Context. Measuring how the physical properties of galaxies change across cosmic times is
essential to understand galaxy formation and evolution. With the advent of numerous ground …

We present a new, publicly available library of dust spectral energy distributions (SEDs).
These SEDs are characterized by only three parameters: the dust mass (M dust), the dust …

We study the dust content of galaxies from z= 0 to z= 9 in semi-analytic models of galaxy
formation that include new recipes to track the production and destruction of dust. We …

We present a" super-deblended" far-infrared (FIR) to (sub) millimeter photometric catalog in
the Cosmic Evolution Survey (COSMOS), prepared with the method recently developed by …

We present new measurements of the cosmic cold molecular gas evolution out to redshift 6
based on systematic mining of the Atacama Large Millimeter/submillimeter Array (ALMA) …

We aim to measure the average dust and molecular gas content of massive star-forming
galaxies (> 3× 10 10 M⊙) up to z= 4 in the COSMOS field to determine if the intense star …

We use spectra from the ALFALFA, GASS and COLD GASS surveys to quantify variations in
the mean atomic and molecular gas mass fractions throughout the SFR–M* plane and along …

Detailed studies of the spectral energy distribution (SED) of normal galaxies have
increasingly been used to understand the physical mechanism dominating their integrated …

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 …

We present a new technique to measure multi-wavelength" super-deblended" photometry
from highly confused images, which we apply to Herschel and ground-based far-infrared …