collaborators

6 papers

astro-ph.IM2025

amc: The Automated Mission Classifier for Telescope Bibliographies

John F. Wu, Joshua E. G. Peek, Sophie J. Miller +3

Telescope bibliographies record the pulse of astronomy research by capturing publication statistics and citation metrics for telescope facilities. Robust and scalable bibliographie…

astro-ph.IM2025

Re-envisioning Euclid Galaxy Morphology: Identifying and Interpreting Features with Sparse Autoencoders

John F. Wu, Michael Walmsley

Sparse Autoencoders (SAEs) can efficiently identify candidate monosemantic features from pretrained neural networks for galaxy morphology. We demonstrate this on Euclid Q1 images u…

astro-ph.IM2025

The Importance of Being Adaptable: An Exploration of the Power and Limitations of Domain Adaptation for Simulation-Based Inference with Galaxy Clusters

Michelle Ntampaka, A. Ciprijanovic, Ana Maria Delgado +4

The application of deep machine learning methods in astronomy has exploded in the last decade, with new models showing remarkably improved performance on benchmark tasks. Not nearl…

astro-ph.GA2025

The SAGA Survey. VI. The Size-Mass Relation for Low-Mass Galaxies Across Environments

Yasmeen Asali, Marla Geha, Erin Kado-Fong +10

We investigate how Milky Way-like environments influence the sizes and structural properties of low-mass galaxies by comparing satellites of Milky Way analogs from the Satellites A…

astro-ph.IM2025

The Platonic Universe: Do Foundation Models See the Same Sky?

UniverseTBD, :, Kshitij Duraphe +3

We test the Platonic Representation Hypothesis (PRH) in astronomy by measuring representational convergence across a range of foundation models trained on different data types. Usi…

astro-ph.GA2024

Estimating Dark Matter Halo Masses in Simulated Galaxy Clusters with Graph Neural Networks

Nikhil Garuda, John F. Wu, Dylan Nelson +1

Galaxies grow and evolve in dark matter halos. Because dark matter is not visible, galaxies' halo masses () must be inferred indirectly. We present a graph neur…