G. Ghirlanda

10.0k citations
136 papers · 4.1k indexed · 1 hit paper · h-index 38

G. Ghirlanda

130 papers receiving 3.9k citations

Hit Papers

General physical properties of bright Fermi blazars3582009202620142020100200300

Peers

G. Ghirlanda
Comparison fields: 5 of 41
  • Astronomy and Astrophysics 4.0k
  • Nuclear and High Energy Physics 1.8k
  • Instrumentation 306
  • Radiation 39
  • Statistical and Nonlinear Physics 42
Replace L. Amati with:
L. Amati Italy
E. Pian Italy
S. D. Ryder Australia
C. Guidorzi Italy
Kunihito Ioka Japan
Jonathan Granot United States
Shigehiro Nagataki Japan
Keiichi Maeda Japan
M. Della Valle Italy
R. A. M. J. Wijers Netherlands
G. Ghirlanda relative to L. Amati Italy L. Amati's profile →
Citations per field
00.5×
L. Amati · 1×
Citations per year

Countries citing papers authored by G. Ghirlanda

Since Specialization
Citations

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

Fields of papers citing papers by G. Ghirlanda

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network

The 25 scholars most cited alongside G. Ghirlanda, 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 G. Ghirlanda Line = papers co-authored together G. Ghirlanda links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown
#Work
1 20242
2 202312
3 202241
4 20221
5 202113
6 20219
7 202111
8 202018
9 202032
10 201946
11 201925
12 201948
13 201843
14 201878
15 20183
16 201677
17
The obscured hyper-energetic GRB 120624B hosted by a luminous compact galaxy at z=2.20
20136
18 200612
19 200618
20 200633

About G. Ghirlanda

G. Ghirlanda is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 136 papers that have together received 4.1k indexed citations. Recurring topics across this work include Gamma-ray bursts and supernovae (121 papers), Pulsars and Gravitational Waves Research (72 papers), Astrophysical Phenomena and Observations (52 papers), Astrophysics and Cosmic Phenomena (37 papers), Astro and Planetary Science (24 papers), Stellar, planetary, and galactic studies (15 papers), Astronomy and Astrophysical Research (14 papers) and Radio Astronomy Observations and Technology (8 papers). The work is most often cited by research in Astronomy and Astrophysics (4.0k citations), Nuclear and High Energy Physics (1.8k citations) and Instrumentation (306 citations). G. Ghirlanda has collaborated with scholars based in Italy, United States and France. Frequent co-authors include G. Ghisellini, Lara Nava, A. Celotti, F. Tavecchio, C. Firmani, Davide Lazzati, O. S. Salafia, L. Foschini, R. Salvaterra and A. Melandri. Their work appears in journals such as Nature, Science and Nature Communications.

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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