E. Belsole

3.4k total citations
18 papers, 776 citations indexed

About

E. Belsole is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Aerospace Engineering. According to data from OpenAlex, E. Belsole has authored 18 papers receiving a total of 776 indexed citations (citations by other indexed papers that have themselves been cited), including 15 papers in Astronomy and Astrophysics, 9 papers in Nuclear and High Energy Physics and 3 papers in Aerospace Engineering. Recurrent topics in E. Belsole's work include Galaxies: Formation, Evolution, Phenomena (15 papers), Astrophysical Phenomena and Observations (11 papers) and Astrophysics and Cosmic Phenomena (9 papers). E. Belsole is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (15 papers), Astrophysical Phenomena and Observations (11 papers) and Astrophysics and Cosmic Phenomena (9 papers). E. Belsole collaborates with scholars based in United Kingdom, France and Germany. E. Belsole's co-authors include M. J. Hardcastle, J. H. Croston, M. Birkinshaw, D. E. Harris, D. M. Worrall, Kyoko Matsushita, H. Böhringer, A. Boselli, D. Pierini and G. Gavazzi and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

E. Belsole

18 papers receiving 760 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
E. Belsole United Kingdom 11 762 380 117 17 12 18 776
G. Hasinger Germany 8 604 0.8× 248 0.7× 107 0.9× 16 0.9× 9 0.8× 21 633
A. T. Steffen United States 11 1.2k 1.5× 458 1.2× 202 1.7× 25 1.5× 5 0.4× 13 1.2k
Robert Nikutta United States 14 1.0k 1.4× 310 0.8× 162 1.4× 22 1.3× 4 0.3× 34 1.1k
F. Vagnetti Italy 17 617 0.8× 273 0.7× 87 0.7× 18 1.1× 4 0.3× 51 644
M. Malkan United States 9 753 1.0× 195 0.5× 168 1.4× 30 1.8× 7 0.6× 13 762
I. M. McHardy United Kingdom 14 486 0.6× 232 0.6× 61 0.5× 28 1.6× 5 0.4× 36 502
E. Fernández Spain 10 256 0.3× 162 0.4× 71 0.6× 24 1.4× 10 0.8× 33 374
L. Bırzan Netherlands 12 534 0.7× 243 0.6× 114 1.0× 9 0.5× 8 0.7× 21 546
C. P. O’Dea United States 10 736 1.0× 389 1.0× 152 1.3× 21 1.2× 7 0.6× 21 751
Dong‐Woo Kim United States 16 1.1k 1.4× 304 0.8× 233 2.0× 20 1.2× 12 1.0× 39 1.1k

Countries citing papers authored by E. Belsole

Since Specialization
Citations

This map shows the geographic impact of E. Belsole'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 E. Belsole with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. Belsole more than expected).

Fields of papers citing papers by E. Belsole

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by E. Belsole. 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 E. Belsole. The network helps show where E. Belsole may publish in the future.

Co-authorship network of co-authors of E. Belsole

This figure shows the co-authorship network connecting the top 25 collaborators of E. Belsole. A scholar is included among the top collaborators of E. Belsole 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 E. Belsole. E. Belsole is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

18 of 18 papers shown
1.
Russell, H. R., A. C. Fabian, G. B. Taylor, et al.. (2012). The X-ray luminous cluster underlying the z = 1.04 quasar PKS 1229−021. Monthly Notices of the Royal Astronomical Society. 422(1). 590–599. 9 indexed citations
2.
Belsole, E., D. M. Worrall, M. J. Hardcastle, & J. H. Croston. (2007). High-redshift Fanaroff-Riley type II radio sources: large-scale X-ray environment. Monthly Notices of the Royal Astronomical Society. 381(3). 1109–1126. 41 indexed citations
3.
Belsole, E., et al.. (2006). High-redshift Faranoff-Riley type II radio galaxies: X-ray properties of the cores. Monthly Notices of the Royal Astronomical Society. 366(1). 339–352. 37 indexed citations
4.
Belsole, E., et al.. (2005). The late merging phase of a galaxy cluster: XMM EPIC observations of A 3266. Astronomy and Astrophysics. 444(3). 673–683. 20 indexed citations
5.
Belsole, E., et al.. (2005). FRII sources at z>0.5: X-ray properties of the core and extended emission. University of Hertfordshire Research Archive (University of Hertfordshire). 604. 573–578. 1 indexed citations
6.
Belsole, E., M. Birkinshaw, & D. M. Worrall. (2005). On the nature of EXO 0423.4−0840. Monthly Notices of the Royal Astronomical Society. 358(1). 120–130. 6 indexed citations
7.
Croston, J. H., M. J. Hardcastle, D. E. Harris, et al.. (2005). An X‐Ray Study of Magnetic Field Strengths and Particle Content in the Lobes of FR II Radio Sources. The Astrophysical Journal. 626(2). 733–747. 195 indexed citations
8.
Belsole, E., et al.. (2005). Merging clusters of galaxies observed with XMM-Newton. Advances in Space Research. 36(4). 630–635. 7 indexed citations
9.
Ferrari, C., Christophe Benoıst, S. Maurogordato, et al.. (2004). Optical and X-ray analysis of the galaxy cluster A3921. Proceedings of the International Astronomical Union. 2004(IAUC195). 1 indexed citations
10.
Belsole, E., D. M. Worrall, M. J. Hardcastle, M. Birkinshaw, & Charles R. Lawrence. (2004). XMM–Newton observations of three high-redshift radio galaxies. Monthly Notices of the Royal Astronomical Society. 352(3). 924–938. 22 indexed citations
11.
Belsole, E., et al.. (2003). The detection of diffuse emission in HCG 16 with XMM-Newton. Springer Link (Chiba Institute of Technology). 14 indexed citations
12.
Sakelliou, I., J. R. Peterson, Takayuki Tamura, et al.. (2002). High resolution soft X-ray spectroscopy of M 87 with the reflection grating spectrometers on $\vec{XMM-Newton}$. Astronomy and Astrophysics. 391(3). 903–909. 40 indexed citations
13.
Matsushita, Kyoko, E. Belsole, A. Finoguenov, & H. Böhringer. (2002). XMM-Newton observation of M87 I. Single-phase temperature structure of intracluster medium. ArXiv.org. 386(1). 77–96. 86 indexed citations
14.
Böhringer, H., E. Belsole, J. A. Kennea, et al.. (2001). XMM-Newton observations of M 87 and its X-ray halo. Springer Link (Chiba Institute of Technology). 101 indexed citations
15.
Belsole, E., J.‐L. Sauvageot, D. M. Worrall, et al.. (2001). An XMM-Newton study of the sub-structure in M 87's halo. Astronomy and Astrophysics. 365(1). L188–L194. 45 indexed citations
16.
Pigot, C., J.‐L. Sauvageot, P. Ferrando, & E. Belsole. (2000). Optimization of spectral performances of the XMM-EPIC MOS camera systems: event selection and energy reconstruction schemes tested on calibration data. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 4140. 500–500. 3 indexed citations
17.
Pigot, C., E. Belsole, P. J. Bennie, et al.. (1999). <title>Ground calibration of the XMM-EPIC MOS cameras at the Orsay Synchrotron Facility</title>. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 3765. 251–264. 1 indexed citations
18.
Gavazzi, G., A. Boselli, M. Scodeggio, D. Pierini, & E. Belsole. (1999). The 3D structure of the Virgo cluster from H-band Fundamental Plane and Tully--Fisher distance determinations. Monthly Notices of the Royal Astronomical Society. 304(3). 595–610. 147 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.

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