A. P. Beardmore

16.7k total citations · 2 hit papers
190 papers, 3.0k citations indexed

About

A. P. Beardmore is a scholar working on Astronomy and Astrophysics, Computational Mechanics and Nuclear and High Energy Physics. According to data from OpenAlex, A. P. Beardmore has authored 190 papers receiving a total of 3.0k indexed citations (citations by other indexed papers that have themselves been cited), including 176 papers in Astronomy and Astrophysics, 49 papers in Computational Mechanics and 34 papers in Nuclear and High Energy Physics. Recurrent topics in A. P. Beardmore's work include Gamma-ray bursts and supernovae (123 papers), Astrophysical Phenomena and Observations (120 papers) and Astronomical Observations and Instrumentation (49 papers). A. P. Beardmore is often cited by papers focused on Gamma-ray bursts and supernovae (123 papers), Astrophysical Phenomena and Observations (120 papers) and Astronomical Observations and Instrumentation (49 papers). A. P. Beardmore collaborates with scholars based in United Kingdom, United States and Italy. A. P. Beardmore's co-authors include J. P. Osborne, K. L. Page, P. T. O’Brien, R. L. C. Starling, P. A. Evans, D. N. Burrows, N. Gehrels, M. Perri, J. A. Kennea and M. R. Goad and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

A. P. Beardmore

172 papers receiving 2.8k citations

Hit Papers

An online repository of Swift/XRT light curves of $\vec \... 2007 2026 2013 2019 2007 2013 100 200 300 400

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
A. P. Beardmore United Kingdom 28 2.9k 1.1k 281 158 107 190 3.0k
J. A. Kennea United States 30 3.0k 1.0× 1.1k 1.1× 341 1.2× 147 0.9× 113 1.1× 285 3.2k
Kinwah Wu United Kingdom 29 2.8k 0.9× 1.2k 1.1× 269 1.0× 96 0.6× 77 0.7× 173 2.9k
Allyn F. Tennant United States 26 1.8k 0.6× 775 0.7× 227 0.8× 90 0.6× 55 0.5× 99 1.9k
N. Masetti Italy 33 3.6k 1.2× 1.5k 1.4× 200 0.7× 190 1.2× 185 1.7× 196 3.7k
N. A. Webb France 24 2.1k 0.7× 572 0.5× 238 0.8× 83 0.5× 91 0.9× 78 2.1k
C. Motch France 29 2.2k 0.7× 511 0.5× 279 1.0× 170 1.1× 111 1.0× 136 2.2k
M. Ehle Germany 23 2.9k 1.0× 1.1k 1.0× 200 0.7× 50 0.3× 135 1.3× 70 3.0k
K. O. Mason United Kingdom 24 2.2k 0.7× 692 0.6× 211 0.8× 134 0.8× 138 1.3× 101 2.3k
L. Zampieri Italy 27 2.3k 0.8× 735 0.7× 156 0.6× 57 0.4× 154 1.4× 133 2.4k
A. De Luca Italy 25 2.4k 0.8× 998 0.9× 338 1.2× 81 0.5× 48 0.4× 125 2.5k

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).

Fields of papers citing papers by A. P. Beardmore

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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.

All Works

20 of 20 papers shown
1.
Cheung, C. C., T. J. Johnson, P. Jean, et al.. (2022). Fermi LAT Gamma-ray Detection of the Recurrent Nova RS Ophiuchi during its 2021 Outburst. The Astrophysical Journal. 935(1). 44–44. 22 indexed citations
2.
Evans, P. A., K. L. Page, J. P. Osborne, et al.. (2020). 2SXPS: An Improved and Expanded Swift X-Ray Telescope Point-source Catalog. The Astrophysical Journal Supplement Series. 247(2). 54–54. 119 indexed citations
3.
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
6.
Ness, Jan‐Uwe, A. P. Beardmore, J. P. Osborne, et al.. (2015). Short-period X-ray oscillations in super-soft novae and persistent super-soft sources. Springer Link (Chiba Institute of Technology). 21 indexed citations
7.
Beardmore, A. P., K. L. Page, & E. Kuulkers. (2015). Swift triggers on V404 Cyg. The astronomer's telegram. 8455. 1. 1 indexed citations
8.
Page, K. L., J. P. Osborne, A. P. Beardmore, et al.. (2014). X-ray and UV observations of V751 Cygni in an optical high state. Springer Link (Chiba Institute of Technology). 4 indexed citations
9.
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
10.
Ness, Jan‐Uwe, J. P. Osborne, M. Henze, et al.. (2013). Obscuration effects in super-soft-source X-ray spectra. Springer Link (Chiba Institute of Technology). 27 indexed citations
11.
Evans, P. A., K. L. Page, J. P. Osborne, et al.. (2013). VizieR Online Data Catalog: 1SXPS Swift X-ray telescope point source catalogue (Evans+ 2014).
12.
Degenaar, N., R. L. C. Starling, P. A. Evans, et al.. (2012). DigitalCommons - WayneState (Wayne State University). 7 indexed citations
13.
Osborne, J. P., K. L. Page, A. A. Henden, et al.. (2011). Swift observations of the March 2011 outburst of the cataclysmic variable NSV 1436: a probable dwarf nova. Springer Link (Chiba Institute of Technology).
14.
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
15.
Page, K. L., J. P. Osborne, A. M. Read, et al.. (2009). X-ray and UV observations of nova V598 Puppis between 147 and 255 days after outburst. Springer Link (Chiba Institute of Technology). 3 indexed citations
16.
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.
19.
Goad, M. R., K. L. Page, O. Godet, et al.. (2007). Swift multi-wavelength observations of the bright flaring burstGRB 051117A. Springer Link (Chiba Institute of Technology). 11 indexed citations
20.
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.

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