Ji Wang
Physics and Astronomy · The Ohio State University
Publications
243
Citations
8,406
Est. group size
~14
Recurring co-author estimate
Active years
34
Publishing since 1993
Ji Wang's research focuses on exoplanets, using high-resolution spectroscopy and direct imaging to study the atmospheres, masses, and orbital architectures of giant planets and brown dwarf companions orbiting other stars. Much of the recent work involves instrumentation and data from the Keck Planet Imager and Characterizer (KPIC), analyzing gases like water in exoplanet atmospheres and linking planetary compositions to their host stars' chemistry and orbital dynamics. Note that the publication list also contains several unrelated titles (e.g., on materials science, steel, and basin geology), which appear to be from different researchers sharing the same name rather than this PI's work.
Publication output grew substantially from 2017 through a peak around 2023, and has been declining somewhat in 2024-2026, though data for the most recent year is likely incomplete.
Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026
- Dynamical Architectures of S-type Transiting Planets in Binaries. II. A Dichotomy in Orbital Alignment of Small Planets in Close Binary Systems
The Astronomical Journal · 2026
- FDM-Printed RGO/Co@C/PLA/TPU Composites Featuring Core-Shell Co@C for Enhanced Electromagnetic Absorption and Mechanical Performance
SSRN Electronic Journal · 2026
- A Novel Tailoring Strategy for Simultaneously Enhancing the Creep Strength and Hydrogen Embrittlement Resistance of Ferritic Heat-resistant Steels
SSRN Electronic Journal · 2026
- Mechanism of overpressure generation of Permian and Triassic source rocks in the central Junggar Basin,northwestern China
SSRN Electronic Journal · 2026
- Chemical Abundances Shape History (CASH). I. A Link between Giant Planets' Orbital Periods and Host Stellar C/O Ratios
The Astronomical Journal · 2026
- Data products from "Atmospheric characterization of six ultra-hot Jupiters from K-band high-resolution spectroscopy"
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Data products from "Atmospheric characterization of six ultra-hot Jupiters from K-band high-resolution spectroscopy"
Zenodo (CERN European Organization for Nuclear Research) · 2026
- Early Accretion of Large Amounts of Solids for Directly Imaged Exoplanets
The Astrophysical Journal · 2025
- Water Dissociation and Rotational Broadening in the Atmosphere of KELT-20 b from High-resolution Spectroscopy
The Astronomical Journal · 2025
- Technical description and performance of the phase II version of the Keck Planet Imager and Characterizer
Journal of Astronomical Telescopes Instruments and Systems · 2025
- True Mass and Atmospheric Composition of the Nontransiting Hot Jupiter HD 143105 b
The Astronomical Journal · 2025
- The Watery Atmosphere of HD 209458 b Revealed by Joint <i>K</i> - and <i>L</i> -band High-resolution Spectroscopy
The Astronomical Journal · 2025
- Fringing analysis and forward modeling of Keck Planet Imager and Characterizer (KPIC) spectra
Journal of Astronomical Telescopes Instruments and Systems · 2025
- Technical description and performance of the phase II version of the Keck Planet Imager and Characterizer
arXiv (Cornell University) · 2025
- Water dissociation and rotational broadening in the atmosphere of KELT-20 b from high-resolution spectroscopy
arXiv (Cornell University) · 2025
- arXiv (Cornell University)×52
- The Astronomical Journal×34
- The Astrophysical Journal×12
- Monthly Notices of the Royal Astronomical Society×5
- SSRN Electronic Journal×5
- Jason Wang
Physics and Astronomy · The Ohio State University
- Lyra Cao
Physics and Astronomy · The Ohio State University
- Alexander P. Stephan
Physics and Astronomy · The Ohio State University
- Caprice L. Phillips
Physics and Astronomy · The Ohio State University
- Marc H. Pinsonneault
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.
Claim or correct this profile