John Wu is an Associate Astronomer and applied AI scientist with a decade of experience at leading institutions including the Space Telescope Science Institute and Johns Hopkins University, specializing in interpretable AI/ML for scientific discovery. He builds and interprets deep learning models that extract physical galaxy properties from imaging, delivering state-of-the-art results such as a novel image-based estimator for cold gas content and the largest-ever sample of faint nearby galaxies. His work blends rigorous statistical methods, convolutional neural networks, and visualization tools (e.g., Grad-CAM and dimensionality reduction) to probe model behavior and astrophysical correlations. John has extensive experience across multi-wavelength datasets (Hubble, Herschel, ALMA, MeerKAT) and in developing data pipelines for large surveys and instruments, including the Roman Telescope. Based in Baltimore, he balances tenure-track research leadership with hands-on model development, collaborating across astronomy and CS to make machine learning both predictive and physically interpretable. An early interest in applied computer vision (CMU CyLab intern) underpins his long-standing commitment to trustworthy, reproducible ML for astronomy.
10 years of coding experience
8 years of employment as a software developer
Doctor of Philosophy - PhD, Astrophysics, Doctor of Philosophy - PhD, Astrophysics at Rutgers University–New Brunswick
Bachelor of Science - BS, Physics/Astrophysics, Bachelor of Science - BS, Physics/Astrophysics at Carnegie Mellon University
Extending the SAGA survey to the wide-field regime using deep learning
Contributions:3 releases, 161 commits, 2 PRs in 11 months
deep-learningsagasaga-surveyfieldsurvey
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