G. A. Wynn
- Astronomy and Astrophysics top 2%
- Astrophysical Phenomena and Observations 52
- Stellar, planetary, and galactic studies 28
- Gamma-ray bursts and supernovae 28
- Pulsars and Gravitational Waves Research 23
- Astrophysics and Star Formation Studies 21
- Astro and Planetary Science 10
- Galaxies: Formation, Evolution, Phenomena 8
- Instrumentation top 5%
- Geophysics top 10%
- High-pressure geophysics and materials 11
- Computational Mechanics top 10%
- Co-authors
- A. R. KingP. T. O’BrienB. P. GompertzA. J. NortonK. HorneM. R. BurleighA. RowlinsonChris Power
- Partner nations
- United KingdomUnited StatesAustralia
In The Last Decade
G. A. Wynn
74 papers receiving 1.5k citations
Peers
Comparison fields: 5 of 35
- Astronomy and Astrophysics 1.5k
- Instrumentation 89
- Nuclear and High Energy Physics 281
- Geophysics 126
- Computational Mechanics 79
Countries citing papers authored by G. A. Wynn
This map shows the geographic impact of G. A. Wynn'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 G. A. Wynn with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. A. Wynn more than expected).
Fields of papers citing papers by G. A. Wynn
This network shows the impact of papers produced by G. A. Wynn. 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 G. A. Wynn. The network helps show where G. A. Wynn may publish in the future.
Co-authorship network
The 25 scholars most cited alongside G. A. Wynn, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | 2024 | 3 | |
| 2 | 2020 | 10 | |
| 3 | 2020 | 9 | |
| 4 | 2018 | 4 | |
| 5 | 2017 | 14 | |
| 6 | 2013 | 22 | |
| 7 | 2011 | 8 | |
| 8 | Broad UV and probable X-ray eclipses in nova U Sco | 2010 | 1 |
| 9 | CSS081007:030559+054715: Swift confirmation of 1.77 day period in X- ray and UV, and a suggestion of a ~45 day period. | 2009 | 1 |
| 10 | 2009 | 15 | |
| 11 | 2009 | 29 | |
| 12 | 2006 | 8 | |
| 13 | 2006 | 43 | |
| 14 | 2004 | 21 | |
| 15 | 2004 | 109 | |
| 16 | 2004 | 2 | |
| 17 | Modelling unstable accretion discs | 2002 | 1 |
| 18 | 1997 | 10 | |
| 19 | 1996 | 7 | |
| 20 | 1992 | 56 |
About G. A. Wynn
G. A. Wynn is a scholar working on Astronomy and Astrophysics, Geophysics and Instrumentation, having authored 74 papers that have together received 1.5k indexed citations. Recurring topics across this work include Astrophysical Phenomena and Observations (52 papers), Stellar, planetary, and galactic studies (28 papers), Gamma-ray bursts and supernovae (28 papers), Pulsars and Gravitational Waves Research (23 papers), Astrophysics and Star Formation Studies (21 papers), High-pressure geophysics and materials (11 papers), Astro and Planetary Science (10 papers) and Galaxies: Formation, Evolution, Phenomena (8 papers). The work is most often cited by research in Astronomy and Astrophysics (1.5k citations), Instrumentation (89 citations) and Nuclear and High Energy Physics (281 citations). G. A. Wynn has collaborated with scholars based in United Kingdom, United States and Australia. Frequent co-authors include A. R. King, P. T. O’Brien, B. P. Gompertz, A. J. Norton, K. Horne, M. R. Burleigh, A. Rowlinson, Chris Power, S. L. Casewell and J. D. Nichols.
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.