R. Beswick
- Astronomy and Astrophysics top 5%
- Nuclear and High Energy Physics top 10%
- Instrumentation top 10%
- Atomic and Molecular Physics, and Optics
- Spectroscopy
- Co-authors
- A. PedlarT. W. B. MuxlowS. AaltoK. A. WillsJ. F. GallimoreM. K. ArgoA. J. HollowayC. G. Mundell
- Topics
- Galaxies: Formation, Evolution, Phenomena (31 papers)Radio Astronomy Observations and Technology (16 papers)Astrophysics and Star Formation Studies (15 papers)
- Partner nations
- United KingdomGermanyUnited States
In The Last Decade
R. Beswick
44 papers receiving 493 citations
Peers
Comparison fields: 5 of 20
- Astronomy and Astrophysics 497
- Nuclear and High Energy Physics 219
- Instrumentation 47
- Atomic and Molecular Physics, and Optics 15
- Spectroscopy 10
Countries citing papers authored by R. Beswick
This map shows the geographic impact of R. Beswick'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 R. Beswick with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. Beswick more than expected).
Fields of papers citing papers by R. Beswick
This network shows the impact of papers produced by R. Beswick. 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 R. Beswick. The network helps show where R. Beswick may publish in the future.
Co-authorship network of co-authors of R. Beswick
This figure shows the co-authorship network connecting the top 25 collaborators of R. Beswick. A scholar is included among the top collaborators of R. Beswick 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 R. Beswick. R. Beswick is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 1 | |
| 3 | 2 | |
| 4 | 5 | |
| 5 | Radio constraints on the mass-loss rate of the Type Ia SN 2018gv | 1 |
| 6 | Mass-loss rate constraints on the Type Ia SN 2018pv from e-MERLIN observations | 1 |
| 7 | 5 | |
| 8 | 30 | |
| 9 | 17 | |
| 10 | 13 | |
| 11 | 7 | |
| 12 | 5 | |
| 13 | 7 | |
| 14 | 5.0 GHz Continuum MERLIN Observations of the Type Ia SN 2013dy | 1 |
| 15 | 14 | |
| 16 | Constraining Star Formation and AGN in z∼2 Massive Galaxies using High Resolution MERLIN Radio Observations | 14 |
| 17 | 9 | |
| 18 | 6 | |
| 19 | 2 | |
| 20 | 6 |
About R. Beswick
R. Beswick is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 46 papers that have together received 503 indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (31 papers), Radio Astronomy Observations and Technology (16 papers) and Astrophysics and Star Formation Studies (15 papers). The work is most often cited by research in Astronomy and Astrophysics (497 citations), Nuclear and High Energy Physics (219 citations) and Instrumentation (47 citations). R. Beswick has collaborated with scholars based in United Kingdom, Germany and United States. Frequent co-authors include A. Pedlar, T. W. B. Muxlow, S. Aalto, K. A. Wills, J. F. Gallimore, M. K. Argo, A. J. Holloway, C. G. Mundell, S. T. Garrington and A. B. Peck. 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.