K. S. de Boer
- Astronomy and Astrophysics top 2%
- Instrumentation top 2%
- Nuclear and High Energy Physics top 10%
- Computational Mechanics top 10%
- Statistical and Nonlinear Physics top 10%
- Topics
- Stellar, planetary, and galactic studies (33 papers)Astrophysics and Star Formation Studies (25 papers)Astronomy and Astrophysical Research (16 papers)
- Partner nations
- GermanyUnited StatesFrance
In The Last Decade
K. S. de Boer
47 papers receiving 1.3k citations
Hit Papers
Peers
Comparison fields: 5 of 49
- Astronomy and Astrophysics 1.3k
- Instrumentation 513
- Nuclear and High Energy Physics 170
- Computational Mechanics 89
- Statistical and Nonlinear Physics 62
Countries citing papers authored by K. S. de Boer
This map shows the geographic impact of K. S. de Boer'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 K. S. de Boer with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites K. S. de Boer more than expected).
Fields of papers citing papers by K. S. de Boer
This network shows the impact of papers produced by K. S. de Boer. 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 K. S. de Boer. The network helps show where K. S. de Boer may publish in the future.
Co-authorship network of co-authors of K. S. de Boer
This figure shows the co-authorship network connecting the top 25 collaborators of K. S. de Boer. A scholar is included among the top collaborators of K. S. de Boer 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 K. S. de Boer. K. S. de Boer is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 10 | |
| 2 | 53 | |
| 3 | 135 | |
| 4 | 7 | |
| 5 | 16 | |
| 6 | 17 | |
| 7 | 8 | |
| 8 | 35 | |
| 9 | 2 | |
| 10 | 1 | |
| 11 | 9 | |
| 12 | 9 | |
| 13 | GAIA: Composition, formation and evolution of the Galaxybreakdown → | 623 |
| 14 | 5 | |
| 15 | 40 | |
| 16 | Location and thickness of the nearest neutral gas cloud in the direction of Auriga-Perseus. | 1 |
| 17 | Hot subluminous stars at high galactic latitudes. I, Spectra and Strömgren photometry | 4 |
| 18 | Spectroscopy of helium-rich subluminous O and B stars. | 1 |
| 19 | Intersstellar absorption lines between 2000 and 3000 A in nearby stars observed with BUSS | 2 |
| 20 | 9 |
About K. S. de Boer
K. S. de Boer is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 50 papers that have together received 1.4k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (33 papers), Astrophysics and Star Formation Studies (25 papers) and Astronomy and Astrophysical Research (16 papers). The work is most often cited by research in Instrumentation (513 citations), Astronomy and Astrophysics (1.3k citations) and Nuclear and High Energy Physics (170 citations). K. S. de Boer has collaborated with scholars based in Germany, United States and France. Frequent co-authors include P. T. de Zeeuw, M. A. C. Perryman, X. Luri, M. G. Lattanzi, O. Pace, G. Gilmore, F. Mignard, E. Høg, Marcel S. Pawlowski and Pavel Kroupa. 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.