D. I. Makarov

73 papers receiving 3.0k citations

Hit Papers

HyperLEDA. III. The catalogue of extragalactic ...200420262011201820142004100200300400500

Peers

D. I. Makarov
Comparison fields: 5 of 56
  • Astronomy and Astrophysics 3.1k
  • Instrumentation 1.3k
  • Nuclear and High Energy Physics 464
  • Atomic and Molecular Physics, and Optics 97
  • Statistical and Nonlinear Physics 93
Replace G. Cresci with:
G. Cresci Italy
Ignacio Martín-Navarro Spain
Joel Leja United States
T. Contini France
Elena Rasia Italy
Helmut Jerjen Australia
C. Gronwall United States
Michaela Hirschmann Italy
Juna A. Kollmeier United States
A. Saintonge United Kingdom
D. I. Makarov relative to G. Cresci Italy G. Cresci's profile →
Citations per field
00.5×1.5×
G. Cresci · 1×
Citations per year

Countries citing papers authored by D. I. Makarov

Since Specialization
Citations

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

Fields of papers citing papers by D. I. Makarov

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of D. I. Makarov

This figure shows the co-authorship network connecting the top 25 collaborators of D. I. Makarov. A scholar is included among the top collaborators of D. I. Makarov 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 D. I. Makarov. D. I. Makarov is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
#WorkIndexed citations
1 5
2 8
3 6
4 21
5 7
6 9
7 34
8 3
9 10
10 0
11 71
12 19
13 13
14 35
15 33
16 100
17 13
18
Edge-on galaxies: A survey of rotation curves
4
19
Orbital velocity of the Sun and the apex of the Galactic center
2
20 120

About D. I. Makarov

D. I. Makarov is a scholar working on Instrumentation, Astronomy and Astrophysics and Statistical and Nonlinear Physics, having authored 82 papers that have together received 3.2k indexed citations. Recurring topics across this work include Galaxies: Formation, Evolution, Phenomena (71 papers), Stellar, planetary, and galactic studies (50 papers) and Astronomy and Astrophysical Research (39 papers). The work is most often cited by research in Instrumentation (1.3k citations), Astronomy and Astrophysics (3.1k citations) and Nuclear and High Energy Physics (464 citations). D. I. Makarov has collaborated with scholars based in Russia, United States and France. Frequent co-authors include И. Д. Караченцев, V. E. Karachentseva, R. Brent Tully, H. M. Courtois, E. Shaya, L. Rizzi, Л. Н. Макарова, W. K. Huchtmeier, P. Prugniel and I. Vauglin. 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.

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