This map shows the geographic impact of Yu. N. Krugly'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 Yu. N. Krugly with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Yu. N. Krugly more than expected).
This network shows the impact of papers produced by Yu. N. Krugly. 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 Yu. N. Krugly. The network helps show where Yu. N. Krugly may publish in the future.
Co-authorship network of co-authors of Yu. N. Krugly
This figure shows the co-authorship network connecting the top 25 collaborators of Yu. N. Krugly.
A scholar is included among the top collaborators of Yu. N. Krugly 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 Yu. N. Krugly. Yu. N. Krugly is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Golubov, Oleksiy, et al.. (2020). Yarkovsky Effect for Tumblers and Non-Convex Shapes: Asteroid (99942) Apophis as a Test Case. 2242. 2072.1 indexed citations
Belskaya, I. N., S. Fornasier, G. P. Tozzi, et al.. (2017). Asteroid polarimetry as a tool to distinguish rare taxonomic types. European Planetary Science Congress.1 indexed citations
7.
Kim, Myung-Jin, Young‐Jun Choi, Yu. N. Krugly, et al.. (2016). Optical observations of NEA 162173 Ryugu (1999 JU3) during the 2016 apparition. 48.
Molotov, I., et al.. (2014). ASPIN-ISON asteroid program: History, current state, and future prospects. 145.1 indexed citations
10.
Slyusarev, I., V. G. Shevchenko, I. N. Belskaya, Yu. N. Krugly, & V. G. Chiorny. (2012). Magnitude Phase Angle Dependences of Jupiter Trojans and Hilda Asteroids. LPI. 1885.2 indexed citations
11.
Shevchenko, V. G., I. N. Belskaya, D. F. Lupishko, et al.. (2010). Kharkiv Asteroid Magnitude-Phase Relations V1.0.2 indexed citations
12.
Ďurech, Josef, David Vokrouhlický, David Polishook, et al.. (2009). Detection of the YORP Effect in Asteroid (3103) Eger.2 indexed citations
13.
Shevchenko, V. G., Yu. N. Krugly, I. N. Belskaya, et al.. (2009). Do Trojan Asteroids Have the Brightness Opposition Effect. LPI. 1391.3 indexed citations
14.
Krugly, Yu. N.. (1999). GSC 614.01209 is a New Variable Star. Information Bulletin on Variable Stars. 4730. 1.1 indexed citations
15.
Krugly, Yu. N. & V. G. Shevchenko. (1999). Magnitude Phase Dependence of Asteroid 433 Eros. LPI. 1595.4 indexed citations
16.
Shevchenko, V. G., et al.. (1996). Magnitude-phase dependences for three asteroids.. Astronomy & Astrophysics Supplement Series. 115. 475–479.13 indexed citations
17.
Busarev, V. V. & Yu. N. Krugly. (1995). A SPOT of Hydrated Silicates on the M Asteroid 201 Penelope. LPI. 26. 197.3 indexed citations
18.
Belskaya, I. N., V. G. Shevchenko, Yu. N. Krugly, D. F. Lupishko, & F. P. Velichko. (1994). Opposition Effect of Asteroids: New Results. Bulletin of the American Astronomical Society. 26. 1549.2 indexed citations
19.
Shevchenko, V. G., Yu. N. Krugly, D. F. Lupishko, Alan W. Harris, & G. P. Chernova. (1993). Light curves and phase relations of the asteroid 55 Pandora. 27(3). 268–272.6 indexed citations
20.
Velichko, F. P., et al.. (1990). Such Unlike Asteroids 1627 Ivar and 1951 Lick. 1546. 39.2 indexed citations
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.