K. Sekiguchi

8.4k total citations
86 papers, 2.3k citations indexed

About

K. Sekiguchi is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, K. Sekiguchi has authored 86 papers receiving a total of 2.3k indexed citations (citations by other indexed papers that have themselves been cited), including 80 papers in Astronomy and Astrophysics, 31 papers in Instrumentation and 13 papers in Computational Mechanics. Recurrent topics in K. Sekiguchi's work include Stellar, planetary, and galactic studies (38 papers), Astronomy and Astrophysical Research (31 papers) and Astrophysical Phenomena and Observations (28 papers). K. Sekiguchi is often cited by papers focused on Stellar, planetary, and galactic studies (38 papers), Astronomy and Astrophysical Research (31 papers) and Astrophysical Phenomena and Observations (28 papers). K. Sekiguchi collaborates with scholars based in Japan, South Africa and United States. K. Sekiguchi's co-authors include Tadafumi Takata, Chris Simpson, Masayuki Akiyama, Yoshihiro Ueda, M. Yoshida, Masanori Iye, Nobunari Kashikawa, I. S. Glass, Sadanori Okamura and Tōru Yamada and has published in prestigious journals such as Nature, Physical Review Letters and The Astrophysical Journal.

In The Last Decade

K. Sekiguchi

79 papers receiving 2.2k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
K. Sekiguchi Japan 24 2.2k 717 478 76 68 86 2.3k
H. E. Smith United States 24 2.4k 1.1× 705 1.0× 667 1.4× 85 1.1× 52 0.8× 97 2.5k
R. Elston United States 27 2.2k 1.0× 623 0.9× 660 1.4× 102 1.3× 60 0.9× 77 2.3k
I. Hook United Kingdom 27 3.0k 1.4× 975 1.4× 755 1.6× 120 1.6× 45 0.7× 88 3.1k
K. A. Misselt United States 29 2.7k 1.2× 689 1.0× 286 0.6× 64 0.8× 48 0.7× 76 2.7k
M. Yoshida Japan 31 3.2k 1.5× 1.1k 1.5× 690 1.4× 168 2.2× 68 1.0× 143 3.3k
N. A. Levenson United States 31 3.3k 1.5× 591 0.8× 679 1.4× 130 1.7× 41 0.6× 102 3.4k
Harland W. Epps United States 15 2.0k 0.9× 742 1.0× 279 0.6× 213 2.8× 56 0.8× 50 2.2k
A. Wolter Italy 25 2.8k 1.3× 538 0.8× 1.4k 3.0× 67 0.9× 60 0.9× 120 3.0k
Alan Uomoto United States 18 3.3k 1.5× 1.3k 1.8× 426 0.9× 142 1.9× 83 1.2× 53 3.4k
Steven Janowiecki United States 18 2.4k 1.1× 798 1.1× 515 1.1× 61 0.8× 65 1.0× 41 2.5k

