C. Fanti
About
In The Last Decade
C. Fanti
67 papers receiving 1.1k citations
Peers
Comparison fields: 5 of 26
- Astronomy and Astrophysics 1.1k
- Nuclear and High Energy Physics 868
- Instrumentation 81
- Aerospace Engineering 55
- Computational Mechanics 26
Countries citing papers authored by C. Fanti
This map shows the geographic impact of C. Fanti'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 C. Fanti with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. Fanti more than expected).
Fields of papers citing papers by C. Fanti
This network shows the impact of papers produced by C. Fanti. 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 C. Fanti. The network helps show where C. Fanti may publish in the future.
Co-authorship network of co-authors of C. Fanti
This figure shows the co-authorship network connecting the top 25 collaborators of C. Fanti. A scholar is included among the top collaborators of C. Fanti 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 C. Fanti. C. Fanti is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 4 | |
| 2 | 9 | |
| 3 | 15 | |
| 4 | 10 | |
| 5 | VLBA POLARIMETRIC OBSERVATIONS OF 3C 286 AT 5 GHZ | 1 |
| 6 | 2 | |
| 7 | Are compact steep-spectrum sources young? | 12 |
| 8 | A sample of small size compact steep-spectrum radio sources. I. VLBI images at 18 cm. | 1 |
| 9 | Are there two engines at the center of 3C 286 | 1 |
| 10 | VLA observations of low luminosity radio galaxies. IV. The B2 sample revisited. | 1 |
| 11 | VLA observations of low-luminosity radio galaxies. VI. Discussion of radio jets. | 2 |
| 12 | Multifrequency observations of low frequency variable sources: a statistical analysis | 0 |
| 13 | VLA observations of low luminosity radio galaxies. III. The A-array observations | 1 |
| 14 | VLA observations of low luminosity radio galaxies. I. Sources with angular size smaller than two arcminutes. | 2 |
| 15 | WSRT radio observations at 1.4 GHz of 32 Abell clusters of distance class 3 and 4. | 1 |
| 16 | Radio and optical observations of 9 nearby Abell Clusters: A 262, A 347, A 569, A 779, A 1213, A 1228, A 2162, A 2666. | 1 |
| 17 | Low frequency variable sources 5 year monitoring program at 408 MHZ. | 4 |
| 18 | Radio and optical data on a complete sample of radio faint galaxies. | 2 |
| 19 | 1 | |
| 20 | A catalogue of 3235 radio sources at 408 MHz | 5 |
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.