E. Tolley
Physics and Astronomy · The Ohio State University
Publications
485
Citations
25,189
Est. group size
—
Recurring co-author estimate
Active years
15
Publishing since 2011
E. Tolley's recent work focuses on applying machine learning and deep learning methods to problems in radio astronomy and cosmology, including detecting radio galaxies and halos, removing foreground noise from 21-cm cosmological signals, and simulating dark matter and cosmic reionization using physics-informed neural networks. The research also explores efficient computational algorithms for radio-interferometric imaging and early-stage applications of quantum computing to astronomical image processing. This work sits at the intersection of astrophysics, signal processing, and computational methods rather than traditional particle physics experimentation.
Publication counts were relatively high and stable from 2017-2021 (averaging roughly 50-70 per year, likely reflecting large collaborative output) but have declined markedly since 2022, dropping to under 10-20 per year through 2024-2025.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- Solving the cosmological Vlasov–Poisson equations with physics-informed Kolmogorov–Arnold networks
Monthly Notices of the Royal Astronomical Society · 2025
- SPINN: Advancing Cosmological Simulations of Fuzzy Dark Matter with Physics Informed Neural Networks
The Astrophysical Journal · 2025
- Radio halo detection in MWA data using deep neural networks and generative data augmentation
Monthly Notices of the Royal Astronomical Society · 2025
- S-R2D2: a spherical extension of the R2D2 deep neural network series paradigm for wide-field radio-interferometric imaging
Monthly Notices of the Royal Astronomical Society · 2025
- SPINN: Advancing Cosmological Simulations of Fuzzy Dark Matter with Physics Informed Neural Networks
arXiv (Cornell University) · 2025
- S-R2D2: a spherical extension of the R2D2 deep neural network series paradigm for wide-field radio-interferometric imaging
arXiv (Cornell University) · 2025
- Deep learning approach for identification of <scp>H ii</scp> regions during reionization in 21-cm observations – II. Foreground contamination
Monthly Notices of the Royal Astronomical Society · 2024
- Quantum radio astronomy: Data encodings and quantum image processing
Astronomy and Computing · 2024
- The stability of deep learning for 21cm foreground removal across various sky models and frequency-dependent systematics
Monthly Notices of the Royal Astronomical Society · 2024
- Wavelet Scattering Networks for Identifying Radio Galaxy Morphologies
2024
- Bipp: An Efficient Hpc Implementation of the Bluebild Algorithm for Radio Astronomy
SSRN Electronic Journal · 2024
- SPC* Separating Point Source Contaminants at the Visibility Level
2024
- Radio Halo Detection in MWA Data using Deep Neural Networks and Generative Data Augmentation
arXiv (Cornell University) · 2024
- BIPP: An efficient HPC implementation of the Bluebild algorithm for radio astronomy
Astronomy and Computing · 2024
- SKA Science Data Challenge 2: analysis and results
Monthly Notices of the Royal Astronomical Society · 2023
- The European Physical Journal C×103
- Journal of High Energy Physics×98
- Physics Letters B×42
- Physical review. D/Physical review. D.×31
- Physical Review Letters×18
- A. Lapertosa
Physics and Astronomy · Purdue University West Lafayette
- A. Li
Physics and Astronomy · Indiana University
- A. G. Myagkov
Physics and Astronomy · Indiana University
- A. J. Myers
Physics and Astronomy · Indiana University
- A. Lounis
Physics and Astronomy · Indiana University
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 19, 2026.
Claim or correct this profile