Xue‐Bing Wu

428 total citations
12 papers, 230 citations indexed

About

Xue‐Bing Wu is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, Xue‐Bing Wu has authored 12 papers receiving a total of 230 indexed citations (citations by other indexed papers that have themselves been cited), including 11 papers in Astronomy and Astrophysics, 4 papers in Instrumentation and 4 papers in Nuclear and High Energy Physics. Recurrent topics in Xue‐Bing Wu's work include Galaxies: Formation, Evolution, Phenomena (7 papers), Astrophysical Phenomena and Observations (7 papers) and Astronomy and Astrophysical Research (4 papers). Xue‐Bing Wu is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (7 papers), Astrophysical Phenomena and Observations (7 papers) and Astronomy and Astrophysical Research (4 papers). Xue‐Bing Wu collaborates with scholars based in China, United States and Taiwan. Xue‐Bing Wu's co-authors include F. K. Liu, Ran Wang, Yongquan Xue, Ye‐Fei Yuan, Zhao‐Yu Li, Gang Zhao, A. A. Zdziarski, Qianggao Hu, Chen Wu and Ronald E. Taam and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Chinese Science Bulletin (Chinese Version).

In The Last Decade

Xue‐Bing Wu

10 papers receiving 215 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Xue‐Bing Wu China 8 221 115 20 9 5 12 230
P. Yu. Minaev Russia 9 211 1.0× 59 0.5× 19 0.9× 5 0.6× 8 1.6× 26 216
Frédéric Marin France 7 193 0.9× 78 0.7× 16 0.8× 10 1.1× 6 1.2× 18 201
B. Nikiel-Wroczyński Poland 7 170 0.8× 121 1.1× 13 0.7× 3 0.3× 5 1.0× 16 176
T. Cantwell United Kingdom 5 127 0.6× 43 0.4× 19 0.9× 4 0.4× 6 1.2× 12 135
A. Tanimoto Japan 8 184 0.8× 75 0.7× 25 1.3× 3 0.3× 6 1.2× 22 198
V. Sudilovsky Germany 9 253 1.1× 99 0.9× 12 0.6× 6 0.7× 2 0.4× 15 256
Hou-Jun Lv China 4 251 1.1× 66 0.6× 23 1.1× 4 0.4× 3 0.6× 6 253
F. J. Virgili United States 5 308 1.4× 92 0.8× 30 1.5× 4 0.4× 3 0.6× 9 310
Z. Igo Italy 6 115 0.5× 58 0.5× 16 0.8× 13 1.4× 3 0.6× 9 119
Ye-Fei Yuan China 7 130 0.6× 47 0.4× 6 0.3× 6 0.7× 10 2.0× 25 136

Countries citing papers authored by Xue‐Bing Wu

Since Specialization
Citations

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

Fields of papers citing papers by Xue‐Bing Wu

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Xue‐Bing Wu. 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 Xue‐Bing Wu. The network helps show where Xue‐Bing Wu may publish in the future.

Co-authorship network of co-authors of Xue‐Bing Wu

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

All Works

12 of 12 papers shown
1.
Yan, Zhen, et al.. (2025). The NuSTAR view of five changing-look active galactic nuclei. Monthly Notices of the Royal Astronomical Society.
2.
Zuo, Wenwen & Xue‐Bing Wu. (2016). The mystery of quasar power. Chinese Science Bulletin (Chinese Version). 61(11). 1157–1163. 1 indexed citations
3.
Wu, Xue‐Bing, Linhua Jiang, Xiaohui Fan, Ran Wang, & Feige Wang. (2015). Observational studies on high-redshift quasars. Chinese Science Bulletin (Chinese Version). 60(25). 2387–2395. 2 indexed citations
4.
Li, Zhao‐Yu, Xue‐Bing Wu, & Ran Wang. (2008). The Black Hole Fundamental Plane: Revisited with a Larger Sample of Radio and X‐Ray–Emitting Broad‐Line AGNs. The Astrophysical Journal. 688(2). 826–836. 46 indexed citations
5.
Hu, Qianggao, Chen Wu, & Xue‐Bing Wu. (2007). The mass and luminosity functions and the formation rate of DA white dwarfs in the Sloan Digital Sky Survey. Springer Link (Chiba Institute of Technology). 17 indexed citations
6.
Yuan, Ye‐Fei, A. A. Zdziarski, Yongquan Xue, & Xue‐Bing Wu. (2007). Modeling the Hard States of XTE J1550−564 during Its 2000 Outburst. The Astrophysical Journal. 659(1). 541–548. 42 indexed citations
7.
Yuan, Ye‐Fei, Ronald E. Taam, Ranjeev Misra, Xue‐Bing Wu, & Yongquan Xue. (2007). Accretion Disk Spectra of the Brightest Ultraluminous X‐Ray Source in M82. The Astrophysical Journal. 658(1). 282–287. 24 indexed citations
8.
Wu, Xue‐Bing, et al.. (2007). Galaxy Bulge Formation: Interplay with Dark Matter Halo and Central Supermassive Black Hole. The Astrophysical Journal. 664(1). 198–203. 8 indexed citations
9.
Qian, Lei, B. F. Liu, & Xue‐Bing Wu. (2007). Disk Evaporation–Fed Corona: Structure and Evaporation Features with Magnetic Field. The Astrophysical Journal. 668(2). 1145–1153. 15 indexed citations
10.
Zhao, Gang, et al.. (2006). Harmonic QPOs and Thick Accretion Disk Oscillations in the BL Lacertae Object AO 0235+164. The Astrophysical Journal. 650(2). 749–762. 37 indexed citations
11.
Wu, Xue‐Bing & F. K. Liu. (2004). Black Hole Mass and Accretion Rate of Active Galactic Nuclei with Double‐peaked Broad Emission Lines. The Astrophysical Journal. 614(1). 91–100. 37 indexed citations
12.
Wu, Xue‐Bing, et al.. (1995). The stability of an isothermal magnetized accretion disk. 295(3). 833. 1 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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