S. T. Bryson
- Astronomy and Astrophysics top 10%
- Instrumentation top 10%
- Computer Vision and Pattern Recognition
- Computer Graphics and Computer-Aided Design top 10%
- Human-Computer Interaction
- Co-authors
- David KenwrightJohan N SiebertDaniel HuberI BíróR. SzabóE. Forgács‐DajkaL. L. KissA. Derekas
- Topics
- Astronomy and Astrophysical Research (5 papers)Stellar, planetary, and galactic studies (5 papers)Astrophysics and Star Formation Studies (4 papers)
- Partner nations
- United StatesAustraliaGermany
In The Last Decade
S. T. Bryson
12 papers receiving 144 citations
Peers
Comparison fields: 5 of 30
- Astronomy and Astrophysics 100
- Instrumentation 47
- Computer Vision and Pattern Recognition 28
- Computer Graphics and Computer-Aided Design 27
- Human-Computer Interaction 15
Countries citing papers authored by S. T. Bryson
This map shows the geographic impact of S. T. Bryson'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. T. Bryson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. T. Bryson more than expected).
Fields of papers citing papers by S. T. Bryson
This network shows the impact of papers produced by S. T. Bryson. 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. T. Bryson. The network helps show where S. T. Bryson may publish in the future.
Co-authorship network of co-authors of S. T. Bryson
This figure shows the co-authorship network connecting the top 25 collaborators of S. T. Bryson. A scholar is included among the top collaborators of S. T. Bryson 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. T. Bryson. S. T. Bryson is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | VizieR Online Data Catalog: K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017) | 2 |
| 2 | Observational Constraints, Stellar Models, and Kepler Data for θ Cyg, the Brightest Star Observable by Kepler | 1 |
| 3 | 9 | |
| 4 | 49 | |
| 5 | 41 | |
| 6 | Detecting Multiple Transiting Planets with the Kepler Mission | 1 |
| 7 | 4 | |
| 8 | 9 | |
| 9 | 9 | |
| 10 | 9 | |
| 11 | 15 | |
| 12 | 2 |
About S. T. Bryson
S. T. Bryson is a scholar working on Instrumentation, Computer Graphics and Computer-Aided Design and Human-Computer Interaction, having authored 12 papers that have together received 151 indexed citations. Recurring topics across this work include Astronomy and Astrophysical Research (5 papers), Stellar, planetary, and galactic studies (5 papers) and Astrophysics and Star Formation Studies (4 papers). The work is most often cited by research in Instrumentation (47 citations), Computer Graphics and Computer-Aided Design (27 citations) and Astronomy and Astrophysics (100 citations). S. T. Bryson has collaborated with scholars based in United States, Australia and Germany. Frequent co-authors include David Kenwright, Johan N Siebert, Daniel Huber, I Bíró, R. Szabó, E. Forgács‐Dajka, L. L. Kiss, A. Derekas, T. R. Bedding and T. Borkovits. Their work appears in journals such as Nature, The Astrophysical Journal 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.