R. Di Stefano
About
In The Last Decade
R. Di Stefano
85 papers receiving 1.4k citations
Peers
Comparison fields: 5 of 62
- Astronomy and Astrophysics 1.4k
- Nuclear and High Energy Physics 299
- Instrumentation 197
- Atomic and Molecular Physics, and Optics 81
- Geophysics 63
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 of co-authors of R. Di Stefano
This figure shows the co-authorship network connecting the top 25 collaborators of R. Di Stefano. A scholar is included among the top collaborators of R. Di Stefano 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 R. Di Stefano. R. Di Stefano is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 7 | |
| 2 | 5 | |
| 3 | 0 | |
| 4 | 4 | |
| 5 | 6 | |
| 6 | 25 | |
| 7 | 30 | |
| 8 | 27 | |
| 9 | 11 | |
| 10 | 21 | |
| 11 | Binary Paths to Type Ia Supernovae Explosions (IAU S281) | 2 |
| 12 | 25 | |
| 13 | Two new supersoft X-ray sources in M31 identified as classical novae | 1 |
| 14 | 4 | |
| 15 | Rebrightening of the Supersoft X-ray Transient in the M31 Globular Cluster Bol 194 | 1 |
| 16 | Supersoft X-ray Sources in M31 | 2 |
| 17 | Globular Cluster X-Ray Sources and Supersoft Sources in NGC 4472 and M87 | 1 |
| 18 | 20 | |
| 19 | Accretion Disks in Supersoft X-ray Sources | 1 |
| 20 | How Large is the Population of Luminous Supersoft X-Ray Sources? | 2 |
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.