B. Kalomeni

909 total citations
30 papers, 573 citations indexed

About

B. Kalomeni is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, B. Kalomeni has authored 30 papers receiving a total of 573 indexed citations (citations by other indexed papers that have themselves been cited), including 29 papers in Astronomy and Astrophysics, 9 papers in Instrumentation and 5 papers in Nuclear and High Energy Physics. Recurrent topics in B. Kalomeni's work include Stellar, planetary, and galactic studies (22 papers), Astrophysics and Star Formation Studies (15 papers) and Astro and Planetary Science (10 papers). B. Kalomeni is often cited by papers focused on Stellar, planetary, and galactic studies (22 papers), Astrophysics and Star Formation Studies (15 papers) and Astro and Planetary Science (10 papers). B. Kalomeni collaborates with scholars based in Türkiye, United States and Australia. B. Kalomeni's co-authors include K. Yakut, A. Levine, T. Borkovits, C. İbanoǧlu, S. Rappaport, I. El Mellah, Katherine M. Deck, Roberto Sanchis-Ojeda, L. A. Nelson and Edwin S. Kite 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

B. Kalomeni

27 papers receiving 557 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
B. Kalomeni Türkiye 13 566 204 38 33 15 30 573
M.-A. Dupret Belgium 15 700 1.2× 333 1.6× 47 1.2× 37 1.1× 11 0.7× 26 719
K. Yakut Türkiye 12 576 1.0× 203 1.0× 32 0.8× 42 1.3× 20 1.3× 41 593
C. Maceroni Italy 11 417 0.7× 184 0.9× 40 1.1× 13 0.4× 14 0.9× 43 427
P. G. Niarchos Greece 13 501 0.9× 188 0.9× 50 1.3× 23 0.7× 17 1.1× 66 514
A. Liakos Greece 13 447 0.8× 171 0.8× 28 0.7× 22 0.7× 19 1.3× 49 456
M. Grosso Argentina 12 565 1.0× 203 1.0× 40 1.1× 13 0.4× 21 1.4× 23 576
A. Derekas Hungary 16 584 1.0× 257 1.3× 51 1.3× 15 0.5× 21 1.4× 48 599
Daniel L. Holdsworth United Kingdom 13 423 0.7× 217 1.1× 52 1.4× 30 0.9× 11 0.7× 38 432
Miloslav Zejda Czechia 17 794 1.4× 268 1.3× 72 1.9× 30 0.9× 21 1.4× 97 812
Elizabeth Jeffery United States 11 517 0.9× 267 1.3× 25 0.7× 26 0.8× 28 1.9× 21 531

Countries citing papers authored by B. Kalomeni

Since Specialization
Citations

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

Fields of papers citing papers by B. Kalomeni

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of B. Kalomeni

This figure shows the co-authorship network connecting the top 25 collaborators of B. Kalomeni. A scholar is included among the top collaborators of B. Kalomeni 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 B. Kalomeni. B. Kalomeni 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.
Yakut, K., B. Kalomeni, & S. Rappaport. (2025). A novel approach to determining the age of stellar clusters: application to NGC 188. Monthly Notices of the Royal Astronomical Society. 542(3). 1817–1826. 1 indexed citations
2.
Yakut, K., B. Kalomeni, S. Rappaport, & Veselin B. Kostov. (2025). A deep look into the intermediate-age open cluster NGC 2506: what binary systems reveal about cluster distance and age. Monthly Notices of the Royal Astronomical Society. 544(1). 271–282.
3.
Kalomeni, B., et al.. (2017). The physical properties and orbital parameters of the triple system V402 Lac. New Astronomy. 60. 65–68. 2 indexed citations
4.
Rappaport, S., Andrew Vanderburg, L. A. Nelson, et al.. (2017). WD 1202-024: the shortest-period pre-cataclysmic variable. Monthly Notices of the Royal Astronomical Society. 471(1). 948–961. 14 indexed citations
5.
Rappaport, S., H. Lehmann, B. Kalomeni, et al.. (2016). A quintuple star system containing two eclipsing binaries. Monthly Notices of the Royal Astronomical Society. 462(2). 1812–1825. 9 indexed citations
6.
Yakut, K., P. P. Eggleton, B. Kalomeni, Christopher A. Tout, & J. J. Eldridge. (2015). A turn-off detached binary star V568 Lyr in theKeplerfield of the oldest open cluster (NGC 6791) in the Galaxy. Monthly Notices of the Royal Astronomical Society. 453(3). 2938–2943. 6 indexed citations
7.
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
8.
Chiang, Eugene, A. Levine, B. Kalomeni, et al.. (2012). POSSIBLE DISINTEGRATING SHORT-PERIOD SUPER-MERCURY ORBITING KIC 12557548. DSpace@MIT (Massachusetts Institute of Technology). 102 indexed citations
9.
Telting, J. H., R. H. Østensen, A. S. Baran, et al.. (2012). Three ways to solve the orbit of KIC 11 558 725: a 10-day beaming sdB+WD binary with a pulsating subdwarf. Astronomy and Astrophysics. 544. A1–A1. 52 indexed citations
10.
Kalomeni, B.. (2012). Short and long time-scale variability in magnetic cataclysmic variables: long-term monitoring of polars. Monthly Notices of the Royal Astronomical Society. 422(2). 1601–1608. 10 indexed citations
11.
Kalomeni, B.. (2011). Long-Term Monitoring of Polars. Proceedings of the International Astronomical Union. 7(S282). 91–92. 1 indexed citations
12.
Kalomeni, B., et al.. (2011). Marginally low mass ratio close binary system V1191 Cyg. New Astronomy. 17(1). 46–49. 17 indexed citations
13.
Kalomeni, B., et al.. (2011). Close binary system GO Cyg. New Astronomy. 17(3). 296–302. 3 indexed citations
14.
Yakut, K., W. Zima, B. Kalomeni, et al.. (2009). Close binary and other variable stars in the solar-age Galactic open cluster M 67. Springer Link (Chiba Institute of Technology).
15.
Yakut, K., W. Zima, B. Kalomeni, et al.. (2009). Close binary and other variable stars in the solar-age Galactic open cluster M 67. Astronomy and Astrophysics. 503(1). 165–176. 28 indexed citations
16.
Kalomeni, B., et al.. (2005). Cyclotron emission from accretion plasma columns in magnetic cataclysmic variable stars. Astronomy and Astrophysics. 439(3). 823–833. 2 indexed citations
17.
Yakut, K., B. Kalomeni, & C. İbanoǧlu. (2004). An analysis of the light curves of the overcontact binary system V2388 Ophiuchi. Astronomy and Astrophysics. 417(2). 725–730. 24 indexed citations
18.
Yakut, K., А. Е. Тарасов, C. İbanoǧlu, et al.. (2003). Basic physical properties of the close binary V497 Cep in the open cluster NGC 7160. Astronomy and Astrophysics. 405(3). 1087–1093. 5 indexed citations
19.
Yakut, K., et al.. (2003). New light curve analysis and period changes of the overcontact binary XY Leonis. Astronomy and Astrophysics. 401(3). 1095–1100. 40 indexed citations
20.
Kalomeni, B., et al.. (2001). Viscous Dissipation of Magnetosonic Waves in Solar Corona. TURKISH JOURNAL OF PHYSICS. 25(3). 195–214. 1 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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