T. Semaan

765 total citations
20 papers, 324 citations indexed

About

T. Semaan is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, T. Semaan has authored 20 papers receiving a total of 324 indexed citations (citations by other indexed papers that have themselves been cited), including 20 papers in Astronomy and Astrophysics, 10 papers in Instrumentation and 4 papers in Computational Mechanics. Recurrent topics in T. Semaan's work include Stellar, planetary, and galactic studies (20 papers), Astrophysics and Star Formation Studies (15 papers) and Astronomy and Astrophysical Research (10 papers). T. Semaan is often cited by papers focused on Stellar, planetary, and galactic studies (20 papers), Astrophysics and Star Formation Studies (15 papers) and Astronomy and Astrophysical Research (10 papers). T. Semaan collaborates with scholars based in Belgium, Switzerland and France. T. Semaan's co-authors include J. Gutiérrez–Soto, Y. Frémat, C. Martayan, A. M. Hubert, N. Mowlavï, P. Eggenberger, L. Eyer, S. Saesen, P. Stee and C. Georgy and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal Supplement Series and Astronomy and Astrophysics.

In The Last Decade

T. Semaan

18 papers receiving 310 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
T. Semaan Belgium 11 309 155 31 9 9 20 324
Á. Sódor Hungary 12 375 1.2× 181 1.2× 42 1.4× 10 1.1× 7 0.8× 41 386
N. Parley United Kingdom 8 423 1.4× 158 1.0× 40 1.3× 13 1.4× 10 1.1× 9 435
A. W. Fullerton United States 12 412 1.3× 150 1.0× 24 0.8× 9 1.0× 8 0.9× 22 416
Fahri Aliçavuş Türkiye 7 279 0.9× 131 0.8× 34 1.1× 4 0.4× 6 0.7× 24 301
G. Banyard Belgium 9 344 1.1× 147 0.9× 20 0.6× 22 2.4× 7 0.8× 12 364
J. L. Provencal United States 11 243 0.8× 119 0.8× 17 0.5× 11 1.2× 19 2.1× 22 254
S. Marshall United States 4 333 1.1× 144 0.9× 67 2.2× 5 0.6× 6 0.7× 7 349
S. Štefl Czechia 12 395 1.3× 113 0.7× 26 0.8× 10 1.1× 11 1.2× 30 400
Yerra Bharat Kumar China 11 362 1.2× 211 1.4× 23 0.7× 14 1.6× 9 1.0× 25 371
L. Fox Machado Mexico 9 247 0.8× 104 0.7× 31 1.0× 8 0.9× 13 1.4× 29 259

Countries citing papers authored by T. Semaan

Since Specialization
Citations

This map shows the geographic impact of T. Semaan'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 T. Semaan with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. Semaan more than expected).

