Kévin Baillié
About
In The Last Decade
Kévin Baillié
22 papers receiving 343 citations
Peers
Comparison fields: 5 of 27
- Astronomy and Astrophysics 354
- Atmospheric Science 61
- Geophysics 38
- Ecology 29
- Spectroscopy 24
Countries citing papers authored by Kévin Baillié
This map shows the geographic impact of Kévin Baillié'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 Kévin Baillié with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Kévin Baillié more than expected).
Fields of papers citing papers by Kévin Baillié
This network shows the impact of papers produced by Kévin Baillié. 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 Kévin Baillié. The network helps show where Kévin Baillié may publish in the future.
Co-authorship network of co-authors of Kévin Baillié
This figure shows the co-authorship network connecting the top 25 collaborators of Kévin Baillié. A scholar is included among the top collaborators of Kévin Baillié 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 Kévin Baillié. Kévin Baillié is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 5 | |
| 2 | 15 | |
| 3 | 3 | |
| 4 | 11 | |
| 5 | 100 | |
| 6 | 1 | |
| 7 | 11 | |
| 8 | 16 | |
| 9 | How Mimas cleared the Cassini Division | 3 |
| 10 | 18 | |
| 11 | 43 | |
| 12 | 16 | |
| 13 | Origin of Refractory Inclusion Diversity by Turbulent Transport in the Inner Solar Nebula | 5 |
| 14 | 12 | |
| 15 | Insights on CAIs Thermal History from Turbulent Transport Simulations of Micron-Sized Precursors in the Early Solar Nebula | 2 |
| 16 | 0 | |
| 17 | 16 | |
| 18 | 36 | |
| 19 | 2 | |
| 20 | 35 |
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.