S. Kiyota

1.9k total citations
27 papers, 357 citations indexed

About

S. Kiyota is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, S. Kiyota has authored 27 papers receiving a total of 357 indexed citations (citations by other indexed papers that have themselves been cited), including 27 papers in Astronomy and Astrophysics, 9 papers in Nuclear and High Energy Physics and 3 papers in Instrumentation. Recurrent topics in S. Kiyota's work include Gamma-ray bursts and supernovae (22 papers), Astrophysical Phenomena and Observations (22 papers) and Pulsars and Gravitational Waves Research (9 papers). S. Kiyota is often cited by papers focused on Gamma-ray bursts and supernovae (22 papers), Astrophysical Phenomena and Observations (22 papers) and Pulsars and Gravitational Waves Research (9 papers). S. Kiyota collaborates with scholars based in Japan, United States and Chile. S. Kiyota's co-authors include Izumi Hachisu, Mariko Kato, Taichi Kato, Hideyuki Saio, F. Marang, Tonny Vanmunster, S. Desidera, P. M. Marrese, R. L. M. Corradi and Federico Boschi and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

S. Kiyota

23 papers receiving 346 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
S. Kiyota Japan 10 355 62 35 32 13 27 357
Reba M. Bandyopadhyay United States 8 229 0.6× 38 0.6× 18 0.5× 31 1.0× 15 1.2× 29 231
A. Domingo Spain 6 238 0.7× 68 1.1× 15 0.4× 15 0.5× 35 2.7× 35 244
Ashley Pagnotta United States 9 342 1.0× 95 1.5× 43 1.2× 18 0.6× 15 1.2× 19 345
E. A. Barsukova Russia 9 222 0.6× 33 0.5× 25 0.7× 15 0.5× 29 2.2× 43 229
S. C. Williams United Kingdom 11 246 0.7× 64 1.0× 39 1.1× 12 0.4× 12 0.9× 41 255
Ryoko Ishioka Japan 9 224 0.6× 46 0.7× 28 0.8× 18 0.6× 5 0.4× 36 228
K. A. Stoyanov Bulgaria 9 176 0.5× 31 0.5× 26 0.7× 27 0.8× 19 1.5× 34 178
I. Traulsen Germany 8 162 0.5× 52 0.8× 22 0.6× 13 0.4× 9 0.7× 17 171
L. E. Rivera Sandoval United States 9 221 0.6× 35 0.6× 15 0.4× 21 0.7× 35 2.7× 24 233
S. Katajainen Finland 9 202 0.6× 125 2.0× 17 0.5× 18 0.6× 7 0.5× 14 212

