Sz. Csizmadia

5.6k total citations
48 papers, 798 citations indexed

About

Sz. Csizmadia is a scholar working on Astronomy and Astrophysics, Instrumentation and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, Sz. Csizmadia has authored 48 papers receiving a total of 798 indexed citations (citations by other indexed papers that have themselves been cited), including 45 papers in Astronomy and Astrophysics, 19 papers in Instrumentation and 3 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in Sz. Csizmadia's work include Stellar, planetary, and galactic studies (42 papers), Astrophysics and Star Formation Studies (20 papers) and Astronomy and Astrophysical Research (19 papers). Sz. Csizmadia is often cited by papers focused on Stellar, planetary, and galactic studies (42 papers), Astrophysics and Star Formation Studies (20 papers) and Astronomy and Astrophysical Research (19 papers). Sz. Csizmadia collaborates with scholars based in Germany, Hungary and Spain. Sz. Csizmadia's co-authors include P. Klagyivik, T. Borkovits, J. Cabrera, H. Rauer, T. Hegedüs, L. L. Kiss, A. Erikson, J. Vinkó, T. Pasternacki and I Bíró 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

Sz. Csizmadia

46 papers receiving 748 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Sz. Csizmadia Germany 18 769 267 54 51 45 48 798
L. Mancini Italy 19 933 1.2× 394 1.5× 93 1.7× 44 0.9× 66 1.5× 60 955
M. Montalto Italy 19 878 1.1× 390 1.5× 34 0.6× 45 0.9× 33 0.7× 46 897
N. Piskunov Sweden 13 878 1.1× 197 0.7× 128 2.4× 21 0.4× 32 0.7× 24 920
S. L. Casewell United Kingdom 20 942 1.2× 346 1.3× 26 0.5× 45 0.9× 72 1.6× 89 974
F. Marang South Africa 19 1.2k 1.6× 353 1.3× 95 1.8× 82 1.6× 40 0.9× 52 1.2k
M. Aurière France 23 1.7k 2.2× 289 1.1× 53 1.0× 40 0.8× 34 0.8× 76 1.7k
Z. Magic Germany 17 1.3k 1.7× 544 2.0× 118 2.2× 40 0.8× 68 1.5× 24 1.4k
A. Mora Spain 15 848 1.1× 198 0.7× 24 0.4× 22 0.4× 20 0.4× 27 869
Guillermo Garcı́a-Segura Mexico 23 1.4k 1.8× 192 0.7× 183 3.4× 20 0.4× 41 0.9× 55 1.4k
F. van Wyk South Africa 19 1.1k 1.5× 443 1.7× 37 0.7× 104 2.0× 59 1.3× 71 1.1k

Countries citing papers authored by Sz. Csizmadia

Since Specialization
Citations

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

Fields of papers citing papers by Sz. Csizmadia

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Sz. Csizmadia

This figure shows the co-authorship network connecting the top 25 collaborators of Sz. Csizmadia. A scholar is included among the top collaborators of Sz. Csizmadia 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 Sz. Csizmadia. Sz. Csizmadia 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.
Csizmadia, Sz., et al.. (2025). Characterising WASP-43b’s interior structure: Unveiling tidal decay and apsidal motion. Astronomy and Astrophysics. 694. A233–A233. 2 indexed citations
2.
Csizmadia, Sz., A. M. S. Smith, H. Rauer, et al.. (2024). Evidence of apsidal motion and a possible co-moving companion star detected in the WASP-19 system. Astronomy and Astrophysics. 684. A78–A78. 8 indexed citations
3.
Szabó, Gy. M., et al.. (2023). Power of wavelets in analyses of transit and phase curves in the presence of stellar variability and instrumental noise. Astronomy and Astrophysics. 675. A107–A107. 5 indexed citations
4.
Szabó, Gy. M., D. Gandolfi, A. Brandeker, et al.. (2021). The changing face of AU Mic b: stellar spots, spin-orbit commensurability, and transit timing variations as seen by CHEOPS and TESS. Repository of the Academy's Library (Library of the Hungarian Academy of Sciences). 14 indexed citations
5.
Carrión-González, Óscar, A. García Muñoz, N. C. Santos, et al.. (2021). Constraining the radius and atmospheric properties of directly imaged exoplanets through multi-phase observations. arXiv (Cornell University). 7 indexed citations
6.
Carrión-González, Óscar, A. García Muñoz, J. Cabrera, et al.. (2020). Directly imaged exoplanets in reflected starlight: the importance of knowing the planet radius. Springer Link (Chiba Institute of Technology). 18 indexed citations
7.
Csizmadia, Sz.. (2020). The Transit and Light Curve Modeller. Monthly Notices of the Royal Astronomical Society. 496(4). 4442–4467. 21 indexed citations
8.
Padovan, Sebastiano, Tilman Spohn, Nicola Tosi, et al.. (2018). Matrix-propagator approach to compute fluid Love numbers and applicability to extrasolar planets. Springer Link (Chiba Institute of Technology). 13 indexed citations
9.
Klagyivik, P., H. J. Deeg, J. Cabrera, Sz. Csizmadia, & J. M. Almenara. (2017). Limits to the presence of transiting circumbinary planets in CoRoT Data. Springer Link (Chiba Institute of Technology). 11 indexed citations
10.
Csizmadia, Sz., et al.. (2016). Extended Meteor Hunting with Smartphones as Surveillance Cameras. elib (German Aerospace Center). 1797.
11.
Sedaghati, Elyar, H. M. J. Boffin, Tereza Jeřabková, et al.. (2016). Potassium detection in the clear atmosphere of a hot-Jupiter: FORS2 transmission spectroscopy of WASP-17b. elib (German Aerospace Center). 15 indexed citations
12.
Borkovits, T., et al.. (2013). THE ANTICORRELATED NATURE OF THE PRIMARY AND SECONDARY ECLIPSE TIMING VARIATIONS FOR THE KEPLER CONTACT BINARIES. DSpace@MIT (Massachusetts Institute of Technology). 30 indexed citations
13.
14.
Pasternacki, T., Sz. Csizmadia, J. Cabrera, et al.. (2011). A VARIABLE STAR CENSUS IN A PERSEUS FIELD. The Astronomical Journal. 142(4). 114–114. 7 indexed citations
15.
Csizmadia, Sz., Z. Nagy, T. Borkovits, et al.. (2008). EM Cygni: A study of its eclipse timings. Astronomische Nachrichten. 329(1). 39–43. 6 indexed citations
16.
Szalai, Tamás, L. L. Kiss, Szabolcs Mészáros, J. Vinkó, & Sz. Csizmadia. (2007). Physical parameters and multiplicity of five southern closeeclipsing binaries. Springer Link (Chiba Institute of Technology). 47 indexed citations
17.
Csizmadia, Sz., et al.. (2007). Updated catalogue of the light curve solutions of contact binary stars. Astronomische Nachrichten. 328(8). 821–824. 2 indexed citations
18.
Csizmadia, Sz., et al.. (2006). New Times of Minima of Some Eclipsing Binary Systems. IBVS. 5736. 1. 4 indexed citations
19.
Kun, M., J. A. Acosta‐Pulido, A. Moór, et al.. (2004). Optical and near infrared observations of V1647 Ori and McNeil's Nebula in February-April 2004. arXiv (Cornell University).
20.
Ábrahám, P., Á. Kóspál, Sz. Csizmadia, et al.. (2004). The infrared properties of the new outburst star\nIRAS 05436–0007 in quiescent phase. Springer Link (Chiba Institute of Technology). 32 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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