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.
Rotation, convection, and magnetic activity in lower main-sequence stars
1984910 citationsR. W. Noyes, S. L. Baliunas et al.The 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 D. K. Duncan'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 D. K. Duncan with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. K. Duncan more than expected).
This network shows the impact of papers produced by D. K. Duncan. 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 D. K. Duncan. The network helps show where D. K. Duncan may publish in the future.
Co-authorship network of co-authors of D. K. Duncan
This figure shows the co-authorship network connecting the top 25 collaborators of D. K. Duncan.
A scholar is included among the top collaborators of D. K. Duncan 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 D. K. Duncan. D. K. Duncan is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Duncan, D. K.. (2006). Success and Failure Using Student Response Systems: "Clickers". American Astronomical Society Meeting Abstracts. 209.1 indexed citations
Duncan, D. K., Brian Chaboyer, Bruce W. Carney, et al.. (2001). Anchoring the Population II Distance Scale: Accurate Ages for Globular Clusters and Field Halo Stars. AAS. 198.3 indexed citations
7.
Duncan, D. K.. (1999). What to Do in a Big Lecture Class, Besides Lecture?. 28(1). 14.3 indexed citations
Deliyannis, Constantine P., Ann Merchant Boesgaard, J. King, & D. K. Duncan. (1996). New observations of Beryllium in the galactic halo. ASPC. 109. 679.1 indexed citations
10.
Duncan, D. K.. (1995). Major NLTE Corrections to HST Boron Observations. 5859.1 indexed citations
Duncan, D. K.. (1991). Rotation of Young Solar-Type Stars in the Orion Nebula Region. Bulletin of the American Astronomical Society. 23. 942.1 indexed citations
Rutten, R. G. M., C. J. Schrijver, C. Zwaan, D. K. Duncan, & R. Mewe. (1989). Magnetic structure in cool stars. XVI. Emissions from the outer atmospheres of M-type dwarfs. NASA Technical Reports Server (NASA). 219. 239–252.2 indexed citations
Duncan, D. K. & George W. Preston. (1979). The Binary δ Delta Scuti System δ Delphini. Bulletin of the American Astronomical Society. 11. 728.2 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.