This map shows the geographic impact of D. Svinkin'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. Svinkin with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. Svinkin more than expected).
This network shows the impact of papers produced by D. Svinkin. 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. Svinkin. The network helps show where D. Svinkin may publish in the future.
Co-authorship network of co-authors of D. Svinkin
This figure shows the co-authorship network connecting the top 25 collaborators of D. Svinkin.
A scholar is included among the top collaborators of D. Svinkin 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. Svinkin. D. Svinkin is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Ridnaia, A., S. Golenetskii, R. Aptekar, et al.. (2020). Konus-Wind observation of a very intense bursting activity of SGR 1935+2154. GCN. 27667. 1.
6.
Frederiks, D., S. Golenetskii, R. Aptekar, et al.. (2020). Konus-Wind observation of GRB 200415A (a magnetar Giant Flare in Sculptor Galaxy?). GRB Coordinates Network. 27596. 1.
7.
Ridnaia, A., S. Golenetskii, R. Aptekar, et al.. (2019). Konus-Wind observation of the recent SGR 1935+2154 activity. GRB Coordinates Network. 26242. 1.1 indexed citations
8.
Svinkin, D., S. Golenetskii, R. Aptekar, et al.. (2019). LIGO/Virgo S190814bv: Konus-Wind observations. GRB Coordinates Network. 25369. 1.
9.
Svinkin, D., S. Golenetskii, R. Aptekar, et al.. (2019). LIGO/Virgo S190425z: Konus-Wind observations.. GRB Coordinates Network. 24417. 1.
10.
Frederiks, D., S. Golenetskii, R. Aptekar, et al.. (2016). GRB 161103A: an ultra-long GRB detected by Konus-Wind.. GRB Coordinates Network. 20141. 1.1 indexed citations
11.
Golenetskii, S., R. Aptekar, D. Frederiks, et al.. (2015). Konus-Wind observation of Galactic transient V404 Cyg in outburst.. GCN. 17938. 1.
12.
Hurley, K., S. Golenetskii, R. Aptekar, et al.. (2014). IPN triangulation of GRB 140801A (Fermi trigger 428612396).. GCN. 16655. 1.
Pal'Shin, V., R. Aptekar, D. Frederiks, et al.. (2013). IPN triangulation of SGR-like burst 130913 - probable association with SGR/AXP 1E1841-045.. GCN. 15245. 1.1 indexed citations
15.
Hurley, K., J. Goldsten, V. Connaughton, et al.. (2013). IPN localization of GRB 130702A (= Fermi 394416326).. GCN. 14974. 1.
16.
Golenetskii, S., R. Aptekar, D. Frederiks, et al.. (2010). Konus-wind observation of short hard GRB 101219A.. GCN. 11470. 1.1 indexed citations
17.
Golenetskii, S., R. Aptekar, E. Mazets, et al.. (2009). Konus-wind detection of very bright SGR-like burst on January 25, 2009.. GCN. 8851. 1.
18.
Golenetskii, S., R. Aptekar, E. Mazets, et al.. (2009). Konus-wind and Konus-RF observations of GRB 090408b.. GRB Coordinates Network. 10166. 1.2 indexed citations
19.
Golenetskii, S., R. Aptekar, E. Mazets, et al.. (2009). Konus-RF GCN on GRB 091018 (from valentin pal'shin).. GCN. 1045. 1.1 indexed citations
20.
Golenetskii, S., R. Aptekar, E. Mazets, et al.. (2008). Konus-wind observations of new Sgr 0501+4516.. GRB Coordinates Network. 8132. 1.1 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.