S. Peng Oh
- Astronomy and Astrophysics top 0.2%
- Nuclear and High Energy Physics top 0.5%
- Instrumentation top 1%
- Aerospace Engineering top 5%
- Statistical and Nonlinear Physics top 5%
- Co-authors
- Steven R. FurlanettoF. H. BriggsMax GrönkeZoltán HaimanFulai GuoMateusz RuszkowskiEvan ScannapiecoClaude‐André Faucher‐Giguère
- Topics
- Galaxies: Formation, Evolution, Phenomena (68 papers)Astrophysics and Star Formation Studies (40 papers)Astrophysics and Cosmic Phenomena (35 papers)
- Partner nations
- United StatesGermanyUnited Kingdom
In The Last Decade
S. Peng Oh
91 papers receiving 5.6k citations
Hit Papers
Peers
Comparison fields: 5 of 61
- Astronomy and Astrophysics 5.6k
- Nuclear and High Energy Physics 2.6k
- Instrumentation 800
- Aerospace Engineering 300
- Statistical and Nonlinear Physics 163
Countries citing papers authored by S. Peng Oh
This map shows the geographic impact of S. Peng Oh's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by S. Peng Oh with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. Peng Oh more than expected).
Fields of papers citing papers by S. Peng Oh
This network shows the impact of papers produced by S. Peng Oh. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by S. Peng Oh. The network helps show where S. Peng Oh may publish in the future.
Co-authorship network of co-authors of S. Peng Oh
This figure shows the co-authorship network connecting the top 25 collaborators of S. Peng Oh. A scholar is included among the top collaborators of S. Peng Oh based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with S. Peng Oh. S. Peng Oh is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 3 | |
| 2 | 3 | |
| 3 | 2 | |
| 4 | 3 | |
| 5 | 2 | |
| 6 | 27 | |
| 7 | 19 | |
| 8 | 12 | |
| 9 | 3 | |
| 10 | Key Physical Processes in the Circumgalactic Mediumbreakdown → | 115 |
| 11 | 65 | |
| 12 | 80 | |
| 13 | 24 | |
| 14 | 58 | |
| 15 | 119 | |
| 16 | 46 | |
| 17 | 82 | |
| 18 | 45 | |
| 19 | 15 | |
| 20 | 154 |
About S. Peng Oh
S. Peng Oh is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 92 papers that have together received 5.9k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (68 papers), Astrophysics and Star Formation Studies (40 papers) and Astrophysics and Cosmic Phenomena (35 papers). The work is most often cited by research in Astronomy and Astrophysics (5.6k citations), Instrumentation (800 citations) and Nuclear and High Energy Physics (2.6k citations). S. Peng Oh has collaborated with scholars based in United States, Germany and United Kingdom. Frequent co-authors include Steven R. Furlanetto, F. H. Briggs, Max Grönke, Zoltán Haiman, Fulai Guo, Mateusz Ruszkowski, Evan Scannapieco, Claude‐André Faucher‐Giguère, Christoph Pfrommer and Matthew Hansen. Their work appears in journals such as The Astrophysical Journal, Physics Reports and Monthly Notices of the Royal Astronomical Society.
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.