M. Haverkorn
- Astronomy and Astrophysics top 1%
- Astrophysics and Star Formation Studies 44
- Stellar, planetary, and galactic studies 38
- Radio Astronomy Observations and Technology 38
- Solar and Space Plasma Dynamics 26
- Galaxies: Formation, Evolution, Phenomena 23
- Astrophysical Phenomena and Observations 13
- Pulsars and Gravitational Waves Research 12
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- Astrophysics and Cosmic Phenomena 61
- Instrumentation top 5%
- Oceanography top 10%
- Co-authors
- B. M. GaenslerN. M. McClure‐GriffithsJ. M. DickeyA. J. GreenL. Staveley‐SmithE. CarrettiJ. C. BrownP. Katgert
- Partner nations
- NetherlandsAustraliaUnited States
In The Last Decade
M. Haverkorn
103 papers receiving 2.6k citations
Peers
Comparison fields: 5 of 48
- Astronomy and Astrophysics 2.6k
- Nuclear and High Energy Physics 1.4k
- Instrumentation 98
- Statistical and Nonlinear Physics 93
- Oceanography 63
Countries citing papers authored by M. Haverkorn
This map shows the geographic impact of M. Haverkorn'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 M. Haverkorn with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Haverkorn more than expected).
Fields of papers citing papers by M. Haverkorn
This network shows the impact of papers produced by M. Haverkorn. 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 M. Haverkorn. The network helps show where M. Haverkorn may publish in the future.
Co-authorship network
The 25 scholars most cited alongside M. Haverkorn, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | 2025 | 0 | |
| 2 | 2025 | 0 | |
| 3 | 2024 | 3 | |
| 4 | 2024 | 6 | |
| 5 | 2024 | 2 | |
| 6 | 2024 | 8 | |
| 7 | 2022 | 5 | |
| 8 | 2021 | 2 | |
| 9 | 2021 | 14 | |
| 10 | 2020 | 1 | |
| 11 | 2019 | 1 | |
| 12 | 2019 | 5 | |
| 13 | 2019 | 4 | |
| 14 | 2019 | 8 | |
| 15 | 2018 | 46 | |
| 16 | 2018 | 22 | |
| 17 | 2018 | 9 | |
| 18 | 2004 | 11 | |
| 19 | 2004 | 21 | |
| 20 | Multi-frequency polarimetry of the Galactic radio background around 350 MHz. II. A region in Horologium around l = 137degr , b = 7degr | 2003 | 32 |
About M. Haverkorn
M. Haverkorn is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation, having authored 108 papers that have together received 2.7k indexed citations. Recurring topics across this work include Astrophysics and Cosmic Phenomena (61 papers), Astrophysics and Star Formation Studies (44 papers), Stellar, planetary, and galactic studies (38 papers), Radio Astronomy Observations and Technology (38 papers), Solar and Space Plasma Dynamics (26 papers), Galaxies: Formation, Evolution, Phenomena (23 papers), Astrophysical Phenomena and Observations (13 papers) and Pulsars and Gravitational Waves Research (12 papers). The work is most often cited by research in Astronomy and Astrophysics (2.6k citations), Nuclear and High Energy Physics (1.4k citations) and Instrumentation (98 citations). M. Haverkorn has collaborated with scholars based in Netherlands, Australia and United States. Frequent co-authors include B. M. Gaensler, N. M. McClure‐Griffiths, J. M. Dickey, A. J. Green, L. Staveley‐Smith, E. Carretti, J. C. Brown, P. Katgert, S. Poppi and G. Bernardi. 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.