Sofya Alexeeva

423 total citations
25 papers, 268 citations indexed

About

Sofya Alexeeva is a scholar working on Astronomy and Astrophysics, Instrumentation and Atmospheric Science. According to data from OpenAlex, Sofya Alexeeva has authored 25 papers receiving a total of 268 indexed citations (citations by other indexed papers that have themselves been cited), including 22 papers in Astronomy and Astrophysics, 7 papers in Instrumentation and 4 papers in Atmospheric Science. Recurrent topics in Sofya Alexeeva's work include Stellar, planetary, and galactic studies (20 papers), Astrophysics and Star Formation Studies (16 papers) and Astronomy and Astrophysical Research (7 papers). Sofya Alexeeva is often cited by papers focused on Stellar, planetary, and galactic studies (20 papers), Astrophysics and Star Formation Studies (16 papers) and Astronomy and Astrophysical Research (7 papers). Sofya Alexeeva collaborates with scholars based in China, Russia and United States. Sofya Alexeeva's co-authors include L. Mashonkina, Gang Zhao, T. Sitnova, T. Ryabchikova, Yu. V. Pakhomov, Jianrong Shi, Hong-Liang Yan, Chiaki Kobayashi, Michael Bolte and Y. Q. Chen and has published in prestigious journals such as Nature Communications, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

Sofya Alexeeva

22 papers receiving 240 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name	h						Papers	Cites
Sofya Alexeeva China	8	258	95	29	14	8	25	268
Henrique Reggiani United States	11	336 1.3×	144 1.5×	27 0.9×	15 1.1×	9 1.1×	34	357
C. Hottier France	4	290 1.1×	69 0.7×	39 1.3×	9 0.6×	10 1.3×	6	300
Giulia De Somma Italy	10	206 0.8×	72 0.8×	51 1.8×	16 1.1×	6 0.8×	25	231
L. Capitanio France	2	274 1.1×	70 0.7×	27 0.9×	13 0.9×	11 1.4×	4	284
R Cabanac France	4	229 0.9×	84 0.9×	30 1.0×	20 1.4×	12 1.5×	4	234
D. T. Andreasen Portugal	8	213 0.8×	97 1.0×	19 0.7×	9 0.6×	19 2.4×	11	217
Benjamin M. Tofflemire United States	12	280 1.1×	67 0.7×	23 0.8×	5 0.4×	15 1.9×	28	285
Н. П. Иконникова Russia	11	333 1.3×	128 1.3×	17 0.6×	10 0.7×	10 1.3×	72	340
G. Cocozza Italy	8	320 1.2×	128 1.3×	34 1.2×	17 1.2×	7 0.9×	11	326
David V. Martin United States	13	449 1.7×	104 1.1×	19 0.7×	9 0.6×	6 0.8×	39	455

Countries citing papers authored by Sofya Alexeeva

Since Specialization

Citations

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

Fields of papers citing papers by Sofya Alexeeva

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Sofya Alexeeva

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

All Works

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20 of 20 papers shown

Shi, Jianrong, Gang Zhao, Haining Li, et al.. (2025). A Systematic NLTE Study of Very Metal-poor Stars with Metallicity down to −4.3 dex. I. Global Stellar Parameters Based on High-resolution Spectra. The Astrophysical Journal. 983(2). 127–127. 1 indexed citations

Alexeeva, Sofya, O. Kochukhov, Е. А. Семенко, et al.. (2025). Chemical abundances and Doppler imaging of the Ap Si/He-wk star HD 100357. Monthly Notices of the Royal Astronomical Society. 542(2). 747–761.

