M. T. Reynolds
Physics and Astronomy · The Ohio State University
Publications
173
Citations
4,212
Est. group size
—
Recurring co-author estimate
Active years
22
Publishing since 2005
M. T. Reynolds works in high-energy astrophysics, studying black holes and related compact objects using X-ray telescopes such as NuSTAR and the Chandra X-ray Observatory, along with multiwavelength data from instruments like JWST. Their work covers black hole spin measurements, X-ray binaries (systems where a black hole pulls material from a companion star), tidal disruption events (when a black hole shreds a passing star), and supermassive black holes such as the one at the center of our galaxy. This research draws on large observational collaborations, including contributions to the Event Horizon Telescope project.
Publication output has been fairly steady over the past decade, fluctuating between about 6 and 15 papers per year, with a modest decline in the most recent couple of years (partial data for 2025-2026).
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- 3-79keV NuSTAR obs. of Swift J1728.9-3613
Strasbourg Astronomical Data Center · 2026
- The Population of NuSTAR Black Hole X-Ray Binaries
The Astrophysical Journal · 2025
- A multiwavelength study of the Galactic center black hole candidate MAXI J1744-294
arXiv (Cornell University) · 2025
- Systematically Revisiting All NuSTAR Spins of Black Holes in X-Ray Binaries
The Astrophysical Journal · 2024
- Evidence for Dust Depletion in a Misaligned Protoplanetary Disk with JWST
The Astrophysical Journal Letters · 2024
- Investigating the Mass of the Black Hole and Possible Wind Outflow of the Accretion Disk in the Tidal Disruption Event AT2021ehb
The Astrophysical Journal · 2024
- Fierce Feedback in an Obscured, Sub-Eddington State of the Seyfert 1.2 Markarian 817
The Astrophysical Journal Letters · 2024
- Prospects for Time-Domain and Multi-Messenger Science with AXIS
Universe · 2024
- Investigating the Mass of the Black Hole and Possible Wind Outflow of the Accretion Disk in the Tidal Disruption Event AT2021ehb
arXiv (Cornell University) · 2024
- Evidence for Dust Depletion in a Misaligned Protoplanetary Disk with JWST
arXiv (Cornell University) · 2024
- A Systematic View of Ten New Black Hole Spins
The Astrophysical Journal · 2023
- Evidence of a Massive Stellar Disruption in the X-Ray Spectrum of ASASSN-14li
The Astrophysical Journal Letters · 2023
- The Spin of a Newborn Black Hole: Swift J1728.9-3613
The Astrophysical Journal · 2023
- The first X-ray look at SMSS J114447.77-430859.3: the most luminous quasar in the last 9 Gyr
Monthly Notices of the Royal Astronomical Society · 2023
- The Black Hole Candidate Swift J1728.9–3613 and the Supernova Remnant G351.9–0.9
The Astrophysical Journal · 2023
- The Astrophysical Journal×16
- UvA-DARE (University of Amsterdam)×15
- Monthly Notices of the Royal Astronomical Society×14
- arXiv (Cornell University)×10
- The astronomer's telegram×9
- Anjan Dutta
Physics and Astronomy · Purdue University West Lafayette
- Jiachen Jiang
Physics and Astronomy · The Ohio State University
- Jin-Hong Chen
Physics and Astronomy · The Ohio State University
- Jack M. M. Neustadt
Physics and Astronomy · The Ohio State University
- R. M. Wagner
Physics and Astronomy · The Ohio State 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.
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