This map shows the geographic impact of A. K. Dambis'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 A. K. Dambis with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. K. Dambis more than expected).
This network shows the impact of papers produced by A. K. Dambis. 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 A. K. Dambis. The network helps show where A. K. Dambis may publish in the future.
Co-authorship network of co-authors of A. K. Dambis
This figure shows the co-authorship network connecting the top 25 collaborators of A. K. Dambis.
A scholar is included among the top collaborators of A. K. Dambis 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 A. K. Dambis. A. K. Dambis is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Melnik, A. M. & A. K. Dambis. (2020). VizieR Online Data Catalog: Kinematic data for high luminosity stars (Melnik+, 2020). 170.1 indexed citations
4.
Joshi, Y. C., A. K. Dambis, A. K. Pandey, & S. C. Joshi. (2016). VizieR Online Data Catalog: Open clusters within 1.8 kpc of the Sun (Joshi+, 2016).1 indexed citations
Бердников, Л. Н., A. K. Dambis, A. Y. Kniazev, В. В. Кравцов, & Ramotholo Sefako. (2014). The 'possible Cepheids' DO Ori and VY CMi are RR Lyrae variables. Observatory. 134. 206–210.2 indexed citations
7.
Melnik, A. M., P. Rautiainen, Л. Н. Бердников, A. K. Dambis, & А. С. Расторгуев. (2014). Classical Cepheids in the Galactic outer ring R1R′2.25 indexed citations
Бердников, Л. Н., A. Y. Kniazev, Ramotholo Sefako, В. В. Кравцов, & A. K. Dambis. (2011). CCD observations of 11 variables classified in the GCVS as RR Lyrae-type stars without light-curve elements. Observatory. 131(6). 386–391.3 indexed citations
10.
Бердников, Л. Н., A. Y. Kniazev, Ramotholo Sefako, В. В. Кравцов, & A. K. Dambis. (2011). CCD observations of three RR Lyrae-type stars: CL Eri, CM Eri, and CN Eri. Observatory. 131(5). 315–317.3 indexed citations
Бердников, Л. Н., A. K. Dambis, & O. V. Vozyakova. (2000). VizieR Online Data Catalog: Galactic Cepheids BVRI photometry (Berdnikov+, 2000).1 indexed citations
13.
Melnik, A. M., A. K. Dambis, & А. С. Расторгуев. (1999). Periodic pattern in the Cepheid space velocity field and the spiral arms of our Galaxy. 25(8). 518–525.2 indexed citations
14.
Расторгуев, А. С., et al.. (1999). Statistical parallaxes and kinematical parameters of classical Cepheids and young star clusters. Astronomy Letters. 25(9). 595–607.12 indexed citations
15.
Dambis, A. K.. (1999). Space-age distribution of young open clusters and observational selection.. Astronomy Letters. 25(1). 10–17.8 indexed citations
16.
Melnik, A. M., et al.. (1998). Kinematic evidence for the wave nature of the Carina-Sagittarius arm. 24(5). 594–602.2 indexed citations
17.
Бердников, Л. Н., O. V. Vozyakova, & A. K. Dambis. (1996). The BVRIJHK period-luminosity relations for Galactic classical Cepheids. Astronomy Letters. 22(6). 839–846.2 indexed citations
18.
Dambis, A. K., A. M. Melnik, & А. С. Расторгуев. (1995). Rotation curve of the system of classical Cepheids and the distance to the galactic center. 21(3). 291–307.1 indexed citations
19.
Dambis, A. K.. (1993). The period-luminosity relation in the K-band for semiregular pulsating red supergiants in the Galaxy and in M33.. Astronomy Letters. 19. 172.2 indexed citations
20.
Dambis, A. K.. (1990). Determination of Normal B-Y/0 Color Indices and Absolute Magnitudes M/v of Blue Supergiants Using Ubvy Beta-Photometry Data. 16. 224.1 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.