Countries citing papers authored by Th. Schmidt‐Kaler
Since
Specialization
Citations
This map shows the geographic impact of Th. Schmidt‐Kaler'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 Th. Schmidt‐Kaler with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Th. Schmidt‐Kaler more than expected).
Fields of papers citing papers by Th. Schmidt‐Kaler
This network shows the impact of papers produced by Th. Schmidt‐Kaler. 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 Th. Schmidt‐Kaler. The network helps show where Th. Schmidt‐Kaler may publish in the future.
Co-authorship network of co-authors of Th. Schmidt‐Kaler
This figure shows the co-authorship network connecting the top 25 collaborators of Th. Schmidt‐Kaler.
A scholar is included among the top collaborators of Th. Schmidt‐Kaler 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 Th. Schmidt‐Kaler. Th. Schmidt‐Kaler is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Schmidt‐Kaler, Th., et al.. (1993). UBV photometry of galactic foreground and LMC member stars. I: Galactic foreground stars. Astronomy & Astrophysics Supplement Series. 99(3). 591–614.2 indexed citations
5.
Kimeswenger, S., Benjamin D. Hoffmann, W. Schlosser, & Th. Schmidt‐Kaler. (1993). Photographic surface photometry of the Milky Way. VII: High-resolution B surface photometry of the southern Milky Way. Astronomy & Astrophysics Supplement Series. 97(2). 517–525.1 indexed citations
6.
Schmidt‐Kaler, Th.. (1992). The Hexapod Telescope: A New Way to Very Large Telescopes. European Southern Observatory Conference and Workshop Proceedings. 42. 117.5 indexed citations
7.
Schlosser, W., Th. Schmidt‐Kaler, & E. F. Milone. (1991). Challenges of Astronomy. CERN Document Server (European Organization for Nuclear Research).3 indexed citations
8.
Brandt, Peter, et al.. (1987). Dynamical Properties of a 12 m Telescope, as Determined by Finite Element Calculations. 70. 281.1 indexed citations
9.
Maitzen, H. M., et al.. (1985). Radial velocities for 28 southern young open clusters.. Astronomy & Astrophysics Supplement Series. 60(3). 355–364.1 indexed citations
10.
Schmidt‐Kaler, Th.. (1984). How to observe an nearby supernova. Observatory. 104. 234–235.1 indexed citations
11.
Feitzinger, J. V., et al.. (1983). A modified method to calibrate photographic surface photometry of galaxies and nebulae.. A&A. 126. 352–356.
Schmidt‐Kaler, Th.. (1982). Advantages, implementation and cost estimate of a long-life version of the Hipparcos payload.. ESASP. 177. 91–92.1 indexed citations
14.
Haupt, Wolfgang, H. M. Maitzen, R. W. RUDOLPH, et al.. (1976). A rapid spectrum scanner for a small telescope.. 50. 85–90.2 indexed citations
Moffat, A. F. J., Wolfgang Haupt, & Th. Schmidt‐Kaler. (1973). On X-Persei as a stellar X-ray source: Comparison with gamma Cassiopeiae.. 23. 433.8 indexed citations
17.
Schmidt‐Kaler, Th. & W. Schlosser. (1972). Flächenphotometrie des Südhimmels mit einer Kugelspiegelkamera.. 11. 120–125.2 indexed citations
Schmidt‐Kaler, Th.. (1961). Überriesen FO-K7 Ia-II in galaktischen Sterhaufen. I. Mittelung von: Leuchtkraft, Alter und Eigenfarben galaktischer Überriesen. Mit 3 Textabbildungen. 53. 1.1 indexed citations
20.
Schmidt‐Kaler, Th.. (1961). On the age of the Galaxy and the helium content of the old population I stars. Observatory. 81. 226–230.1 indexed citations
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
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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.