Overview
The faintest galaxies in the nearby universe
Our research group explores the faintest and most elusive galaxies in the nearby universe — systems so diffuse and low-mass that they often escape traditional surveys.
By combining ultra-deep observations from ground- and space-based telescopes with creative, data-driven discovery techniques, we uncover hidden populations of dwarf and low-surface-brightness galaxies beyond the Milky Way.
These galaxies serve as powerful laboratories for understanding how galaxies form, how dark matter shapes structure on small scales, and how visible and invisible matter co-evolve across cosmic time.
Our big questions
What we're chasing
- How common are low-mass and ultra-faint galaxies beyond the Local Group, and what is their true census in the nearby universe?
- How does dark matter shape the structure and dynamics of the smallest galaxies?
- What is the relationship between dark matter and visible matter in galaxies at the lowest masses?
- Which physical processes govern the formation and evolution of low-mass galaxies?
- What new astrophysical phenomena emerge when we push observations into the low-surface-brightness universe?