R. Di Stefano
- Astronomy and Astrophysics top 2%
- Astrophysical Phenomena and Observations 42
- Stellar, planetary, and galactic studies 36
- Gamma-ray bursts and supernovae 26
- Galaxies: Formation, Evolution, Phenomena 24
- Pulsars and Gravitational Waves Research 16
- Astrophysics and Star Formation Studies 10
- Instrumentation top 5%
- Astronomy and Astrophysical Research 14
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- Astrophysics and Cosmic Phenomena 7
- Architecture top 10%
- Co-authors
- S. RappaportA. K. H. KongDaniel J. D’OrazioJ. GreinerShude MaoPhilipp PodsiadlowskiZhanwen HanP. C. Joss
- Partner nations
- United StatesGermanyItaly
In The Last Decade
R. Di Stefano
85 papers receiving 1.4k citations
Peers
Comparison fields: 5 of 62
- Astronomy and Astrophysics 1.4k
- Instrumentation 197
- Nuclear and High Energy Physics 299
- Geophysics 63
- Architecture 7
Countries citing papers authored by R. Di Stefano
This map shows the geographic impact of R. Di Stefano'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 R. Di Stefano with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. Di Stefano more than expected).
Fields of papers citing papers by R. Di Stefano
This network shows the impact of papers produced by R. Di Stefano. 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 R. Di Stefano. The network helps show where R. Di Stefano may publish in the future.
Co-authorship network
The 25 scholars most cited alongside R. Di Stefano, 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 | 7 | |
| 2 | 2024 | 5 | |
| 3 | 2024 | 0 | |
| 4 | 2023 | 4 | |
| 5 | 2022 | 6 | |
| 6 | 2021 | 25 | |
| 7 | 2020 | 30 | |
| 8 | 2019 | 27 | |
| 9 | 2018 | 11 | |
| 10 | 2015 | 21 | |
| 11 | Binary Paths to Type Ia Supernovae Explosions (IAU S281) | 2013 | 2 |
| 12 | 2012 | 25 | |
| 13 | Two new supersoft X-ray sources in M31 identified as classical novae | 2008 | 1 |
| 14 | 2008 | 4 | |
| 15 | Rebrightening of the Supersoft X-ray Transient in the M31 Globular Cluster Bol 194 | 2007 | 1 |
| 16 | Supersoft X-ray Sources in M31 | 2003 | 2 |
| 17 | Globular Cluster X-Ray Sources and Supersoft Sources in NGC 4472 and M87 | 2002 | 1 |
| 18 | 2002 | 20 | |
| 19 | Accretion Disks in Supersoft X-ray Sources | 1996 | 1 |
| 20 | How Large is the Population of Luminous Supersoft X-Ray Sources? | 1995 | 2 |
About R. Di Stefano
R. Di Stefano is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 89 papers that have together received 1.5k indexed citations. Recurring topics across this work include Astrophysical Phenomena and Observations (42 papers), Stellar, planetary, and galactic studies (36 papers), Gamma-ray bursts and supernovae (26 papers), Galaxies: Formation, Evolution, Phenomena (24 papers), Pulsars and Gravitational Waves Research (16 papers), Astronomy and Astrophysical Research (14 papers), Astrophysics and Star Formation Studies (10 papers) and Astrophysics and Cosmic Phenomena (7 papers). The work is most often cited by research in Astronomy and Astrophysics (1.4k citations), Instrumentation (197 citations) and Nuclear and High Energy Physics (299 citations). R. Di Stefano has collaborated with scholars based in United States, Germany and Italy. Frequent co-authors include S. Rappaport, A. K. H. Kong, Daniel J. D’Orazio, J. Greiner, Shude Mao, Philipp Podsiadlowski, Zhanwen Han, P. C. Joss, Maxwell Moe and S. S. Murray. Their work appears in journals such as Nature, The Astrophysical Journal and Physics Today.
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.