I. W. Harry
- Astronomy and Astrophysics top 1%
- Geophysics top 5%
- Nuclear and High Energy Physics top 5%
- Atomic and Molecular Physics, and Optics top 10%
- Oceanography top 5%
- Co-authors
- A. P. LundgrenD. KeitelL. K. NuttallA. NitzD. BrownS. FairhurstA. BohéAlessandra Buonanno
- Topics
- Pulsars and Gravitational Waves Research (51 papers)Gamma-ray bursts and supernovae (27 papers)Astrophysical Phenomena and Observations (11 papers)
- Journals
- The Astrophysical JournalMonthly Notices of the Royal Astronomical SocietyPhysics Letters A
- Partner nations
- United KingdomUnited StatesGermany
In The Last Decade
I. W. Harry
55 papers receiving 2.7k citations
Hit Papers
Peers
Comparison fields: 5 of 49
- Astronomy and Astrophysics 2.6k
- Geophysics 530
- Nuclear and High Energy Physics 477
- Atomic and Molecular Physics, and Optics 323
- Oceanography 308
Countries citing papers authored by I. W. Harry
This map shows the geographic impact of I. W. Harry'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 I. W. Harry with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites I. W. Harry more than expected).
Fields of papers citing papers by I. W. Harry
This network shows the impact of papers produced by I. W. Harry. 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 I. W. Harry. The network helps show where I. W. Harry may publish in the future.
Co-authorship network of co-authors of I. W. Harry
This figure shows the co-authorship network connecting the top 25 collaborators of I. W. Harry. A scholar is included among the top collaborators of I. W. Harry 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 I. W. Harry. I. W. Harry is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 6 | |
| 2 | 7 | |
| 3 | 3 | |
| 4 | 10 | |
| 5 | 4 | |
| 6 | 10 | |
| 7 | 11 | |
| 8 | 9 | |
| 9 | 46 | |
| 10 | 48 | |
| 11 | 62 | |
| 12 | 93 | |
| 13 | 542 | |
| 14 | 95 | |
| 15 | 32 | |
| 16 | 93 | |
| 17 | Charging Issues in LIGO | 2 |
| 18 | Reduction of tantala mechanical losses in Ta2O5/SiO2 coatings for the next generation of VIRGO and LIGO interferometric gravitational waves detectors | 1 |
| 19 | 11 | |
| 20 | Wideband Resonant-Lever Transducer for Massive Spherical Gravitational Wave Detectors | 1 |
About I. W. Harry
I. W. Harry is a scholar working on Astronomy and Astrophysics, Geophysics and Oceanography, having authored 57 papers that have together received 2.8k indexed citations. Recurring topics across this work include Pulsars and Gravitational Waves Research (51 papers), Gamma-ray bursts and supernovae (27 papers) and Astrophysical Phenomena and Observations (11 papers). The work is most often cited by research in Astronomy and Astrophysics (2.6k citations), Geophysics (530 citations) and Nuclear and High Energy Physics (477 citations). I. W. Harry has collaborated with scholars based in United Kingdom, United States and Germany. Frequent co-authors include A. P. Lundgren, D. Keitel, L. K. Nuttall, A. Nitz, D. Brown, S. Fairhurst, A. Bohé, Alessandra Buonanno, Tanja Hinderer and S. Privitera. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Physics Letters A.
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.