J. Richard Bond
- Astronomy and Astrophysics top 0.1%
- Cosmology and Gravitation Theories 53
- Galaxies: Formation, Evolution, Phenomena 53
- Radio Astronomy Observations and Technology 23
- Stellar, planetary, and galactic studies 11
- Instrumentation top 0.5%
- Astronomy and Astrophysical Research 12
- Nuclear and High Energy Physics top 0.2%
- Dark Matter and Cosmic Phenomena 16
- Astrophysics and Cosmic Phenomena 15
- Statistical and Nonlinear Physics top 0.5%
- Scientific Research and Discoveries 12
- Oceanography top 5%
J. Richard Bond
85 papers receiving 9.4k citations
Hit Papers
Peers
Comparison fields: 5 of 100
- Astronomy and Astrophysics 9.3k
- Instrumentation 1.9k
- Nuclear and High Energy Physics 4.1k
- Statistical and Nonlinear Physics 951
- Oceanography 362
Countries citing papers authored by J. Richard Bond
This map shows the geographic impact of J. Richard Bond'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 J. Richard Bond with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites J. Richard Bond more than expected).
Fields of papers citing papers by J. Richard Bond
This network shows the impact of papers produced by J. Richard Bond. 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 J. Richard Bond. The network helps show where J. Richard Bond may publish in the future.
Co-authorship network
The 25 scholars most cited alongside J. Richard Bond, 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 | 2025 | 0 | |
| 2 | 2024 | 2 | |
| 3 | 2024 | 2 | |
| 4 | 2024 | 2 | |
| 5 | 2023 | 9 | |
| 6 | 2023 | 5 | |
| 7 | 2023 | 5 | |
| 8 | 2021 | 72 | |
| 9 | 2020 | 4 | |
| 10 | 2020 | 65 | |
| 11 | 2019 | 37 | |
| 12 | 2013 | 19 | |
| 13 | 2012 | 0 | |
| 14 | 2009 | 69 | |
| 15 | 1999 | 157 | |
| 16 | 1998 | 5 | |
| 17 | Cosmic Web: Origin and Observables | 1998 | 1 |
| 18 | How filaments of galaxies are woven into the cosmic webbreakdown → | 1996 | 704 |
| 19 | 1994 | 72 | |
| 20 | 1984 | 18 |
About J. Richard Bond
J. Richard Bond is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 88 papers that have together received 9.7k indexed citations. Recurring topics across this work include Cosmology and Gravitation Theories (53 papers), Galaxies: Formation, Evolution, Phenomena (53 papers), Radio Astronomy Observations and Technology (23 papers), Dark Matter and Cosmic Phenomena (16 papers), Astrophysics and Cosmic Phenomena (15 papers), Astronomy and Astrophysical Research (12 papers), Scientific Research and Discoveries (12 papers) and Stellar, planetary, and galactic studies (11 papers). The work is most often cited by research in Astronomy and Astrophysics (9.3k citations), Instrumentation (1.9k citations) and Nuclear and High Energy Physics (4.1k citations). J. Richard Bond has collaborated with scholars based in Canada, United States and United Kingdom. Frequent co-authors include G. Efstathiou, N. Kaiser, J. Bardeen, D. S. Salopek, Alexander S. Szalay, Shaun Cole, Lev Kofman, Dmitry Pogosyan, B. J. Carr and S. T. Myers. Their work appears in journals such as Nature, Proceedings of the National Academy of Sciences and Physical Review Letters.
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.