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.
This map shows the geographic impact of R. W. Argyle'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 R. W. Argyle with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. W. Argyle more than expected).
This network shows the impact of papers produced by R. W. Argyle. 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 R. W. Argyle. The network helps show where R. W. Argyle may publish in the future.
Co-authorship network of co-authors of R. W. Argyle
This figure shows the co-authorship network connecting the top 25 collaborators of R. W. Argyle.
A scholar is included among the top collaborators of R. W. Argyle 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 R. W. Argyle. R. W. Argyle is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Argyle, R. W., P. Bunclark, & James R. Lewis. (2008). Astronomical data analysis software and systems XVII : proceedings of a conference held in Kensington Town Hall, London, United Kingdom, 23-26 September 2007. Astronomical Society of the Pacific eBooks.1 indexed citations
Argyle, R. W.. (2007). Thomas Cooke (1807-1868) - a great English telescope maker. Observatory. 127. 392–400.1 indexed citations
6.
Fresneau, A., A. E. Vaughan, & R. W. Argyle. (2007). Sydney observatory Galactic survey. Astronomy and Astrophysics. 469(3). 1221–1229.4 indexed citations
Argyle, R. W.. (2004). The 50th anniversary of the last observation with the Airy Transit Circle at Greenwich. Observatory. 124. 229–232.1 indexed citations
Argyle, R. W.. (1999). Treasure hunting in astronomical plate archives. Observatory. 119. 269.6 indexed citations
13.
Garrington, S. T., R. J. Davis, L. V. Morrison, & R. W. Argyle. (1998). Linking the Radio and Optical Frames with Merlin. Symposium - International Astronomical Union. 179. 389–391.1 indexed citations
14.
Irwin, M., et al.. (1997). Transferring HIPPARCOS frame to Schmidt surveys. 23. 12.
15.
Lagerkvist, C.–I., et al.. (1992). Physical studies of asteroids. XXIV - Phase relations for 48 asteroids obtained with the Carlsberg Meridian Circle. Astronomy & Astrophysics Supplement Series. 94(1). 43–71.7 indexed citations
16.
Argyle, R. W., et al.. (1990). Optical positions of Seyfert galaxies - III.. Monthly Notices of the Royal Astronomical Society. 243(3). 504–508.12 indexed citations
17.
Argyle, R. W., et al.. (1990). Optical positions of miscellaneous galaxies. Observatory. 110. 93–95.3 indexed citations
18.
Morrison, L. V., et al.. (1990). Comparison of FK5 with Bordeaux and Carlsberg meridian circle observations.. Research at the University of Copenhagen (University of Copenhagen). 240(1). 173–177.3 indexed citations
Argyle, R. W.. (1983). Probable Supernova in NGC 4220. IAUC. 3839. 2.1 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.