By compiling a comprehensive census of literature studies, we investigate the evolution of
the main sequence (MS) of star-forming galaxies (SFGs) in the widest range of redshift (0< …

The PHANGS collaboration has been building a reference data set for the multiscale,
multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With …

Context. The efficiency of the different processes responsible for the evolution of interstellar
dust on the scale of a galaxy are, to date, very uncertain, spanning several orders of …

We present maps tracing the fraction of dust in the form of polycyclic aromatic hydrocarbons
(PAHs) in IC 5332, NGC 628, NGC 1365, and NGC 7496 from JWST/MIRI observations. We …

Aims. We perform a homogeneous analysis of an unprecedented set of spatially resolved
scaling relations (SRs) between interstellar medium (ISM) components, that is to say dust …

Mapping star-formation rates (SFR) within galaxies is key to unveiling their assembly and
evolution. Calibrations exist for computing the SFR from a combination of ultraviolet and …

We study the dust evolution in galaxies by implementing a detailed dust prescription in the
SAGE semi-analytical model (SAM) for galaxy formation. The new model, called Dusty …

Aims. The general consensus is that late-type galaxies undergo intense star-formation,
activity while early-type galaxies are mostly inactive. We question this general rule and …

We apply the radiative transfer (RT) code skirt on a sample of low-redshift (z≤ 0.1) galaxies
extracted from the TNG50 simulation to enable an apples-to-apples comparison with …

We perform a spectral energy distribution fitting analysis on a COSMOS photometric sample
covering the ultra-violet up to the far-infrared wavelengths and including emission lines from …