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.
Atlas of quasar energy distributions
19941.1k citationsM. Elvis, B. J. Wilkes et al.The Astrophysical Journal Supplement Seriesprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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This map shows the geographic impact of B. J. Wilkes'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. J. Wilkes with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. J. Wilkes more than expected).
This network shows the impact of papers produced by B. J. Wilkes. 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. J. Wilkes. The network helps show where B. J. Wilkes may publish in the future.
Co-authorship network of co-authors of B. J. Wilkes
This figure shows the co-authorship network connecting the top 25 collaborators of B. J. Wilkes.
A scholar is included among the top collaborators of B. J. Wilkes 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. J. Wilkes. B. J. Wilkes is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Lonsdale, Carol J., Mark Lacy, Amy Kimball, et al.. (2015). RADIO JET FEEDBACK AND STAR FORMATION IN HEAVILY OBSCURED, HYPERLUMINOUS QUASARS AT REDSHIFTS ~ 0.5–3. I. ALMA OBSERVATIONS. DSpace@MIT (Massachusetts Institute of Technology).28 indexed citations
10.
Leipski, C., Martin Haas, H. Meusinger, et al.. (2007). Narrow-line AGN in the ISO-2MASS survey\n. Springer Link (Chiba Institute of Technology).5 indexed citations
11.
Polletta, M., B. J. Wilkes, Brian Siana, et al.. (2006). The Most Obscured AGN in the Chandra/SWIRE Survey in the Lockman Hole. ESASP. 604. 807.
12.
Garcia, M. R. & B. J. Wilkes. (2002). Magnitudes of X-ray Nova XTE J1650-500 in Quiescence. ATel. 104. 1.1 indexed citations
13.
Brotherton, M. S., Ari Laor, D. Wills, et al.. (1999). The PG X-Ray QSO sample: Links between the UV-X-Ray Continuum and Emission Lines. ASPC. 162. 373.
14.
Kuhn, O., Aneta Siemiginowska, M. Elvis, B. J. Wilkes, & Jonathan McDowell. (1991). Optical Variations in Blue Bump Quasars. Bulletin of the American Astronomical Society. 23. 926.1 indexed citations
15.
Wilkes, B. J.. (1991). The emerging picture of quasars.. 19(12). 34–41.1 indexed citations
Wilkes, B. J.. (1982). Broad emission-line profiles in QSO spectra.. 94. 761.1 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.