works on

From the 1 of 12 linked papers with an AI index.

activity
20242026
collaborators

12 papers

astro-ph.IM2026

Enhancing WISE Infrared Imaging to Spitzer Resolution Using Deep Learning Super-Resolution

Saeed Rezaee, Shoubaneh Hemmati, Bahram Mobasher +4

The paper introduces a deep‑learning model that upscales WISE infrared images to near‑Spitzer resolution, achieving about 4.6× higher spatial detail and improved flux recovery and…

astro-ph.CO2026

Diffusion-based Galaxy Simulations for the Roman High Latitude Survey

Diana Scognamiglio, Jake H. Lee, Eric Huff +2

Future weak lensing analyses with the Nancy Grace Roman Space Telescope will require highly realistic image simulations to control shear systematics at unprecedented precision. A k…

astro-ph.GA2026

Learning to See Sharper: A Physics-Informed Artificial Intelligence Framework for Super-Resolving Galaxy Spectra

Aryana Haghjoo, Shoubaneh Hemmati, Bahram Mobasher +6

The information recoverable from galaxy spectra depends fundamentally on spectral resolution, yet assembling large samples at high resolution remains observationally expensive. We…

astro-ph.GA2026

Reducing the Dimensions of AGN Lightcurve Manifolds

Shoubaneh Hemmati, Jessica Krick, Daniel Stern +10

The Active Galactic Nuclei (AGN) glossary is vast and complex. Depending on selection method, observing wavelength, and brightness, AGNs are assigned distinct labels, yet the relat…

astro-ph.GA2025

Mapping the Galaxy Color-Star Formation Rate Relation with Manifold Learning and Infrared Image Stacking

Yu-Heng Lin, Daniel Masters, Andreas L. Faisst +7

Modern surveys present us with billions of faint galaxies for which we only have broadband images in 6-8 optical-to-near-infrared (NIR) filters. Galaxy star formation rates (…

astro-ph.GA2025

Selection of Dwarf Galaxies Hosting AGNs: A Measure of Bias and Contamination using Unsupervised Machine Learning Techniques

Sogol Sanjaripour, Archana Aravindan, Gabriela Canalizo +4

Identifying AGNs in dwarf galaxies is critical for understanding black hole formation but remains challenging due to their low luminosities, low metallicities, and star formation-d…