrared, and sub-mm (24–
850μm) emission at the position of one of 41 UV-bright () z≃ 6.6–6.9 Lyman-break galaxy …