ABSTRACT The Dwarf Galaxy Survey (DGS) program is studying low-metallicity galaxies
using 230 hr of far-infrared (FIR) and submillimetre (submm) photometric and spectroscopic …

The use of integral field spectroscopy is since recently allowing to measure the emission line
fluxes of an increasingly large number of star-forming galaxies, both locally and at high …

Aims. We propose to infer the output of the ionising continuum-leaking properties of galaxies
based upon their Lyα line profiles. Methods. We carried out Lyα radiation transfer …

The sensitive infrared telescopes, Spitzer and Herschel, have been used to target low-
metallicity star-forming galaxies, allowing us to investigate the properties of their interstellar …

Context. We present new photometric data from our Herschel guaranteed time key
programme, the Dwarf Galaxy Survey (DGS), dedicated to the observation of the gas and …

Physical properties of galaxies at z> 7 are of interest for understanding both the early
phases of star formation and the process of cosmic reionization. Chemical abundance …

We combine samples of nearby galaxies with Herschel photometry selected on their dust,
metal, H i and stellar mass content, and compare these to chemical evolution models in …

With the aim of understanding the coevolution of star formation rate (SFR), stellar mass (M*),
and oxygen abundance (O/H) in galaxies up to redshift z≃ 3.7, we have compiled the largest …

Abstract 2+ We present a methodology for the use of sulphur as global metallicity tracer in
galaxies, allowing performing a complete abundance analysis using only the red-to-near …

ABSTRACT Using new Very Large Telescope (VLT)/XShooter spectral observations we
analyse the physical properties of five z∼ 0.3–0.4 confirmed Lyman continuum (LyC) …