activity
20192026
most citedEnhanced mass-loss rate evolution of stars with and missing optically-observed type II core-collapse supernovae

8 citations · 10 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

The Deep Learning Halo Definer: A Multimodal Framework for Halo Mass and Gas Fraction Inference on Galaxy Groups and Clusters

Caleb Ogle, Kalvyn N. Poncelet Adams, Benjamin D. Oppenheimer +5

Accurately inferring dark matter halo properties like the total halo mass (M_{halo}) and gas fractions (f_{gas}) remains particularly challenging at group scales, where low member…

astro-ph.GA2026

CNN-Based Inference of Gaseous Halo Properties from Synthetic X-ray and 21-cm HI Observations

Kalvyn N. Poncelet Adams, Benjamin D. Oppenheimer, Naomi Gluck +3

Quantifying the information content in multi-wavelength observations is critical for setting exposure times for upcoming X-ray and 21-cm HI radio surveys. We train convolutional ne…

astro-ph.SR2026

Benchmarking Machine Learning Emulators of Stellar Evolution for Precision Asteroseismology

Naomi Gluck, Earl P. Bellinger, Yan Liang +5

Fast and accurate stellar evolution emulators---surrogate models that approximate expensive simulation outputs with machine learning (ML)---are powerful tools for modern stellar ch…

astro-ph.GA2023★ 2 cited

An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks

Naomi Gluck, Benjamin D. Oppenheimer, Daisuke Nagai +2

The circum-galactic medium (CGM) can feasibly be mapped by multiwavelength surveys covering broad swaths of the sky. With multiple large datasets becoming available in the near fut…

astro-ph.SR2019★ 8 cited

Enhanced mass-loss rate evolution of stars with and missing optically-observed type II core-collapse supernovae

Roni Anna Gofman, Naomi Gluck, Noam Soker

We evolve stellar models with zero-age main sequence (ZAMS) mass of under the assumption that they experience an enhanced mass-loss rate when cros…