The Observational Cosmology and Astrophysics Lab develops radio instrumentation and data‑analysis pipelines for observations spanning meter to millimeter wavelengths. We use these capabilities to detect and map galaxies, galaxy clusters, and supermassive black holes, with the broader goal of uncovering the physical processes that govern their formation and evolution.
Three-dimensional X-ray/SZ/WL inference and CLUMP-3D methodology
Development of a 12–20 GHz prototype receiver and COMAP × galaxy/Lyα cross-correlation analysis
Establishing a Korea–Australia pathfinder baselines toward SKA-Low VLBI