collaborators

14 papers

astro-ph.CO2026

A Multimodal Approach to Star--Galaxy Separation using SPHEREx Spectrophotometry and DESI Legacy Survey Imaging

Kendrick Nguyen, Richard M. Feder, Sean Bruton +1

Stellar contamination is a critical systematic for increasingly precise large-scale structure analyses from ongoing and next-generation surveys. Experiments targeting constraints o…

cs.LG2026

Can Microcanonical Langevin Dynamics Leverage Mini-Batch Gradient Noise?

Emanuel Sommer, Kangning Diao, Jakob Robnik +2

Scaling inference methods such as Markov chain Monte Carlo to high-dimensional models remains a central challenge in Bayesian deep learning. A promising recent proposal, microcanon…

astro-ph.CO2026

Field-Level Inference from Galaxies: BAO Reconstruction

Adrian E. Bayer, Liam Parker, David Valcin +3

Baryon acoustic oscillations (BAO) underpin the key cosmological results from modern spectroscopic galaxy surveys, but nonlinear gravitational evolution limits the precision achiev…

cs.AI2026

The Future of Artificial Intelligence and the Mathematical and Physical Sciences (AI+MPS)

Andrew Ferguson, Marisa LaFleur, Lars Ruthotto +97

This community paper developed out of the NSF Workshop on the Future of Artificial Intelligence (AI) and the Mathematical and Physics Sciences (MPS), which was held in March 2025 w…

astro-ph.EP2026

Exoplanet transit search at the detection limit: detection and false alarm vetting pipeline

Jakob Robnik, Uroš Seljak, Jon M. Jenkins +1

One of the primary mission goals of the Kepler space telescope was to detect Earth-like terrestrial planets in the habitable zone around Sun-like stars. These planets are at the de…

astro-ph.EP2025

Reassessment of Kepler's habitable zone Earth-like exoplanets with data-driven null-signal templates

Jakob Robnik, Uroš Seljak

One of the primary mission goals of the Kepler space telescope is to detect Earth-like terrestrial planets in the habitable zone around Sun-like stars. Unfortunately, such planets…