Marco Chianese
- Nuclear and High Energy Physics top 5%
- Astronomy and Astrophysics top 5%
- Atomic and Molecular Physics, and Optics
- Statistical and Nonlinear Physics
- Oceanography
- Co-authors
- Gennaro MieleStefano MorisiChristoph WenigerStephen F. KingDamiano F. G. FiorilloNinetta SavianoT. EdwardsO. Pisanti
- Topics
- Dark Matter and Cosmic Phenomena (29 papers)Astrophysics and Cosmic Phenomena (24 papers)Neutrino Physics Research (15 papers)
- Journals
- Physical Review LettersSHILAP Revista de lepidopterologíaThe Astrophysical Journal
- Partner nations
- ItalyNetherlandsDenmark
In The Last Decade
Marco Chianese
37 papers receiving 545 citations
Peers
Comparison fields: 5 of 18
- Nuclear and High Energy Physics 485
- Astronomy and Astrophysics 355
- Atomic and Molecular Physics, and Optics 38
- Statistical and Nonlinear Physics 20
- Oceanography 8
Countries citing papers authored by Marco Chianese
This map shows the geographic impact of Marco Chianese'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 Marco Chianese with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Marco Chianese more than expected).
Fields of papers citing papers by Marco Chianese
This network shows the impact of papers produced by Marco Chianese. 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 Marco Chianese. The network helps show where Marco Chianese may publish in the future.
Co-authorship network of co-authors of Marco Chianese
This figure shows the co-authorship network connecting the top 25 collaborators of Marco Chianese. A scholar is included among the top collaborators of Marco Chianese 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 Marco Chianese. Marco Chianese is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 5 | |
| 2 | 10 | |
| 3 | 2 | |
| 4 | 12 | |
| 5 | 4 | |
| 6 | 10 | |
| 7 | 1 | |
| 8 | 5 | |
| 9 | 27 | |
| 10 | 0 | |
| 11 | 0 | |
| 12 | 1 | |
| 13 | 10 | |
| 14 | 20 | |
| 15 | 28 | |
| 16 | 2 | |
| 17 | 1 | |
| 18 | 30 | |
| 19 | 23 | |
| 20 | 25 |
About Marco Chianese
Marco Chianese is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Oceanography, having authored 40 papers that have together received 553 indexed citations. Recurring topics across this work include Dark Matter and Cosmic Phenomena (29 papers), Astrophysics and Cosmic Phenomena (24 papers) and Neutrino Physics Research (15 papers). The work is most often cited by research in Nuclear and High Energy Physics (485 citations), Astronomy and Astrophysics (355 citations) and Statistical and Nonlinear Physics (20 citations). Marco Chianese has collaborated with scholars based in Italy, Netherlands and Denmark. Frequent co-authors include Gennaro Miele, Stefano Morisi, Christoph Weniger, Stephen F. King, Damiano F. G. Fiorillo, Ninetta Saviano, T. Edwards, O. Pisanti, Roberta Calabrese and Antonio Ambrosone. Their work appears in journals such as Physical Review Letters, SHILAP Revista de lepidopterología and The Astrophysical Journal.
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.