W.-J. Kim
- Astronomy and Astrophysics top 10%
- Spectroscopy
- Atmospheric Science
- Atomic and Molecular Physics, and Optics
- Nuclear and High Energy Physics
- Co-authors
- F. WyrowskiK. M. MentenJ. S. UrquhartT. CsengeriKee‐Tae KimDo‐Young ByunChung Sik OhT. J. T. Moore
- Topics
- Astrophysics and Star Formation Studies (20 papers)Stellar, planetary, and galactic studies (9 papers)Galaxies: Formation, Evolution, Phenomena (8 papers)
- Journals
- Monthly Notices of the Royal Astronomical SocietyThe Astrophysical Journal Supplement SeriesAstronomy and Astrophysics
- Partner nations
- GermanyUnited KingdomSpain
In The Last Decade
W.-J. Kim
19 papers receiving 157 citations
Peers
Comparison fields: 5 of 16
- Astronomy and Astrophysics 153
- Spectroscopy 67
- Atmospheric Science 43
- Atomic and Molecular Physics, and Optics 22
- Nuclear and High Energy Physics 15
Countries citing papers authored by W.-J. Kim
This map shows the geographic impact of W.-J. 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 W.-J. Kim with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W.-J. Kim more than expected).
Fields of papers citing papers by W.-J. Kim
This network shows the impact of papers produced by W.-J. 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 W.-J. Kim. The network helps show where W.-J. Kim may publish in the future.
Co-authorship network of co-authors of W.-J. Kim
This figure shows the co-authorship network connecting the top 25 collaborators of W.-J. Kim. A scholar is included among the top collaborators of W.-J. 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 W.-J. Kim. W.-J. Kim is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 2 | |
| 3 | 3 | |
| 4 | 2 | |
| 5 | 30 | |
| 6 | 7 | |
| 7 | 4 | |
| 8 | 9 | |
| 9 | 5 | |
| 10 | 5 | |
| 11 | 3 | |
| 12 | 6 | |
| 13 | 5 | |
| 14 | 15 | |
| 15 | 17 | |
| 16 | 10 | |
| 17 | 17 | |
| 18 | 9 | |
| 19 | 1 | |
| 20 | 21 |
About W.-J. Kim
W.-J. Kim is a scholar working on Astronomy and Astrophysics, Atmospheric Science and Nuclear and High Energy Physics, having authored 20 papers that have together received 171 indexed citations. Recurring topics across this work include Astrophysics and Star Formation Studies (20 papers), Stellar, planetary, and galactic studies (9 papers) and Galaxies: Formation, Evolution, Phenomena (8 papers). The work is most often cited by research in Astronomy and Astrophysics (153 citations), Spectroscopy (67 citations) and Atmospheric Science (43 citations). W.-J. Kim has collaborated with scholars based in Germany, United Kingdom and Spain. Frequent co-authors include F. Wyrowski, K. M. Menten, J. S. Urquhart, T. Csengeri, Kee‐Tae Kim, Do‐Young Byun, Chung Sik Oh, T. J. T. Moore, S. Leurini and Jaehan Bae. Their work appears in journals such as Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal Supplement Series and Astronomy and Astrophysics.
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.