Philip Rosenfield
About
In The Last Decade
Philip Rosenfield
22 papers receiving 1.6k citations
Hit Papers
Peers
Comparison fields: 5 of 42
- Astronomy and Astrophysics 1.7k
- Instrumentation 834
- Nuclear and High Energy Physics 82
- Atomic and Molecular Physics, and Optics 58
- Geophysics 55
Countries citing papers authored by Philip Rosenfield
This map shows the geographic impact of Philip Rosenfield'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 Philip Rosenfield with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Philip Rosenfield more than expected).
Fields of papers citing papers by Philip Rosenfield
This network shows the impact of papers produced by Philip Rosenfield. 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 Philip Rosenfield. The network helps show where Philip Rosenfield may publish in the future.
Co-authorship network of co-authors of Philip Rosenfield
This figure shows the co-authorship network connecting the top 25 collaborators of Philip Rosenfield. A scholar is included among the top collaborators of Philip Rosenfield 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 Philip Rosenfield. Philip Rosenfield is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 40 | |
| 2 | 35 | |
| 3 | 85 | |
| 4 | 14 | |
| 5 | A NEW GENERATION OF PARSEC-COLIBRI STELLAR ISOCHRONES INCLUDING THE TP-AGB PHASE breakdown → | 564 |
| 6 | 1 | |
| 7 | 26 | |
| 8 | 5 | |
| 9 | New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star-forming dwarf galaxies breakdown → | 296 |
| 10 | 35 | |
| 11 | 27 | |
| 12 | 28 | |
| 13 | 52 | |
| 14 | 6 | |
| 15 | 43 | |
| 16 | 6 | |
| 17 | 209 | |
| 18 | 102 | |
| 19 | 3 | |
| 20 | 1 |
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.