C. S. Crawford

6.2k citations
81 papers · 3.7k indexed · h-index 26
Topics
Galaxies: Formation, Evolution, Phenomena (69 papers)Astrophysical Phenomena and Observations (43 papers)Astrophysics and Star Formation Studies (33 papers)

In The Last Decade

C. S. Crawford

79 papers receiving 3.6k citations

Peers

C. S. Crawford
Comparison fields: 5 of 44
  • Astronomy and Astrophysics 3.6k
  • Nuclear and High Energy Physics 1.3k
  • Instrumentation 629
  • Atomic and Molecular Physics, and Optics 87
  • Computational Mechanics 54
Replace G. Trinchieri with:
G. Trinchieri Italy
Jill Bechtold United States
T. Miyaji United States
J. Bergeron France
R.‐J. Dettmar Germany
H. E. Smith United States
David A. Turnshek United States
A. E. Hornschemeier United States
K. Sekiguchi Japan
P. A. Shaver Germany
C. S. Crawford relative to G. Trinchieri Italy G. Trinchieri's profile →
Citations per field
00.5×1.7×
G. Trinchieri · 1×
Citations per year

Countries citing papers authored by C. S. Crawford

Since Specialization
Citations

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

Fields of papers citing papers by C. S. Crawford

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of C. S. Crawford

This figure shows the co-authorship network connecting the top 25 collaborators of C. S. Crawford. A scholar is included among the top collaborators of C. S. Crawford 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. S. Crawford. C. S. Crawford 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
#WorkIndexed citations
1 0
2 5
3 15
4 97
5 48
6 118
7 41
8 28
9 3
10 22
11 46
12 12
13 7
14 11
15 15
16 13
17 41
18 7
19 15
20 4

About C. S. Crawford

C. S. Crawford is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 81 papers that have together received 3.7k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (69 papers), Astrophysical Phenomena and Observations (43 papers) and Astrophysics and Star Formation Studies (33 papers). The work is most often cited by research in Astronomy and Astrophysics (3.6k citations), Instrumentation (629 citations) and Nuclear and High Energy Physics (1.3k citations). C. S. Crawford has collaborated with scholars based in Russia, United Kingdom and United States. Frequent co-authors include A. C. Fabian, R. M. Johnstone, S. W. Allen, J. S. Sanders, A. C. Edge, K. Iwasawa, G. B. Taylor, H. Ebeling, J. P. Huchra and H. Böhringer. 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.

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2026