Dorottya Szécsi
- Astronomy and Astrophysics top 2%
- Instrumentation top 5%
- Nuclear and High Energy Physics top 10%
- Geophysics
- Oceanography
- Co-authors
- S. P. StevensonN. LangerIlya MandelCoenraad J. NeijsselAlejandro Vigna-GómezS. E. de MinkJim W. BarrettPhilipp Podsiadlowski
- Topics
- Gamma-ray bursts and supernovae (18 papers)Stellar, planetary, and galactic studies (16 papers)Astrophysics and Star Formation Studies (8 papers)
- Journals
- The Astrophysical JournalMonthly Notices of the Royal Astronomical SocietyAstronomy and Astrophysics
- Partner nations
- GermanyCzechiaUnited Kingdom
In The Last Decade
Dorottya Szécsi
22 papers receiving 855 citations
Hit Papers
Peers
Comparison fields: 5 of 33
- Astronomy and Astrophysics 931
- Instrumentation 161
- Nuclear and High Energy Physics 87
- Geophysics 29
- Oceanography 24
Countries citing papers authored by Dorottya Szécsi
This map shows the geographic impact of Dorottya Szécsi'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 Dorottya Szécsi with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Dorottya Szécsi more than expected).
Fields of papers citing papers by Dorottya Szécsi
This network shows the impact of papers produced by Dorottya Szécsi. 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 Dorottya Szécsi. The network helps show where Dorottya Szécsi may publish in the future.
Co-authorship network of co-authors of Dorottya Szécsi
This figure shows the co-authorship network connecting the top 25 collaborators of Dorottya Szécsi. A scholar is included among the top collaborators of Dorottya Szécsi 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 Dorottya Szécsi. Dorottya Szécsi is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 3 | |
| 2 | 17 | |
| 3 | 11 | |
| 4 | 8 | |
| 5 | 13 | |
| 6 | 3 | |
| 7 | 39 | |
| 8 | 36 | |
| 9 | 17 | |
| 10 | 108 | |
| 11 | The effect of the metallicity-specific star formation history on double compact object mergersbreakdown → | 192 |
| 12 | 23 | |
| 13 | 15 | |
| 14 | 11 | |
| 15 | On the formation history of Galactic double neutron starsbreakdown → | 204 |
| 16 | How may short-duration GRBs form? A review of progenitor theories | 1 |
| 17 | 0 | |
| 18 | 91 | |
| 19 | 55 | |
| 20 | 106 |
About Dorottya Szécsi
Dorottya Szécsi is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 26 papers that have together received 976 indexed citations. Recurring topics across this work include Gamma-ray bursts and supernovae (18 papers), Stellar, planetary, and galactic studies (16 papers) and Astrophysics and Star Formation Studies (8 papers). The work is most often cited by research in Astronomy and Astrophysics (931 citations), Instrumentation (161 citations) and Nuclear and High Energy Physics (87 citations). Dorottya Szécsi has collaborated with scholars based in Germany, Czechia and United Kingdom. Frequent co-authors include S. P. Stevenson, N. Langer, Ilya Mandel, Coenraad J. Neijssel, Alejandro Vigna-Gómez, S. E. de Mink, Jim W. Barrett, Philipp Podsiadlowski, Sung-Chul Yoon and D. Sanyal. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society 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.