Francesco Shankar
- Astronomy and Astrophysics top 0.5%
- Instrumentation top 0.2%
- Nuclear and High Energy Physics top 2%
- Ecology top 10%
- Computer Vision and Pattern Recognition top 5%
- Co-authors
- Mariangela BernardiRavi K. ShethS. MeiV. VikramA. MeertMolly S. PeeplesDavid H. WeinbergAndrea Lapi
- Topics
- Galaxies: Formation, Evolution, Phenomena (110 papers)Astronomy and Astrophysical Research (66 papers)Astrophysical Phenomena and Observations (47 papers)
- Partner nations
- United KingdomUnited StatesItaly
In The Last Decade
Francesco Shankar
114 papers receiving 4.2k citations
Hit Papers
Peers
Comparison fields: 5 of 63
- Astronomy and Astrophysics 4.4k
- Instrumentation 2.1k
- Nuclear and High Energy Physics 795
- Ecology 191
- Computer Vision and Pattern Recognition 182
Countries citing papers authored by Francesco Shankar
This map shows the geographic impact of Francesco Shankar'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 Francesco Shankar with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Francesco Shankar more than expected).
Fields of papers citing papers by Francesco Shankar
This network shows the impact of papers produced by Francesco Shankar. 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 Francesco Shankar. The network helps show where Francesco Shankar may publish in the future.
Co-authorship network of co-authors of Francesco Shankar
This figure shows the co-authorship network connecting the top 25 collaborators of Francesco Shankar. A scholar is included among the top collaborators of Francesco Shankar 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 Francesco Shankar. Francesco Shankar is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 0 | |
| 2 | 0 | |
| 3 | 6 | |
| 4 | 3 | |
| 5 | 3 | |
| 6 | 9 | |
| 7 | 19 | |
| 8 | 5 | |
| 9 | 33 | |
| 10 | 11 | |
| 11 | 5 | |
| 12 | 15 | |
| 13 | 10 | |
| 14 | 2 | |
| 15 | 16 | |
| 16 | 13 | |
| 17 | The galaxy’s gas content regulated by the dark matter halo mass results in a superlinear M BH–M ⋆ Relation | 11 |
| 18 | 18 | |
| 19 | The morphologies of massive galaxies from z ~ 3-witnessing the two channels of bulge growth | 49 |
| 20 | 27 |
About Francesco Shankar
Francesco Shankar is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 118 papers that have together received 4.5k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (110 papers), Astronomy and Astrophysical Research (66 papers) and Astrophysical Phenomena and Observations (47 papers). The work is most often cited by research in Instrumentation (2.1k citations), Astronomy and Astrophysics (4.4k citations) and Nuclear and High Energy Physics (795 citations). Francesco Shankar has collaborated with scholars based in United Kingdom, United States and Italy. Frequent co-authors include Mariangela Bernardi, Ravi K. Sheth, S. Mei, V. Vikram, A. Meert, Molly S. Peeples, David H. Weinberg, Andrea Lapi, Jordi Miralda‐Escudé and A. Marconi. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Hypertension.
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.