K. S. de Boer

2.5k total citations · 1 hit paper
50 papers, 1.4k citations indexed

About

K. S. de Boer is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, K. S. de Boer has authored 50 papers receiving a total of 1.4k indexed citations (citations by other indexed papers that have themselves been cited), including 47 papers in Astronomy and Astrophysics, 16 papers in Instrumentation and 9 papers in Computational Mechanics. Recurrent topics in K. S. de Boer's work include Stellar, planetary, and galactic studies (33 papers), Astrophysics and Star Formation Studies (25 papers) and Astronomy and Astrophysical Research (16 papers). K. S. de Boer is often cited by papers focused on Stellar, planetary, and galactic studies (33 papers), Astrophysics and Star Formation Studies (25 papers) and Astronomy and Astrophysical Research (16 papers). K. S. de Boer collaborates with scholars based in Germany, United States and France. K. S. de Boer's co-authors include G. Gilmore, O. Pace, M. A. C. Perryman, X. Luri, M. G. Lattanzi, E. Høg, F. Mignard, P. T. de Zeeuw, Pavel Kroupa and Blair D. Savage and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

K. S. de Boer

47 papers receiving 1.3k citations

Hit Papers

GAIA: Composition, formation and evolution of the Galaxy 2001 2026 2009 2017 2001 200 400 600

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
K. S. de Boer Germany 15 1.3k 513 170 89 62 50 1.4k
G. Jasniewicz France 8 1.5k 1.1× 573 1.1× 194 1.1× 149 1.7× 22 0.4× 30 1.6k
T. D. Oswalt United States 21 1.4k 1.1× 580 1.1× 121 0.7× 72 0.8× 22 0.4× 77 1.4k
S. Laloë France 2 1.2k 0.9× 472 0.9× 173 1.0× 131 1.5× 18 0.3× 5 1.3k
M. Konacki Poland 21 1.4k 1.0× 611 1.2× 57 0.3× 98 1.1× 38 0.6× 83 1.4k
S. Borde France 2 1.2k 0.9× 471 0.9× 173 1.0× 131 1.5× 18 0.3× 5 1.3k
Justin Harker United States 10 1.0k 0.8× 442 0.9× 166 1.0× 35 0.4× 57 0.9× 11 1.1k
A. Vallenari Italy 20 1.7k 1.3× 970 1.9× 69 0.4× 100 1.1× 36 0.6× 84 1.8k
W. Saunders United Kingdom 20 1.2k 0.9× 628 1.2× 255 1.5× 34 0.4× 76 1.2× 38 1.3k
J. Blazek United States 13 1.0k 0.8× 434 0.8× 203 1.2× 42 0.5× 46 0.7× 20 1.1k
S. Zaggia Italy 27 2.2k 1.6× 1.0k 2.0× 185 1.1× 67 0.8× 27 0.4× 91 2.2k

Countries citing papers authored by K. S. de Boer

Since Specialization
Citations

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

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

20 of 20 papers shown
1.
Richter, P., K. S. de Boer, K. Werner, & T. Rauch. (2015). High-velocity gas toward the LMC resides in the Milky Way halo. Springer Link (Chiba Institute of Technology). 10 indexed citations
2.
Richter, P., et al.. (2010). Interstellar absorptions towards the LMC: Small-scale density variations in Milky Way disc gas. arXiv (Cornell University). 6 indexed citations
3.
Boer, K. S. de, et al.. (2005). Kinematics of RHB stars to trace the structure of the Galaxy. Springer Link (Chiba Institute of Technology). 16 indexed citations
4.
Boer, K. S. de. (2004). The contribution of halo red giant mass loss to the high-velocity gas falling onto the Milky Way disk. Springer Link (Chiba Institute of Technology). 8 indexed citations
5.
Altmann, M., H. Edelmann, & K. S. de Boer. (2004). Studying the populations of our Galaxy using the kinematics of sdB stars. Astronomy and Astrophysics. 414(1). 181–201. 35 indexed citations
6.
Bailer‐Jones, C. A. L., et al.. (2003). Automated determination of stellar parameters from simulated dispersed images for DIVA. Astronomy and Astrophysics. 401(3). 1203–1213. 2 indexed citations
7.
Bluhm, Harald, K. S. de Boer, O. Marggraf, & P. Richter. (2001). ORFEUS echelle spectra: Molecular hydrogen in disk, IVC, and HVC gas in front of the LMC. Astronomy and Astrophysics. 367(1). 299–310. 9 indexed citations
8.
Richter, P., et al.. (1999). Discovery of molecular hydrogen in a high-velocity cloud of the Galactic halo. Nature. 402(6760). 386–387. 40 indexed citations
9.
Richter, P., K. S. de Boer, D. J. Bomans, et al.. (1999). ORFEUS II echelle spectra: On the H-2/CO ratio in LMC gas towards LH 10. University of Groningen research database (University of Groningen / Centre for Information Technology). 351(1). 323–329. 1 indexed citations
10.
Wakker, Bart P., Hugo van Woerden, U. J. Schwarz, et al.. (1996). Distance and Metallicity of HVCs. Symposium - International Astronomical Union. 169. 605–606.
11.
King, David L., G. Vladilo, K. S. de Boer, et al.. (1995). NGC 4526 gas, high velocity clouds, and Galactic halo gas: the interstellar medium towards SN 1994D.. CERN Bulletin. 300. 881. 1 indexed citations
12.
Boer, K. S. de, et al.. (1991). Location and thickness of the nearest neutral gas cloud in the direction of Auriga-Perseus.. Astronomy & Astrophysics Supplement Series. 87(3). 471–479. 1 indexed citations
13.
Moehler, S., T. Richtler, K. S. de Boer, R.‐J. Dettmar, & U. Heber. (1990). Hot subluminous stars at high galactic latitudes. I, Spectra and Strömgren photometry. Astronomy & Astrophysics Supplement Series. 86(1). 53–74. 4 indexed citations
14.
Dreizler, S., U. Heber, K. Werner, S. Moehler, & K. S. de Boer. (1990). Hot subliminous stars at high galactic latitudes. III, Non-LTE analysis of extremely helium rich sdO-stars. 235. 234–241. 3 indexed citations
15.
Savage, Blair D., E. B. Jenkins, Charles L. Joseph, & K. S. de Boer. (1989). Ultraviolet observations of interstellar absorption lines toward SN 1987A. The Astrophysical Journal. 345. 393–393. 8 indexed citations
16.
Heber, U., S. Dreizler, K. S. de Boer, S. Moehler, & T. Richtler. (1988). Spectroscopy of helium-rich subluminous O and B stars.. 1. 16. 1 indexed citations
17.
Boer, K. S. de, et al.. (1986). Intersstellar absorption lines between 2000 and 3000 A in nearby stars observed with BUSS. NASA Technical Reports Server (NASA). 157(1). 119–128. 2 indexed citations
18.
Boer, K. S. de & A. G. Nash. (1982). Ultraviolet absorption by interstellar gas near the LMC star HD 36402 in the interstellar bubble N51D. The Astrophysical Journal. 255. 447–447. 9 indexed citations
19.
Savage, Blair D. & K. S. de Boer. (1979). Observational evidence for a hot gaseous Galactic corona. The Astrophysical Journal. 230. L77–L77. 39 indexed citations
20.
Boer, K. S. de, R. Hoekstra, & K. A. van der Hucht. (1972). UV interstellar absorption lines in the spectrum of zeta Pup.. 21. 447. 3 indexed citations

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.

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