We describe the sample design for the SDSS-IV MaNGA survey and present the final
properties of the main samples along with important considerations for using these samples …

Galaxy mergers trigger both star formation and accretion on to the central supermassive
black hole. As a result of subsequent energetic feedback processes, it has long been …

At fixed galaxy stellar mass, there is a clear observational connection between structural
asymmetry and offset from the star-forming main sequence, ΔSFMS. Herein, we use the …

We present an analysis of the instantaneous supermassive black hole (SMBH) accretion
rates in a collection of 1563 post-merger galaxies drawn from the IllustrisTNG simulation …

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 …

Machine learning is becoming a popular tool to quantify galaxy morphologies and identify
mergers. However, this technique relies on using an appropriate set of training data to be …

We investigate the spatial structure and evolution of star formation and the interstellar
medium (ISM) in interacting galaxies. We use an extensive suite of parsec-scale galaxy …

ABSTRACT The Canada–France Imaging Survey (CFIS) will consist of deep, high-resolution
r-band imaging over∼ 5000 deg2 of the sky, representing a first-rate opportunity to identify …

We use the IllustrisTNG cosmological hydrodynamical simulations to investigate how the
specific star formation rates (sSFRs) of massive galaxies (M*> 1010 M⊙) depend on the …

We present a comprehensive suite of high-resolution (parsec-scale), idealized (non-
cosmological) galaxy merger simulations (24 runs, stellar mass ratio∼ 2.5: 1) to investigate …