Harald Pfeiffer
- Astronomy and Astrophysics top 0.1%
- Nuclear and High Energy Physics top 0.5%
- Geophysics top 2%
- Oceanography top 2%
- Atomic and Molecular Physics, and Optics top 5%
- Co-authors
- Larry KidderMark ScheelMichael BoyleSaul A. TeukolskyAlessandra BuonannoBéla SzilágyiFrançois FoucartAbdul Mroué
- Topics
- Pulsars and Gravitational Waves Research (147 papers)Astrophysical Phenomena and Observations (106 papers)Gamma-ray bursts and supernovae (57 papers)
- Partner nations
- United StatesGermanyCanada
In The Last Decade
Harald Pfeiffer
187 papers receiving 8.9k citations
Hit Papers
Peers
Comparison fields: 5 of 84
- Astronomy and Astrophysics 7.9k
- Nuclear and High Energy Physics 2.5k
- Geophysics 1.1k
- Oceanography 757
- Atomic and Molecular Physics, and Optics 603
Countries citing papers authored by Harald Pfeiffer
This map shows the geographic impact of Harald Pfeiffer'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 Harald Pfeiffer with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Harald Pfeiffer more than expected).
Fields of papers citing papers by Harald Pfeiffer
This network shows the impact of papers produced by Harald Pfeiffer. 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 Harald Pfeiffer. The network helps show where Harald Pfeiffer may publish in the future.
Co-authorship network of co-authors of Harald Pfeiffer
This figure shows the co-authorship network connecting the top 25 collaborators of Harald Pfeiffer. A scholar is included among the top collaborators of Harald Pfeiffer 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 Harald Pfeiffer. Harald Pfeiffer is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 3 | |
| 3 | 13 | |
| 4 | 1 | |
| 5 | 18 | |
| 6 | 5 | |
| 7 | 5 | |
| 8 | 10 | |
| 9 | 1 | |
| 10 | 5 | |
| 11 | 41 | |
| 12 | 13 | |
| 13 | 42 | |
| 14 | 9 | |
| 15 | 4 | |
| 16 | 30 | |
| 17 | 6 | |
| 18 | 53 | |
| 19 | 21 | |
| 20 | A catalog of 171 high-quality binary black-hole simulations for gravitational-wave astronomy | 2 |
About Harald Pfeiffer
Harald Pfeiffer is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Oceanography, having authored 191 papers that have together received 9.2k indexed citations. Recurring topics across this work include Pulsars and Gravitational Waves Research (147 papers), Astrophysical Phenomena and Observations (106 papers) and Gamma-ray bursts and supernovae (57 papers). The work is most often cited by research in Astronomy and Astrophysics (7.9k citations), Nuclear and High Energy Physics (2.5k citations) and Geophysics (1.1k citations). Harald Pfeiffer has collaborated with scholars based in United States, Germany and Canada. Frequent co-authors include Larry Kidder, Mark Scheel, Michael Boyle, Saul A. Teukolsky, Alessandra Buonanno, Béla Szilágyi, François Foucart, Abdul Mroué, Tony Chu and Yi Pan. Their work appears in journals such as Physical Review Letters, PLoS ONE 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.