Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

We present the catalog of∼ 31,500 extragalactic H i line sources detected by the completed
Arecibo Legacy Fast ALFA (ALFALFA) survey out to z< 0.06, including both high signal-to …

Here we introduce the interstellar dust modelling framework THEMIS (The Heterogeneous
dust Evolution Model for Interstellar Solids), which takes a global view of dust and its …

We present a synthesis of the astronomical observations constraining the wavelength-
dependent extinction, emission, and polarization from interstellar dust from UV to microwave …

The Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) is a blind narrow-
band (NB) Hα+[NII] imaging survey carried out with MegaCam at the Canada–France …

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 …

Context. Studying the coupling between the energy output produced by the central quasar
and the host galaxy is fundamental to fully understand galaxy evolution. Quasar feedback is …

Aims. We aim to study the fraction of stellar radiation absorbed by dust, f abs, in 814 galaxies
of different morphological types. The targets constitute the vast majority (93%) of the …

The dust mass absorption coefficient, κd is the conversion function used to infer physical
dust masses from observations of dust emission. However, it is notoriously poorly …

Unbiased sky background modeling is crucial for the analysis of deep wide-field images, but
it remains a major challenge in low surface brightness astronomy. Traditional image …