R. Salvaterra
- Astronomy and Astrophysics top 0.5%
- Nuclear and High Energy Physics top 2%
- Instrumentation top 2%
- Geophysics top 10%
- Statistical and Nonlinear Physics top 10%
- Co-authors
- Andrea FerraraB. CiardiG. GhirlandaS. CampanaG. GhiselliniRaffaella SchneiderA. MelandriG. Tagliaferri
- Topics
- Gamma-ray bursts and supernovae (78 papers)Astrophysical Phenomena and Observations (68 papers)Pulsars and Gravitational Waves Research (37 papers)
- Partner nations
- ItalyFranceUnited States
In The Last Decade
R. Salvaterra
110 papers receiving 2.7k citations
Hit Papers
Peers
Comparison fields: 5 of 49
- Astronomy and Astrophysics 2.8k
- Nuclear and High Energy Physics 823
- Instrumentation 393
- Geophysics 82
- Statistical and Nonlinear Physics 52
Countries citing papers authored by R. Salvaterra
This map shows the geographic impact of R. Salvaterra'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 R. Salvaterra with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. Salvaterra more than expected).
Fields of papers citing papers by R. Salvaterra
This network shows the impact of papers produced by R. Salvaterra. 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 R. Salvaterra. The network helps show where R. Salvaterra may publish in the future.
Co-authorship network of co-authors of R. Salvaterra
This figure shows the co-authorship network connecting the top 25 collaborators of R. Salvaterra. A scholar is included among the top collaborators of R. Salvaterra 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 R. Salvaterra. R. Salvaterra is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 4 | |
| 2 | 2 | |
| 3 | 6 | |
| 4 | 1 | |
| 5 | 3 | |
| 6 | 13 | |
| 7 | 8 | |
| 8 | 25 | |
| 9 | 21 | |
| 10 | 78 | |
| 11 | 77 | |
| 12 | 16 | |
| 13 | 24 | |
| 14 | 23 | |
| 15 | 40 | |
| 16 | High redshift GRBs and the epoch of reionization . | 1 |
| 17 | 15 | |
| 18 | GRB 111228A: possible detection of the SN with the TNG. | 1 |
| 19 | GRB 110328A / Swift J164449.3+573451: beamed emission. | 0 |
| 20 | GRB 090423: TNG amici spectrum. | 0 |
About R. Salvaterra
R. Salvaterra is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 116 papers that have together received 2.8k indexed citations. Recurring topics across this work include Gamma-ray bursts and supernovae (78 papers), Astrophysical Phenomena and Observations (68 papers) and Pulsars and Gravitational Waves Research (37 papers). The work is most often cited by research in Astronomy and Astrophysics (2.8k citations), Instrumentation (393 citations) and Nuclear and High Energy Physics (823 citations). R. Salvaterra has collaborated with scholars based in Italy, France and United States. Frequent co-authors include Andrea Ferrara, B. Ciardi, G. Ghirlanda, S. Campana, G. Ghisellini, Raffaella Schneider, A. Melandri, G. Tagliaferri, P. D’Avanzo and S. Covino. Their work appears in journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.
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.