research

My research is in observational and computational astrophysics, with a focus on weak gravitational lensing and its application to galaxy cluster science and cosmology.

Currently, I work on the SuperBIT balloon-borne telescope, developing the end-to-end weak-lensing shape-measurement pipeline — including PSF characterization and modelling, shear calibration, and neural-network-based shape measurement.

My PhD work focused on Bayesian inference methods for the Cosmic Microwave Background (CMB), including maximum a posteriori (MAP) estimators for galaxy cluster mass measurement from CMB lensing, and Hamiltonian Monte Carlo methods for inferring our local motion from small-scale CMB anisotropies.

More to come soon.