Current research

The VERTICO view of star forming gas in the Virgo Cluster
The VERTICO view of star forming gas in the Virgo Cluster

I investigate how galaxies form, evolve, and cease forming stars using observations from ALMA, MUSE, HST, LOFAR, and ASKAP. As we prepare for the SKA era, our group focuses on two scientific frontiers plus digital infrastructure. The areas below highlight active collaborations and projects with opportunities for students and postdocs.

Environmental Regulation of Star Formation

How dense environments reshape the interstellar medium. I co-lead MAUVE and VERTICO—using MUSE and ALMA to trace ram-pressure stripping and quantify how external pressures and stellar feedback regulate star formation down to ~50–100 parsec scales. Projects available.

MAUVE view of Virgo cluster galaxies
MAUVE view of stars and ionized gas in the Virgo galaxies

Evolution and Feedback in Dwarf Galaxies

Building a framework to understand how low-mass systems sustain or suppress star formation. Our collaborations combine UNIONS, LSST, LOFAR, and WALLABY data to characterize the interplay between star formation, cosmic rays, and AGN activity. Projects available.

Digital Infrastructure & CANFAR

At the Canadian Astronomy Data Centre, our group guides the CANFAR Science Platform and leads the SKA Regional Centre Network (SRCNet)—designing the distributed network to support SKA science. The Canadian SKA Regional Centre will require infrastructure two orders of magnitude more powerful than current Canadian capacity. Projects available.

Canadian SKA Regional Centre
Canadian SKA Regional Centre infrastructure

The group bridges observational astrophysics and advanced data science to handle the exabyte-scale challenges of the next decade. If you're interested in joining these efforts, see opportunities.