Marshall C. Johnson
Physics and Astronomy · The Ohio State University
Publications
169
Citations
2,088
Est. group size
~5
Recurring co-author estimate
Active years
27
Publishing since 2000
Marshall C. Johnson studies exoplanets—planets orbiting stars beyond our solar system—with a focus on how their orbits are tilted or aligned relative to their host stars' spin, and on characterizing planetary atmospheres using high-resolution spectroscopy. Much of the recent work involves large surveys (such as SOYSAUCE and PEPSI-based projects) that measure orbital alignment in young planetary systems and study atmospheric composition and escape in giant, hot planets like hot Jupiters. This research combines ground-based telescope observations with data from missions like TESS to find, confirm, and study these distant planetary systems.
Publication output has fluctuated over the last decade with a dip around 2020-2021, followed by a resurgence to a fairly steady average of about 13 papers per year over the last five years.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- SOYSAUCE: Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape
Zenodo (CERN European Organization for Nuclear Research) · 2026
- SOYSAUCE: Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE). II. A 135 Myr Planet on an Aligned Orbit with Transit Timing Variations
The Astronomical Journal · 2026
- Wide Binary Orbits Are Preferentially Aligned with the Orbits of Small Planets, but Probably Not Hot Jupiters
The Astronomical Journal · 2025
- Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE): A Likely Aligned Orbit for the 3 Myr Planet TIDYE-1 b
The Astrophysical Journal Letters · 2025
- HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth
The Astronomical Journal · 2025
- The Multiband Imaging Survey for High-alpha PlanetS (MISHAPS). I. Preliminary Constraints on the Occurrence Rate of Hot Jupiters in 47 Tucanae
The Astronomical Journal · 2025
- HD 35843: A Sun-like star hosting a long period sub-Neptune and inner super-Earth
arXiv (Cornell University) · 2025
- PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). IV. High-Resolution Phased-Resolved Spectroscopy of The Ultra Hot Jupiter KELT-20 b
arXiv (Cornell University) · 2025
- PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). IV. High-resolution Phased-resolved Spectroscopy of the Ultra-hot-Jupiter KELT-20 b
The Astronomical Journal · 2025
- Identification of the Top TESS Objects of Interest for Atmospheric Characterization of Transiting Exoplanets with JWST
The Astronomical Journal · 2024
- TOI-1994b: A Low-mass Eccentric Brown Dwarf Transiting A Subgiant Star
The Astronomical Journal · 2024
- The PEPSI Exoplanet Transit Survey (PETS). V: New Na D transmission spectra indicate a quieter atmosphere on HD 189733b
arXiv (Cornell University) · 2024
- Resting places: on wounds, war and the Irish Revolution
Irish Studies Review · 2024
- Overfitting Affects the Reliability of Radial Velocity Mass Estimates of the V1298 Tau Planets
The Astronomical Journal · 2023
- arXiv (Cornell University)×30
- The Astronomical Journal×26
- Monthly Notices of the Royal Astronomical Society×13
- VizieR Online Data Catalog×9
- UNC Libraries×9
- Marc H. Pinsonneault
Physics and Astronomy · The Ohio State University
- Zachary G. Maas
Physics and Astronomy · Indiana University
- Lyra Cao
Physics and Astronomy · The Ohio State University
- Marcelo Tala Pinto
Physics and Astronomy · The Ohio State University
- Constantine P. Deliyannis
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.
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