D. Pogosyan

10.4k citations
50 papers · 1.9k indexed · h-index 22

D. Pogosyan

50 papers receiving 1.8k citations

Peers

D. Pogosyan
Comparison fields: 5 of 56
  • Astronomy and Astrophysics 1.8k
  • Instrumentation 337
  • Nuclear and High Energy Physics 519
  • Statistical and Nonlinear Physics 181
  • Atmospheric Science 80
Replace M. R. Calabretta with:
M. R. Calabretta Australia
N. Aghanim France
Noam I. Libeskind Germany
S. Prunet France
G. de Zotti Italy
Jessica K. Werk United States
Shun Saito Japan
Steven Janowiecki United States
B. Koribalski Australia
Nissim Kanekar India
D. Pogosyan relative to M. R. Calabretta Australia M. R. Calabretta's profile →
Citations per field
00.5×4.1×
M. R. Calabretta · 1×
Citations per year

Countries citing papers authored by D. Pogosyan

Since Specialization
Citations

This map shows the geographic impact of D. Pogosyan'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 D. Pogosyan with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. Pogosyan more than expected).

Fields of papers citing papers by D. Pogosyan

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by D. Pogosyan. 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 D. Pogosyan. The network helps show where D. Pogosyan may publish in the future.

Co-authorship network

The 25 scholars most cited alongside D. Pogosyan, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.

Border = papers with D. Pogosyan Line = papers co-authored together D. Pogosyan links everyone, so they are left out of the graph.

All Works

20 of 20 papers shown
#Work
1 20243
2 20244
3 20241
4 202314
5 202111
6 20201
7 201815
8 201719
9 201712
10 201624
11 201573
12 20155
13 2014104
14 201114
15
Line-of-sight statistical methods for turbulent medium: VCS for emission and absorption lines
20092
16 200531
17
Quest for H I Turbulence Statistics: New Techniques
20022
18
Velocity Modification of HI Spectrum and Clouds in Velocity Space
19991
19
Origin and observables of the cosmic web.
19982
20 19973

About D. Pogosyan

D. Pogosyan is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics, having authored 50 papers that have together received 1.9k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (24 papers), Cosmology and Gravitation Theories (23 papers), Astrophysics and Star Formation Studies (20 papers), Stellar, planetary, and galactic studies (17 papers), Solar and Space Plasma Dynamics (15 papers), Astronomy and Astrophysical Research (8 papers), Dark Matter and Cosmic Phenomena (6 papers) and Scientific Research and Discoveries (6 papers). The work is most often cited by research in Astronomy and Astrophysics (1.8k citations), Instrumentation (337 citations) and Nuclear and High Energy Physics (519 citations). D. Pogosyan has collaborated with scholars based in Canada, United States and France. Frequent co-authors include A. Lazarian, Christophe Pichon, Lev Kofman, S. Prunet, Yohan Dubois, Sandrine Codis, Adrianne Slyz, Julien Devriendt, T. Sousbie and D. Kandel. Their work appears in journals such as Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal, Physics Letters B, The Astrophysical Journal Supplement Series and Monthly Notices of the Royal Astronomical Society Letters.

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.

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