G Cañas-Herrera
Impact in
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- Cosmology and Gravitation Theories
- Pulsars and Gravitational Waves Research
- Galaxies: Formation, Evolution, Phenomena
- Radio Astronomy Observations and Technology
- Gamma-ray bursts and supernovae
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- Black Holes and Theoretical Physics
- Dark Matter and Cosmic Phenomena
Papers in ⓘ
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- Cosmology and Gravitation Theories 5
- Galaxies: Formation, Evolution, Phenomena 3
- Pulsars and Gravitational Waves Research 1
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- Dark Matter and Cosmic Phenomena 2
- Black Holes and Theoretical Physics 1
- Co-authors
- Valeri Vardanyan (1 shared paper)Jesús Torrado (1 shared paper)Ana Achúcarro (1 shared paper)Fabrizio Renzi (1 shared paper)M. Martinelli (2 shared papers)Guillermo Franco Abellán (1 shared paper)C. J. A. P. Martins (1 shared paper)D Sciotti (1 shared paper)
- Partner nations
- NetherlandsSpainItaly
In The Last Decade
G Cañas-Herrera
6 papers receiving 55 citations
Peers
Comparison fields: 5 of 12
- Astronomy and Astrophysics 55
- Nuclear and High Energy Physics 21
- Instrumentation 5
- Oceanography 6
- Statistical and Nonlinear Physics 5
Countries citing papers authored by G Cañas-Herrera
This map shows the geographic impact of G Cañas-Herrera'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 Cañas-Herrera with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G Cañas-Herrera more than expected).
Fields of papers citing papers by G Cañas-Herrera
This network shows the impact of papers produced by G Cañas-Herrera. 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 Cañas-Herrera. The network helps show where G Cañas-Herrera may publish in the future.
Co-authors
The 14 scholars most cited alongside G Cañas-Herrera, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | 2020 | 22 | |
| 2 | 2021 | 15 | |
| 3 | 2022 | 7 | |
| 4 | 2024 | 6 | |
| 5 | 2021 | 4 | |
| 6 | 2024 | 2 |
About G Cañas-Herrera
G Cañas-Herrera is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics, Instrumentation, Signal Processing and Computational Mechanics, having authored 6 papers that have together received 56 indexed citations. Recurring topics across this work include Cosmology and Gravitation Theories (5 papers), Galaxies: Formation, Evolution, Phenomena (3 papers), Dark Matter and Cosmic Phenomena (2 papers), Blind Source Separation Techniques (1 paper), Black Holes and Theoretical Physics (1 paper), Astronomy and Astrophysical Research (1 paper), Gaussian Processes and Bayesian Inference (1 paper) and Pulsars and Gravitational Waves Research (1 paper). The work is most often cited by research in Astronomy and Astrophysics (55 citations), Nuclear and High Energy Physics (21 citations), Instrumentation (5 citations), Oceanography (6 citations) and Statistical and Nonlinear Physics (5 citations). G Cañas-Herrera has collaborated with scholars based in Netherlands, Spain and Italy. Frequent co-authors include Valeri Vardanyan, Jesús Torrado, Ana Achúcarro, Fabrizio Renzi, M. Martinelli, Guillermo Franco Abellán, C. J. A. P. Martins, D Sciotti, L. Vacher and Christoph Weniger. Their work appears in journals such as Physical review. D and Journal of Cosmology and Astroparticle Physics.
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.