R. R. Burman
About
In The Last Decade
R. R. Burman
26 papers receiving 310 citations
Peers
Comparison fields: 5 of 30
- Astronomy and Astrophysics 307
- Nuclear and High Energy Physics 107
- Atomic and Molecular Physics, and Optics 25
- Oceanography 24
- Geophysics 23
Countries citing papers authored by R. R. Burman
This map shows the geographic impact of R. R. Burman'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. R. Burman with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. R. Burman more than expected).
Fields of papers citing papers by R. R. Burman
This network shows the impact of papers produced by R. R. Burman. 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. R. Burman. The network helps show where R. R. Burman may publish in the future.
Co-authorship network of co-authors of R. R. Burman
This figure shows the co-authorship network connecting the top 25 collaborators of R. R. Burman. A scholar is included among the top collaborators of R. R. Burman 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. R. Burman. R. R. Burman is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 86 | |
| 2 | The Swift short gamma-ray burst rate density: prospects for detecting binary neutron star mergers by aLIGO | 1 |
| 3 | 4 | |
| 4 | 21 | |
| 5 | 23 | |
| 6 | 8 | |
| 7 | 26 | |
| 8 | 4 | |
| 9 | 1 | |
| 10 | 2 | |
| 11 | 26 | |
| 12 | 3 | |
| 13 | Attenuation of Whistler Mode Waves Excited in the Insterstellar Medium by Pulsars(Note) | 2 |
| 14 | 3 | |
| 15 | 1 | |
| 16 | 2 | |
| 17 | On the physical nature of cosmic neutrino absorption II: cosmological models without continuous creation | 4 |
| 18 | 3 | |
| 19 | 1 | |
| 20 | 2 |
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.