B. M. Gaensler
- Astronomy and Astrophysics top 0.1%
- Nuclear and High Energy Physics top 0.2%
- Geophysics top 5%
- Oceanography top 5%
- Computational Mechanics top 5%
- Co-authors
- N. M. McClure‐GriffithsM. HaverkornJ. M. DickeyA. J. GreenF. CamiloPatrick SlaneV. M. KaspiR. N. Manchester
- Topics
- Astrophysics and Cosmic Phenomena (143 papers)Pulsars and Gravitational Waves Research (111 papers)Gamma-ray bursts and supernovae (100 papers)
- Partner nations
- AustraliaUnited StatesCanada
In The Last Decade
B. M. Gaensler
258 papers receiving 8.1k citations
Peers
Comparison fields: 5 of 64
- Astronomy and Astrophysics 8.1k
- Nuclear and High Energy Physics 4.6k
- Geophysics 436
- Oceanography 306
- Computational Mechanics 222
Countries citing papers authored by B. M. Gaensler
This map shows the geographic impact of B. M. Gaensler'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 B. M. Gaensler with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. M. Gaensler more than expected).
Fields of papers citing papers by B. M. Gaensler
This network shows the impact of papers produced by B. M. Gaensler. 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 B. M. Gaensler. The network helps show where B. M. Gaensler may publish in the future.
Co-authorship network of co-authors of B. M. Gaensler
This figure shows the co-authorship network connecting the top 25 collaborators of B. M. Gaensler. A scholar is included among the top collaborators of B. M. Gaensler 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 B. M. Gaensler. B. M. Gaensler 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 | 0 | |
| 3 | 1 | |
| 4 | 11 | |
| 5 | 7 | |
| 6 | 16 | |
| 7 | 12 | |
| 8 | 4 | |
| 9 | 5 | |
| 10 | 8 | |
| 11 | 1 | |
| 12 | 8 | |
| 13 | 46 | |
| 14 | 7 | |
| 15 | 2 | |
| 16 | 10 | |
| 17 | 1 | |
| 18 | Probing the Galactic Magnetic Field with the Allen Telescope Array | 1 |
| 19 | The Scale Height and Filling Factor of Warm Ionized Gas in the Milky Way | 0 |
| 20 | Further VLA observations of Sgr 1806-20. | 1 |
About B. M. Gaensler
B. M. Gaensler is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation, having authored 280 papers that have together received 8.5k indexed citations. Recurring topics across this work include Astrophysics and Cosmic Phenomena (143 papers), Pulsars and Gravitational Waves Research (111 papers) and Gamma-ray bursts and supernovae (100 papers). The work is most often cited by research in Astronomy and Astrophysics (8.1k citations), Nuclear and High Energy Physics (4.6k citations) and Instrumentation (220 citations). B. M. Gaensler has collaborated with scholars based in Australia, United States and Canada. Frequent co-authors include N. M. McClure‐Griffiths, M. Haverkorn, J. M. Dickey, A. J. Green, F. Camilo, Patrick Slane, V. M. Kaspi, R. N. Manchester, Shami Chatterjee and L. Staveley‐Smith. Their work appears in journals such as Nature, Science and The Astrophysical Journal.
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.