P. Székely

712 total citations
24 papers, 299 citations indexed

About

P. Székely is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, P. Székely has authored 24 papers receiving a total of 299 indexed citations (citations by other indexed papers that have themselves been cited), including 20 papers in Astronomy and Astrophysics, 8 papers in Instrumentation and 2 papers in Computational Mechanics. Recurrent topics in P. Székely's work include Stellar, planetary, and galactic studies (14 papers), Astrophysics and Star Formation Studies (12 papers) and Astronomy and Astrophysical Research (8 papers). P. Székely is often cited by papers focused on Stellar, planetary, and galactic studies (14 papers), Astrophysics and Star Formation Studies (12 papers) and Astronomy and Astrophysical Research (8 papers). P. Székely collaborates with scholars based in Hungary, Australia and United States. P. Székely's co-authors include L. L. Kiss, T. R. Bedding, Geraint F. Lewis, A. Siebert, Rodrigo Ibata, Richard R. Lane, Gyula M. Szabó, A. Derekas, Z. Balog and B. Csák 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

P. Székely

21 papers receiving 296 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
P. Székely Hungary 10 285 118 26 14 10 24 299
G. Casali Italy 11 263 0.9× 145 1.2× 24 0.9× 18 1.3× 5 0.5× 21 281
Sarah Ballard United States 9 243 0.9× 95 0.8× 9 0.3× 10 0.7× 10 1.0× 26 247
E. Jofré Argentina 9 297 1.0× 121 1.0× 19 0.7× 15 1.1× 17 1.7× 23 313
Eric Stempels United States 8 349 1.2× 101 0.9× 12 0.5× 7 0.5× 14 1.4× 73 357
Keith Y. Matthews United States 4 238 0.8× 117 1.0× 17 0.7× 8 0.6× 11 1.1× 5 258
A. Milone Brazil 8 254 0.9× 118 1.0× 25 1.0× 11 0.8× 12 1.2× 17 268
A. Garofalo Italy 11 283 1.0× 168 1.4× 17 0.7× 24 1.7× 8 0.8× 19 300
D. T. Andreasen Portugal 8 213 0.7× 97 0.8× 19 0.7× 19 1.4× 10 1.0× 11 217
I. Toledo Chile 6 339 1.2× 156 1.3× 27 1.0× 13 0.9× 5 0.5× 13 343
S. Duffau Chile 12 414 1.5× 192 1.6× 22 0.8× 19 1.4× 5 0.5× 22 417

Countries citing papers authored by P. Székely

Since Specialization
Citations

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

Fields of papers citing papers by P. Székely

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of P. Székely

This figure shows the co-authorship network connecting the top 25 collaborators of P. Székely. A scholar is included among the top collaborators of P. Székely 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 P. Székely. P. Székely 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.
Barna, Barbara P., Tamás Szalai, J. Vinkó, et al.. (2025). SN 2022xlp: The second-known well-observed, intermediate-luminosity Iax supernova. Astronomy and Astrophysics. 703. A64–A64.
2.
Nagy, Andrea, Réka Könyves-Tóth, Tamás Szalai, et al.. (2023). Three is the magic number: Distance measurement of NGC 3147 using SN 2021hpr and its siblings. Astronomy and Astrophysics. 677. A183–A183.
3.
Székely, P., et al.. (2020). Learning Approaches and Attitudes Toward Cognitive Enhancers in UK University Students. Journal of Psychoactive Drugs. 52(3). 248–254. 4 indexed citations
4.
Szabados, L., A. Derekas, L. L. Kiss, et al.. (2013). Discovery of the spectroscopic binary nature of six southern Cepheids. Monthly Notices of the Royal Astronomical Society. 430(3). 2018–2028. 8 indexed citations
5.
Anderson, Richard I., A. Derekas, L. L. Kiss, et al.. (2013). Discovery of the spectroscopic binary nature of three bright southern Cepheids. Monthly Notices of the Royal Astronomical Society. 434(1). 870–877. 9 indexed citations
6.
Lane, Richard R., L. L. Kiss, Geraint F. Lewis, et al.. (2011). AAOmega spectroscopy of 29 351 stars in fields centered on ten Galactic globular clusters. Springer Link (Chiba Institute of Technology). 33 indexed citations
7.
Lane, Richard R., L. L. Kiss, Geraint F. Lewis, et al.. (2010). Halo globular clusters observed with AAOmega: dark matter content, metallicity and tidal heating. Monthly Notices of the Royal Astronomical Society. 406(4). 2732–2742. 71 indexed citations
8.
Lane, Richard R., L. L. Kiss, Geraint F. Lewis, et al.. (2009). Testing Newtonian gravity with AAOmega: mass-to-light profiles and metallicity calibrations from 47 Tuc and M55. Monthly Notices of the Royal Astronomical Society. 401(4). 2521–2530. 38 indexed citations
9.
Derekas, A., L. L. Kiss, T. R. Bedding, et al.. (2009). Binarity and multiperiodicity in high-amplitude δ Scuti stars. Monthly Notices of the Royal Astronomical Society. 394(2). 995–1008. 16 indexed citations
10.
Kiss, L. L., P. Székely, T. R. Bedding, G. Á. Bakos, & Geraint F. Lewis. (2007). A Wide-Field Kinematic Survey for Tidal Tails around Five Globular Clusters. The Astrophysical Journal. 659(2). L129–L132. 12 indexed citations
11.
Székely, P., L. L. Kiss, R. J. Jackson, et al.. (2006). RR Lyrae stars in the southern globular cluster NGC 362. Springer Link (Chiba Institute of Technology). 17 indexed citations
12.
Szabó, Gy. M., Gábor Fürész, P. Székely, & Á. Szentgyörgyi. (2006). Kinematics and Variable Stars in NGC 1907 and NGC 1912. 349. 339.
13.
Uemura, Makoto, R. E. Mennickent, Rod Stubbings, et al.. (2005). Outburst of a Black Hole X-ray Binary V4641 Sgr in 2004 July. IBVS. 5626. 1. 1 indexed citations
14.
Griffin, Julian L., L. L. Kiss, Makoto Uemura, et al.. (2005). New clues on outburst mechanisms and improved spectroscopic elements of the black hole binary V4641 Sagittarii★. Monthly Notices of the Royal Astronomical Society. 363(3). 882–890. 12 indexed citations
15.
Székely, P., L. L. Kiss, Gy. M. Szabó, et al.. (2005). CCD photometry of 23 minor planets. Planetary and Space Science. 53(9). 925–936. 5 indexed citations
16.
Csorba, Roland, et al.. (2004). [Child sexual abuse].. PubMed. 145(5). 223–7. 2 indexed citations
17.
Szabó, Gy. M., K. Sárneczky, J. Vinkó, et al.. (2003). Photometry of SN 2002bo with template image subtraction. Springer Link (Chiba Institute of Technology). 4 indexed citations
18.
Székely, P.. (2003). A CCD Photometric Search for Pulsations in SZ Her. Information Bulletin on Variable Stars. 5467. 1. 1 indexed citations
19.
Derekas, A., L. L. Kiss, P. Székely, et al.. (2003). A photometric monitoring of bright high-amplitudeδScuti stars. Astronomy and Astrophysics. 402(2). 733–743. 12 indexed citations
20.
Kiss, L. L., A. Derekas, Szabolcs Mészáros, & P. Székely. (2002). A photometric monitoring of bright high-amplitudeδScuti stars. Astronomy and Astrophysics. 394(3). 943–948. 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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