Guo, Yanjun, et al.. (2024). Non-local thermodynamic equilibrium (NLTE) abundances of europium (Eu) for a sample of metal-poor stars in the galactic halo and metal-poor disk with 1D and 〈3D〉 models. Astronomy and Astrophysics. 693. A211–A211. 3 indexed citations

Yuan, Zhen, Tadafumi Matsuno, L. Mashonkina, et al.. (2024). HR-GO. Astronomy and Astrophysics. 690. A331–A331. 1 indexed citations

Alexeeva, Sofya, Gang Zhao, Feng Wang, et al.. (2023). NLTE Analysis of Y i and Y ii in the Atmospheres of FGK Stars. The Astrophysical Journal. 957(1). 10–10. 7 indexed citations

Alexeeva, Sofya, Gang Zhao, Zeming Zhou, et al.. (2023). Sodium Abundances in Very Metal-poor Stars. Research in Astronomy and Astrophysics. 23(7). 75019–75019. 3 indexed citations

Alexeeva, Sofya, Feng Wang, Yong Wu, et al.. (2023). Theoretical study of inelastic processes in collisions of Y and Y+ with hydrogen atom. Monthly Notices of the Royal Astronomical Society. 527(2). 2083–2092. 1 indexed citations

Alexeeva, Sofya & Gang Zhao. (2022). Spectroscopic Study of M33 with the LAMOST Survey. I. Chemical Gradients from Nebulae. The Astrophysical Journal. 925(1). 76–76. 6 indexed citations

Cui, Wenyuan, et al.. (2022). Origins of B-type stars at high Galactic latitudes based on abundances and kinematics. Monthly Notices of the Royal Astronomical Society. 519(1). 995–1012. 7 indexed citations

10.

Cui, Wenyuan, et al.. (2022). Chemical Composition of B-type Stars from LAMOST DR5. The Astrophysical Journal. 937(2). 110–110. 4 indexed citations

11.

Hu, Shaoming, et al.. (2022). Exploration of the origin of the 2020 X-ray outburst in OJ 287. Monthly Notices of the Royal Astronomical Society. 515(2). 2778–2789. 2 indexed citations

12.

Alexeeva, Sofya, et al.. (2021). Author Correction: Spectroscopic evidence for a large spot on the dimming Betelgeuse. Nature Communications. 12(1). 5252–5252.

13.

Alexeeva, Sofya, et al.. (2021). Spectroscopic evidence for a large spot on the dimming Betelgeuse. Nature Communications. 12(1). 4719–4719. 4 indexed citations

14.

Alexeeva, Sofya, et al.. (2020). Impact of the convective mixing-length parameter α on stellar metallicity. Astronomy and Astrophysics. 635. A176–A176. 8 indexed citations

15.

Alexeeva, Sofya, et al.. (2020). Influence of the convective mixing-length parameter α on the chemical abundances in the case of metal-poor giant HD 122563. Research in Astronomy and Astrophysics. 20(8). 121–121. 1 indexed citations

16.

Zhao, Gang, L. Mashonkina, Hong-Liang Yan, et al.. (2016). SYSTEMATIC NON-LTE STUDY OF THE −2.6 ≤ [Fe/H] ≤ 0.2 F AND G DWARFS IN THE SOLAR NEIGHBORHOOD. II. ABUNDANCE PATTERNS FROM Li TO Eu*. The Astrophysical Journal. 833(2). 225–225. 101 indexed citations

17.

Wu, Xiaoshu, Sofya Alexeeva, L. Mashonkina, et al.. (2015). Calibrating theαparameter of convective efficiency using observed stellar properties. Astronomy and Astrophysics. 577. A134–A134. 8 indexed citations

18.

Соболев, А. М., et al.. (2015). Star formation in the S233 region. Monthly Notices of the Royal Astronomical Society. 452(3). 2306–2317. 10 indexed citations

19.

Ryabchikova, T., N. Piskunov, Yu. V. Pakhomov, et al.. (2015). Accuracy of atmospheric parameters of FGK dwarfs determined by spectrum fitting. Monthly Notices of the Royal Astronomical Society. 456(2). 1221–1234. 31 indexed citations

20.

Alexeeva, Sofya, et al.. (2013). Orbital and physical parameters of the spectroscopic binary HD37737. Astrophysical Bulletin. 68(2). 169–176. 5 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.

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