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 …

Observations of evolution in the dust-to-metal ratio allow us to constrain the dominant dust
processing mechanisms. In this work, we present a study of the dust-to-metal and dust-to …

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will
scan thousands of square degrees of the northern sky with a unique set of 56 filters using …

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 accurate resolved WISE photometry of galaxies in the combined SINGS and
KINGFISH sample. The luminosities in the W3 12 μm and W4 23 μm bands are calibrated to …

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 …

Aims. Within the framework of the DustPedia project we investigate the properties of cosmic
dust and its interaction with stellar radiation (originating from different stellar populations) for …

Aims. The purpose of this work is the characterization of the radial distribution of dust, stars,
gas, and star-formation rate (SFR) in a sub-sample of 18 face-on spiral galaxies extracted …

We present a new method to accurately describe the ionization fraction and the size
distribution of polycyclic aromatic hydrocarbons (PAHs) within astrophysical sources. To this …

Aims. The DustPedia project is capitalising on the legacy of the Herschel Space
Observatory, using cutting-edge modelling techniques to study dust in the 875 DustPedia …