M. Capalbi

1.6k total citations
5 papers, 34 citations indexed

About

M. Capalbi is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, M. Capalbi has authored 5 papers receiving a total of 34 indexed citations (citations by other indexed papers that have themselves been cited), including 5 papers in Astronomy and Astrophysics, 3 papers in Nuclear and High Energy Physics and 1 paper in Instrumentation. Recurrent topics in M. Capalbi's work include Astrophysical Phenomena and Observations (4 papers), Gamma-ray bursts and supernovae (3 papers) and Astrophysics and Cosmic Phenomena (3 papers). M. Capalbi is often cited by papers focused on Astrophysical Phenomena and Observations (4 papers), Gamma-ray bursts and supernovae (3 papers) and Astrophysics and Cosmic Phenomena (3 papers). M. Capalbi collaborates with scholars based in Italy, Netherlands and United Kingdom. M. Capalbi's co-authors include L. Piro, A. Malizia, F. Fiore, L. A. Antonelli, F. Frontera, E. Montanari, Alessandro Coletta, Mike Smith, D. Ricci and L. Vetere and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Springer Link (Chiba Institute of Technology).

In The Last Decade

M. Capalbi

3 papers receiving 34 citations

Peers

M. Capalbi
Comparison fields: 5 of 9
  • Astronomy and Astrophysics 33
  • Nuclear and High Energy Physics 24
  • Instrumentation 2
  • Statistical and Nonlinear Physics 1
  • Radiation 1
Replace Andrea Bonchi with:
Andrea Bonchi Italy
D. Lennarz Germany
Itay Rabinak Israel
M. Seglar-Arroyo France
A. A. Nikiforova Russia
B. Carpenter Germany
M. Marongiu Italy
L. Popa Romania
Y. Uchiyama Japan
A. Homeier Germany
Andrea Bonchi Italy View profile →
Citations per field, relative to M. Capalbi
M. Capalbi · 1×
Citations per year, relative to M. Capalbi
M. Capalbi · 1×

Countries citing papers authored by M. Capalbi

Since Specialization
Citations

This map shows the geographic impact of M. Capalbi'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 M. Capalbi with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Capalbi more than expected).

Fields of papers citing papers by M. Capalbi

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. Capalbi. 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 M. Capalbi. The network helps show where M. Capalbi may publish in the future.

Co-authorship network of co-authors of M. Capalbi

This figure shows the co-authorship network connecting the top 25 collaborators of M. Capalbi. A scholar is included among the top collaborators of M. Capalbi 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 M. Capalbi. M. Capalbi is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

5 of 5 papers shown
# Work Indexed citations
1 0
2
Swift follow-up of the blazar 4C+21.35 (PKS 1222+21) after a bright gamma-ray flare
0
3 14
4 5
5 15

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.

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2026