C. J. Schalinski

581 total citations
29 papers, 326 citations indexed

About

C. J. Schalinski is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Aerospace Engineering. According to data from OpenAlex, C. J. Schalinski has authored 29 papers receiving a total of 326 indexed citations (citations by other indexed papers that have themselves been cited), including 24 papers in Astronomy and Astrophysics, 14 papers in Nuclear and High Energy Physics and 6 papers in Aerospace Engineering. Recurrent topics in C. J. Schalinski's work include Radio Astronomy Observations and Technology (15 papers), Astrophysics and Cosmic Phenomena (14 papers) and GNSS positioning and interference (6 papers). C. J. Schalinski is often cited by papers focused on Radio Astronomy Observations and Technology (15 papers), Astrophysics and Cosmic Phenomena (14 papers) and GNSS positioning and interference (6 papers). C. J. Schalinski collaborates with scholars based in Germany, United States and France. C. J. Schalinski's co-authors include T. P. Krichbaum, A. Witzel, D. S. Heeschen, C. A. Hummel, A. Quirrenbach, A. Alberdi, A. Witzel, K. J. Johnston, S. Britzen and J. A. Zensus and has published in prestigious journals such as Nature, Proceedings of the National Academy of Sciences and The Astrophysical Journal.

In The Last Decade

C. J. Schalinski

27 papers receiving 317 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
C. J. Schalinski Germany 9 307 245 29 18 18 29 326
J. N. Chengalur India 6 302 1.0× 114 0.5× 31 1.1× 12 0.7× 29 1.6× 8 319
R. Wegner Germany 9 357 1.2× 359 1.5× 17 0.6× 14 0.8× 12 0.7× 11 383
D. A. Graham Germany 7 248 0.8× 120 0.5× 15 0.5× 27 1.5× 20 1.1× 44 265
H. E. Hardebeck United States 5 176 0.6× 88 0.4× 22 0.8× 14 0.8× 10 0.6× 8 200
S. Kenderdine United Kingdom 8 242 0.8× 141 0.6× 40 1.4× 19 1.1× 8 0.4× 19 272
Yoshiharu Asaki Japan 12 321 1.0× 107 0.4× 52 1.8× 17 0.9× 8 0.4× 40 332
P. A. Heckert United States 11 354 1.2× 173 0.7× 18 0.6× 9 0.5× 7 0.4× 33 384
A. A. Stepanian Armenia 11 274 0.9× 229 0.9× 9 0.3× 10 0.6× 16 0.9× 48 338
C. H. Costain Canada 10 279 0.9× 188 0.8× 44 1.5× 10 0.6× 9 0.5× 25 312
R. A. Preston United States 11 396 1.3× 170 0.7× 35 1.2× 34 1.9× 11 0.6× 44 412

Countries citing papers authored by C. J. Schalinski

Since Specialization
Citations

This map shows the geographic impact of C. J. Schalinski'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 C. J. Schalinski with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. J. Schalinski more than expected).

Fields of papers citing papers by C. J. Schalinski

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by C. J. Schalinski. 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 C. J. Schalinski. The network helps show where C. J. Schalinski may publish in the future.

