V. S. Tamazian
- Astronomy and Astrophysics top 5%
- Instrumentation top 5%
- Computational Mechanics
- Atomic and Molecular Physics, and Optics
- Spectroscopy
- Co-authors
- J. Á. DocoboO. Yu. MalkovJ. WoitasR. J. WhiteYu. Yu. BalegaY. Y. BalegaManuel Correia de AndradeD. Schertl
- Topics
- Stellar, planetary, and galactic studies (46 papers)Astrophysics and Star Formation Studies (26 papers)Astro and Planetary Science (25 papers)
In The Last Decade
V. S. Tamazian
45 papers receiving 321 citations
Peers
Comparison fields: 5 of 30
- Astronomy and Astrophysics 323
- Instrumentation 92
- Computational Mechanics 38
- Atomic and Molecular Physics, and Optics 28
- Spectroscopy 15
Countries citing papers authored by V. S. Tamazian
This map shows the geographic impact of V. S. Tamazian'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 V. S. Tamazian with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites V. S. Tamazian more than expected).
Fields of papers citing papers by V. S. Tamazian
This network shows the impact of papers produced by V. S. Tamazian. 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 V. S. Tamazian. The network helps show where V. S. Tamazian may publish in the future.
Co-authorship network of co-authors of V. S. Tamazian
This figure shows the co-authorship network connecting the top 25 collaborators of V. S. Tamazian. A scholar is included among the top collaborators of V. S. Tamazian 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 V. S. Tamazian. V. S. Tamazian is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 3 | |
| 2 | Catalog of binary UV ceti type flare stars | 1 |
| 3 | 0 | |
| 4 | 57 | |
| 5 | INTERNATIONAL WORKSHOP ON DOUBLE AND MULTIPLE STARS: DYNAMICS, PHYSICS, AND INSTRUMENTATION | 1 |
| 6 | 1 | |
| 7 | 2 | |
| 8 | Tracing the Dynamic Orbit of the Young, Massive High-Eccentricity Binary System θ1 Orionis C. First results from VLTI aperture-synthesis imaging and ESO 3.6-metre visual speckle interferometry | 1 |
| 9 | 53 | |
| 10 | 8 | |
| 11 | 0 | |
| 12 | 8 | |
| 13 | Binary Star Speckle Measurements with the 1.52-M Telescope at Calar Alto | 0 |
| 14 | 9 | |
| 15 | 0 | |
| 16 | 9 | |
| 17 | 8 | |
| 18 | 6 | |
| 19 | 0 | |
| 20 | 1 |
About V. S. Tamazian
V. S. Tamazian is a scholar working on Instrumentation, Astronomy and Astrophysics and Computational Mechanics, having authored 54 papers that have together received 336 indexed citations. Recurring topics across this work include Stellar, planetary, and galactic studies (46 papers), Astrophysics and Star Formation Studies (26 papers) and Astro and Planetary Science (25 papers). The work is most often cited by research in Instrumentation (92 citations), Astronomy and Astrophysics (323 citations) and Computational Mechanics (38 citations). V. S. Tamazian has collaborated with scholars based in Spain, Armenia and Russia. Frequent co-authors include J. Á. Docobo, O. Yu. Malkov, J. Woitas, R. J. White, Yu. Yu. Balega, Y. Y. Balega, Manuel Correia de Andrade, D. Schertl, G. Weigelt and J. F. Ling. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.
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.