W. H. G. Lewin
- Astronomy and Astrophysics top 2%
- Nuclear and High Energy Physics top 5%
- Geophysics top 10%
- Biomedical Engineering
- Radiation top 10%
- Co-authors
- G. W. ClarkJ. van ParadijsH. W. SchnopperT. H. MarkertWilliam B. SmithM. van der KlisJ. DotyF. A. Primini
- Topics
- Astrophysical Phenomena and Observations (42 papers)Gamma-ray bursts and supernovae (27 papers)Pulsars and Gravitational Waves Research (14 papers)
- Partner nations
- United StatesNetherlandsGermany
In The Last Decade
W. H. G. Lewin
66 papers receiving 870 citations
Peers
Comparison fields: 5 of 48
- Astronomy and Astrophysics 820
- Nuclear and High Energy Physics 293
- Geophysics 214
- Biomedical Engineering 101
- Radiation 76
Countries citing papers authored by W. H. G. Lewin
This map shows the geographic impact of W. H. G. Lewin'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. H. G. Lewin with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. H. G. Lewin more than expected).
Fields of papers citing papers by W. H. G. Lewin
This network shows the impact of papers produced by W. H. G. Lewin. 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. H. G. Lewin. The network helps show where W. H. G. Lewin may publish in the future.
Co-authorship network of co-authors of W. H. G. Lewin
This figure shows the co-authorship network connecting the top 25 collaborators of W. H. G. Lewin. A scholar is included among the top collaborators of W. H. G. Lewin 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. H. G. Lewin. W. H. G. Lewin is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 2 | |
| 2 | The XMM-Newton Spectrum of 4U 1543-475 in the Low/Hard State and a Comment on Accretion Flow Constraints in this Regime | 1 |
| 3 | The likely optical counterpart of X-ray transient KS 1731-260 | 2 |
| 4 | 7 | |
| 5 | 14 | |
| 6 | New supernova remnant candidates in M31 | 1 |
| 7 | Supernova 1993J in NGC 3031 | 1 |
| 8 | 18 | |
| 9 | 29 | |
| 10 | 12 | |
| 11 | 9 | |
| 12 | The High Energy Transient Explorer (HETE). | 1 |
| 13 | 3 | |
| 14 | 3 | |
| 15 | 7 | |
| 16 | Hard X-ray Observations of a 38 sec Pulsar | 1 |
| 17 | 30 | |
| 18 | 92 | |
| 19 | 11 | |
| 20 | 31 |
About W. H. G. Lewin
W. H. G. Lewin is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Radiation, having authored 71 papers that have together received 911 indexed citations. Recurring topics across this work include Astrophysical Phenomena and Observations (42 papers), Gamma-ray bursts and supernovae (27 papers) and Pulsars and Gravitational Waves Research (14 papers). The work is most often cited by research in Astronomy and Astrophysics (820 citations), Nuclear and High Energy Physics (293 citations) and Geophysics (214 citations). W. H. G. Lewin has collaborated with scholars based in United States, Netherlands and Germany. Frequent co-authors include G. W. Clark, J. van Paradijs, H. W. Schnopper, T. H. Markert, William B. Smith, M. van der Klis, J. Doty, F. A. Primini, C. R. Canizares and P. L. Nolan. Their work appears in journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.
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.