Research focus
About the research
How can improved analysis methods extract cosmological information from large imaging surveys with minimal bias?
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The group develops and applies weak gravitational lensing and related analysis techniques to measure cosmic shear and galaxy properties from survey data. Current projects focus on Hyper Suprime-Cam data and preparations for Rubin Observatory LSST and the Roman Space Telescope, developing methods for shear estimation, PSF systematics removal, and redshift distribution inference. Researchers design generative and machine-learning approaches for galaxy morphology and ensemble redshift estimation to enable precision cosmology with upcoming wide-field surveys.
Selected publications
2 listedPeople & alumni
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