G. Chon

7.9k total citations
21 papers, 284 citations indexed

About

G. Chon is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, G. Chon has authored 21 papers receiving a total of 284 indexed citations (citations by other indexed papers that have themselves been cited), including 20 papers in Astronomy and Astrophysics, 10 papers in Instrumentation and 7 papers in Nuclear and High Energy Physics. Recurrent topics in G. Chon's work include Galaxies: Formation, Evolution, Phenomena (19 papers), Astrophysical Phenomena and Observations (11 papers) and Astronomy and Astrophysical Research (10 papers). G. Chon is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (19 papers), Astrophysical Phenomena and Observations (11 papers) and Astronomy and Astrophysical Research (10 papers). G. Chon collaborates with scholars based in Germany, Italy and United Kingdom. G. Chon's co-authors include H. Böhringer, A. Challinor, Klaus Dolag, C. A. Collins, L. Guzzo, N. Nowak, G. P. Smith, M. Lerchster, J. Trümper and M. Verdugo and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Astronomische Nachrichten.

In The Last Decade

G. Chon

20 papers receiving 278 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
G. Chon Germany 11 276 96 95 10 7 21 284
G. Bazin United States 5 226 0.8× 74 0.8× 70 0.7× 6 0.6× 10 1.4× 6 235
Subhabrata Majumdar India 8 293 1.1× 98 1.0× 96 1.0× 14 1.4× 8 1.1× 20 300
R. Carballo Spain 14 374 1.4× 96 1.0× 145 1.5× 8 0.8× 4 0.6× 29 379
G. Gozaliasl Finland 12 257 0.9× 149 1.6× 54 0.6× 13 1.3× 10 1.4× 32 272
Timothy Garn United Kingdom 11 386 1.4× 158 1.6× 134 1.4× 14 1.4× 9 1.3× 11 390
G. Castignani Italy 9 198 0.7× 84 0.9× 62 0.7× 8 0.8× 6 0.9× 25 209
Édouard Tollet France 6 305 1.1× 145 1.5× 106 1.1× 19 1.9× 7 1.0× 7 327
Ryu Makiya Japan 10 304 1.1× 69 0.7× 176 1.9× 12 1.2× 5 0.7× 23 333
Estelle Pons United Kingdom 9 249 0.9× 86 0.9× 61 0.6× 6 0.6× 4 0.6× 11 262
Alex Krolewski Canada 9 211 0.8× 43 0.4× 91 1.0× 16 1.6× 4 0.6× 21 223

Countries citing papers authored by G. Chon

Since Specialization
Citations

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

Fields of papers citing papers by G. Chon

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of G. Chon

This figure shows the co-authorship network connecting the top 25 collaborators of G. Chon. A scholar is included among the top collaborators of G. Chon 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 G. Chon. G. Chon 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.
Barrena, R., Lorenzo Pizzuti, G. Chon, & H. Böhringer. (2024). Unveiling the shape: A multi-wavelength analysis of the galaxy clusters Abell 76 and Abell 1307. Astronomy and Astrophysics. 691. A135–A135. 1 indexed citations
2.
Han, J. L., et al.. (2023). More relaxed intracluster gas than galaxies in clusters in quasi-equilibrium. Monthly Notices of the Royal Astronomical Society. 523(1). 1364–1372. 3 indexed citations
3.
Barrena, R., G. Chon, H. Böhringer, J. Méndez‐Abreu, & A. Ferragamo. (2023). RXCJ1111.6+4050 galaxy cluster: Observational evidence of a transitional fossil group. Astronomy and Astrophysics. 679. A147–A147.
4.
Barrena, R., H. Böhringer, & G. Chon. (2022). The dynamical state of RXCJ1230.7+3439: A multi-substructured merging galaxy cluster. Astronomy and Astrophysics. 663. A78–A78. 2 indexed citations
5.
Böhringer, H., G. Chon, Richard S. Ellis, R. Barrena, & Nicolas Laporte. (2022). XMM-Newton study of six massive, X-ray luminous galaxy cluster systems in the redshift range z = 0.25–0.5. Astronomy and Astrophysics. 664. A57–A57. 2 indexed citations
6.
Böhringer, H., G. Chon, & J. Trümper. (2021). The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey. Astronomy and Astrophysics. 651. A15–A15. 9 indexed citations
7.
Böhringer, H., et al.. (2017). Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters. Springer Link (Chiba Institute of Technology). 12 indexed citations
8.
Chon, G., et al.. (2017). From the core to the outskirts: structure analysis of three massive galaxy clusters. Astronomy and Astrophysics. 601. A145–A145. 14 indexed citations
9.
Böhringer, H. & G. Chon. (2015). The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II). Astronomy and Astrophysics. 574. L8–L8. 6 indexed citations
10.
Ota, Naomi, et al.. (2013). Suzakuobservations of the low surface brightness cluster A76. Astronomy and Astrophysics. 556. A21–A21. 4 indexed citations
11.
Böhringer, H., et al.. (2013). The extended ROSAT-ESO flux limited X-ray galaxy cluster survey (REFLEX II) II. Construction and properties of the survey. Astronomy and Astrophysics. 555. A30–A30. 50 indexed citations
12.
Chon, G. & H. Böhringer. (2013). Cluster science from ROSAT to eROSITA. Astronomische Nachrichten. 334(4-5). 478–481. 2 indexed citations
13.
Verdugo, M., M. Lerchster, H. Böhringer, et al.. (2012). The Cosmic Web and galaxy evolution around the most luminous X-ray cluster: RX J1347.5−1145. Monthly Notices of the Royal Astronomical Society. 421(3). 1949–1968. 12 indexed citations
14.
Chon, G., H. Böhringer, & G. P. Smith. (2012). Statistics and implications of substructure detected in a representative sample of X-ray clusters. Astronomy and Astrophysics. 548. A59–A59. 22 indexed citations
15.
Böhringer, H., Klaus Dolag, & G. Chon. (2012). Modelling self-similar appearance of galaxy clusters in X-rays. Astronomy and Astrophysics. 539. A120–A120. 36 indexed citations
16.
Chon, G. & H. Böhringer. (2012). The ROSAT-ESO flux limited X-ray galaxy cluster survey (REFLEX II) - I. Newly identified X-ray luminous clusters at z ≥ 0.2. MPG.PuRe (Max Planck Society). 538. 1–9. 17 indexed citations
17.
Chon, G. & H. Böhringer. (2011). The ROSAT-ESO flux limited X-ray galaxy cluster survey (REFLEX II). Astronomy and Astrophysics. 538. A35–A35. 22 indexed citations
18.
Fassbender, R., H. Böhringer, Joana Santos, et al.. (2010). A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 atz= 0.975. Astronomy and Astrophysics. 527. A78–A78. 11 indexed citations
19.
Fassbender, R., H. Böhringer, Joana Santos, et al.. (2010). A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 at z=0.975 - Observing the assembly of a massive system. arXiv (Cornell University). 527. 1–26. 11 indexed citations
20.
Challinor, A. & G. Chon. (2005). Error analysis of quadratic power spectrum estimates for cosmic microwave background polarization: sampling covariance. Monthly Notices of the Royal Astronomical Society. 360(2). 509–532. 47 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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