I. Saviane
- Instrumentation top 1%
- Astronomy and Astrophysical Research 58
- Astronomy and Astrophysics top 1%
- Stellar, planetary, and galactic studies 81
- Astrophysics and Star Formation Studies 45
- Galaxies: Formation, Evolution, Phenomena 27
- Astro and Planetary Science 16
- Gamma-ray bursts and supernovae 11
- Astrophysical Phenomena and Observations 7
- Nuclear and High Energy Physics top 10%
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- Adaptive optics and wavefront sensing 6
I. Saviane
95 papers receiving 1.9k citations
Peers
Comparison fields: 5 of 44
- Instrumentation 900
- Astronomy and Astrophysics 1.9k
- Nuclear and High Energy Physics 199
- Global and Planetary Change 51
- Atomic and Molecular Physics, and Optics 71
Countries citing papers authored by I. Saviane
This map shows the geographic impact of I. Saviane'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 I. Saviane with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites I. Saviane more than expected).
Fields of papers citing papers by I. Saviane
This network shows the impact of papers produced by I. Saviane. 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 I. Saviane. The network helps show where I. Saviane may publish in the future.
Co-authorship network
The 25 scholars most cited alongside I. Saviane, 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 | 2024 | 1 | |
| 2 | 2023 | 2 | |
| 3 | 2022 | 12 | |
| 4 | 2021 | 6 | |
| 5 | 2021 | 17 | |
| 6 | 2019 | 12 | |
| 7 | When nature tries to trick us An eclipsing eccentric close binary superposed on the central star of the planetary nebula M 3-2 | 2018 | 5 |
| 8 | 2017 | 28 | |
| 9 | 2016 | 26 | |
| 10 | 2015 | 10 | |
| 11 | 2014 | 17 | |
| 12 | 2014 | 36 | |
| 13 | 2014 | 4 | |
| 14 | POPIPlaN: A Deep Morphological Catalogue of Newly Discovered Southern Planetary Nebulae | 2012 | 3 |
| 15 | 2011 | 7 | |
| 16 | 2010 | 7 | |
| 17 | La Silla 2010 | 2009 | 0 |
| 18 | 2007 | 25 | |
| 19 | Circular Polarimetry Now Offered at EFOSC2 | 2007 | 2 |
| 20 | 2003 | 29 |
About I. Saviane
I. Saviane is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 104 papers that have together received 2.0k indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (81 papers), Astronomy and Astrophysical Research (58 papers), Astrophysics and Star Formation Studies (45 papers), Galaxies: Formation, Evolution, Phenomena (27 papers), Astro and Planetary Science (16 papers), Gamma-ray bursts and supernovae (11 papers), Astrophysical Phenomena and Observations (7 papers) and Adaptive optics and wavefront sensing (6 papers). The work is most often cited by research in Instrumentation (900 citations), Astronomy and Astrophysics (1.9k citations) and Nuclear and High Energy Physics (199 citations). I. Saviane has collaborated with scholars based in Chile, Italy and United States. Frequent co-authors include E. V. Held, G. Piotto, Marco Gullieuszik, Alfred Rosenberg, A. Aparicio, S. Ortolani, G. S. Da Costa, B. Barbuy, R. Michael Rich and Y. Momany. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Sensors.
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.