G. F. Bignami
About
In The Last Decade
G. F. Bignami
154 papers receiving 2.5k citations
Peers
Comparison fields: 5 of 103
- Astronomy and Astrophysics 2.2k
- Nuclear and High Energy Physics 1.4k
- Geophysics 327
- Atomic and Molecular Physics, and Optics 155
- Oceanography 133
Countries citing papers authored by G. F. Bignami
This map shows the geographic impact of G. F. Bignami'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. F. Bignami with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. F. Bignami more than expected).
Fields of papers citing papers by G. F. Bignami
This network shows the impact of papers produced by G. F. Bignami. 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. F. Bignami. The network helps show where G. F. Bignami may publish in the future.
Co-authorship network of co-authors of G. F. Bignami
This figure shows the co-authorship network connecting the top 25 collaborators of G. F. Bignami. A scholar is included among the top collaborators of G. F. Bignami 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 G. F. Bignami. G. F. Bignami is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | HST observation of the Crab Nebula following the September 2010 gamma-ray flare | 1 |
| 2 | 50 | |
| 3 | Optical observations of pulsars: the ESO contribution. | 2 |
| 4 | Proper motion as a tool to identiy the optical counterparts of pulsars: the case of PSR 0656+14. | 7 |
| 5 | Multiwavelength phenomenology of isolated neutron stars. | 2 |
| 6 | Nearly-aligned rotator model of gamma ray pulsars. | 1 |
| 7 | Geminga, 10 years of optical observations. | 4 |
| 8 | ROSAT and optical observations of two X-ray transients: MX 0836-42 and GS 0834-430 | 2 |
| 9 | Optical identification of celestial high energy sources. | 0 |
| 10 | On the Colours of G" ,the Proposed Optical Counterpart of Geminga * | 2 |
| 11 | The local interstellar medium as traced by gamma rays | 0 |
| 12 | COS-B gamma-ray measurements, cosmic rays and the local interstellar medium | 0 |
| 13 | 1 | |
| 14 | Further COS-B evidence for gamma-ray emission from 3C273 | 1 |
| 15 | The Cos-B Experiment and Mission | 2 |
| 16 | COS-B Observations of Localised Gamma-Ray Emission | 1 |
| 17 | COS-B observations of pulsed gamma -ray emission from PSR 0531+21 and PSR 0833-45. | 1 |
| 18 | Distribution of cosmic gamma rays in the galactic anticenter region as observed by SAS-2 | 1 |
| 19 | High Energy Galactic Gamma Radiation Observed by the SAS-2 Satellite | 1 |
| 20 | An Accelerator Evaluation of the Performance of the COSB Experiment for Gamma-Ray Astronomy | 1 |
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.