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.
A Catalog of Parameters for Globular Clusters in the Milky Way
Countries citing papers authored by William E. Harris
Since
Specialization
Citations
This map shows the geographic impact of William E. Harris'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 William E. Harris with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites William E. Harris more than expected).
Fields of papers citing papers by William E. Harris
This network shows the impact of papers produced by William E. Harris. 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 William E. Harris. The network helps show where William E. Harris may publish in the future.
Co-authorship network of co-authors of William E. Harris
This figure shows the co-authorship network connecting the top 25 collaborators of William E. Harris.
A scholar is included among the top collaborators of William E. Harris 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 William E. Harris. William E. Harris is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
McKay, Adam, A. L. Cochran, Neil Dello Russo, et al.. (2014). Evolution of fragment-species production in comet C/2012 S1 (ISON) from 1.6 au to 0.4 au. 344.4 indexed citations
12.
Russo, Neil Dello, Ronald J. Vervack, Harold F. Weaver, et al.. (2014). The evolving chemical composition of C/2012 S1 ISON as it approached the Sun. Open Repository and Bibliography (University of Liège). 130.1 indexed citations
13.
Kaplan, G. H., et al.. (2012). NOVAS: Naval Observatory Vector Astrometry Software. Astrophysics Source Code Library.4 indexed citations
14.
Kaplan, G. H., et al.. (2012). Naval Observatory Vector Astrometry Software (NOVAS) Version 3.1:Fortran, C, and Python Editions. 24.
15.
Geisler, D., et al.. (2004). Wide-Field Washington Photometry of the NGC 5128 Globular Cluster System. 204.4 indexed citations
Durrell, Patrick R., William E. Harris, C. J. Pritchet, & T. J. Davidge. (1999). Photometry of the Outer Halo of M31. AAS. 195.1 indexed citations
18.
Stetson, P. B., J. E. Hesser, R. D. McClure, et al.. (1996). Pal 3 and Eridanus: HST CMDs of second-parameter globular clusters in the outer halo.. Bulletin of the American Astronomical Society. 28. 1362.3 indexed citations
19.
Harris, William E.. (1996). VizieR Online Data Catalog: Globular Clusters in the Milky Way (Harris, 1996).2 indexed citations
20.
Harris, William E.. (1953). Effect of Five Antibiotics in Varying Concentrations on Growth of Young Corn Plants. Digital Commons @ Butler University (Butler University). 11(1). 6.2 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.