This map shows the geographic impact of B. Warner'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. Warner with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. Warner more than expected).
This network shows the impact of papers produced by B. Warner. 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. Warner. The network helps show where B. Warner may publish in the future.
Co-authorship network of co-authors of B. Warner
This figure shows the co-authorship network connecting the top 25 collaborators of B. Warner.
A scholar is included among the top collaborators of B. Warner 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. Warner. B. Warner is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
20 of 20 papers shown
1.
Warner, B.. (2018). Charles Darwin and John Herschel. SHILAP Revista de lepidopterología.
Woudt, P. A., et al.. (2013). CSS121123:045020-093113: A WZ Sge-type dwarf nova amongst the AM CVn systems. The astronomer's telegram. 4726. 1.
4.
Stephens, Robert D., B. Warner, Michael K. Shepard, & Alan W. Harris. (2008). Lightcurve and Radar Observations and Analysis of 11 Parthenope and 678 Fredegundis.2 indexed citations
5.
Harris, Alan W., B. Warner, & Petr Pravec. (2005). Asteroid Lightcurve Derived Data.4 indexed citations
6.
Warner, B.. (2002). Asteroid Photometry at the Palmer Divide Observatory: Results for 1333 Cevenola and 2460 Mitlincoln. 29. 74–75.2 indexed citations
7.
Warner, B.. (2001). Asteroid Photometry at the Palmer Divide Observatory. The Minor planet bulletin. 28. 31.2 indexed citations
8.
Stephens, Robert D., et al.. (2001). New Period Determination for 27 Euterpe, a Collaborative Project. 28. 1–2.
9.
Warner, B.. (2000). The Minor Planet Observer. The Minor planet bulletin. 27. 11–12.2 indexed citations
10.
O’Donoghue, D., B. Warner, D. Kilkenny, et al.. (1990). Whole Earth Telescope observations of the interacting binary white dwarf V803 CEN in its low state.. Monthly Notices of the Royal Astronomical Society. 245(1). 140–146.2 indexed citations
11.
Warner, B.. (1988). University of Cape Town Report. 47. 35.1 indexed citations
12.
Warner, B.. (1987). The William Herschel 14-foot Telescope. 46. 158.1 indexed citations
Livio, Mario & B. Warner. (1984). Wind accretion onto white dwarfs. Observatory. 104. 152–159.13 indexed citations
15.
Warner, B.. (1982). The Large Southern Telescope - Cape or Melbourne. Quarterly journal of the Royal Astronomical Society. 23. 505.1 indexed citations
16.
Warner, B.. (1978). A History of Scientific Endeavour in South Africa. 37. 15.41 indexed citations
17.
Warner, B.. (1977). The Double Star Discoveries of Fearon Fallows. 36. 134.1 indexed citations
18.
Warner, B.. (1968). Transition Probabilities in n p and n p 5 Configurations. 69. 399.1 indexed citations
19.
Lambert, David L. & B. Warner. (1968). ABUNDANCES OF THE ELEMENTS IN THE SOLAR PHOTOSPHERE. III. SILICON.. Monthly Notices of the Royal Astronomical Society.1 indexed citations
20.
Warner, B.. (1963). High resolution spectra of Comet Seki-Lines (1962c). Observatory. 83. 223–225.3 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.