Citations per year, relative to P. A. Curran P. A. Curran (= 1×)
peers
J. Gofford
Countries citing papers authored by P. A. Curran
Since
Specialization
Citations
This map shows the geographic impact of P. A. Curran'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. A. Curran with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites P. A. Curran more than expected).
This network shows the impact of papers produced by P. A. Curran. 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. A. Curran. The network helps show where P. A. Curran may publish in the future.
Co-authorship network of co-authors of P. A. Curran
This figure shows the co-authorship network connecting the top 25 collaborators of P. A. Curran.
A scholar is included among the top collaborators of P. A. Curran 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. A. Curran. P. A. Curran 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.
Curran, P. A.. (2015). MCSpearman: Monte Carlo error analyses of Spearman's rank test. Astrophysics Source Code Library.1 indexed citations
2.
Kennea, J. A., D. N. Burrows, M. J. Coe, et al.. (2015). Swift observations show MAXI J0051-736 is a new outburst of SMC X-2. ATel. 8091. 1.1 indexed citations
Kennea, J. A., M. Linares, H. A. Krimm, et al.. (2013). MAXI J1828-249: Swift UV counterpart and XRT spectral fit. The astronomer's telegram. 5479. 1.1 indexed citations
5.
Miller‐Jones, J. C. A., T. D. Russell, G. R. Sivakoff, & P. A. Curran. (2013). Radio non-detection of MAXI J1828-249. The astronomer's telegram. 5484. 1.1 indexed citations
6.
Coriat, M., P. G. Edwards, R. P. Fender, et al.. (2013). Swift J1745.1-2624 is still active in radio. ATel. 4760. 1.1 indexed citations
7.
Altamirano, D., T. Belloni, P. Casella, et al.. (2011). IGR J17091-3624 undergoes 'heartbeat' oscillations similar to those of GRS 1915+105. UvA-DARE (University of Amsterdam).2 indexed citations
8.
Kennea, J. A., E. A. Hoversten, M. H. Siegel, et al.. (2011). MAXI J1836-194: Swift localization and optical counterpart. ATel. 3613. 1.3 indexed citations
9.
Altamirano, D., T. Belloni, H. A. Krimm, et al.. (2011). RXTE observations strengthen the similarities between the black hole candidates IGR J17091-3624 and GRS 1915+105.. UvA-DARE (University of Amsterdam). 3299. 1.2 indexed citations
Curran, P. A., et al.. (2011). Forth Replacement Crossing – Tender Design. 1.
13.
Kennea, J. A., H. A. Krimm, V. Mangano, et al.. (2010). MAXI J1659-152: Swift localization and monitoring. ATel. 2877. 1.2 indexed citations
14.
Curran, P. A., Phil Evans, M. Still, C. Brocksopp, & Chris Done. (2010). Swift Pointed Observations of XTE J1752-223. ATel. 2424. 1.1 indexed citations
15.
Kennea, J. A., P. A. Curran, P. Romano, et al.. (2010). Swift detection of an ~500s period in MAXI J1409-619. ATel. 3060. 1.1 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.
Levan, A. J., P. A. Curran, K. Wiersema, & P. Groot. (2009). GRB 090621B: optical observations.. GRB Coordinates Network. 9547. 1.1 indexed citations
18.
Curran, P. A., S. D. Barthelmy, A. P. Beardmore, et al.. (2009). GRB 090621B: Swift detection of a short hard burst.. GCN. 9545. 1.1 indexed citations
19.
Linares, M., Paolo Soleri, P. A. Curran, et al.. (2008). The cooling tail of a long X-ray burst from XTE J1701-407. UvA-DARE (University of Amsterdam). 1618. 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.