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.
The Chandra Deep Field North Survey. XIII. 2 Ms Point-Source Catalogs
2003447 citationsDonald P. Schneider, W. L. W. Sargent et al.The Astronomical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by W. L. W. Sargent
Since
Specialization
Citations
This map shows the geographic impact of W. L. W. Sargent'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 W. L. W. Sargent with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. L. W. Sargent more than expected).
Fields of papers citing papers by W. L. W. Sargent
This network shows the impact of papers produced by W. L. W. Sargent. 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 W. L. W. Sargent. The network helps show where W. L. W. Sargent may publish in the future.
Co-authorship network of co-authors of W. L. W. Sargent
This figure shows the co-authorship network connecting the top 25 collaborators of W. L. W. Sargent.
A scholar is included among the top collaborators of W. L. W. Sargent 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 W. L. W. Sargent. W. L. W. Sargent is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Barlow, T. A., F. Hamann, & W. L. W. Sargent. (1997). Partial Coverage and Time Variability of Narrow-Line Intrinsic QSO Absorption Systems. CERN Bulletin. 128. 13.2 indexed citations
Sargent, W. L. W.. (1991). Pluto-Charon: A Double Planet on the Ragged Edge of the Solar System. Bulletin of the American Astronomical Society. 23. 962.1 indexed citations
Myers, S. T., et al.. (1988). A Limit on the Anisotropy of the Microwave Background on Arcminute Scales. Bulletin of the American Astronomical Society. 20. 987.3 indexed citations
Lo, K. Y., W. L. W. Sargent, C. T. Kowal, & I. A. Smith. (1986). Search for dwarf galaxies in nearby groups.. Bulletin of the American Astronomical Society. 18. 450.1 indexed citations
Roxburgh, I. W., W. L. W. Sargent, & P. A. Strittmatter. (1966). Determination of rotational velocity and aspect for stars in clusters. Observatory. 86. 118–120.2 indexed citations
19.
Sargent, W. L. W. & Leonard Searle. (1966). The interpretation of B star spectra having weak helium lines. Observatory. 86. 27–29.1 indexed citations
20.
Sargent, W. L. W.. (1965). Forbidden emission lines in the spectrum of a G-type supergiant. Observatory. 85. 33–35.2 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.