S.‐B. Qian

3.5k total citations
177 papers, 2.7k citations indexed

About

S.‐B. Qian is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, S.‐B. Qian has authored 177 papers receiving a total of 2.7k indexed citations (citations by other indexed papers that have themselves been cited), including 177 papers in Astronomy and Astrophysics, 46 papers in Instrumentation and 9 papers in Computational Mechanics. Recurrent topics in S.‐B. Qian's work include Stellar, planetary, and galactic studies (170 papers), Astrophysics and Star Formation Studies (149 papers) and Astro and Planetary Science (84 papers). S.‐B. Qian is often cited by papers focused on Stellar, planetary, and galactic studies (170 papers), Astrophysics and Star Formation Studies (149 papers) and Astro and Planetary Science (84 papers). S.‐B. Qian collaborates with scholars based in China, Thailand and Argentina. S.‐B. Qian's co-authors include Li-Ying Zhu, J.-J. He, Boonrucksar Soonthornthum, Yuangui Yang, Linsheng Liu, Wuping Liao, Z.-B. Dai, Wen-Ping Liao, E. Fernández Lajús and Jia Zhang and has published in prestigious journals such as SHILAP Revista de lepidopterología, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

S.‐B. Qian

168 papers receiving 2.5k 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.‐B. Qian China 30 2.6k 652 150 134 93 177 2.7k
Li-Ying Zhu China 27 1.9k 0.7× 531 0.8× 138 0.9× 105 0.8× 60 0.6× 141 1.9k
J. O. Sundqvist Belgium 31 2.2k 0.8× 521 0.8× 165 1.1× 111 0.8× 139 1.5× 87 2.3k
T. E. Harrison United States 24 1.9k 0.7× 447 0.7× 127 0.8× 96 0.7× 187 2.0× 91 1.9k
P. Rodríguez-Gil Spain 27 2.2k 0.8× 523 0.8× 144 1.0× 116 0.9× 208 2.2× 108 2.2k
J. J. Hermes United States 28 2.2k 0.8× 788 1.2× 131 0.9× 111 0.8× 85 0.9× 127 2.3k
S. Geier Germany 30 2.5k 1.0× 1.2k 1.8× 187 1.2× 84 0.6× 68 0.7× 120 2.6k
Eiji Kambe Japan 23 1.7k 0.6× 670 1.0× 75 0.5× 31 0.2× 85 0.9× 90 1.8k
H. Todt Germany 24 1.9k 0.7× 593 0.9× 108 0.7× 40 0.3× 100 1.1× 73 1.9k
J.‐C. Bouret France 30 2.9k 1.1× 779 1.2× 117 0.8× 44 0.3× 51 0.5× 74 3.0k
R. A. Saffer United States 24 1.8k 0.7× 802 1.2× 91 0.6× 47 0.4× 41 0.4× 49 1.8k

