Dong‐Woo Kim

1.8k total citations
39 papers, 1.1k citations indexed

About

Dong‐Woo Kim is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, Dong‐Woo Kim has authored 39 papers receiving a total of 1.1k indexed citations (citations by other indexed papers that have themselves been cited), including 37 papers in Astronomy and Astrophysics, 13 papers in Instrumentation and 9 papers in Nuclear and High Energy Physics. Recurrent topics in Dong‐Woo Kim's work include Galaxies: Formation, Evolution, Phenomena (33 papers), Astrophysical Phenomena and Observations (24 papers) and Astronomy and Astrophysical Research (13 papers). Dong‐Woo Kim is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (33 papers), Astrophysical Phenomena and Observations (24 papers) and Astronomy and Astrophysical Research (13 papers). Dong‐Woo Kim collaborates with scholars based in United States, Italy and United Kingdom. Dong‐Woo Kim's co-authors include G. Fabbiano, Bram Boroson, G. R. Knapp, Puragra Guhathakurta, Michael Jura, Paul Green, Wayne Barkhouse, Silvia Pellegrini, J. D. Silverman and Paul B. Eskridge and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

Dong‐Woo Kim

34 papers receiving 1.1k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Dong‐Woo Kim United States 16 1.1k 304 233 26 20 39 1.1k
A. P. Thomson United Kingdom 15 885 0.8× 211 0.7× 290 1.2× 13 0.5× 17 0.8× 32 919
W. Ishibashi Switzerland 14 898 0.8× 184 0.6× 206 0.9× 9 0.3× 23 1.1× 33 928
Tiago Costa Germany 16 922 0.9× 170 0.6× 286 1.2× 14 0.5× 13 0.7× 28 982
George C. Privon United States 19 899 0.8× 182 0.6× 264 1.1× 21 0.8× 37 1.9× 50 940
Dan Oravetz United States 3 944 0.9× 245 0.8× 247 1.1× 14 0.5× 26 1.3× 3 963
S. G. Neff United States 19 802 0.7× 146 0.5× 270 1.2× 11 0.4× 33 1.6× 46 825
E. Gonzales-Solares United Kingdom 3 949 0.9× 268 0.9× 232 1.0× 6 0.2× 31 1.6× 3 968
Myriam Gitti Italy 21 1.1k 1.1× 550 1.8× 166 0.7× 9 0.3× 24 1.2× 67 1.2k
Michele Perna Italy 17 801 0.7× 136 0.4× 242 1.0× 19 0.7× 16 0.8× 43 843

Countries citing papers authored by Dong‐Woo Kim

Since Specialization
Citations

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

Fields of papers citing papers by Dong‐Woo Kim

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Dong‐Woo Kim. 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 Dong‐Woo Kim. The network helps show where Dong‐Woo Kim may publish in the future.

