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.
An online repository of Swift/XRT light curves of $\vec \gamma$-ray bursts
2007452 citationsP. A. Evans, A. P. Beardmore et al.profile →
Calibration of X-ray absorption in our Galaxy
2013426 citationsR. L. C. Starling, A. P. Beardmore et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
Countries citing papers authored by A. P. Beardmore
Since
Specialization
Citations
This map shows the geographic impact of A. P. Beardmore'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 A. P. Beardmore with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. P. Beardmore more than expected).
This network shows the impact of papers produced by A. P. Beardmore. 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 A. P. Beardmore. The network helps show where A. P. Beardmore may publish in the future.
Co-authorship network of co-authors of A. P. Beardmore
This figure shows the co-authorship network connecting the top 25 collaborators of A. P. Beardmore.
A scholar is included among the top collaborators of A. P. Beardmore 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 A. P. Beardmore. A. P. Beardmore is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Beardmore, A. P., et al.. (2017). Detection of a 9.4 min periodicity in the XMM-Newton and Chandra X-ray light curves of V407 Lup (Nova Lup 2016). ATel. 10749. 1.1 indexed citations
4.
Singh, K. P., Gordon Stewart, S. Chandra, et al.. (2016). In-orbit performance of SXT aboardAstroSat. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 9905. 99051E–99051E.54 indexed citations
5.
Page, K. L., N. P. M. Kuin, A. P. Beardmore, J. P. Osborne, & G. J. Schwarz. (2015). Nova V5668 Sgr (N Sgr 2015 no. 2) enters the super-soft X-ray phase. ATel. 8054. 1.1 indexed citations
Beardmore, A. P., J. P. Osborne, & K. L. Page. (2014). Fading and probable quasi-periodic oscillation in the Swift X-ray observations of symbiotic recurrent nova V745 Sco. ATel. 5897. 1.3 indexed citations
Stamatikos, M., S. D. Barthelmy, A. P. Beardmore, et al.. (2011). GRB 111123A: Swift detection of a burst.. GRB Coordinates Network. 12587. 1.1 indexed citations
Schady, P., W. H. Baumgartner, A. P. Beardmore, et al.. (2009). GRB 090618: Swift detection of a bright burst with optical afterglow.. GCN. 9512. 1.
17.
Markwardt, C. B., et al.. (2009). Updated Position, Flux and Spectrum of XTE J1652-453. ATel. 2120. 1.3 indexed citations
18.
Krimm, H. A., A. P. Beardmore, N. Gehrels, et al.. (2008). Swift discovery of a new soft gamma repeater Sgr 1550-5418.. GRB Coordinates Network. 8312. 1.
Evans, P. A., A. P. Beardmore, M. R. Goad, et al.. (2007). GRB 070328: Swift/XRT refined analysis. UvA-DARE (University of Amsterdam). 1085. 1.
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.