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 P. Bunclark'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 P. Bunclark with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites P. Bunclark more than expected).
This network shows the impact of papers produced by P. Bunclark. 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 P. Bunclark. The network helps show where P. Bunclark may publish in the future.
Co-authorship network of co-authors of P. Bunclark
This figure shows the co-authorship network connecting the top 25 collaborators of P. Bunclark.
A scholar is included among the top collaborators of P. Bunclark 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 P. Bunclark. P. Bunclark 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.
Rots, A. H., P. Bunclark, M. R. Calabretta, et al.. (2014). Representations of Time Coordinates in FITS Time and Relative Dimension in Space.4 indexed citations
Lewis, J., M. Irwin, & P. Bunclark. (2010). Pipeline Processing for VISTA. ASPC. 434. 91.1 indexed citations
4.
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., 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 ... Society of the Pacific Conference).2 indexed citations
Emerson, J. P., Jim Lewis, S. T. Hodgkin, et al.. (2004). VISTA data flow system: overview. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 5493. 401–401.38 indexed citations
9.
Emerson, J. P., Jim Lewis, S. T. Hodgkin, et al.. (2004). Optimizing Scientific Return for Astronomy through Information Technologies.5 indexed citations
10.
Audard, M., K. W. Smith, I. A. Bonnell, et al.. (1999). 3. Second "Three-Islands" Euroconference on Stellar Clusters and Associations: Convection, Rotation and Dynamos.1 indexed citations
Irwin, M. J., et al.. (1990). A new satellite galaxy of the Milky Way in the constellation of Sextans.. Monthly Notices of the Royal Astronomical Society. 244(2).
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.