Co-authorship network of co-authors of Dong‐Woo Kim

This figure shows the co-authorship network connecting the top 25 collaborators of Dong‐Woo Kim. A scholar is included among the top collaborators of Dong‐Woo Kim 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 Dong‐Woo Kim. Dong‐Woo Kim 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.
Kim, Dong‐Woo, et al.. (2023). The Chandra Source Catalog Normal Galaxy Sample. The Astrophysical Journal Supplement Series. 268(1). 17–17. 2 indexed citations
2.
Kim, Dong‐Woo, et al.. (2023). Revisiting X-Ray-bright Optically Normal Galaxies with the Chandra Source Catalog. The Astrophysical Journal. 955(1). 56–56.
3.
Wang, Yunchong, Mark Vogelsberger, Dong‐Woo Kim, et al.. (2023). X-ray scaling relations of early-type galaxies in IllustrisTNG and a new way of identifying backsplash objects. Monthly Notices of the Royal Astronomical Society. 527(3). 6763–6778. 1 indexed citations
4.
Kim, Dong‐Woo, et al.. (2021). Origin of operating voltage increase in deep UV light-emitting diodes with ITO/Al reflector. Japanese Journal of Applied Physics. 60(11). 112002–112002. 2 indexed citations
5.
Kim, Dong‐Woo, et al.. (2019). Revisiting the X-ray – Mass scaling relations of early-type galaxies with the mass of their globular cluster systems as a proxy for the total galaxy mass. Monthly Notices of the Royal Astronomical Society. 8 indexed citations
6.
Kim, Dong‐Woo, A. Paggi, Ewan O’Sullivan, et al.. (2019). Temperature profiles of hot gas in early-type galaxies. Monthly Notices of the Royal Astronomical Society. 492(2). 2095–2118. 5 indexed citations
7.
Kim, Dong‐Woo, et al.. (2018). The Mass of the Globular Cluster Systems of Early Type Galaxies as Proxy for the Total Galaxy Mass. arXiv (Cornell University). 1 indexed citations
8.
Kim, Dong‐Woo, C. S. Anderson, D. J. Burke, et al.. (2018). Disturbed Fossil Group Galaxy NGC 1132. The Astrophysical Journal. 853(2). 129–129. 6 indexed citations
9.
Hornschemeier, A. E., A. Wolter, & Dong‐Woo Kim. (2015). What dominates the X-ray emission of normal galaxies?. Proceedings of the International Astronomical Union. 11(A29B). 124–135. 1 indexed citations
10.
Kim, Dong‐Woo & G. Fabbiano. (2015). X-RAY SCALING RELATIONS OF “CORE” AND “CORELESS” E AND S0 GALAXIES. The Astrophysical Journal. 812(2). 127–127. 38 indexed citations
11.
Kim, Dong‐Woo & Paul Green. (2014). X-ray View of Galaxy Ecosystems. 2 indexed citations
12.
Paggi, A., G. Fabbiano, Dong‐Woo Kim, et al.. (2014). ACTIVE GALACTIC NUCLEUS FEEDBACK IN THE HOT HALO OF NGC 4649. The Astrophysical Journal. 787(2). 134–134. 9 indexed citations
13.
Strader, Jay, G. Fabbiano, Bin Luo, et al.. (2012). DEEPCHANDRAMONITORING OBSERVATIONS OF NGC 4649. II. WIDE-FIELDHUBBLE SPACE TELESCOPEIMAGING OF THE GLOBULAR CLUSTERS. The Astrophysical Journal. 760(1). 87–87. 22 indexed citations
14.
Haggard, Daryl, Paul Green, Scott F. Anderson, et al.. (2010). THE FIELD X-RAY AGN FRACTION TOz= 0.7 FROM THECHANDRAMULTIWAVELENGTH PROJECT AND THE SLOAN DIGITAL SKY SURVEY. The Astrophysical Journal. 723(2). 1447–1468. 57 indexed citations
15.
Fabbiano, G., N. J. Brassington, L. Lentati, et al.. (2010). FIELD AND GLOBULAR CLUSTER LOW-MASS X-RAY BINARIES IN NGC 4278. The Astrophysical Journal. 725(2). 1824–1847. 14 indexed citations
16.
Fragos, Tassos, V. Kalogera, B. Willems, et al.. (2009). TRANSIENT LOW-MASS X-RAY BINARY POPULATIONS IN ELLIPTICAL GALAXIES NGC 3379 AND NGC 4278. The Astrophysical Journal. 702(2). L143–L147. 20 indexed citations
17.
Kim, Dong‐Woo & M. Elvis. (1999). Radio‐quiet Red Quasars. The Astrophysical Journal. 516(1). 9–17. 28 indexed citations
18.
Eskridge, Paul B., G. Fabbiano, & Dong‐Woo Kim. (1995). A Multiparametric Analysis of the Einstein Sample of Early-Type Galaxies. III. Comparisons with the kappa -Parameters. The Astrophysical Journal. 448. 70–70. 5 indexed citations
19.
Kim, Dong‐Woo. (1991). The X-ray Spectra of Galaxies. 16. 19–19. 1 indexed citations
20.
Kim, Dong‐Woo. (1988). Interstellar Matter in Early Type Galaxies.. PhDT.

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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026