Countries citing papers authored by K. Sekiguchi

Since Specialization
Citations

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

Fields of papers citing papers by K. Sekiguchi

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of K. Sekiguchi

This figure shows the co-authorship network connecting the top 25 collaborators of K. Sekiguchi. A scholar is included among the top collaborators of K. Sekiguchi 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 K. Sekiguchi. K. Sekiguchi 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.
Fiúza, Frederico, et al.. (2024). Electron-Ion Temperature Ratio in Transrelativistic Unmagnetized Shock Waves. arXiv (Cornell University). 11–11. 1 indexed citations
2.
Spitkovsky, Anatoly, et al.. (2024). Electron Heating in High Mach Number Collisionless Shocks. Physical Review Letters. 132(26). 265201–265201. 4 indexed citations
3.
Totorica, Samuel, Seiji Zenitani, Shuichi Matsukiyo, et al.. (2023). Exact Calculation of Nonideal Fields Demonstrates Their Dominance of Injection in Relativistic Reconnection. The Astrophysical Journal Letters. 952(1). L1–L1. 5 indexed citations
4.
Ishiguro, Masateru, Yoshiharu Shinnaka, Tatsuya Nakaoka, et al.. (2018). High polarization degree of the continuum of comet 2P/Encke based on spectropolarimetric signals during its 2017 apparition. Springer Link (Chiba Institute of Technology). 4 indexed citations
5.
Magliocchetti, M., M. Cirasuolo, R. J. McLure, et al.. (2007). On the evolution of clustering of 24-μm-selected galaxies. Monthly Notices of the Royal Astronomical Society. 383(3). 1131–1142. 18 indexed citations
6.
Lane, K., O. Almaini, Sylvie Foucaud, et al.. (2007). The colour selection of distant galaxies in the UKIDSS Ultra Deep Survey Early Data Release. Leicester Research Archive (University of Leicester). 22 indexed citations
7.
Watson, M. G., et al.. (2004). The Subaru XMM-Newton Deep Survey (SXDS). 14 indexed citations
8.
Motch, C., K. Sekiguchi, F. Haberl, et al.. (2004). The proper motion of the isolated neutron star RX J1605.3+3249. Astronomy and Astrophysics. 429(1). 257–265. 25 indexed citations
9.
Severgnini, P., A. Caccianiga, V. Braito, et al.. (2003). XMM-Newtonobservations reveal AGN in apparently normal galaxies. Astronomy and Astrophysics. 406(2). 483–492. 59 indexed citations
10.
Ramsay, Gavin, Kinwah Wu, M. Cropper, et al.. (2002). Optical/infrared spectroscopy and photometry of the short-period binary RX J1914+24. Monthly Notices of the Royal Astronomical Society. 333(3). 575–582. 21 indexed citations
11.
Kajisawa, Masaru, Tōru Yamada, Ichi Tanaka, et al.. (1999). Color–Magnitude Sequence in the Clusters at z ∼ 1.2 near the Radio Galaxy 3C 324. 13 indexed citations
12.
Buckley, D. A. H., D. O’Donoghue, B. J. M. Hassall, et al.. (1993). Discovery of an EUV-bright polar in the period gap from the ROSAT Wide Field Camera sky survey. Monthly Notices of the Royal Astronomical Society. 262(1). 93–108. 9 indexed citations
13.
Scarrott, S. M., et al.. (1990). The nature of the bipolar nebula associated with IRAS 07131−0147. Monthly Notices of the Royal Astronomical Society. 245(3). 484–492. 3 indexed citations
14.
Sekiguchi, K., P. A. Whitelock, M. W. Feast, et al.. (1990). The 1989 outburst of the recurrent nova V745 Sco. Monthly Notices of the Royal Astronomical Society. 246(1). 78–83. 7 indexed citations
15.
Sekiguchi, K., M. W. Feast, A. P. Fairall, & Hartmut Winkler. (1989). Spectral evolution of Nova Centauri 1986 (V842 Cen). Monthly Notices of the Royal Astronomical Society. 241(2). 311–323. 6 indexed citations
16.
Sekiguchi, K., D. Kilkenny, Hartmut Winkler, & J. G. Doyle. (1989). Optical spectroscopy of Nova LMC 1988 No. 2 during its early decline stage. Monthly Notices of the Royal Astronomical Society. 241(4). 827–837. 6 indexed citations
17.
Sekiguchi, K., R. M. Catchpole, A. P. Fairall, et al.. (1989). The recurrent nova V394 Coronae Austrinae – the 1987 outburst. Monthly Notices of the Royal Astronomical Society. 236(3). 611–619. 12 indexed citations
18.
Sekiguchi, K., et al.. (1988). The Cambridge Astronomy Guide. 47. 12. 2 indexed citations
19.
Sekiguchi, K. & Kurt S. Anderson. (1987). The initial mass function for early-type stars in starburst galaxies. The Astronomical Journal. 94. 644–644. 5 indexed citations
20.
Sekiguchi, K. & Kurt S. Anderson. (1987). Mass to line-strength relations from IUE spectra of early-type stars. The Astronomical Journal. 94. 129–129. 4 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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