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.
Parameter estimation in X-ray astronomy
1976451 citationsM. Lampton, B. Margon et al.The Astrophysical Journalprofile →
Author Peers
Peers are selected by citation overlap in the author's most active subfields.
citations ·
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This map shows the geographic impact of B. Margon'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 B. Margon with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. Margon more than expected).
This network shows the impact of papers produced by B. Margon. 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 B. Margon. The network helps show where B. Margon may publish in the future.
Co-authorship network of co-authors of B. Margon
This figure shows the co-authorship network connecting the top 25 collaborators of B. Margon.
A scholar is included among the top collaborators of B. Margon 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 B. Margon. B. Margon is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Margon, B., et al.. (2015). The Kinematics of Dwarf Carbon Stars. AAS. 225.
4.
Levitan, D., S. R. Kulkarni, Thomas A. Prince, et al.. (2013). The Search for AM CVn Systems with the Palomar Transient Factory. Radboud Repository (Radboud University). 221.1 indexed citations
Margon, B., Eric W. Deutsch, A. Silber, et al.. (1994). Very deep x-ray observation sof three globular clusters. UvA-DARE (University of Amsterdam). 26(2). 872–872.2 indexed citations
Margon, B., Eric Wilcots, & Michael Bolte. (1991). Main Sequence Close Binary Stars in NGC 288. Bulletin of the American Astronomical Society. 23. 948.1 indexed citations
Stockman, H. S., Gary D. Schmidt, & B. Margon. (1980). A Direct Measurement of the Magnetic Field in AM Herculis. Bulletin of the American Astronomical Society. 12. 851.
15.
Margon, B., S. A. Grandi, R. A. Downes, et al.. (1979). The 164 and 13 Day Periods of SS 433. Bulletin of the American Astronomical Society. 11. 671.1 indexed citations
16.
Margon, B., S. A. Grandi, & R. A. Downes. (1979). The Kinematics of SS 433.. Bulletin of the American Astronomical Society. 11. 786.
17.
Margon, B., S. De Grandi, & H. A. Ford. (1979). Enormous Periodic Doppler Shifts in SS 433. Bulletin of the American Astronomical Society. 11. 446.9 indexed citations
18.
Margon, B.. (1978). The Optical Counterparts of Compact Galactic X-Ray Sources (invited). Bulletin of the American Astronomical Society. 10. 499.1 indexed citations
19.
Greenstein, George, B. Margon, S. Bowyer, et al.. (1976). A Search for Thermal Extreme Ultraviolet Radiation from Nearby Pulsars.. Bulletin of the American Astronomical Society. 54. 548–625.2 indexed citations
20.
Lampton, M., B. Margon, Robert A. Stern, Francesco Paresce, & S. Bowyer. (1976). An Intense Extreme Ultraviolet Source in Cetus. Bulletin of the American Astronomical Society. 8. 360.1 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.