Fields of papers citing papers by T. Semaan

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of T. Semaan

This figure shows the co-authorship network connecting the top 25 collaborators of T. Semaan. A scholar is included among the top collaborators of T. Semaan 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 T. Semaan. T. Semaan 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.
Semaan, T., A. M. Hubert, J. Zorec, et al.. (2018). Study of a sample of faint Be stars in the exofield of CoRoT. Astronomy and Astrophysics. 613. A70–A70. 21 indexed citations
2.
Mahy, L., E. Gosset, Jean Manfroid, et al.. (2018). The triple system HD 150136: From periastron passage to actual masses. Astronomy and Astrophysics. 616. A75–A75. 11 indexed citations
3.
Granada, A., C. E. Jones, T. A. A. Sigut, et al.. (2018). Quiescent and Active Phases in Be Stars: A WISE Snapshot of Young Galactic Open Clusters. The Astronomical Journal. 155(1). 50–50. 8 indexed citations
4.
Zorec, J., Y. Frémat, A. Domiciano de Souza, et al.. (2017). Critical study of the distribution of rotational velocities of Be stars. Astronomy and Astrophysics. 602. A83–A83. 9 indexed citations
5.
Morel, T., Yaël Nazé, G. Rauw, et al.. (2017). Chemical abundances of fast-rotating massive stars. Astronomy and Astrophysics. 603. A56–A56. 22 indexed citations
6.
Saio, Hideyuki, Sylvia Ekström, N. Mowlavï, et al.. (2017). Period–luminosity relations of fast-rotating B-type stars in the young open cluster NGC 3766. Monthly Notices of the Royal Astronomical Society. 467(4). 3864–3873. 14 indexed citations
7.
Morel, T., Yaël Nazé, G. Rauw, et al.. (2017). Chemical abundances of fast-rotating massive stars. I. Description of the methods and individual results. Open Repository and Bibliography (University of Liège). 603. 13 indexed citations
8.
Zorec, J., Y. Frémat, A. Domiciano de Souza, et al.. (2017). Critical study of the distribution of rotational velocities of Be stars; II: Differential rotation and some hidden effects interfering with the interpretation of the Vsin i parameter. SPIRE - Sciences Po Institutional REpository. 602. 4 indexed citations
9.
Frémat, Y., A. Domiciano de Souza, F. Royer, et al.. (2016). Critical study of the distribution of rotational velocities of Be stars. Astronomy and Astrophysics. 595. A132–A132. 58 indexed citations
10.
Mowlavï, N., S. Saesen, T. Semaan, et al.. (2016). Stellar variability in open clusters. Astronomy and Astrophysics. 595. L1–L1. 21 indexed citations
11.
Anderson, Richard I., Stefano Casertano, Adam G. Riess, et al.. (2016). VETTING GALACTIC LEAVITT LAW CALIBRATORS USING RADIAL VELOCITIES: ON THE VARIABILITY, BINARITY, AND POSSIBLE PARALLAX ERROR OF 19 LONG-PERIOD CEPHEIDS. The Astrophysical Journal Supplement Series. 226(2). 18–18. 20 indexed citations
12.
Mowlavï, N., S. Saesen, T. Semaan, et al.. (2016). Stellar variability in open clusters. II. Discovery of a new period-luminosity relation in a class of fast-rotating pulsating stars in NGC 3766. arXiv (Cornell University). 7 indexed citations
13.
Anderson, Richard I., A. Mérand, P. Kervella, et al.. (2015). Investigating Cepheid ℓ Carinae's cycle-to-cycle variations via contemporaneous velocimetry and interferometry. Monthly Notices of the Royal Astronomical Society. 455(4). 4231–4248. 24 indexed citations
14.
Blomme, R., Y. Frémat, E. Gosset, et al.. (2014). The Gaia-ESO Survey and Massive Stars. Proceedings of the International Astronomical Union. 9(S307). 88–89.
15.
Mantegazza, L., E. Poretti, E. Michel, et al.. (2012). Pulsation spectrum ofδScuti stars: the binary HD 50870 as seen with CoRoT and HARPS. Astronomy and Astrophysics. 542. A24–A24. 23 indexed citations
16.
Semaan, T., Alex Hubert, J. Zorec, et al.. (2012). Study of a sample of faint Be stars in the exofield of CoRoT. Astronomy and Astrophysics. 551. A130–A130. 7 indexed citations
17.
Lehmann, H., A. Tkachenko, T. Semaan, et al.. (2010). Spectral analysis of Kepler SPB andβ Cephei candidate stars. Astronomy and Astrophysics. 526. A124–A124. 54 indexed citations
18.
Semaan, T., Christophe Martayan, Y. Frémat, et al.. (2010). Spectral and photometric study of Be Stars in the first exoplanet fields of CoRoT. Proceedings of the International Astronomical Union. 6(S272). 547–548. 4 indexed citations
19.
Martayan, Christophe, R. Blomme, J.-B. Le Bouquin, et al.. (2010). High-angular resolution observations of the Pistol star. Proceedings of the International Astronomical Union. 6(S272). 616–617.
20.
Gutiérrez–Soto, J., C. Neiner, J. Fabregat, et al.. (2010). Short-term variations in Be stars observed by the CoRoT and Kepler space missions. Proceedings of the International Astronomical Union. 6(S272). 451–456. 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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