Abdurrouf
Physics and Astronomy · Indiana University
Publications
114
Citations
2,463
Est. group size
~1
Recurring co-author estimate
Active years
26
Publishing since 2001
Abdurrouf studies galaxies in the distant, early universe, using data from space telescopes such as JWST (James Webb Space Telescope) and the Euclid mission to examine how galaxies form and evolve, including very high-redshift objects seen when the universe was young. The work involves measuring stellar mass, chemical abundances, and star-formation activity in galaxies through techniques like spectral energy distribution fitting. A smaller set of publications also touches on molecular simulations and machine learning for signal processing.
Publication activity has grown over the past decade, rising from a few papers per year in the late 2010s to a peak around 2024, averaging about 15 publications per year over the last five years.
Generated by claude-opus-4-8 from public bibliographic data · Jul 9, 2026
Typically publishes in teams of ~10 · 19% small-team papers (≤3 authors) · across 30 venues
- GalSyn (Galaxy Synthesizer), a Forward-Modeling Software for Synthetic Galaxy Observations from Hydrodynamical Simulations
Zenodo (CERN European Organization for Nuclear Research) · 2026
- GalSyn First Data Release (DR1)
Zenodo (CERN European Organization for Nuclear Research) · 2026
- GalSyn (Galaxy Synthesizer), a Forward-Modeling Software for Synthetic Galaxy Observations from Hydrodynamical Simulations
Open MIND · 2026
- GalSyn First Data Release (DR1)
Open MIND · 2026
- High-redshift Galaxy Candidates at z = 6+ as Revealed by JWST Observations of MACS0647
The Astrophysical Journal · 2026
- VENUS: When red meets blue
Astronomy and Astrophysics · 2026
- Euclid preparation. LXXXI. The impact of nonparametric star formation histories on spatially resolved galaxy property estimation using synthetic Euclid images
Astronomy and Astrophysics · 2026
- BEACON: JWST NIRCam Pure-parallel Imaging Survey. IV. A Systematic Search for Galaxy Overdensities and Evidence for Gas Accretion Mode Transition
The Astrophysical Journal · 2026
- The z = 9.625 Cosmic Gems Galaxy was a "Compact Blue Monster" Propelled by Massive Star Clusters
arXiv (Cornell University) · 2025
- Little red dot variability over a century reveals black hole envelope via a giant Einstein cross
arXiv (Cornell University) · 2025
- Unveiling the Cosmic Gems Arc at z ∼ 10 with JWST NIRCam
The Astrophysical Journal · 2025
- The z = 9.625 Cosmic Gems galaxy was a compact “blue monster” propelled by massive star clusters
Astronomy and Astrophysics · 2025
- Implication of Galaxy-scale Negative Feedback by One of the Most Powerful Multiphase Outflows in a Hyperluminous Infrared Galaxy at Intermediate Redshift
The Astrophysical Journal · 2025
- Enhancing ECG Signal Quality in Noisy Environments: Comparative Evaluation of Signal Processing, Deep Learning, and Embedded Implementation
Research Square · 2025
- Physics-Based Explainable AI for ECG Segmentation: A Lightweight Model
arXiv (Cornell University) · 2025
- arXiv (Cornell University)×31
- The Astrophysical Journal×15
- Astronomy and Astrophysics×14
- Journal of Physics Conference Series×10
- AIP conference proceedings×6
- Zheng Zheng
Physics and Astronomy · The Ohio State University
- Vital Fernández
Physics and Astronomy · University of Michigan
- Sean D. Johnson
Physics and Astronomy · University of Michigan
- Keren Sharon
Physics and Astronomy · University of Michigan
- David J. Carr
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 Sep 1, 2026.
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