R. K. Cochrane
- Astronomy and Astrophysics top 2%
- Instrumentation top 2%
- Nuclear and High Energy Physics top 10%
- Ecology
- Electrical and Electronic Engineering
- Co-authors
- R. MaiolinoY. PengChristopher C. HaywardDaniel Anglés‐AlcázarClaude‐André Faucher‐GiguèreP. N. BestAndrew WetzelD. J. B. Smith
- Topics
- Galaxies: Formation, Evolution, Phenomena (36 papers)Astronomy and Astrophysical Research (17 papers)Astrophysics and Star Formation Studies (13 papers)
- Partner nations
- United KingdomUnited StatesNetherlands
In The Last Decade
R. K. Cochrane
37 papers receiving 929 citations
Hit Papers
Peers
Comparison fields: 5 of 36
- Astronomy and Astrophysics 1.0k
- Instrumentation 505
- Nuclear and High Energy Physics 210
- Ecology 41
- Electrical and Electronic Engineering 32
Countries citing papers authored by R. K. Cochrane
This map shows the geographic impact of R. K. Cochrane'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. K. Cochrane with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. K. Cochrane more than expected).
Fields of papers citing papers by R. K. Cochrane
This network shows the impact of papers produced by R. K. Cochrane. 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. K. Cochrane. The network helps show where R. K. Cochrane may publish in the future.
Co-authorship network of co-authors of R. K. Cochrane
This figure shows the co-authorship network connecting the top 25 collaborators of R. K. Cochrane. A scholar is included among the top collaborators of R. K. Cochrane 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. K. Cochrane. R. K. Cochrane is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 0 | |
| 3 | 0 | |
| 4 | 2 | |
| 5 | 6 | |
| 6 | 7 | |
| 7 | 11 | |
| 8 | 8 | |
| 9 | 3 | |
| 10 | 11 | |
| 11 | 10 | |
| 12 | Bursty Star Formation Naturally Explains the Abundance of Bright Galaxies at Cosmic Dawnbreakdown → | 86 |
| 13 | 15 | |
| 14 | 20 | |
| 15 | 35 | |
| 16 | 23 | |
| 17 | 17 | |
| 18 | 7 | |
| 19 | 57 | |
| 20 | 27 |
About R. K. Cochrane
R. K. Cochrane is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 40 papers that have together received 1.1k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (36 papers), Astronomy and Astrophysical Research (17 papers) and Astrophysics and Star Formation Studies (13 papers). The work is most often cited by research in Instrumentation (505 citations), Astronomy and Astrophysics (1.0k citations) and Nuclear and High Energy Physics (210 citations). R. K. Cochrane has collaborated with scholars based in United Kingdom, United States and Netherlands. Frequent co-authors include R. Maiolino, Y. Peng, Christopher C. Hayward, Daniel Anglés‐Alcázar, Claude‐André Faucher‐Giguère, P. N. Best, Andrew Wetzel, D. J. B. Smith, Philip F. Hopkins and Guochao Sun. 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.