Countries citing papers authored by S.‐B. Qian

Since Specialization
Citations

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

Fields of papers citing papers by S.‐B. Qian

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S.‐B. Qian

This figure shows the co-authorship network connecting the top 25 collaborators of S.‐B. Qian. A scholar is included among the top collaborators of S.‐B. Qian 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.‐B. Qian. S.‐B. Qian 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.
Shi, Xiang-Dong, et al.. (2024). Observational Properties of 155 β Cephei Pulsating Variable Stars. The Astrophysical Journal Supplement Series. 271(1). 28–28. 4 indexed citations
2.
Li, Min-Yu, S.‐B. Qian, Li-Ying Zhu, et al.. (2024). Pulsation phases and mode identification of tidally excited oscillations in fourteen Kepler Heartbeat Stars. Monthly Notices of the Royal Astronomical Society. 530(1). 586–596. 3 indexed citations
3.
4.
Qian, S.‐B., Li-Ying Zhu, Wen-Ping Liao, et al.. (2024). A New Window for Studying Intermediate Polars and Tilted Accretion Disk Precession. The Astrophysical Journal. 966(1). 83–83. 5 indexed citations
5.
6.
Qian, S.‐B., et al.. (2024). Detection of Two Totally Eclipsing B-type Binaries with Extremely Low Mass Ratios. The Astrophysical Journal. 972(1). 119–119. 1 indexed citations
7.
Qian, S.‐B., Miloslav Zejda, Zdeněk Mikulášek, et al.. (2023). First photometric investigation of OGLE-SMC-ECL-2063: A low-metallicity massive contact binary in the SMC. Publications of the Astronomical Society of Japan. 75(2). 358–367. 1 indexed citations
8.
Qian, S.‐B., et al.. (2023). New evidence for the precession of tilted disc in SDSS J081256.85+191157.8. Monthly Notices of the Royal Astronomical Society. 526(3). 3730–3743. 11 indexed citations
9.
Qian, S.‐B., Min-Yu Li, Er-Gang Zhao, et al.. (2023). Five Massive Contact Binaries with Twin Components in LMC. The Astrophysical Journal. 956(1). 49–49. 4 indexed citations
10.
Shi, Xiang-Dong, et al.. (2023). A Catalog of New Slowly Pulsating B-type Stars. The Astrophysical Journal Supplement Series. 268(1). 16–16. 4 indexed citations
11.
Li, L.-J., S.‐B. Qian, Xiang-Dong Shi, & Li-Ying Zhu. (2023). Two Different Weak Modulations in ab-type RR Lyrae Variable V838 Cyg, and Potential Influence of Metal Abundance on Blazhko Modulation. The Astronomical Journal. 166(3). 83–83. 2 indexed citations
12.
Qian, S.‐B., Lìyǐng Zhū, Ai‐Jun Dong, et al.. (2022). First discovery of quasi-periodic oscillations in the dwarf nova HS 2325+8205 based on TESS photometry. Monthly Notices of the Royal Astronomical Society. 518(3). 3901–3907. 10 indexed citations
13.
Qian, S.‐B., Ai‐Jun Dong, Qi‐Jun Zhi, et al.. (2022). Study on the variation of orbital period, quasi-periodic oscillations and negative superhumps in V729 Sgr. New Astronomy. 93. 101751–101751. 8 indexed citations
14.
Zhou, X. & S.‐B. Qian. (2021). Orbital period correction and light curve modeling of the W-subtype shallow contact binary OW Leo. Research in Astronomy and Astrophysics. 21(2). 27–27. 2 indexed citations
15.
Shi, Xiang-Dong, et al.. (2020). ASAS J174406+2446.8 is identified as a marginal-contact binary with a possible cool third body. Research in Astronomy and Astrophysics. 20(6). 96–96. 8 indexed citations
16.
Qian, S.‐B., Miloslav Zejda, Jingjing Wang, et al.. (2019). A photometric study of the short-period eclipsing binary 1SWASP J204932.94-654025.8, showing strong third light. New Astronomy. 76. 101324–101324. 3 indexed citations
17.
Zhu, Li-Ying, et al.. (2019). A Close-in Substellar Object Orbiting the sdOB-type Eclipsing-Binary System NSVS14256825. Conicet. 8 indexed citations
18.
Qian, S.‐B., Guang Shi, S. Zoła, et al.. (2013). A search for substellar objects orbiting the sdB eclipsing binary HS 0705+6700. Monthly Notices of the Royal Astronomical Society. 436(2). 1408–1414. 22 indexed citations
19.
Liao, Wuping, S.‐B. Qian, Kaitao Li, et al.. (2013). THE MULTI-COLOR LIGHT CURVES OF THE W UMa TYPE CONTACT BINARY EP ANDROMEDAE. The Astronomical Journal. 146(4). 79–79. 17 indexed citations
20.
Liao, Wuping & S.‐B. Qian. (2010). The most plausible explanation of the cyclic period changes in close binaries: the case of the RS CVn-type binary WW Dra. Monthly Notices of the Royal Astronomical Society. no–no. 98 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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