Irina Zhuravleva
- Astronomy and Astrophysics top 1%
- Galaxies: Formation, Evolution, Phenomena 43
- Astrophysics and Star Formation Studies 27
- Astrophysical Phenomena and Observations 26
- Stellar, planetary, and galactic studies 19
- Gamma-ray bursts and supernovae 9
- Instrumentation top 2%
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- Astrophysics and Cosmic Phenomena 9
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- Thermal and Kinetic Analysis 8
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- Synthesis and properties of polymers 6
- Co-authors
- E. ChurazovW. FormanNorbert WernerS. W. AllenA. SimionescuA. A. SchekochihinA. VikhlininA. C. Fabian
- Partner nations
- United StatesGermanyRussia
In The Last Decade
Irina Zhuravleva
65 papers receiving 1.6k citations
Hit Papers
Peers
Comparison fields: 5 of 49
- Astronomy and Astrophysics 1.6k
- Instrumentation 276
- Nuclear and High Energy Physics 444
- Statistical and Nonlinear Physics 31
- Computational Mechanics 50
Countries citing papers authored by Irina Zhuravleva
This map shows the geographic impact of Irina Zhuravleva'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 Irina Zhuravleva with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Irina Zhuravleva more than expected).
Fields of papers citing papers by Irina Zhuravleva
This network shows the impact of papers produced by Irina Zhuravleva. 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 Irina Zhuravleva. The network helps show where Irina Zhuravleva may publish in the future.
Co-authorship network
The 25 scholars most cited alongside Irina Zhuravleva, 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 | 2024 | 0 | |
| 2 | 2024 | 7 | |
| 3 | 2024 | 19 | |
| 4 | 2023 | 14 | |
| 5 | 2023 | 15 | |
| 6 | Evidence for heavy-seed origin of early supermassive black holes from a z ≈ 10 X-ray quasarbreakdown → | 2023 | 139 |
| 7 | 2023 | 23 | |
| 8 | 2022 | 16 | |
| 9 | 2022 | 35 | |
| 10 | 2021 | 6 | |
| 11 | 2021 | 12 | |
| 12 | 2020 | 54 | |
| 13 | 2018 | 27 | |
| 14 | 2016 | 40 | |
| 15 | 2016 | 25 | |
| 16 | 2014 | 79 | |
| 17 | 2014 | 217 | |
| 18 | 2012 | 27 | |
| 19 | 2012 | 71 | |
| 20 | 2011 | 47 |
About Irina Zhuravleva
Irina Zhuravleva is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 67 papers that have together received 1.7k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (43 papers), Astrophysics and Star Formation Studies (27 papers), Astrophysical Phenomena and Observations (26 papers), Stellar, planetary, and galactic studies (19 papers), Gamma-ray bursts and supernovae (9 papers), Astrophysics and Cosmic Phenomena (9 papers), Thermal and Kinetic Analysis (8 papers) and Synthesis and properties of polymers (6 papers). The work is most often cited by research in Astronomy and Astrophysics (1.6k citations), Instrumentation (276 citations) and Nuclear and High Energy Physics (444 citations). Irina Zhuravleva has collaborated with scholars based in United States, Germany and Russia. Frequent co-authors include E. Churazov, W. Forman, Norbert Werner, S. W. Allen, A. Simionescu, A. A. Schekochihin, A. Vikhlinin, A. C. Fabian, J. S. Sanders and P. Arévalo. Their work appears in journals such as Nature, The Astrophysical Journal and Macromolecules.
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.