C. Feruglio

8.5k citations
85 papers · 3.2k indexed · 4 hit papers · h-index 27

C. Feruglio

83 papers receiving 3.0k citations

Hit Papers

AGN wind scaling relations and the co-evolution ...3472010202620152020100200300

Peers

C. Feruglio
Comparison fields: 5 of 41
  • Instrumentation 853
  • Astronomy and Astrophysics 3.1k
  • Nuclear and High Energy Physics 625
  • Global and Planetary Change 72
  • Spectroscopy 38
Replace C. Cicone with:
C. Cicone Italy
Elisabete da Cunha United States
N. P. H. Nesvadba France
David S. N. Rupke United States
M. J. Michałowski United Kingdom
M. Pannella Germany
Roberto J. Assef United States
A. J. Baker United States
Jacqueline Hodge Germany
M. Sargent United Kingdom
C. Feruglio relative to C. Cicone Italy C. Cicone's profile →
Citations per field
00.5×1.5×
C. Cicone · 1×
Citations per year

Countries citing papers authored by C. Feruglio

Since Specialization
Citations

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

Fields of papers citing papers by C. Feruglio

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network

The 25 scholars most cited alongside C. Feruglio, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with C. Feruglio Line = papers co-authored together C. Feruglio links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown
#Work
1 20250
2 20235
3 20236
4 202333
5 20238
6 202316
7 20218
8 202153
9 20206
10 202023
11 202034
12 202026
13 20205
14 201954
15 201810
16 201834
17 201818
18 201729
19 201690
20 2015108

About C. Feruglio

C. Feruglio is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 85 papers that have together received 3.2k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (79 papers), Astrophysical Phenomena and Observations (55 papers), Astrophysics and Star Formation Studies (35 papers), Astronomy and Astrophysical Research (25 papers), Gamma-ray bursts and supernovae (21 papers), Astrophysics and Cosmic Phenomena (13 papers), Stellar, planetary, and galactic studies (10 papers) and Radio Astronomy Observations and Technology (3 papers). The work is most often cited by research in Instrumentation (853 citations), Astronomy and Astrophysics (3.1k citations) and Nuclear and High Energy Physics (625 citations). C. Feruglio has collaborated with scholars based in Italy, United Kingdom and Germany. Frequent co-authors include F. Fiore, E. Piconcelli, R. Maiolino, C. Cicone, N. Menci, A. Lamastra, M. Bischetti, E. Sturm, Stefano Carniani and A. Bongiorno. Their work appears in journals such as Astronomy and Astrophysics, Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal, The Astrophysical Journal Letters and Nature.

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