Co-authorship network of co-authors of C. J. Schalinski

This figure shows the co-authorship network connecting the top 25 collaborators of C. J. Schalinski. A scholar is included among the top collaborators of C. J. Schalinski 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 C. J. Schalinski. C. J. Schalinski 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.
Penny, A. J., et al.. (1998). Darwin interferometer. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 3350. 666–666. 3 indexed citations
2.
Röser, S., U. Bastian, K. S. de Boer, et al.. (1997). DIVA - towards microarcsecond global astrometry. Research at the University of Copenhagen (University of Copenhagen). 402. 777–782. 7 indexed citations
3.
Bastian, U., H. Mandel, W. Seifert, et al.. (1996). DIVA ‐ An interferometric minisatellite for astrometry and photometry. Astronomische Nachrichten. 317(4). 281–288. 7 indexed citations
4.
Guirado, J. C., J. M. Marcaide, P. Elósegui, et al.. (1995). VLBI differential astrometry of the radio sources 1928+738 and 2007+777 at 5 GHz.. A&A. 293. 613–625.
5.
Schalinski, C. J., K. J. Johnston, A. Witzel, et al.. (1995). VLBI Observations of Cygnus X-3 during the 1985 October Radio Outburst. The Astrophysical Journal. 447. 752–752. 27 indexed citations
6.
Lichti, G., T. J. Balonek, T. Courvoisier, et al.. (1995). Simultaneous and quasi-simultaneous observations of the continuum emission of the quasar 3C 273 from radio to γ-ray energies. University of New Hampshire Scholars Repository (University of New Hampshire at Manchester). 298. 711. 3 indexed citations
7.
Krichbaum, T. P., et al.. (1994). MM-VLBI: Bending of Jets in the Vicinity of AGN. 39. 2 indexed citations
8.
Krichbaum, T. P., et al.. (1994). mm-VLBI: Jets in the Vicinity of Galaxy-Cores. Symposium - International Astronomical Union. 159. 187–188. 4 indexed citations
9.
Greve, A., et al.. (1994). Disk brightness temperature of the planets at 43 GHz (and 43 GHz flux densities of some continuum sources).. 286. 654–658. 4 indexed citations
10.
Krichbaum, T. P., A. Witzel, D. A. Graham, C. J. Schalinski, & J. A. Zensus. (1993). New results from VLBI at 43 GHz. 181. 2 indexed citations
11.
Hummel, C. A., T. W. B. Muxlow, T. P. Krichbaum, et al.. (1992). MERLIN and VLBI observations of the quasar 0836+710 : morphology of a parsec-kiloparsec scale jet.. 266(1). 93–100. 2 indexed citations
12.
Hummel, C. A., C. J. Schalinski, T. P. Krichbaum, et al.. (1992). The jets of quasar 1928+738 : superluminal motion and large-scale structure. 257(2). 489–500. 2 indexed citations
13.
Quirrenbach, A., A. Witzel, C. A. Hummel, et al.. (1992). Statistics of intraday variability in extragalactic radio sources. 258(2). 279–284. 21 indexed citations
14.
Marcaide, J. M., A. Alberdi, P. Elósegui, et al.. (1990). Detection of a New Component in the Peculiar Superluminal Quasar 4C 39.25. 59. 1 indexed citations
15.
Quirrenbach, A., A. Witzel, T. P. Krichbaum, et al.. (1989). Rapid variability of extragalactic radio sources. Nature. 337(6206). 442–444. 27 indexed citations
16.
Schalinski, C. J., W. Alef, A. Witzel, Jim Campbell, & Harald Schuh. (1988). First Results of the VLBI-Investigation of Sources from Geodetic IRIS-Experiments. Symposium - International Astronomical Union. 129. 359–360. 2 indexed citations
17.
Eckart, A., A. Witzel, Peter L. Biermann, et al.. (1987). Investigation of a complete sample of flat spectrum radio sources from the S5 survey. II. Results.. Astronomy & Astrophysics Supplement Series. 67(1). 121–146. 2 indexed citations
18.
Heeschen, D. S., T. P. Krichbaum, C. J. Schalinski, & A. Witzel. (1987). Rapid variability of extragalactic radio sources. The Astronomical Journal. 94. 1493–1493. 101 indexed citations
19.
Johnston, K. J., R. Simon, A. Eckart, et al.. (1987). 1928 + 738 - A superluminal source with large-scale structure. The Astrophysical Journal. 313. L85–L85. 7 indexed citations
20.
Eckart, A., A. Witzel, Peter L. Biermann, et al.. (1986). Investigation of a complete sample of flat spectrum radio sources from the S5 survey. I: Analysis. 168. 17–24. 2 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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