Takuma Suda

3.8k total citations
89 papers, 1.1k citations indexed

About

Takuma Suda is a scholar working on Astronomy and Astrophysics, Instrumentation and Computer Networks and Communications. According to data from OpenAlex, Takuma Suda has authored 89 papers receiving a total of 1.1k indexed citations (citations by other indexed papers that have themselves been cited), including 61 papers in Astronomy and Astrophysics, 22 papers in Instrumentation and 17 papers in Computer Networks and Communications. Recurrent topics in Takuma Suda's work include Stellar, planetary, and galactic studies (45 papers), Astrophysics and Star Formation Studies (28 papers) and Gamma-ray bursts and supernovae (25 papers). Takuma Suda is often cited by papers focused on Stellar, planetary, and galactic studies (45 papers), Astrophysics and Star Formation Studies (28 papers) and Gamma-ray bursts and supernovae (25 papers). Takuma Suda collaborates with scholars based in Japan, United States and Germany. Takuma Suda's co-authors include Masayuki Y. Fujimoto, Wako Aoki, Yutaka Komiya, Tadafumi Matsuno, Kenichi Fujii, M. Aikawa, Masahiro N. Machida, M. Y. Fujimoto, Haining Li and Miho N. Ishigaki and has published in prestigious journals such as Journal of Geophysical Research Atmospheres, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

Takuma Suda

72 papers receiving 1.1k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Takuma Suda Japan 20 893 372 151 109 83 89 1.1k
Sarah Loebman United States 20 1.3k 1.4× 540 1.5× 38 0.3× 131 1.2× 33 0.4× 40 1.4k
Giuliano Taffoni Italy 10 586 0.7× 342 0.9× 68 0.5× 104 1.0× 28 0.3× 42 679
Naohito Nakasato Japan 14 547 0.6× 121 0.3× 102 0.7× 106 1.0× 24 0.3× 43 765
K. Barbary United States 9 320 0.4× 127 0.3× 35 0.2× 47 0.4× 33 0.4× 19 430
J. Goldstein United States 10 572 0.6× 99 0.3× 167 1.1× 230 2.1× 57 0.7× 17 792
R. Geyer Germany 4 557 0.6× 304 0.8× 80 0.5× 21 0.2× 51 0.6× 9 715
Xuefei Chen China 21 1.1k 1.3× 341 0.9× 36 0.2× 66 0.6× 33 0.4× 94 1.3k
Ted Kremenek United States 7 612 0.7× 49 0.1× 79 0.5× 164 1.5× 195 2.3× 7 879
Uwe Wolter Germany 17 558 0.6× 226 0.6× 26 0.2× 7 0.1× 109 1.3× 59 784
William O’Mullane Spain 10 266 0.3× 136 0.4× 77 0.5× 17 0.2× 27 0.3× 34 392

Countries citing papers authored by Takuma Suda

Since Specialization
Citations

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

Fields of papers citing papers by Takuma Suda

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Takuma Suda

This figure shows the co-authorship network connecting the top 25 collaborators of Takuma Suda. A scholar is included among the top collaborators of Takuma Suda 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 Takuma Suda. Takuma Suda 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
1.
Zhao, Jingkun, Guangwei Li, Wako Aoki, et al.. (2025). Chemical Abundances of Seven Stars in the GD-1 Stream. The Astrophysical Journal Letters. 989(2). L52–L52.
2.
Matsuno, Tadafumi, Haining Li, Wako Aoki, et al.. (2024). Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties. The Astrophysical Journal. 966(2). 174–174. 4 indexed citations
3.
Zhao, Gang, Wako Aoki, Haining Li, et al.. (2024). Detection of the Actinide Th in an r-process-enhanced Star with Accretion Origin. The Astrophysical Journal. 965(1). 79–79. 3 indexed citations
4.
Aoki, Wako, Haining Li, Tadafumi Matsuno, et al.. (2022). Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency. The Astrophysical Journal. 931(2). 146–146. 15 indexed citations
5.
Li, Haining, Wako Aoki, Tadafumi Matsuno, et al.. (2022). Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances. The Astrophysical Journal. 931(2). 147–147. 69 indexed citations
6.
Matsuno, Tadafumi, Helmer H. Koppelman, A. Helmi, et al.. (2022). High-precision chemical abundances of Galactic building blocks. Astronomy and Astrophysics. 661. A103–A103. 25 indexed citations
7.
Suda, Takuma, et al.. (2021). s-process enrichment of ultrafaint dwarf galaxies. Monthly Notices of the Royal Astronomical Society. 505(3). 3755–3766. 5 indexed citations
8.
Li, Haining, Wako Aoki, Tadafumi Matsuno, et al.. (2018). Enormous Li Enhancement Preceding Red Giant Phases in Low-mass Stars in the Milky Way Halo∗. The Astrophysical Journal Letters. 852(2). L31–L31. 26 indexed citations
9.
Ishizuka, Chikako, Takuma Suda, Hideyuki Suzuki, et al.. (2015). EOSDB: The database for nuclear equations of state. Kyoto University Research Information Repository (Kyoto University). 6 indexed citations
10.
Suda, Takuma, Jun Hidaka, Miho N. Ishigaki, et al.. (2014). Stellar Abundances for Galactic Archaeology database for stars in dwarf galaxies. MmSAI. 85. 600. 1 indexed citations
11.
Gil-Pons, Pilar, C. L. Doherty, Herbert H. B. Lau, et al.. (2013). Evolution and CNO yields ofZ= 10-5stars and possible effects on carbon-enhanced metal-poor production. Astronomy and Astrophysics. 557. A106–A106. 27 indexed citations
12.
Aoki, Wako, Miho N. Ishigaki, Takuma Suda, Takuji Tsujimoto, & N. Arimoto. (2012). Galactic archaeology : near-field cosmology and the formation of the milky way. Astronomical Society of the Pacific eBooks. 36 indexed citations
13.
Suda, Takuma & M. Y. Fujimoto. (2010). Evolution of low- and intermediate-mass stars with [Fe/H]≤− 2.5. Monthly Notices of the Royal Astronomical Society. 39 indexed citations
14.
Tanaka, Masaomi, Keiichi Maeda, P. A. Mazzali, et al.. (2008). Multi-Dimensional Simulations of Radiative Transfer in Aspherical Core-Collapse Supernovae. AIP conference proceedings. 1016. 249–254. 1 indexed citations
15.
Suda, Takuma, Takaya Nozawa, Akira Ohnishi, et al.. (2008). ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System. AIPC. 1016. 3 indexed citations
16.
Gil-Pons, Pilar, Takuma Suda, Masayuki Y. Fujimoto, & E. Garcı́a–Berro. (2005). Carbon burning in intermediate-mass primordial stars. Astronomy and Astrophysics. 433(3). 1037–1046. 22 indexed citations
17.
Suda, Takuma, M. Aikawa, Masahiro N. Machida, M. Y. Fujimoto, & Icko Iben. (2004). Is HE0107-5240 A Primordial Star?. arXiv (Cornell University).
18.
Suda, Takuma, et al.. (1981). Cosmic ray N-S asymmetry and interplanetary magnetic field. ICRC. 10. 187–189. 2 indexed citations
19.
Suda, Takuma & M. Wada. (1979). Average Features of Cosmic Ray Variations at Magnetic Sudden Commencements. International Cosmic Ray Conference. 3. 433. 1 indexed citations
20.
Suda, Takuma, et al.. (1977). The Spectrum of Forbush Decrease and the Velocity of Blast Wave. International Cosmic Ray Conference. 3. 312.

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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