Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Realization of Accurate Close-Binary Light Curves: Application to MR Cygni
19711.6k citationsR. E. Wilson, E. J. DevinneyThe Astrophysical Journalprofile →
Accuracy and efficiency in the binary star reflection effect
1990678 citationsR. E. WilsonThe Astrophysical Journalprofile →
Eccentric orbit generalization and simultaneous solution of binary star light and velocity curves
1979658 citationsR. E. WilsonThe Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of R. E. Wilson'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 R. E. Wilson with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. E. Wilson more than expected).
This network shows the impact of papers produced by R. E. Wilson. 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 R. E. Wilson. The network helps show where R. E. Wilson may publish in the future.
Co-authorship network of co-authors of R. E. Wilson
This figure shows the co-authorship network connecting the top 25 collaborators of R. E. Wilson.
A scholar is included among the top collaborators of R. E. Wilson 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 R. E. Wilson. R. E. Wilson 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.
Wilson, R. E., E. J. Devinney, & W. Van Hamme. (2020). WD: Wilson-Devinney binary star modeling. Astrophysics Source Code Library.1 indexed citations
2.
Wilson, R. E., C. A. Pilachowski, & D. Terrell. (2017). THE M DWARF ECLIPSING BINARY CU CANCRI. The Astrophysical Journal. 835(2). 251–251.6 indexed citations
3.
Wilson, R. E. & W. Van Hamme. (2015). Computing Binary Star Observables.17 indexed citations
4.
Wilson, R. E. & W. Van Hamme. (2010). Eclipsing Binary Modeling Advances - Recent and On the Way. ASPC. 435. 45.3 indexed citations
5.
Wilson, R. E.. (2006). Binary Stars and their Light Curves. ASPC. 349. 71.5 indexed citations
6.
Wilson, R. E., et al.. (2003). Toward optimal processing of large eclipsing binary data sets. ASPC. 298. 313.1 indexed citations
Hamme, W. Van & R. E. Wilson. (1994). Binary star radial velocities weighted by line strength.. Memorie della Societa Astronomica Italiana. 65. 89–92.2 indexed citations
14.
Wilson, R. E.. (1994). Invited Review Paper Understanding Binary Stars Via Light Curves. 55. 1.3 indexed citations
15.
Terrell, D., et al.. (1992). Binary stars : a pictorial atlas.5 indexed citations
16.
Wilson, R. E.. (1986). Timing Within the Western Area Power Administration. Defense Technical Information Center (DTIC). 467–490.2 indexed citations
17.
Thompson, G. I., K. Nandy, C. Jamar, et al.. (1980). Book-Review - Catalogue of Stellar Ultraviolet Fluxes. Observatory. 100. 14.1 indexed citations
18.
Wilson, R. E. & Christy Caldwell. (1978). A model of V356 Sagittarii. The Astrophysical Journal. 221. 917–917.9 indexed citations
19.
Paterson, W. R., et al.. (1976). Photoelectric Photometry of AK Her. Bulletin of the American Astronomical Society. 8. 306.1 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.