Xue-Bing Wu

4.9k citations
111 papers · 2.1k indexed · 1 hit paper · h-index 22
Topics
Galaxies: Formation, Evolution, Phenomena (74 papers)Astrophysical Phenomena and Observations (59 papers)Astronomy and Astrophysical Research (36 papers)

In The Last Decade

Xue-Bing Wu

99 papers receiving 1.9k citations

Hit Papers

An ultraluminous quasar with a twelve-billion-solar-mass ...20152026201820222015100200300400

Peers

Xue-Bing Wu
Comparison fields: 5 of 79
  • Astronomy and Astrophysics 1.9k
  • Nuclear and High Energy Physics 553
  • Instrumentation 453
  • Atomic and Molecular Physics, and Optics 58
  • Computational Mechanics 57
Replace M. Vaccari with:
M. Vaccari Italy
S. Paltani Switzerland
Eilat Glikman United States
F. J. Carrera Spain
Laura Blecha United States
Yongquan Xue China
Bret Lehmer United States
Tinggui Wang China
P. Marziani Italy
Fuyan Bian United States
Xue-Bing Wu relative to M. Vaccari Italy M. Vaccari's profile →
Citations per field
00.5×1.5×2.2×
M. Vaccari · 1×
Citations per year

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

20 of 20 papers shown
#WorkIndexed citations
1 5
2 1
3 0
4 3
5 7
6 2
7 10
8 8
9 30
10 34
11 11
12 20
13 46
14 64
15 94
16 3
17 16
18 51
19 33
20 38

About Xue-Bing Wu

Xue-Bing Wu is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 111 papers that have together received 2.1k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (74 papers), Astrophysical Phenomena and Observations (59 papers) and Astronomy and Astrophysical Research (36 papers). The work is most often cited by research in Instrumentation (453 citations), Astronomy and Astrophysics (1.9k citations) and Nuclear and High Energy Physics (553 citations). Xue-Bing Wu has collaborated with scholars based in China, United States and Germany. Frequent co-authors include Xiaohui Fan, Feige Wang, Jinyi Yang, Linhua Jiang, Ran Wang, Fuyan Bian, Ian D. McGreer, Qian Yang, Weimin Yi and Wenwen Zuo. Their work appears in journals such as Nature, Science and The Astrophysical Journal.

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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