Countries citing papers authored by S. Kiyota

Since Specialization
Citations

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

Fields of papers citing papers by S. Kiyota

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. Kiyota

This figure shows the co-authorship network connecting the top 25 collaborators of S. Kiyota. A scholar is included among the top collaborators of S. Kiyota 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 S. Kiyota. S. Kiyota 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.
Kiyota, S., J. Brimacombe, R. A. Koff, et al.. (2017). ASASSN-17cu and ASASSN-17cv: Discovery of Two Probable Supernovae. ATel. 10113. 1.
2.
Imada, Akira, Taichi Kato, Keisuke Isogai, et al.. (2017). The 2015 superoutburst of QZ Virginis: Detection of growing superhumps between the precursor and main superoutburst. Publications of the Astronomical Society of Japan. 69(4). 1 indexed citations
3.
Vallely, P., J. L. Prieto, K. Z. Stanek, et al.. (2017). The highly luminous Type Ibn supernova ASASSN-14ms. Monthly Notices of the Royal Astronomical Society. 475(2). 2344–2354. 7 indexed citations
4.
Noguchi, T., S. Kiyota, G. Masi, et al.. (2015). Supernova 2015G in NGC 6951 = Psn J20372558+6607115. 4087. 1.
5.
Pagnotta, Ashley, Bradley E. Schaefer, James L. Clem, et al.. (2015). THE 2010 ERUPTION OF THE RECURRENT NOVA U SCORPII: THE MULTI-WAVELENGTH LIGHT CURVE. Leicester Research Archive (University of Leicester). 5 indexed citations
6.
Holoien, T. W. S., K. Z. Stanek, C. S. Kochanek, et al.. (2014). ASAS-SN Discovery of A Probable Supernova in PGC 006399. The astronomer's telegram. 6714. 1. 1 indexed citations
7.
Kiyota, S., T. W. S. Holoien, K. Z. Stanek, et al.. (2014). ASAS-SN Discovery of A Possible Supernova in NGC 1566. ATel. 6460. 1.
8.
Hachisu, Izumi, Mariko Kato, S. Kiyota, et al.. (2008). Optical Light Curves of RS Oph (2006) and Hydrogen Burning Turnoff. ASPC. 401. 206. 1 indexed citations
9.
Hachisu, Izumi, Mariko Kato, S. Kiyota, et al.. (2006). The Hydrogen-Burning Turnoff of RS Ophiuchi (2006). The Astrophysical Journal. 651(2). L141–L144. 34 indexed citations
10.
Uemura, Makoto, R. E. Mennickent, Ryoko Ishioka, et al.. (2005). TV Corvi revisited: Precursor and superhump period derivative linkedto the disk instability model. Springer Link (Chiba Institute of Technology). 14 indexed citations
11.
Uemura, Makoto, Taichi Kato, Ryoko Ishioka, et al.. (2004). A Deeply Eclipsing SU UMa-Type Dwarf Nova with the Shortest Orbital Period, XZ Eridani. Publications of the Astronomical Society of Japan. 56(sp1). S141–S146. 2 indexed citations
12.
Nogami, Daisaku, Makoto Uemura, Ryoko Ishioka, et al.. (2004). A New SU UMa-Type Dwarf Nova, QW Serpentis (= TmzV46). Publications of the Astronomical Society of Japan. 56(sp1). S99–S107. 3 indexed citations
13.
Ishioka, Ryoko, Taichi Kato, Makoto Uemura, et al.. (2003). Period Change of Superhumps in a WZ Sge-Type Dwarf Nova, HV Virginis. Publications of the Astronomical Society of Japan. 55(3). 683–690. 7 indexed citations
14.
Munari, U., A. A. Henden, S. Kiyota, et al.. (2002). The mysterious eruption of V838 Mon. Springer Link (Chiba Institute of Technology). 89 indexed citations
15.
Uemura, Makoto, Taichi Kato, Ryoko Ishioka, et al.. (2002). Rapid Optical Fluctuations in the Black Hole Binary V4641 Sagittarii. Publications of the Astronomical Society of Japan. 54(5). L79–L82. 12 indexed citations
16.
Ishioka, Ryoko, Taichi Kato, Makoto Uemura, et al.. (2001). The 2000–2001 Superoutburst of the WZ Sge-Type Star RZ Leonis: A Clue to Understanding the Origin of Viscosity in Quiescent Dwarf Nova Disks. Publications of the Astronomical Society of Japan. 53(5). 905–914. 21 indexed citations
17.
Matsumoto, Katsura, Makoto Uemura, Takeo Kato, et al.. (2001). Detailed optical behavior of the 2000 outburst of the eclipsing recurrent nova CI Aquilae. Astronomy and Astrophysics. 378(2). 487–494. 11 indexed citations
18.
Kato, Taichi, et al.. (2001). 1998 Superoutburst of the Large-Amplitude SU UMa-Type Dwarf Nova WX Ceti. Publications of the Astronomical Society of Japan. 53(5). 893–900. 16 indexed citations
19.
Skillman, David R., David A. Harvey, J. Patterson, et al.. (1998). Superhumps and Accretion Disk Precession in TT Arietis. The Astrophysical Journal. 503(1). L67–L70. 30 indexed citations
20.
Patterson, J., Jonathan Kemp, David R. Skillman, et al.. (1998). Superhumps in Cataclysmic Binaries. XV. EG Cancri, King of the Echo Outbursts. Publications of the Astronomical Society of the Pacific. 110(753). 1290–1303. 43 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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