Eva Šrámková

614 total citations
28 papers, 373 citations indexed

About

Eva Šrámková is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Geophysics. According to data from OpenAlex, Eva Šrámková has authored 28 papers receiving a total of 373 indexed citations (citations by other indexed papers that have themselves been cited), including 28 papers in Astronomy and Astrophysics, 7 papers in Nuclear and High Energy Physics and 6 papers in Geophysics. Recurrent topics in Eva Šrámková's work include Pulsars and Gravitational Waves Research (27 papers), Astrophysical Phenomena and Observations (24 papers) and Astrophysics and Cosmic Phenomena (7 papers). Eva Šrámková is often cited by papers focused on Pulsars and Gravitational Waves Research (27 papers), Astrophysical Phenomena and Observations (24 papers) and Astrophysics and Cosmic Phenomena (7 papers). Eva Šrámková collaborates with scholars based in Czechia, Poland and Sweden. Eva Šrámková's co-authors include Gabriel Török, Z. Stuchlík, M. A. Abramowicz, Zdeněk Stuchlík, Martin Urbanec, Ulf Torkelsson, Jiří Horák, O. Straub, W. Kluźniak and Omer Blaes 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

Eva Šrámková

25 papers receiving 362 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Eva Šrámková Czechia 11 365 201 41 32 14 28 373
P. Rebusco Germany 9 395 1.1× 164 0.8× 54 1.3× 32 1.0× 7 0.5× 16 404
Ding-Xiong Wang China 11 372 1.0× 203 1.0× 19 0.5× 16 0.5× 8 0.6× 62 385
Alejandra Jiménez-Rosales Germany 8 289 0.8× 170 0.8× 19 0.5× 19 0.6× 17 1.2× 11 300
Sean M. Ressler United States 12 551 1.5× 327 1.6× 54 1.3× 25 0.8× 5 0.4× 24 566
Christian Alig Germany 8 436 1.2× 100 0.5× 33 0.8× 31 1.0× 23 1.6× 13 445
Petr Slaný Czechia 13 615 1.7× 419 2.1× 16 0.4× 17 0.5× 12 0.9× 31 626
Menglei Zhou China 13 363 1.0× 209 1.0× 21 0.5× 29 0.9× 7 0.5× 26 372
Gibwa Musoke Netherlands 8 338 0.9× 184 0.9× 22 0.5× 25 0.8× 5 0.4× 12 357
M. L. Trippe United States 10 353 1.0× 130 0.6× 15 0.4× 21 0.7× 18 1.3× 13 358
Lorenzo Sironi United States 9 304 0.8× 232 1.2× 22 0.5× 8 0.3× 17 1.2× 12 333

Countries citing papers authored by Eva Šrámková

Since Specialization
Citations

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

Fields of papers citing papers by Eva Šrámková

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Eva Šrámková

This figure shows the co-authorship network connecting the top 25 collaborators of Eva Šrámková. A scholar is included among the top collaborators of Eva Šrámková 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 Eva Šrámková. Eva Šrámková 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.
Török, Gabriel, Jiří Horák, O. Straub, et al.. (2024). Accretion tori around rotating neutron stars. Astronomy and Astrophysics. 691. A168–A168.
2.
Török, Gabriel, Jiří Horák, Martin Urbanec, et al.. (2024). Accretion tori around rotating neutron stars. Astronomy and Astrophysics. 691. A167–A167. 2 indexed citations
3.
Karas, V., et al.. (2023). Timing of accreting neutron stars with future X-ray instruments: towards new constraints on dense matter equation of state. Contributions of the Astronomical Observatory Skalnaté Pleso. 53(4).
4.
Török, Gabriel, et al.. (2022). Simple Analytic Formula Relating the Mass and Spin of Accreting Compact Objects to Their Rapid X-Ray Variability. The Astrophysical Journal. 929(1). 28–28. 6 indexed citations
5.
Šrámková, Eva, Jiří Horák, O. Straub, et al.. (2022). Oscillations of fluid tori around neutron stars. Astronomische Nachrichten. 344(1-2). 1 indexed citations
6.
Šrámková, Eva, Gabriel Török, Jiří Horák, et al.. (2020). Models of high-frequency quasi-periodic oscillations and black hole spin estimates in Galactic microquasars. Springer Link (Chiba Institute of Technology). 19 indexed citations
7.
Török, Gabriel, et al.. (2019). Mass of the active galactic nucleus black hole XMMUJ134736.6+173403. Astronomy and Astrophysics. 622. L8–L8. 8 indexed citations
8.
Stuchlík, Zdeněk, Jan Schee, Eva Šrámková, & Gabriel Török. (2017). Superspinning Quark Stars Limited by Twin High-FrequencyQuasiperiodic Oscillations. Acta Astronomica. 67(2). 181–201. 2 indexed citations
9.
Šrámková, Eva, et al.. (2017). Super-spinning compact objects and models of high-frequency quasi-periodic oscillations observed in Galactic microquasars. Astronomy and Astrophysics. 607. A69–A69. 10 indexed citations
10.
Török, Gabriel, et al.. (2015). Twin peak high-frequency quasi-periodic oscillations as a spectral imprint of dual oscillation modes of accretion tori. Springer Link (Chiba Institute of Technology). 8 indexed citations
11.
Šrámková, Eva, et al.. (2015). Black hole spin inferred from 3:2 epicyclic resonance model of high-frequency quasi-periodic oscillations. Springer Link (Chiba Institute of Technology). 11 indexed citations
12.
Török, Gabriel, et al.. (2015). Twin peak quasi-periodic oscillations as signature of oscillating cusp torus. Monthly Notices of the Royal Astronomical Society Letters. 457(1). L19–L23. 29 indexed citations
13.
Török, Gabriel, V. Karas, Michal Dovčiak, et al.. (2014). Power density spectra of modes of orbital motion in strongly curved space–time: obtaining the observable signal. Monthly Notices of the Royal Astronomical Society. 439(2). 1933–1939. 18 indexed citations
14.
Török, Gabriel, et al.. (2014). Super-spinning compact objects and models of high-frequency quasi-periodic oscillations observed in Galactic microquasars. Astronomy and Astrophysics. 572. A79–A79. 10 indexed citations
15.
Mazur, Grzegorz P., F. Vincent, Maria C. Johansson, et al.. (2013). Towards modeling quasi-periodic oscillations of microquasars with oscillating slender tori. Springer Link (Chiba Institute of Technology). 8 indexed citations
16.
Török, Gabriel, et al.. (2011). Confronting the models of 3:2 quasiperiodic oscillations with the rapid spin of the microquasar GRS 1915+105. Astronomy and Astrophysics. 531. A59–A59. 90 indexed citations
17.
Urbanec, Martin, et al.. (2010). Disc-oscillation resonance and neutron star QPOs: 3:2 epicyclic orbital model. Astronomy and Astrophysics. 522. A72–A72. 13 indexed citations
18.
Šrámková, Eva, et al.. (2008). On magnetic-field induced non-geodesic corrections to the relativistic precession QPO model. AIP conference proceedings. 1054. 123–128. 1 indexed citations
19.
Šrámková, Eva, Ulf Torkelsson, & M. A. Abramowicz. (2007). Oscillations of tori in the pseudo-Newtonian potential. Astronomy and Astrophysics. 467(2). 641–646. 18 indexed citations
20.
Šrámková, Eva. (2005). Epicyclic oscillation modes of a Newtonian, non‐slender torus. Astronomische Nachrichten. 326(9). 835–837. 7 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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026